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Proceedings of the 2010 Australian Geothermal Energy Conference

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G E O S C I E N C E A U S T R A L I A<strong>Proceedings</strong> <strong>of</strong> <strong>the</strong> <strong>2010</strong> <strong>Australian</strong>Geo<strong>the</strong>rmal <strong>Energy</strong> <strong>Conference</strong>Gurgenci, H. and Weber, R. D.Record<strong>2010</strong>/35GeoCat #71204APPLYING GEOSCIENCE TO AUSTR ALIA’S MOST IMPORTANT CHALLENGES


<strong>Proceedings</strong> <strong>of</strong> <strong>the</strong> <strong>2010</strong> <strong>Australian</strong>Geo<strong>the</strong>rmal <strong>Energy</strong> <strong>Conference</strong>GEOSCIENCE AUSTRALIA Record <strong>2010</strong>/35Edited byHal Gurgenci 1 and Rikki Weber 21 Queensland Geo<strong>the</strong>rmal <strong>Energy</strong> Centre, The University <strong>of</strong> Queensland, St Lucia 40722 Geoscience Australia, GPO Box 378, Canberra, ACT 2601


Department <strong>of</strong> Resources, <strong>Energy</strong> and TourismMinister for Resources and <strong>Energy</strong>: The Hon. Martin Ferguson, AM MPSecretary: Mr Drew ClarkeGeoscience AustraliaChief Executive Officer: Dr Chris Pigram© Commonwealth <strong>of</strong> Australia, <strong>2010</strong>This work is copyright. Apart from any fair dealings for <strong>the</strong> purpose <strong>of</strong> study, research, criticism,or review, as permitted under <strong>the</strong> Copyright Act 1968, no part may be reproduced by any processwithout written permission. Copyright is <strong>the</strong> responsibility <strong>of</strong> <strong>the</strong> Chief Executive Officer,Geoscience Australia. Requests and enquiries should be directed to <strong>the</strong> Chief Executive Officer,Geoscience Australia, GPO Box 378 Canberra ACT 2601.Geoscience Australia has tried to make <strong>the</strong> information in this product as accurate as possible.However, it does not guarantee that <strong>the</strong> information is totally accurate or complete. Therefore, youshould not solely rely on this information when making a commercial decision.ISSN 1448-2177 ISBN 978-1-921781-38-4GeoCat # 71204Recommended bibliographic reference: Gurgenci, H. and Weber, R. D. (editors), <strong>2010</strong>.<strong>Proceedings</strong> <strong>of</strong> <strong>the</strong> <strong>2010</strong> <strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong> <strong>Conference</strong>, Geoscience Australia,Record <strong>2010</strong>/35.Recommended bibliographic citation: Glikson, A. and Uysal, T.<strong>2010</strong>. Evidence <strong>of</strong> impactshock metamorphism in basement granitoids, Cooper Basin, South Australia, in: Gurgenci andWeber (editors), <strong>Proceedings</strong> <strong>of</strong> <strong>the</strong> <strong>2010</strong> <strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong> <strong>Conference</strong>, GeoscienceAustralia, Record <strong>2010</strong>/35.Cover illustration: 3D image <strong>of</strong> gravity inversion modelling in <strong>the</strong> area between Mt Isa and <strong>the</strong>Georgetown Inlier, Queensland, viewed obliquely from <strong>the</strong> south. The red bodies enclose regions<strong>of</strong> low density interpreted as granites located at depth beneath Millungera Basin sediments, <strong>the</strong>base <strong>of</strong> which is shown as <strong>the</strong> yellow surface. The interpreted granites are shown projected abovean image <strong>of</strong> <strong>the</strong> Bouguer Gravity field, from which <strong>the</strong> inversion model was generated. Courtesy<strong>of</strong> Alison Kirkby, Geoscience Australia.


The Convenors would like to thank <strong>the</strong> following sponsors for <strong>the</strong>ir kind support:Gold SponsorsSilver SponsorsBronze Sponsors<strong>Conference</strong> Dinner SponsorHappy Hour Sponsors


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>IntroductionThis volume is a compilation <strong>of</strong> Extended Abstracts presented at <strong>the</strong> <strong>2010</strong> <strong>Australian</strong>Geo<strong>the</strong>rmal <strong>Energy</strong> <strong>Conference</strong>, 17-19 November <strong>2010</strong>, Adelaide Convention Centre,Adelaide, organised by <strong>the</strong> <strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong> Association and <strong>the</strong> <strong>Australian</strong>Geo<strong>the</strong>rmal <strong>Energy</strong> Group.As editors <strong>of</strong> <strong>the</strong>se proceedings, we first would like to thank <strong>the</strong> Technical Committeewho have been very generous with <strong>the</strong>ir time to review <strong>the</strong> submissions and to workwith <strong>the</strong> authors <strong>of</strong> <strong>the</strong> accepted submissions to improve <strong>the</strong> quality <strong>of</strong> <strong>the</strong> Abstractsand <strong>the</strong> presentations.We also thank <strong>the</strong> <strong>Conference</strong> Chair Tony Hill and <strong>the</strong> rest <strong>of</strong> <strong>the</strong> Organising Committeewho were brave enough to take on <strong>the</strong> job organising this second event on behalf <strong>of</strong> <strong>the</strong><strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong> Association and <strong>the</strong> <strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong> Group.Rob Bulfield and Sapro <strong>Conference</strong> Management have done an excellent job in assisting<strong>the</strong> organisation.We also thank again <strong>the</strong> sponsoring companies for <strong>the</strong>ir generous support.We thank Geoscience Australia for publishing <strong>the</strong> proceedings.Finally, we thank all delegates without whose participation none <strong>of</strong> this is worthwhile.Hal GurgenciRikki Weberi


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong><strong>Conference</strong> Organising CommitteeSusan Jeans, AGEAVicki Cleavland, AGEADr Graeme Beardsmore, Hot Dry Rocks Pty LtdDr Betina Bendall, PIRSADr Anthony Budd, Geoscience AustraliaBarry Goldstein, PIRSAPr<strong>of</strong>essor Hal Gurgenci, University QueenslandChris Mat<strong>the</strong>ws, AGEAJonathan Teubner, Petra<strong>the</strong>rmProgram Technical PanelPr<strong>of</strong>essor Hal Gurgenci (chair), Queensland Geo<strong>the</strong>rmal <strong>Energy</strong> Centre <strong>of</strong> Excellence,Dr Anthony Budd, Geoscience Australia,Delton Chen, Geodynamics Ltd,Gareth Cooper, Hot Dry Rocks Pty LtdPeter Dowd, The University <strong>of</strong> AdelaideDes Fitzgerald, Intrepid Geophysics,Dr Massimo Gasparon, The University <strong>of</strong> QueenslandHelen Gibson, GeoIntrepidAlison Kirkby, Geoscience AustraliaAlan Knights, Green Rock Pty LtdChris Mat<strong>the</strong>ws, AGEA,Tony Meixner, Geoscience AustraliaPr<strong>of</strong>essor Behdad Moghtaderi, The University <strong>of</strong> NewcastlePr<strong>of</strong>essor Klaus Regenauer-Lieb, The University <strong>of</strong> Western AustraliaPeter Reid, Petra<strong>the</strong>rm LtdMichel Rosener, Geodynamics LtdDr Ca<strong>the</strong>rine Stafford, Granite Power LtdJonathan Teubner, Petra<strong>the</strong>rmDr Adrian Williams, Geodynamics Ltd DrDoone Wyborn, Geodynamics LtdDr Yung Ngothai, The University <strong>of</strong> Adelaide<strong>Conference</strong> OrganisersRob Bulfield Sapro <strong>Conference</strong> Management Ph: 08 8274 6043 Fax: 08 8274 6000www.sapro.com.auii


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Stream OneA.R. Budd, E.J. Gerner, A.M. Kirkby, R.D. Weber, A.J. Meixner and D.C.ChampionGeoscience Australia’s Onshore <strong>Energy</strong> Security Program: progress by <strong>the</strong> Geo<strong>the</strong>rmal<strong>Energy</strong> ProjectCara Danis and Craig O’Neill3D <strong>the</strong>rmal modelling VS down-hole temperature extrapolation and <strong>the</strong> implications fortargeting potential geo<strong>the</strong>rmal anomalies: a Sydney Basin case studM. Hand and Y. NgothaiSouth <strong>Australian</strong> Geo<strong>the</strong>rmal Research CentreHearst Ghabri Mehran, Robert B. Retallcik, Trent and Killin KevinApplication <strong>of</strong> magnetotellurics in geo<strong>the</strong>rmal reservoir characterizationDavid Jenson, Kerry Parker, Ron Palmer and Bertus de GraffHutton Sandstone – a viable geo<strong>the</strong>rmal developmentAshok A. Kaniyal, Jonathan J. Pincus and Graham J. NathanInvestment in common-use network infrastructure to trigger incremental expansion ingeo<strong>the</strong>rmal energy generating capital stockIvan Kočiš, Tomáš Krišt<strong>of</strong>ič, and Igor KočišUltra deep drilling technologies for geo<strong>the</strong>rmal energy productionp1p4p9p11p14p20p21Gideon B. Kuncoro, Yung Ngothai, Brian O’Neill, Allan Pring and Joel BruggerA Preliminary Study on Na-Cl-H 2 O-Rock Interactions <strong>of</strong> <strong>the</strong> Hot Fractured Rock Geo<strong>the</strong>rmalSystem in Cooper Basin, South Australiap24Adrian Larking and Gary MeyerGeo<strong>the</strong>rmal <strong>Energy</strong> in <strong>the</strong> Perth Basin, AustraliaComparisons with <strong>the</strong> Rhine Grabenp30A.D. Long, A.R. Budd, H. Gurgenci, M. Hand, C. Huddlestone-Holmes, B. Moghtaderi and K.Regenauer-LiebAustralia’s Geo<strong>the</strong>rmal Research Activitiesp35V. Marshall, J. Van Zyl, S.E. Byron, T. Uysal and M. GasparonComparative petrology & geochemistry <strong>of</strong> high heat-producing granites in Australia & Europep41Craig McClarren, Massimo Gasparon and I. Tonguç UysalGeo<strong>the</strong>rmal Prospection Using Existing Groundwater Geochemical and Thermal Datasets:Identifying Regions <strong>of</strong> Interest in Queensland from Government Well and Bore Datap48Malcolm B. McInnesGenie Impact Drilling: Synopsis <strong>of</strong> a New Hard Rock Drilling DevelopmentAlexander W. Middleton, I Tonguç Uysal, Massimo Gasparon and Scott BryanHydro<strong>the</strong>rmal alteration aspects <strong>of</strong> high heat producing granites in Australia & EuropeThomas Poulet, Soazig Corbel and Michael StegherrA Geo<strong>the</strong>rmal Web Catalog Service for <strong>the</strong> Perth Basinp52p59p64Martin Pujol, Grant Bolton and Fabrice GolfierFlow and heat modelling <strong>of</strong> a Hot Sedimentary Aquifer (HSA) for direct-use geo<strong>the</strong>rmal heatiii


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>production in <strong>the</strong> Perth urban area, Western Australia (WA)p69Sukanta RoyGeo<strong>the</strong>rmal Exploration in Indiap75Behnam Talebi, Mark Maxwell, Sarah Sargent and Steven BowdenQueensland Coastal Geo<strong>the</strong>rmal <strong>Energy</strong> Initiative – An Approach to a Regional Assessmentp81David H. Taylor, Ben Harrison, Michelle Ayling and Kate BassanoGeo<strong>the</strong>rmal Exploration in Victoria, AustraliaI. Tonguç Uysal, Alexander W. Middleton, Robert Bolhar and Massimo GasparonGeochemistry <strong>of</strong> silica rocks in <strong>the</strong> Drummond Basin as a record <strong>of</strong> geo<strong>the</strong>rmal potentialp87p91Gordon Webb and Ben HarrisonEstimates <strong>of</strong> <strong>the</strong> magnitude <strong>of</strong> topographical effects on surface heat flow from finite elementmodellingp94Doone Wyborn, Robert Hogarth, Delton Chen and Michel RosenerThe next <strong>Australian</strong> EGS Resevoir – Jolokia 1 stimulationChaoshui XuOptimised Fracture Network Model for Habanero Reservoirp97p98Stream TwoAleks D. Atrens, Hal Gurgenci and Victor RudolphProgress in CO 2 -based EGSp104Peter Barnett and Tim EvansExploration and assessment <strong>of</strong> Hot Sedimentary Aquifer (HSA) geo<strong>the</strong>rmal resources in <strong>the</strong>Otway Basin Victoriap106J.E. Davey and J.T. KeetleyValidation <strong>of</strong> Geo<strong>the</strong>rmal Exploration Techniques for Analysing Hot Sedimentary Aquifer andEnhanced Geo<strong>the</strong>rmal Systemsp112Bertus de Graaf, Ian Reid, Ron Palmer, David Jenson and Kerry ParkerSalamander-1 – a geo<strong>the</strong>rmal well based on petroleum exploration resultsp117Ben Clennel, Lionel Esteban, Ludovic Ricard, Mat<strong>the</strong>w Josh, Cameron Huddlestone-Holmes,Jie Liu and Klaus Regenauer-LiebPetrophysical Methods for Characterization <strong>of</strong> Geo<strong>the</strong>rmal Reservoirsp123Farizal and Prashanti Amelia AnisaGeo<strong>the</strong>rmal Power Plant Competitiveness in Indonesia: Economic and Fiscal Policy Analysisp130Desmond Fitzgerald and Raymond SeikelA Method For Calibrating <strong>Australian</strong> Temperature-Depth ModelsAndrew Y. Glikson and I. Tonguç UysalEvidence <strong>of</strong> impact shock metamorphism in basement granitoids, Cooper Basin, SouthAustraliaT. HarinarayanaGeo<strong>the</strong>rmal <strong>Energy</strong> in India: Past, Present and Future Plansp138p141p148Peter Leary, Peter Malin, Eylon Shalev and Stephen Onachaiv


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Aquifer heterogeneity – is it properly assessed by wellbore samples and does it matter foraquifer heat extraction?p149Yan Liu, Huilin Xing, Zhenqun Guan and Hongwu ZhangAutomatic Meshing and Construction <strong>of</strong> a 3D Reservoir System: From Visualization towardsSimulationp157Luke Mortimer, Adnan Aydin and Craig T. SimmonsTargeting Faults <strong>of</strong> Geo<strong>the</strong>rmal Fluid Production: Exploring for Zones <strong>of</strong> Enhanced Permeabilityp163Grahame J.H. OliverAn EGS/HAS concept for SingaporeJared Peacock, Stephan Thiel, Graham Heinson and Louise McAllisterMonitoring EGS Reservoirs Using Magnetotelluricsp169p175Joshua Koh, Nima Gholizadeh-Doonechaly, Abdul Ravo<strong>of</strong> and Sheik RahmanReservoir characterisation and numerical modelling to reduce project risk and maximise <strong>the</strong>chance <strong>of</strong> success. An example <strong>of</strong> how to design a stimulation program and assess fluidproduction from <strong>the</strong> Soultz geo<strong>the</strong>rmal field, Francep179P. W. Reid, L. McAllister and M. MesseillerStatus <strong>of</strong> <strong>the</strong> Paralana 2 Hydraulic Stimulation ProgramAlvin I. Remoroza, Behdad Moghtaderi and Elham DoroodchiThree Dimensional Reservoir Simulations <strong>of</strong> Supercritical CO 2 EGSCa<strong>the</strong>rine E. StaffordMeasuring <strong>the</strong> Success <strong>of</strong> EGS Projects: An Historical to Present Day Perspectivep203p206p210J.F. Wellmann, F.G. Horowitz, L.P. Ricard and K. Regenauer-LiebEstimates <strong>of</strong> sustainable pumping in Hot Sedimentary Aquifers: Theoretical considerations,numerical simulations and <strong>the</strong>ir application to resource mappingp215Thomas W. Wideman, Jared M. Potter, Brett O’Leary and Adrian WilliamsHydro<strong>the</strong>rmal Spallation for <strong>the</strong> Treatment <strong>of</strong> Hydro<strong>the</strong>rmal and EGS Wells: a Cost-EffectiveMethod for Substantially Increasing Reservoir Production Flow Ratesp222Bisheng Wu, Bailin Wu, Xi Zhang and Rob JeffreyThermal effects on <strong>the</strong> wellbore stabilityMat<strong>the</strong>w Zengerer, Chris Mat<strong>the</strong>ws and Jerome Randabel3D Geological Modelling for Geo<strong>the</strong>rmal Exploration in <strong>the</strong> Torrens Hinge ZoneJ. Zhang and H.L. XingNumerical simulation <strong>of</strong> geo<strong>the</strong>rmal reservoir systems with multiphase fluidsXi Zhang and Robert G. JeffreyDevelopment <strong>of</strong> Hydraulic Fractures and Conductivity near a Wellborep226p232p243p247Stream ThreeDavid L. Battye, Peter J. Ashman and GUS J. NathanEconomics <strong>of</strong> geo<strong>the</strong>rmal feedwater heating for steam Rankine cyclesGraeme Beardsmore, Ladislaus Rybach, David Blackwell and Charles BaronA Protocol for Estimating and Mapping Global EGS Potentialp253p257v


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>G. Beardsmore, A. Budd, B. Goldstein, F. Holgate, G. Jeffress, A. Larking, J. Lawless, J. Libby,M. Middleton, P. Reid, C. Stafford, M. Ward and A. WilliamsChanges to Geo<strong>the</strong>rmal Reporting Code and Guidelines on Company Reporting p263Anna Collyer, Nadia Harrison and Natasha McNamaraGeo<strong>the</strong>rmal <strong>Energy</strong>’s Transition from Resource to Power: Legal Challengesp269Barry Goldstein, Betina Bendall, Alexandra Long, Michael Malavazos, David Dockshell andDavid LoveTrusted Regulation for Geo<strong>the</strong>rmal Resource Development (Including Induced SeismicityAssociated with EGS Operations)p273B.A. Goldstein, G. Hiriart, J.Tester, B. Bertani, R. Bromley, L.C.J. Gutierrez-Negrin, E.Huenges, H. Ragnarsson, A. Mongillo, M.A. Muraoka and V.I. ZuiGreat Expectations For Geo<strong>the</strong>rmal <strong>Energy</strong> – Forecast to 2100Hal Gurgenci and Zhiqiang GuanNew Design Concepts for Natural Draft Cooling TowersKamel HoomanQGECE Research on Heat Exchangers and Air-Cooled Condensersp281p290p294Robert McKibbin, Franklin Horowitz, Neville Fowkes and Brenda FlorioEquation-Free Summary <strong>of</strong> <strong>the</strong> <strong>2010</strong> Ma<strong>the</strong>matics in Industry Study Group on Geo<strong>the</strong>rmal DataAnalysis and Optimizationp298Jim LawlessStatus <strong>of</strong> Compliance With The Geo<strong>the</strong>rmal Reporting CodeJim LawlessApplication <strong>of</strong> <strong>the</strong> <strong>Australian</strong> Geo<strong>the</strong>rmal Reporting Code to “Conventional” Geo<strong>the</strong>rmalProjectsDavid N. Love, Gary Gibson, Russell Cuthbertson and Wayne PeckSmall <strong>Australian</strong> seismic events and <strong>the</strong>ir effectsSteve Kennedy, Chris Mat<strong>the</strong>ws, Damia Ettakadoumi and Cynthia CroweCommunity Consultation Best Practice ManualCraig Morgan and David PaulOptimising ORC use in <strong>Australian</strong> Geo<strong>the</strong>rmal Applicationsp302p305p306p400p402Yung Ngothai, Norio Yanagisawa, Allan Pring, Peter Rose, Brian O’Neill and Joel BruggerMineral scaling in geo<strong>the</strong>rmal fields: A reviewp405Donald J.B. Payne and Dezso KiralyDirect GeoExhange Cooling for <strong>the</strong> <strong>Australian</strong> Square Kilometer Array Pathfinder – Field Trialp410Klaus Regenauer-Lieb and <strong>the</strong> WAGCoE team, Peter Malin and <strong>the</strong> IESE team, Steve Harveyand <strong>the</strong> CSIRO CESRE team, Edson Nakagawa and CSIRO’s Geo<strong>the</strong>rmal & PetroleumPortfolio and Hal Gurgenci and <strong>the</strong> QGECE teamA Research Well for <strong>the</strong> Pawsey Geo<strong>the</strong>rmal Supercomputer Cooling Projectp416Kyra ReznikovFracture Stimulation – legal risks and liabilitiesAndrew S. Rowlands and Jason CzaplaQGECE Mobile Geo<strong>the</strong>rmal Test Plant & ORC Cycle Challengesp421p422vi


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Jonathan Teubner<strong>Australian</strong> geo<strong>the</strong>rmal Industry working with Investors – Defining <strong>the</strong> key parameterscontributing to <strong>the</strong> long run marginal cost <strong>of</strong> geo<strong>the</strong>rmal and providing a comparison benchmarkon <strong>the</strong> key unknownsp426O. Bouchel, T. Hazou, C. Scott and Roger WindersCOMMUNITY TRUST – Engagement & CommunicationMelissa Zillmann and Myria MakrasGeo<strong>the</strong>rmal energy legislation and developments in Queenslandp427p434vii


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Geoscience Australia’s Onshore <strong>Energy</strong> Security Program: progressby <strong>the</strong> Geo<strong>the</strong>rmal <strong>Energy</strong> ProjectA.R. Budd,* E.J. Gerner, A.L. Kirkby, R.D. Weber, A.J. Meixner and D.C. ChampionGeoscience Australia. GPO Box 378, Canberra, ACT 2601.*Corresponding author: Anthony.Budd@ga.gov.auAbstractGeoscience Australia’s $58.9M 5-year Onshore<strong>Energy</strong> Security Program began in 2006 andincludes a new Geo<strong>the</strong>rmal <strong>Energy</strong> Project.The project aims to assist <strong>the</strong> development <strong>of</strong> ageo<strong>the</strong>rmal industry in Australia by: providingprecompetitive geoscience information, includingacquisition <strong>of</strong> new data; informing <strong>the</strong> public andgovernment about Australia’s geo<strong>the</strong>rmalpotential; providing technical advice togovernment; and partnering with industry ininternational promotional events for <strong>the</strong> purpose<strong>of</strong> attracting investment.This abstract gives a brief summation <strong>of</strong> activitiesundertaken by Geoscience Australia within <strong>the</strong>Onshore <strong>Energy</strong> Security Program, principallythose <strong>of</strong> <strong>the</strong> Geo<strong>the</strong>rmal <strong>Energy</strong> Project.Keywords: data acquisition, modelling,Geo<strong>the</strong>rmal Play SystemsThe Geo<strong>the</strong>rmal <strong>Energy</strong> ProjectFollowing consultation with industry and State andNor<strong>the</strong>rn Territory geological surveys, a number<strong>of</strong> activities were identified where GA could ei<strong>the</strong>rfill gaps where no o<strong>the</strong>r organisation was able t<strong>of</strong>ulfil, or could complement activities by o<strong>the</strong>rpartners.Advice to governmentGeoscience Australia (GA) is a prescribed agencywithin <strong>the</strong> Department <strong>of</strong> Resources, <strong>Energy</strong> andTourism. GA provides advice to government ongeoscience-related matters, including resources.GA participated in <strong>the</strong> development <strong>of</strong> <strong>the</strong>Geo<strong>the</strong>rmal Industry Development Frameworkand Geo<strong>the</strong>rmal Industry Technology Roadmap.GA was involved in <strong>the</strong> program design andsubsequent technical assessment <strong>of</strong> <strong>the</strong>Geo<strong>the</strong>rmal Drilling Program. GA co-authored(with ABARE) <strong>the</strong> geo<strong>the</strong>rmal chapter <strong>of</strong> <strong>the</strong><strong>Australian</strong> <strong>Energy</strong> Resource Assessment. GA hasbeen involved in <strong>the</strong> development <strong>of</strong> <strong>the</strong><strong>Australian</strong> Code for Reporting <strong>of</strong> ExplorationResults, Geo<strong>the</strong>rmal Resources and Geo<strong>the</strong>rmalReserves, and sits on <strong>the</strong> Joint AGEA-AGEGCode Committee for <strong>the</strong> purpose <strong>of</strong> one daycompiling and reporting geo<strong>the</strong>rmal resource andreserve estimates in <strong>the</strong> same way as is done formineral and oil & gas commodities.OZTEMPGA has released OZTEMP, an updated datasetand map <strong>of</strong> predicted temperatures at 5 km depth,available from <strong>the</strong> project’s webpage(www.ga.gov.au/minerals/research/national/geo<strong>the</strong>rmal). Extensive QA/QC was conducted on <strong>the</strong>dataset <strong>of</strong> bottom hole temperatures, and whereavailable new data was included. For <strong>the</strong> map, <strong>the</strong>OZSeeBase dataset was used (FrOG Tech,2006), and <strong>the</strong> Bureau <strong>of</strong> Meteorology’s MeanAnnual Average Air Temperature (BoM <strong>2010</strong>) wasalso used with a correction for surfacetemperature. For <strong>the</strong> first time, heat flow data wasalso incorporated into <strong>the</strong> map.Data acquisitionThere is a paucity <strong>of</strong> temperature-specific data inAustralia, and to address this GA has establisheda capability for measuring surface heat flow via<strong>the</strong>rmal gradient logging and <strong>the</strong>rmal conductivitymeasurement.Thermal gradient loggingWithout <strong>the</strong> possibility <strong>of</strong> drilling new holes, GAhas worked with State geological surveys andminerals exploration companies to accessexploration and water bores. Figure 1 shows <strong>the</strong>distribution <strong>of</strong> logged bores as <strong>of</strong> July <strong>2010</strong>.Figure 1. Map showing existing heat flow measurements for <strong>the</strong><strong>Australian</strong> continent, and <strong>the</strong> distribution <strong>of</strong> bores logged fortemperature by Geoscience Australia (black stars).Thermal conductivityGA operates an Anter 2022 Uni<strong>the</strong>rm <strong>the</strong>rmalconductivity meter and associated samplepreparation equipment. Project staff have beeninvolved in establishing operating procedures for<strong>the</strong> instrument, a process which has includedinter-lab comparison testing with Torrens <strong>Energy</strong>,Hot Dry Rocks Pty Ltd, and Sou<strong>the</strong>rn MethodistUniversity. In addition, GA has engaged Hot Dry1


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Rocks Pty Ltd to measure two batches <strong>of</strong>samples.Samples have been taken from <strong>the</strong> majority <strong>of</strong> <strong>the</strong>bores measured by Geoscience Australia for <strong>the</strong>ir<strong>the</strong>rmal gradient, as well as o<strong>the</strong>r bores for‘stratigraphic’ conductivity values.PromotionUndoubtedly <strong>the</strong> greatest impediment to <strong>the</strong>development <strong>of</strong> <strong>the</strong> <strong>Australian</strong> geo<strong>the</strong>rmalindustry since <strong>the</strong> Global Financial Crisis hasbeen <strong>the</strong> lack <strong>of</strong> capital investment. GeoscienceAustralia has participated in “Team AustraliaGeo<strong>the</strong>rmal” events at <strong>the</strong> Geo<strong>the</strong>rmal <strong>Energy</strong>Expo, Reno 2009, and <strong>the</strong> World Geo<strong>the</strong>rmalCongress, Bali <strong>2010</strong>. The collaboration <strong>of</strong>industry, government and associations has beenaimed at portraying Australia as a favourableinvestment destination.Resource assessmentsIn 2007 GA produced an estimate <strong>of</strong> <strong>the</strong>contained heat above 150°C in <strong>the</strong> top 5 km <strong>of</strong> <strong>the</strong><strong>Australian</strong> crust. Understandably this produced avery large estimate <strong>of</strong> energy. To provide a morerelevant estimate 1% <strong>of</strong> <strong>the</strong> <strong>the</strong>rmal resource wasassumed to be accessible and convertible, andthis equates to ~26,000 years <strong>of</strong> energyconsumption (Budd et al., 2009).The production <strong>of</strong> <strong>the</strong> <strong>Australian</strong> <strong>Energy</strong> ResourceAssessment highlighted <strong>the</strong> need for a betterunderstanding <strong>of</strong> Australia’s geo<strong>the</strong>rmalresources potential. This contrasts with o<strong>the</strong>rrenewable energy resources where <strong>the</strong>knowledge-base is quite advanced. There is aneed for geo<strong>the</strong>rmal to be better understood sothat it can be compared more directly to o<strong>the</strong>renergy sources. With a limitation on <strong>the</strong>availability <strong>of</strong> temperature data, o<strong>the</strong>r geosciencedatasets must be used to inform or deriveestimates <strong>of</strong> geo<strong>the</strong>rmal resource potential.Geo<strong>the</strong>rmal Play SystemsAs mentioned above, <strong>the</strong>re is a paucity <strong>of</strong>temperature-specific data publicly available inAustralia. There is, however, a wealth <strong>of</strong> highqualitygeoscientific data available throughout <strong>the</strong>country, much <strong>of</strong> which can be used to makeassessments <strong>of</strong> geo<strong>the</strong>rmal potential from aconceptual view point. Like some companies ando<strong>the</strong>r organisations, GA has developed 2.5D and3D methods for processing geological,geophysical and geochemical data to produceresource potential assessments and estimates. A‘systems’ approach has been utilised to enable<strong>the</strong>se data sets to be used as ‘mappable proxies’to estimate heat production and <strong>the</strong>rmal insulationat regional scales (Budd et al., 2009). Conceptualand empirical methods <strong>of</strong> developing <strong>the</strong>Geo<strong>the</strong>rmal Play Systems approach have beenpursued, and are still in development.3D <strong>the</strong>rmal modellingThrough a Primary Industries and ResourcesSouth Australia (PIRSA) <strong>Australian</strong> Geo<strong>the</strong>rmal<strong>Energy</strong> Group (AGEG) Technical Interest Group 9Tied Grant, a <strong>the</strong>rmal calculation module was builtfor GeoModeller s<strong>of</strong>tware by Intrepid Geophysics(Siekel et al., 2009). This has been used todevelop <strong>the</strong>rmal models <strong>of</strong> <strong>the</strong> Millungerra Basin(unpublished), and <strong>the</strong> Cooper Basin (such asGibson et al., <strong>2010</strong>).We have also undertaken syn<strong>the</strong>tic <strong>the</strong>rmalmodelling tests. This involved <strong>the</strong> development <strong>of</strong>a syn<strong>the</strong>tic grid <strong>of</strong> granites buried under flat-lyingsediments that was used to model <strong>the</strong> effects <strong>of</strong>changing <strong>the</strong>rmal and geometric variables (one ata time). Modelled variables include <strong>the</strong>rmalconductivity, heat production and density <strong>of</strong> <strong>the</strong>sediments and granite, as well as <strong>the</strong> thickness,radius and depth extent <strong>of</strong> <strong>the</strong> granites and totalsediment thickness. This has resulted in 5,400individual test models, and we are in <strong>the</strong> process<strong>of</strong> interpreting <strong>the</strong>se results. These interpretationswill <strong>the</strong>n serve as a guide for a first-passassessment <strong>of</strong> <strong>the</strong>rmal potential <strong>of</strong> <strong>the</strong> wholecontent based on estimates <strong>of</strong> granite size, basingeometry and composition (Meixner, 2009).North Queensland <strong>Energy</strong> AssessmentA GIS-based approach was used to qualify <strong>the</strong>Hot Rock and Hot Sedimentary Aquifergeo<strong>the</strong>rmal systems <strong>of</strong> nor<strong>the</strong>rn Queensland(Huston, <strong>2010</strong>).ReferencesBoM, <strong>2010</strong>, Climate Data Onlinehttp://www.bom.gov.au/climate/data/Budd, A.R., Barnicoat, A.C., Ayling, B.F., Gerner,E.J., Meixner, A.J. and Kirkby, A.M., 2009, AGeo<strong>the</strong>rmal Play Systems approach forexploration Australia, in: Budd and Gurgenci(editors), <strong>Proceedings</strong> <strong>of</strong> <strong>the</strong> 2009 <strong>Australian</strong>Geo<strong>the</strong>rmal <strong>Energy</strong> <strong>Conference</strong>, GeoscienceAustralia, Record 2009/35.FrOG Tech, 2006, OZ SEEBASE ProterozoicBasins Study. PR107.Gibson, H., Seikel, R., and Meixner, T. <strong>2010</strong>,Characterising uncertainty when solving for 3Dtemperature: New tools for <strong>the</strong> <strong>Australian</strong>geo<strong>the</strong>rmal energy exploration sector. ASEGExtended Abstracts <strong>2010</strong>, 1–3.doi:10.1071/ASEG<strong>2010</strong>ab290.Huston, D.L., <strong>2010</strong>, An assessment <strong>of</strong> <strong>the</strong>uranium and geo<strong>the</strong>rmal potential <strong>of</strong> northQueensland / edited by Huston, D.L. withcontributions by Ayling, B., Connolly, D., Huston,D.L., Lewis, B., Mernagh, T.P., Sch<strong>of</strong>ield, A.,Skirrow, R.S. and van der Wielen, S.E.Geoscience Australia Record <strong>2010</strong>/14, Canberra2


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>https://www.ga.gov.au/products/servlet/controller?event=GEOCAT_DETAILS&catno=69711Meixner, T., Johnston, S., Kirkby, A., Gibson, H.,Seikel, R., Stuwe, K., Fitzgerald, D., Horspool, N.Lane, R. and Budd, A., 2009, Establishing hotrock exploration models: from syn<strong>the</strong>tic <strong>the</strong>rmalmodelling to <strong>the</strong> Cooper Basin 3D geological map.Siekel R., Stuwe K., Gibson H., Bendall B.,McAllister L., Reid P., Budd A., 2009, Forwardprediction <strong>of</strong> spatial temperature variation from 3Dgeology models. ASEG Extended Abstracts 2009,–. doi:10.1071/ASEG2009ab117.3


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>3D <strong>the</strong>rmal modelling VS down-hole temperature extrapolation and<strong>the</strong> implications for targeting potential geo<strong>the</strong>rmal anomalies: aSydney Basin case studyCara Danis 1* and Craig O’Neill 11 GEMOC Macquarie University, Dept Earth & Planetary Science, NSW 2109, Australia* Corresponding author: cara.danis@mq.edu.auGeo<strong>the</strong>rmal exploration programs requireaccurate subsurface temperature information andcurrently this information primarily comes fromtemperature maps created from <strong>the</strong> extrapolation<strong>of</strong> shallow down-hole temperature measurements.These extrapolations are <strong>of</strong>ten taken frommeasurements made in non-equilibratedboreholes and do not account for variations ingeological structure or <strong>the</strong>rmal conductivity. Herewe present a case study for <strong>the</strong> Sydney basinwhere we explore temperature maps at 5kmcreated from extrapolated equilibrated and nonequilibratedborehole measurements and frommodelled basin temperatures and <strong>the</strong> implicationsfor targeting potential geo<strong>the</strong>rmal anomalies. Themodelled temperatures are derived from finiteelement models using 3D basin geology anddefined <strong>the</strong>rmal properties.Keywords: Sydney Basin, 3D <strong>the</strong>rmal modelling,temperature extrapolation, geo<strong>the</strong>rmal explorationCase Study – Sydney BasinThe Sydney Basin, part <strong>of</strong> <strong>the</strong> Sydney-Gunnedah-Bowen Basin system, is a major sedimentarybasin in <strong>the</strong> east coast <strong>of</strong> Australia and animportant economic resource. Much attention isgiven to <strong>the</strong> coal and coal seam gas prospects butrecently <strong>the</strong> focus has shifted to <strong>the</strong> basins<strong>the</strong>rmal structure and geo<strong>the</strong>rmal potential.Previous work in <strong>the</strong> Gunnedah Basin (Danis etal., <strong>2010</strong>) has shown that basin architecture andinsulating sediments have a pr<strong>of</strong>ound impact on<strong>the</strong> <strong>the</strong>rmal structure. Heat refracts aroundinsulating coal and sediment layers, into adjacentzones <strong>of</strong> lower <strong>the</strong>rmal resistance, resulting inlarge lateral variations in <strong>the</strong> subsurfacetemperature.In order to determine areas for potentialgeo<strong>the</strong>rmal resource exploration an assessment<strong>of</strong> <strong>the</strong> temperature at depth is required. Short <strong>of</strong>drilling deep and expensive boreholes, currentmethods extrapolate down-hole temperaturesfrom shallow boreholes to 5km using shallowgeo<strong>the</strong>rmal gradients. This method relies on nonequilibratedtemperature information andgeo<strong>the</strong>rmal gradients, which fails to account forlateral variations in geology and <strong>the</strong>rmalconductivity. Such extrapolations may differsignificantly to actual temperatures at depth andmy result in false target anomalies. 3D <strong>the</strong>rmalmodelling provides a more representative analysis<strong>of</strong> <strong>the</strong> <strong>the</strong>rmal structure, with <strong>the</strong> ability to setmodel parameters for lateral geological variationand define <strong>the</strong>rmal characteristics.The work presented here compares <strong>the</strong> results <strong>of</strong>extrapolated equilibrated and non equilibratedtemperature information from shallow boreholesto 5km depth and <strong>the</strong>rmal modelling usinggeological models for target anomaly location.There is a significant difference in temperaturestructure at depth between equilibrated and nonequilibratedextrapolated temperatures as well as<strong>the</strong>rmal modelled temperatures. Thesedifferences have significant implications fortargeting resource areas for geo<strong>the</strong>rmalexploration.Methods and ResultsDown-hole Temperature Measurements:Equilibrated and Non-equilibratedRoutinely temperature measurements inboreholes are not conducted for <strong>the</strong> purpose <strong>of</strong>geo<strong>the</strong>rmal exploration, instead <strong>the</strong>y <strong>of</strong>ten aredesigned to assess groundwater aquifer locationsand cement setting during construction <strong>of</strong>groundwater bores. In exploration drillholestemperatures are recorded at <strong>the</strong> bottom <strong>of</strong> <strong>the</strong>hole during airlift tests or geophysical surveys(o<strong>the</strong>r than temperature). These results are takenimmediately following drilling, generally within24hrs, and are <strong>the</strong>refore considered nonequilibrated.On rare occasions temperatureinformation is collected several months or evenyears after drilling, this is considered equilibrated.To assess <strong>the</strong> impact <strong>of</strong> non-equilibrated andequilibrated temperature maps we collected alarge amount <strong>of</strong> temperature results from bothnon-equilibrated and equilibrated boreholes. Mostequilibrated data is collected in <strong>the</strong> field usingmethodology outlined in detail in Danis et al.(<strong>2010</strong>). As Beardsmore & Cull (2001) recommendequilibrated measurements can be recorded afterwaiting 3 times <strong>the</strong> drilling time length, ourtemperature results were divided accordingly. Ingeneral any measurements taken one month orgreater after drilling were considered asequilibrated results.Geo<strong>the</strong>rmal gradients were determined for eachequilibrated and non-equilibrated borehole using4


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong><strong>the</strong> 1D two layer extrapolation method (outlinedby Chopra & Holgate, 2006) and temperature at5km depth below surface contour map produced(Figure 1). All temperatures were corrected forclimatic variations based on Cull (1979). Whereonly a bottom hole temperature measurementwas recorded a surface temperature average <strong>of</strong>15°C was used to calculate <strong>the</strong> geo<strong>the</strong>rmalgradient. Where possible only temperatures frombelow 100m ground surface were used, to try andavoid diurnal/seasonal temperature influences.Figure 1: Shallow borehole temperatures extrapolated to 5km(a) equilibrated and (b) non-equilibrated. Location <strong>of</strong>boreholes used shown as crosses.(a)(b)The first layer (sediments) is defined from ourSydney Basin geological model and used <strong>the</strong>calculated geo<strong>the</strong>rmal gradient. The second layer(basement) is also defined from our geologicalmodel and uses <strong>the</strong> uniform geo<strong>the</strong>rmal gradient<strong>of</strong> 25°C/km so as to be comparable to <strong>the</strong> currenttemperature at 5km map.Figure 1 shows a distinctive difference between<strong>the</strong> extrapolated equilibrated and non-equilibratedmeasurements for temperature observed at 5km.The equilibrated boreholes (Figure 1a) show lowtemperatures (60-120°C) in <strong>the</strong> central part <strong>of</strong> <strong>the</strong>Sydney Basin, where sediment thickness isgreatest, whilst near <strong>the</strong> edges <strong>of</strong> <strong>the</strong> basin (i.eUlan and Singleton) temperatures areapproaching 200 - 250°C. The non-equilibratedbores also show a similar trend, however on aslightly different scale, with several elevatedanomalies in <strong>the</strong> generally colder parts <strong>of</strong> <strong>the</strong>central and sou<strong>the</strong>rn Sydney Basin.The position <strong>of</strong> temperature highs (or in somecases lows) will shift depending on whe<strong>the</strong>requilibrated or non-equilibrated temperatures areused. Three highs appear around <strong>the</strong> Sydney-Campbelltown-Wollongong region in <strong>the</strong> nonequilibrateddata which are not prominent in <strong>the</strong>equilibrated map. The high near Singleton is alsomore localised with <strong>the</strong> non-equilibratedmeasurements.The pattern in temperature distribution <strong>of</strong> lowsover <strong>the</strong> centre and highs on <strong>the</strong> edge <strong>of</strong> <strong>the</strong>Sydney Basin, were an expected feature. They tiein with <strong>the</strong> fact that <strong>the</strong> coal measures provide a<strong>the</strong>rmal insulator, thus temperatures measuredabove coal measures would be expected to becooler than those measure in or below coalmeasures. On <strong>the</strong> edge <strong>of</strong> <strong>the</strong> basin heatrefracting around <strong>the</strong> coal measures produces <strong>the</strong>elevated temperatures.Previous <strong>the</strong>rmal modelling <strong>of</strong> <strong>the</strong> GunnedahBasin (Danis et al., <strong>2010</strong>) showed basinarchitecture and <strong>the</strong> refraction <strong>of</strong> heat around <strong>the</strong>coal interval to be major controlling factors in <strong>the</strong><strong>the</strong>rmal pr<strong>of</strong>ile. Therefore to better understand <strong>the</strong>impact <strong>of</strong> extrapolating shallow <strong>the</strong>rmalmeasurements to depth we created 15 <strong>the</strong>rmalmodel pr<strong>of</strong>iles along <strong>the</strong> lines shown in Figure 1.Thermal Modelling: UnderworldThermal models were developed using <strong>the</strong> finiteelement code Underworld. The code solves <strong>the</strong>non-steady state heat equation with internal heatsources in two dimensions. Distinct layers fromour 3D geological model are imported as differentmaterials into <strong>the</strong> code, with constant temperaturetop and bottom boundary conditions. The <strong>the</strong>rmalproperties for each material layer are outlined inTable 1, and are aggregates <strong>of</strong> measurements oneach unit/rock type. In addition <strong>the</strong>re is one quasi-5


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>material called ‘air’. This top air layer has a largeconductivity and its purpose is to allow direct<strong>the</strong>rmal coupling <strong>of</strong> <strong>the</strong> varying topographicsurface with <strong>the</strong> top boundary condition. The sideboundary conditions are reflecting, and an extra10km has been added to ei<strong>the</strong>r side <strong>of</strong> <strong>the</strong> modelpr<strong>of</strong>ile to avoid any reflecting edge effects.Rock TypeDensity(kg/m 3 )Table 1Conductivity(W/m-K)HeatProduction(µW/m 3 )Basement 2700 3 2Mafics 2950 3 0.5Sediments 2460 2 1.25Coal Interval 1900 0.3 1.25The main free parameter is <strong>the</strong> bottomtemperature condition at 12km, which wasextrapolated from <strong>the</strong> National Temperature at5km map (e.g Budd, 2007) to be ~350°C. Heatproduction in <strong>the</strong> basement is taken fromrepresentative Lachlan Fold Belt granites in <strong>the</strong>OZCHEM database. The model considers <strong>the</strong>rmalconduction only, it doesn’t take into accountadvective effects or <strong>the</strong> effects <strong>of</strong> varying surfacetemperature conditions.The model boundary conditions were calibratedusing limited available equilibrated temperaturefrom shallow boreholes (Figure 2).equipment, whilst pr<strong>of</strong>iles 2, 11 and 13 have beengeophysical logged. The precision <strong>of</strong> <strong>the</strong> Hobologging equipment is 0.37°C at 20°C and <strong>the</strong>general precision <strong>of</strong> geophysical temperaturelogging equipment is 0.1°C (from AUSLOG). Theuncertainty <strong>of</strong> <strong>the</strong> climate correction applied to <strong>the</strong>equilibrated measurements is approximately ±5°C at <strong>the</strong> surface, ±3°C at 500m and ± 1°C at1km. We <strong>the</strong>refore allow an uncertainty buffer <strong>of</strong> ±10°C in our measured temperatures whencomparing <strong>the</strong>m to <strong>the</strong> modelled geo<strong>the</strong>rms. It isimportant to note in pr<strong>of</strong>ile 2 <strong>the</strong> greenmeasurements are <strong>the</strong> equilibrated results andare lower than expected due to cleaning <strong>of</strong> <strong>the</strong>borehole before logging. The red and bluemeasurements represent non-equilibratedtemperatures.In order to compare <strong>the</strong> results <strong>of</strong> extrapolatedtemperature measurements with <strong>the</strong>rmalmodelling, a series <strong>of</strong> temperature pr<strong>of</strong>iles weretaken along a selected <strong>the</strong>rmal model line. Here<strong>the</strong> equilibrated and non-equilibrated temperaturemeasurements were extracted at 500m and 5kmdepth and compared to those <strong>of</strong> <strong>the</strong> <strong>the</strong>rmalmodel pr<strong>of</strong>ile at <strong>the</strong> same depths, as shown inFigure 3.Figure 2: Geo<strong>the</strong>rm calibration checks using shallowequilibrated borehole temperatures for four selected pr<strong>of</strong>iles.Ground surface (green line) varies from model depth zerodepending on topography. Gray shaded area represents±10°C <strong>of</strong> <strong>the</strong> model geo<strong>the</strong>rm.Figure 3: Thermal model Line 12 temperature output wi<strong>the</strong>xtrapolated temperatures (green = equilibrated, blue = nonequilibrated)at (a) 500m and (b) 5000m below groundsurface and showing model geology.The equilibrated borehole temperatures (Figure 2)compare well with <strong>the</strong> model geo<strong>the</strong>rms and arefrom boreholes in <strong>the</strong> Permian sequence.Equilibrated temperatures in pr<strong>of</strong>ile 1 are fromfield measurements using Hobo loggingFrom Figure 3 a distinctive difference in anomalystructure can be seen between <strong>the</strong> 500m and 5kmdepths. In both cases <strong>the</strong> extrapolated6


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>equilibrated and non-equilibrated measurementsunderestimate <strong>the</strong> modelled temperatures. Evenat 500m, above <strong>the</strong> influence <strong>of</strong> <strong>the</strong> coalmeasures <strong>the</strong> extrapolated temperatures are stilllower than <strong>the</strong> modelled temperatures.At 5km <strong>the</strong> model temperature also shows verylittle variation as <strong>the</strong>y are predominately in <strong>the</strong>Lachlan Fold Belt basement. At 500m shallowsurface variations in <strong>the</strong> modelled temperaturesare observed and are most likely related to <strong>the</strong>geology and/or influences <strong>of</strong> shallow groundwateraquifers.In both pr<strong>of</strong>iles (Figure 3) <strong>the</strong> effects <strong>of</strong> <strong>the</strong>insulating coal interval on extrapolatedequilibrated or non-equilibrated versus modelledtemperatures can be seen. It appears that <strong>the</strong>extrapolation <strong>of</strong> shallow measurements, withoutany consideration <strong>of</strong> <strong>the</strong> geology and/or <strong>the</strong>rmalconductivity, to depth propagates shallow surfacefeatures and produces false anomalies.To fur<strong>the</strong>r illustrate <strong>the</strong> difference between <strong>the</strong>extrapolated and modelled temperatures Figure 4is a contour map <strong>of</strong> modelled temperatures at5km below ground surface for <strong>the</strong> Sydney Basin.Figure 4: Modelled temperatures at 5km depth below groundsurface. Thermal model lines are numbered 1 to 15, outline<strong>of</strong> <strong>the</strong> Sydney Basin shown in grey and edge <strong>of</strong> continentalshelf is <strong>the</strong> <strong>of</strong>fshore black line.Modelled temperatures (Figure 4) in <strong>the</strong> SydneyBasin at 5km are hottest where <strong>the</strong> thickest layers<strong>of</strong> sediment and coal intervals are. This is mostprominent around Sydney and north towards <strong>the</strong>Hunter/Newcastle Coalfields, where sedimentthickness ranges from 3 to 4km, and a thick layer<strong>of</strong> basal volcanics are also present. Thetemperature anomaly observed wast <strong>of</strong> Singletonin <strong>the</strong> equilibrated extrapolation map appears in asimilar location with <strong>the</strong> modelled temperatures,but is less pronounced. The high on Line 12 north<strong>of</strong> Mossvale in <strong>the</strong> equilibrated extrapolation mapis not apparent in Figure 4. High basementtemperatures <strong>of</strong>fshore <strong>of</strong> Newcastle in <strong>the</strong>Newcastle Syncline are a new feature observedwith <strong>the</strong> modelled temperatures. Where basementis shallow, i.e. <strong>the</strong> sou<strong>the</strong>rn parts <strong>of</strong> <strong>the</strong> SydneyBasin, modelled temperatures at 5km are lowerthan those fur<strong>the</strong>r north with greater sedimentcover, predominately because <strong>the</strong> coal interval isgenerally absent, removing <strong>the</strong> insulating effect,and sediment thickness is less than 1km.Modelled temperatures show high (210+°C)temperatures under areas <strong>of</strong> thick sedimentcover, whilst shallow extrapolated temperaturemeasurements <strong>of</strong>ten reflect <strong>the</strong> insulating effect <strong>of</strong><strong>the</strong> coal interval (if above <strong>the</strong> coal interval) withtemperatures ranging from 60°C to 230°C.SummaryThese results show that <strong>the</strong> temperaturevariations observed in maps created fromextrapolated shallow borehole measurements arelikely to be inaccurate. The simple linearextrapolations shown here <strong>of</strong> both equilibratedand non-equilibrated show shallow temperaturemeasurements propagate near surface features todepth which, when compared to modelledtemperatures, are not true anomalies. Thereforegiven most <strong>of</strong> <strong>the</strong> measurements used in <strong>the</strong>creation <strong>of</strong> temperature at 5km maps are takenfrom non-equilibrated boreholes extreme cautionshould be exercised when considering <strong>the</strong>temperatures.However <strong>the</strong>rmal modelling did show thatequilibrated measurements are an excellentcalibration tool. The modelled geo<strong>the</strong>rms fit wellwith <strong>the</strong> shallow equilibrated measurements. Awell calibrated <strong>the</strong>rmal model will better accountfor basin structure and changes in <strong>the</strong>rmalconductivity than extrapolated temperature maps.Extrapolation doesn’t take into account <strong>the</strong><strong>the</strong>rmal effects <strong>of</strong> basin architectural structure andshould be avoided as a geo<strong>the</strong>rmal explorationtool. Not only is <strong>the</strong>re a risk <strong>of</strong> <strong>the</strong> targetanomalies being false positives, possible positivetargets may be incorrectly located as a result <strong>of</strong>refracted heat from <strong>the</strong> basin structure.ReferencesBeardsmore, G.R., Cull, J.P., 2001, Crustal heatflow: a guide to measurement and modelling.Cambridge University Press 324p.Budd, A.R., 2007, <strong>Australian</strong> radiogenic graniteand sedimentary basin geo<strong>the</strong>rmal hot rock7


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>potential map (preliminary edition), 1:5 000 000scale. Geoscience Australia, Canberra.Cull, J.P., 1982, An appraisal <strong>of</strong> <strong>Australian</strong> heatflow data. BMR Journal <strong>of</strong> <strong>Australian</strong> Geology &Geophysics v.7, p. 11-21.Danis, C., O’Neill, C., and Lackie, M., <strong>2010</strong>, 3Darchitecture and upper crustal temperatures <strong>of</strong> <strong>the</strong>Gunnedah Basin. <strong>Australian</strong> Journal <strong>of</strong> EarthSciences 57, 483-505.8


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>South <strong>Australian</strong> Geo<strong>the</strong>rmal Research CentreM. Hand and Y. NgothaiSACGER, IMER, The University <strong>of</strong> Adelaide, South Australia, 5005.*Corresponding author: martin.hand@adelaide.edu.auThe emergence <strong>of</strong> <strong>the</strong> <strong>Australian</strong> Geo<strong>the</strong>rmalSector has focussed attention on <strong>the</strong> potential <strong>of</strong><strong>the</strong> Australia’s non volcanic <strong>the</strong>rmal systems toprovide both direct and indirect energy. However<strong>the</strong> challenges are significant, and require acoordinated effort between <strong>the</strong> private,government and R&D sectors to focus expertiseand bring projects to demonstration. TheDevelopment Framework and TechnologyRoadmap (DRET, 2008) outlines a clear plan forproject development. A key aspect <strong>of</strong> thisroadmap is consultation between <strong>the</strong> privatesector and research organisations that prioritisesresearch gaols that directly aid <strong>the</strong> sector. In thiscontext <strong>the</strong>re are now a number <strong>of</strong> researchcentres within Australia that are seeking to form acohesive national R&D effort to assist <strong>the</strong> sector.This paper provides an overview <strong>of</strong> <strong>the</strong> South<strong>Australian</strong> Geo<strong>the</strong>rmal Research Centre(SACGER), which is hosted at <strong>the</strong> University <strong>of</strong>Adelaide, and provides a compliment to <strong>the</strong>national overview presented by Long et al (thisvolume).Keywords: South <strong>Australian</strong> Geo<strong>the</strong>rmalResearch Centre.South <strong>Australian</strong> Centre for Geo<strong>the</strong>rmal<strong>Energy</strong> Research - SACGERThe South <strong>Australian</strong> Centre for Geo<strong>the</strong>rmal<strong>Energy</strong> Research is based at <strong>the</strong> University <strong>of</strong>Adelaide within <strong>the</strong> Institute for Minerals and<strong>Energy</strong> Resources (IMER),www.adelaide.edu.au/imer. The centre is fundedfrom <strong>the</strong> South <strong>Australian</strong> Renewable <strong>Energy</strong>Fund, established with a grant <strong>of</strong> AU$1.6M overtwo years from 1 July 2009. However initiation <strong>of</strong>expenditure was delayed until July <strong>2010</strong>. TheUniversity <strong>of</strong> Adelaide is providing AU$400,000over <strong>the</strong> same period. Within IMER <strong>the</strong> South<strong>Australian</strong> Centre for Geo<strong>the</strong>rmal <strong>Energy</strong>Research forms part <strong>of</strong> a broader R&D portfolioon energy that includes <strong>the</strong> Centre for <strong>Energy</strong>Technologies which has a focus that includes <strong>the</strong>energy conversion and hybrid technologies whoseaim is to optimise <strong>the</strong> geo<strong>the</strong>rmal energydelivered to <strong>the</strong> surface.The SACGER research program has threeprincipal foci which compliment <strong>the</strong> researchprograms <strong>of</strong> o<strong>the</strong>r centres around <strong>the</strong> country andbuild on strengths in subsurface modelling andcharacterisation to foster reliable estimates andefficient development <strong>of</strong> geo<strong>the</strong>rmal resources.Program 1: Development <strong>of</strong>Electromagnetic tools to monitor andassess geo<strong>the</strong>rmal reservoirbehaviourThis program is designed to <strong>the</strong> development <strong>of</strong>technologies and methods to make surface-basedmagnetotelluric (MT) surveys useful in (1)predicting <strong>the</strong> presence <strong>of</strong> fractured reservoirsahead <strong>of</strong> <strong>the</strong> drill bit and (2) monitoring fluid flowsin Engineered Geo<strong>the</strong>rmal Systems.Under certain conditions, MT surveys can indicate<strong>the</strong> presence <strong>of</strong> naturally occurring hot fracturedrock targets that are susceptible to reservoirenhancement with fracture stimulation to createEngineered Geo<strong>the</strong>rmal Systems. MT surveyscan provide measurements that indicate <strong>the</strong>nature <strong>of</strong> changed fracture networks and postreservoir enhancement with hydraulic fracturestimulation. The development <strong>of</strong> MT technologiesand MT interpretation methods is identified as apriority for research in <strong>the</strong> <strong>Australian</strong>Government’s Geo<strong>the</strong>rmal Industry DevelopmentFramework and its associated Geo<strong>the</strong>rmalTechnology Roadmap as requiring immediateattention. The University <strong>of</strong> Adelaide isinternationally recognised for its expertise in <strong>the</strong>use and development <strong>of</strong> MT techniques, and iswell positioned to become an international leaderin <strong>the</strong> development <strong>of</strong> electromagnetically basedtools for <strong>the</strong> geo<strong>the</strong>rmal industry.The initiation and propagation <strong>of</strong> <strong>the</strong> undergroundfluid-reservoir is dependent on severalparameters, including <strong>the</strong> stress regime, geometry<strong>of</strong> pre-existing faults, and reservoir lithologies.Currently, measurements <strong>of</strong> shear-wave splitting(SWS) is deployed to define EGS stress regimes,while refined measurement <strong>of</strong> seismicity (naturaland induced during EGS field operations) is astandard approach to determine <strong>the</strong> location <strong>of</strong><strong>the</strong> enhanced extent in <strong>the</strong> subsurface <strong>of</strong> EGSreservoirs (by locating seismic events associatedwith <strong>the</strong> creation <strong>of</strong> fractures during EGSoperations). Because MT surveys can, undercertain conditions, detect fluid flow patterns,advances in MT technologies and interpretationmethods hold promise to foster more accuratedelineation <strong>of</strong> EGS reservoirs, and models <strong>of</strong> fluidflows in EGS reservoirs. Locating MTmeasurement stations alongside micro-seismicdetectors is a way to better understand <strong>the</strong>relationship between <strong>the</strong> two datasets and9


delineate <strong>the</strong> location <strong>of</strong> fracture zones in EGSfields.The proposed research leverages on knowledgeobtained from a pilot project concluded by <strong>the</strong>University <strong>of</strong> Adelaide with Petra<strong>the</strong>rm Ltd. Initialstudies and field surveys indicate close sitespacing <strong>of</strong> <strong>the</strong> MT sites and high data quality arecrucial for successfully monitoring <strong>the</strong> reservoirdevelopment.The technologies and approaches developed willbe readily transferable to o<strong>the</strong>r potential EGSsites in South Australia and more globally.Program 2: Fluid-rock interactions ingeo<strong>the</strong>rmal reservoirsFracture and flowAustralia’s three flagship geo<strong>the</strong>rmal projects areall located in South Australia (Geodynamics’Cooper Basin project; Petra<strong>the</strong>rm’s Paralanaproject; and Panax’s Salamander (Penola)project. The Geodynamics and Petra<strong>the</strong>rmprojects represent two <strong>of</strong> <strong>the</strong> world’s mostsignificant Engineered Geo<strong>the</strong>rmal Systems(EGS) projects. Both projects entail <strong>the</strong>enhancement <strong>of</strong> naturally fractured rocks withhydraulic fracture stimulation. Additionallydependent on <strong>the</strong> reservoir nature, HotSedimentary Aquifer systems such as thosetargeted in Panax’s Salamander project may alsorequire stimulation.Reliably predictive flow modelling <strong>of</strong> EGSreservoirs is a recognised critical researchchallenge that is driving a peak internationalconsortia (<strong>the</strong> International Partnership forGeo<strong>the</strong>rmal Technologies; <strong>the</strong> IPGT) to focus onimproving 3-D modelling <strong>of</strong> reservoir performancethrough <strong>the</strong> life <strong>of</strong> a geo<strong>the</strong>rmal field life e.g.models that couple heat exchange, pressure,rock-fluid interaction, fluid flow dynamics,geomechanical properties and o<strong>the</strong>r geo<strong>the</strong>rmalreservoir and geo<strong>the</strong>rmal well parameters overlife-cycle production history. The aim <strong>of</strong> researchin SACGER will be to:(1) Improve 3D models with new informationfrom <strong>the</strong> EGS projects, and work incollaboration with <strong>the</strong> R&D expertise inAustralia and internationally. This work willhave implications for <strong>the</strong> risk management <strong>of</strong>induced seismicity by characterising <strong>the</strong>geometry <strong>of</strong> naturally existing fracturepatterns, and improving knowledge <strong>of</strong> <strong>the</strong> insitustresses and potential overpressureregimes.(2) Develop laboratory procedures using coreflooding under stress aimed at predictingformation damage in production/injectionwells and removal <strong>of</strong> well damage.<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Program 3: Chemical reactivity ingeo<strong>the</strong>rmal systemsArea-specific research to mitigate fouling andgeo<strong>the</strong>rmal reservoir (pore and fracture) blockingis essential for efficient geo<strong>the</strong>rmal energydevelopment projects. This research will build onpilot studies using a hydro<strong>the</strong>rmal cell atrepresentative reservoir temperatures (100-250 o C) to study fluid-rock interactions ingeo<strong>the</strong>rmal reservoirs. However, <strong>the</strong> pilot studycell operated at pressures (roughly 50 bar, <strong>the</strong>saturation pressure <strong>of</strong> fluid) well below pressures(~ 300 bar) typical <strong>of</strong> EGS reservoirs in SouthAustralia. More realistic reservoir conditions willbe simulated by <strong>the</strong> creation <strong>of</strong> a hightemperature, high pressure flow through cell toexperimentally explore <strong>the</strong> risks <strong>of</strong> fouling andreservoir blockage at conditions that mimicsconditions in <strong>the</strong> South <strong>Australian</strong> EGS projects.The research will also allow <strong>the</strong> chemicalprocesses in HSA systems to be examined. Thiswill allow prediction <strong>of</strong> permeability for down-dip(<strong>the</strong>rmally viable) targets HSA targets as well asscaling and fouling.Development and application <strong>of</strong> tracers andsmart particles to track fluid flow withinreservoirsTracer technologies are a critical factor incalibrating reservoir performance models in allgeo<strong>the</strong>rmal projects and can be used todetermine <strong>the</strong> reactiveConservative tracers for characterizing inter-wellreservoir flow processes are:- Thermally stable to 350 o C- Detectible to low parts per trillion- Environmentally friendly and non-toxicReactive tracers for characterizing fracturesurface areas in injection/backflow tests are:- Thermally decomposing- Reversibly sorbing- Possessing contrasting diffusivitiesIn addition to <strong>the</strong>se research programs is workcurrently underway within <strong>the</strong> within <strong>the</strong> Centre for<strong>Energy</strong> Technologies that is experimentingverification <strong>of</strong> underground cooling for efficient<strong>the</strong>rmal cycles and examination <strong>of</strong> lowtemperature <strong>the</strong>rmal processing using geo<strong>the</strong>rmalenergy aimed at optimising geo<strong>the</strong>rmal energyinvestments.For more information seewww.adelaide.edu.au/geo<strong>the</strong>rmal/or contact <strong>the</strong> centre: imer@adelaide.edu.au ormartin.hand@adelaide.edu.au10


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Application <strong>of</strong> magnetotellurics in geo<strong>the</strong>rmal reservoircharacterizationGharibi 1 Mehran, Hearst 1* Robert B. , Retallick 2 Trent and Killin 1 Kevin1 Quantec Geoscience Ltd., 146 Sparks Ave., Toronto, ON, Canada M2H 2S42 Quantec Geoscience Pty. Ltd., Unit 2/77 Araluen Street, Kedron, Qld., 4031*Corresponding author: rhearst@quantecgeoscience.comIn this paper we examine Magnetotelluric (MT)data and analysis from a few different styles <strong>of</strong>geo<strong>the</strong>rmal resource. The geo<strong>the</strong>rmal resourcesexamined include both shallow (2000m) scenarios. The implicationswith respect to survey and limitations imposed bysurvey design on <strong>the</strong> interpretation <strong>of</strong> <strong>the</strong> resultsare discussed. The results <strong>of</strong> 1-D, 2-D and 3-Dinversions are compared and discussed in terms<strong>of</strong> <strong>the</strong>ir vertical and spatial resolutions and <strong>the</strong>reliability <strong>of</strong> <strong>the</strong> results in conjunction with <strong>the</strong>geology <strong>of</strong> <strong>the</strong> study areas. The continuedimprovement in <strong>the</strong> power and affordability inmulti-core PC-platform computing allows for <strong>the</strong>relatively rapid inversion <strong>of</strong> MT data in 3-D. In <strong>the</strong>past it had been necessary to invert in 3-D withonly a subset <strong>of</strong> <strong>the</strong> original dataset and with alimited number <strong>of</strong> frequencies (<strong>of</strong>ten 2000m) andfor reconnaissance type surveys whereby a largeamount <strong>of</strong> ground must be covered in a limitedamount <strong>of</strong> time and hence relatively wide siteintervals are required (> 500m). Detailed pr<strong>of</strong>ilingcan also be accomplished.The past decade has seen <strong>the</strong> development <strong>of</strong>array type systems whereby a large number <strong>of</strong>MT sites can be deployed in a rapid fashionallowing for a detailed investigation to becompleted in a short period time. Often <strong>the</strong>sesystems include <strong>the</strong> ability to acquire o<strong>the</strong>rcomplementary geophysical data sets (e.g. DCresistivity, IP chargeability, TEM). An example <strong>of</strong>such a system is illustrated by Figure 2. Ingeneral, <strong>the</strong>se array type systems can beextremely effective in <strong>the</strong> delineation <strong>of</strong> nearsurface (


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>1-D and 2-D inversions and <strong>the</strong> data must bemitigated or removed before <strong>the</strong> inversion. On <strong>the</strong>contrary, <strong>the</strong> 3-D inversion uses impedance dataand is capable to handle this type <strong>of</strong> data; making<strong>the</strong> inversion a robust tool to produce a realisticrepresentation <strong>of</strong> <strong>the</strong> subsurface.In this discussion we contrast <strong>the</strong> differencesbetween not only <strong>the</strong> 1-D, 2-D and 3-D inversionsbut also <strong>the</strong> effect <strong>of</strong> variations in MT field sampleintervals and spacing on <strong>the</strong> effectiveness <strong>of</strong> <strong>the</strong>various inversion methods on <strong>the</strong> ability to discernand characterize geo<strong>the</strong>rmal reservoirs.Figure 2: Example <strong>of</strong> an Array Type MT Acquisition SystemInversion MethodologiesInterpretation <strong>of</strong> <strong>the</strong> MT data is performed using<strong>the</strong> maps <strong>of</strong> true resistivity <strong>of</strong> <strong>the</strong> subsurface.Inversion algorithms in one-dimension (1-D), twodimension(2-D), and three-dimension (3-D) areused to invert <strong>the</strong> apparent resistivity and phasedata in to <strong>the</strong> maps <strong>of</strong> true resistivity <strong>of</strong> <strong>the</strong>subsurface. A simple layered subsurface structuregenerally can adequately be reproduced using <strong>the</strong>1-D inversion. In <strong>the</strong> case <strong>of</strong> more complex 2-D or3-D structures, <strong>the</strong> MT response will be affectedby lateral variations in resistivity. Consequently, a2-D or 3-D inversion algorithm is required to allow<strong>the</strong> lateral resistivity variations.In 1-D earth assumption, <strong>the</strong> 1-D inversion <strong>of</strong> <strong>the</strong>MT data produces a resistivity-depth pr<strong>of</strong>ile foreach MT site. The results represent a first orderapproximation <strong>of</strong> <strong>the</strong> resistivity variations withdepth using a layered-earth model. Often <strong>the</strong>seinversion results are presented in pseudo-sectionform as “stitched” 1-D inversion sections.If <strong>the</strong>re are lateral variations in <strong>the</strong> resistivity <strong>of</strong><strong>the</strong> subsurface along one direction only(perpendicular to <strong>the</strong> strike) <strong>the</strong>n a 2-D inversionand interpretation is required. A cross-section <strong>of</strong><strong>the</strong> true resistivity variations perpendicular to <strong>the</strong>assumed strike direction is created in <strong>the</strong> 2-Dinversion and is used in interpretation.For more complex geological structures a 3-Dinversion is essential to adequately describe <strong>the</strong>resistivity variation <strong>of</strong> <strong>the</strong> subsurface. This isusually <strong>the</strong> case when mapping <strong>the</strong> geologicalsettings hosting a geo<strong>the</strong>rmal system. In this caseno simplifying assumption is made in terms <strong>of</strong>property <strong>of</strong> <strong>the</strong> MT data and dimensionality <strong>of</strong> <strong>the</strong>underlying subsurface. In highly heterogeneousenvironments MT phase data <strong>of</strong>ten exhibit an out<strong>of</strong>-phase(phase-wrap) behaviour; caused by <strong>the</strong>complexity <strong>of</strong> <strong>the</strong> current paths in <strong>the</strong> subsurface.Modelling <strong>of</strong> <strong>the</strong>se data is essential in order toresolve <strong>the</strong> heterogeneity <strong>of</strong> <strong>the</strong> subsurface. Thiskind <strong>of</strong> data, however, cannot be modelled usingReferencesBaars, R.M., Owens, L., Tobin, H., Norman, D.,Cumming, W., and Hill, G., 2006, Exploration andtargeting <strong>of</strong> <strong>the</strong> Socorro, New Mexico direct usegeo<strong>the</strong>rmal exploration well, a GRED III Project:<strong>Proceedings</strong>, Thirty-First Workshop onGeo<strong>the</strong>rmal Reservoir Engineering, StanfordUniversity, Stanford, California, January 30-February 1, 2006, SGP-TR-179.Bahr, K., and Simpson, F., 2005, PracticalMagnetotellurics, Cambridge University Press.Brophy, P., 2007, A brief classification <strong>of</strong>geo<strong>the</strong>rmal systems: Geophysical Techniques inGeo<strong>the</strong>rmal Exploration Workshop, GRC AnnualMeeting, 2007, Sparks, Nevada.Constable, S.C., Parker, R.L., and Constable,C.G., 1987. Occam’s inversion - A practicalalgorithm for generating smooth models fromelectromagnetic sounding data. Geophysics, 52(3), 289-300.de Lugao, P.P., and Wannamaker, P.E., 1996.Calculating <strong>the</strong> two-dimensional magnetotelluricJacobian in finite elements using reciprocity.Geophysical Journal International, 127, 806-810.Marquardt, D.W., 1963. An algorithm for leastsquaresestimation <strong>of</strong> non-linear parameters. J.Sot. Ind. Appl. Math., 11, 431–441.Nabighian, M.N., 1987. Electromagnetic Methodsin Applied Geophysics, Volume 2: Application(Parts A and B). Society <strong>of</strong> ExplorationGeophysicists (SEG), Tulsa.Orange, A.S., 1989. Magnetotelluric explorationfor hydrocarbons. <strong>Proceedings</strong> <strong>of</strong> <strong>the</strong> IEEE, 77,287-317.Rodi, W., and Mackie, R.L., 2001. Nonlinearconjugate gradients algorithm for 2Dmagnetotelluric inversions. Geophysics, 66, 174-187.Siripunvaraporn, W., Egbert, G., Lenbury, Y., andUyeshima, M., 2005. Three-DimensionalMagnetotelluric: Data Space Method. Physics <strong>of</strong><strong>the</strong> Earth and Planetary Interiors, 150, 3-14.12


Ussher, G., Harvey, C., Johnstone, R., Anderson,E., 2000, Understanding <strong>the</strong> resistivities observedin geo<strong>the</strong>rmal systems: <strong>Proceedings</strong> WorldGe<strong>the</strong>rmal Congress 2000, Kyushu-Tohoku,Japan, May 28-June 10, 2000, p.1915-1920.Voz<strong>of</strong>f, K., 1972. The Magnetotelluric method in<strong>the</strong> Exploration <strong>of</strong> Sedimentary basins.Geophysics, 37, 98-141.Wannamaker, P.E., Stodt, J.A., and Rijo, L., 1987.A stable finite-element solution for twodimensionalmagnetotelluric modeling.Geophysical Journal <strong>of</strong> <strong>the</strong> Royal AstronomicalSociety, 88, 277-296.Wight, D.E., 1987. MT/EMAP Data InterchangeStandard, Revision 1.0. Society <strong>of</strong> ExplorationGeophysicists (SEG). (Document available at <strong>the</strong>SEG web site: www.seg.org).<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>13


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Hutton Sandstone – a viable geo<strong>the</strong>rmal developmentDavid Jenson*, Kerry Parker, Ron Palmer, Bertus de GraafPanax Geo<strong>the</strong>rmal Ltd. PO Box 2142, Milton, Qld 4064*Corresponding author: djenson@panaxgeo<strong>the</strong>rmal.com.auPanax Geo<strong>the</strong>rmal Limited (Panax) holds fourGeo<strong>the</strong>rmal Exploration Licences (GEL’s) in <strong>the</strong>north east <strong>of</strong> South Australia, namely GEL’s 220,221, 281 and 502. These licences overlap <strong>the</strong>Great Artesian Basin and in particular <strong>the</strong> HuttonSandstone (“Hutton”), a known prolific reservoir.It has been demonstrated in existing wells andextrapolated using seismic data that <strong>the</strong> Huttonare recognized as a very porous and permeableaquifer and can be found at depths greater than2,000m and temperatures <strong>of</strong> up to 145 °C.Reviewing core samples in <strong>the</strong> region suggeststhat <strong>the</strong>re is a high likelihood for transmissibilityup to 90-100 Dm.The Hutton Project is based on producing aninitial artesian flow <strong>of</strong> hot water sufficient togenerate about 1 MWe. Although greater flowscould be produced, ei<strong>the</strong>r by artesian flow or bypumping, capable <strong>of</strong> generating up to 5-6 MWeper production well, a smaller development ismore appropriate whilst <strong>the</strong> market evolves.Initially, <strong>the</strong> focus is on replacing diesel or gasgeneration in <strong>the</strong> local oil fields, small settlementsand pastoral leases.This study is based on small scale generationbased on multiple (between 2 and 5) proprietaryPureCycle 280kW units (580kW – 1400kW grosspower output) receiving flows <strong>of</strong> artesian hotwater between 135 and 145 °C from a single150mm nominal diameter well. The maximumflow that may be required is about 51 kg/s whichis less than half <strong>of</strong> <strong>the</strong> natural artesian flow thatcould be expected.Geo<strong>the</strong>rmal potential <strong>of</strong> Panax’sHutton Sandstone project licencesPanax Geo<strong>the</strong>rmal Limited (Panax) holds fourGeo<strong>the</strong>rmal Exploration Licences (GEL’s) in <strong>the</strong>Cooper Basin region, north east <strong>of</strong> SouthAustralia, see Figure 1. GEL’s 220 and 221 are in<strong>the</strong> Nappamerri Trough and GEL’s 281 and part<strong>of</strong> 502 are in <strong>the</strong> Patchawarra Trough. Both areasare covered by <strong>the</strong> hydrogeological GreatArtesian Basin.Figure 1. Panax's geo<strong>the</strong>rmal licences located in NE SouthAustralia. All four licences are in <strong>the</strong> hydro-geological GreatArtesian BasinBeardsmore (2009) assessed GEL 281 for itsgeo<strong>the</strong>rmal potential and determined a “MeasuredGeo<strong>the</strong>rmal Resource” <strong>of</strong> 11,000PJcomplemented by an additional 30,000 PJ <strong>of</strong>“Indicated Geo<strong>the</strong>rmal Resource”, see tablebelow. This resource classification was inaccordance with <strong>the</strong> <strong>Australian</strong> Code forReporting <strong>of</strong> Exploration Results, Geo<strong>the</strong>rmalResources and Geo<strong>the</strong>rmal Reserves, 2008edition.The ability to positively assess <strong>the</strong> significantgeo<strong>the</strong>rmal resource potential is due to <strong>the</strong> longhistory <strong>of</strong> petroleum exploration with numerouswells and seismic surveys (Figure 2).This highly encouraging resource classification,<strong>the</strong> third in Australia and second resourceclassification <strong>of</strong> a Hot Sedimentary Aquiferconfirmed <strong>the</strong> high potential <strong>of</strong> geo<strong>the</strong>rmal energydevelopment in sedimentary basins.Table 1. Geo<strong>the</strong>rmal Resource, GEL281Measured Indicated Inferred Total[PJ] [PJ] [PJ] [PJ]11,000 30,000 0 41,00014


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Figure 2. GEL281 - outlines <strong>of</strong> Measured Geo<strong>the</strong>rmalResources showing existing petroleum wells.In <strong>the</strong> following Geo<strong>the</strong>rmal SystemsAssessment, Cooper et al. (2009) found that <strong>the</strong>Hutton Sandstone has potential for low enthalpygeo<strong>the</strong>rmal energy generation. Cooper points outthat <strong>the</strong> temperature modeling may have beenunderstating <strong>the</strong> temperature as <strong>the</strong> data points atthis stratigraphic level are sparse and that it ispossible that advective (lateral) heat flow mayoccur that has not been included in <strong>the</strong> modelling.Cooper’s positive assessment <strong>of</strong> <strong>the</strong> GreatArtesian Basin in GELs 220 and 221 confirmedtoge<strong>the</strong>r with earlier work over GEL 281 thatPanax’s GEL’s in <strong>the</strong> region represents a largearea with a significant geo<strong>the</strong>rmal resourcePanax commissioned Hot Dry Rocks Pty Ltd(“HDRPL”) to review depth and temperaturepotential <strong>of</strong> GEL’s 220, 221 and 281 (GEL 502was not granted at <strong>the</strong> time <strong>of</strong> this review). Walsh(2009A) found in this brief review that preliminarytemperature models using ‘best fit’ indicated that<strong>the</strong> temperature at <strong>the</strong> top <strong>of</strong> <strong>the</strong> Hutton where itis at its deepest was estimated to be in <strong>the</strong> order<strong>of</strong> 142°C (see Figure ?) and that <strong>the</strong> top <strong>of</strong> HuttonSandstone in <strong>the</strong> area <strong>of</strong> maximum thickness isinterpreted to lie between 2,150 and 2,200mdepth.Walsh (2009B), finally, also assessedpermeability assessments from 246 core samplescollected from 12 petroleum wells in a depthrange <strong>of</strong> 1,700m to 2,000m in <strong>the</strong> area andconcluded that <strong>the</strong> permeability appeared to behigh, with <strong>the</strong> bulk <strong>of</strong> <strong>the</strong> values in <strong>the</strong>encouraging 100 to 2,000 mD region.Interestingly, though data presented by Walshshowed a wide range <strong>of</strong> permeabilities, <strong>the</strong>y doindicate that even a less thick horizon <strong>of</strong> <strong>the</strong>Hutton Sandstone has <strong>the</strong> ability to sustainreasonable flow rates.Concluding, <strong>the</strong> Hutton sandstone in GEL 220 ismodeled at a depth in excess <strong>of</strong> 2,000m and witha temperature at its top <strong>of</strong> 142 deg C.Permeability estimates from 12 wells with porosityand permeability estimates <strong>of</strong> <strong>the</strong> HuttonSandstone indicate a bi-modal population with <strong>the</strong>larger population in <strong>the</strong> vicinity <strong>of</strong> 50mD to2,000mD. If a conservative value <strong>of</strong>, say, 250mDis chosen assuming not all parts are productive,<strong>the</strong>n at <strong>the</strong> estimated thickness <strong>of</strong> HuttonSandstone <strong>of</strong> 380m, <strong>the</strong>re is a potential <strong>of</strong> areservoir with a transmissivity <strong>of</strong> 90-100 Dm.These highly encouraging estimates suggest that<strong>the</strong> Hutton sandstone represents a strongprospect for developing a low risk hot sedimentaryaquifer, geo<strong>the</strong>rmal energy.Great Artesian Basin and HuttonSandstoneThe Eromanga basin was deposited as an uninterruptedsequence from <strong>the</strong> Early Jurassic toMid-Late Cretaceous, see Figure below. Thebasal units are mainly non-marine to marginalmarine, however, marine influences dominate <strong>the</strong>silts and mudstones <strong>of</strong> <strong>the</strong> Marree Subgroup.Non-marine sandstones were deposited in <strong>the</strong>final stages (Winton Formation). Of petroleumand geo<strong>the</strong>rmal interest are <strong>the</strong> terrestrialsandstones <strong>of</strong> <strong>the</strong> Hutton, Namur, and CadnaowieFormations. These units, in particular <strong>the</strong>Cadna-owie Formation, constitute much <strong>of</strong> <strong>the</strong>Great Artesian Basin.Figure 3. Preliminary 1D temperature prediction for HuttonSandstone based on temperature data from nearby wells15


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Figure 5. GAB extent and ground water temperatures (afterHabermehl, 2001).supply, as is <strong>the</strong> case at Birdsville, as well as forstock use. Ground temperatures at <strong>the</strong> well headsrange from 30deg C to 100deg C. Groundwatertemperatures from 1,880 water wells tapping in to<strong>the</strong> Cadna-owie aquifer, above <strong>the</strong> deeper HuttonSandstone, from are presented in Figure 5.Figure 4. General stratigraphy <strong>of</strong> <strong>the</strong> Eromanga and LakeEyre Basin sequences in <strong>the</strong> Cooper Basin (Gravestock et al,1998.The Jurassic Hutton Sandstone is a sandstonedominatedunit that has been interpreted to havebeen deposited in a continent-scale, braidedstreamenvironment, and to have beenunconfined across a broad alluvial plain extendingover much <strong>of</strong> Queensland and South Australia.The Canterbury Plain in New Zealand isconsidered as a close modern analogue. TheHutton Sandstone is well-known as a regionalaquifer in a number <strong>of</strong> fields in both SouthAustralia and Queensland.Habermehl (reference?) notes that <strong>the</strong> GreatArtesian Basin is a well known aquifer with some4,700 artesian water bores drilled in to it. Most <strong>of</strong><strong>the</strong>se artesian wells tap in to <strong>the</strong> Cadna-owieaquifer, <strong>the</strong> uppermost artesian aquifer <strong>of</strong> thismulti-layered sequence. Groundwater in <strong>the</strong>Cadna-owie aquifer is <strong>of</strong> good quality, containingbetween 500mg/l to 1,000mg/l total dissolvedsolids. It is suitable for domestic, town-waterGeo<strong>the</strong>rmal developmentThe Hutton Project aims to produce an artesianflow <strong>of</strong> hot water sufficient to generate about 1MWe. Although greater flows could be produced,ei<strong>the</strong>r by artesian flow or by pumping, capable <strong>of</strong>generating up to 5MWe per production well,sufficient demand to justify such a developmentdoes not exist and so <strong>the</strong> focus is on smallerplants to replace diesel or gas generation in <strong>the</strong>local oil fields, small settlements and pastoralleases.Artesian flows at adequate temperature can beproduced from <strong>the</strong> Hutton Sandstone at welldepths down to 2,500m. Artesian pressures <strong>of</strong> atleast 10bar are expected which will be easilysufficient for a hot water flow <strong>of</strong> about 30 kg/swhich will be required for 1 MWe Geo<strong>the</strong>rmalPower Plant.It is intended that <strong>the</strong> cooled exhaust water will bereinjected back into <strong>the</strong> same formation. For <strong>the</strong>small flows that are required, it is anticipated thatno or minimal reinjection pumping power will berequired. ie if pressures can be maintained in a16


Top Hutton Sandstone > 2000 mbslclosed circuit, it is expected that a <strong>the</strong>rmosiphonwill be established.The Hutton Sandstone can be found at suitabledepths over relatively wide areas <strong>of</strong> <strong>the</strong> GELs andso <strong>the</strong>re is a possibility that a number <strong>of</strong> standaloneplants based on a production/reinjectionwell pair could be developed.The development scenarios considered are basedon <strong>the</strong> use <strong>of</strong> two to five PureCycle © units asmarketed by Pratt and Whitney Power Systems.These units have a nominal 280 kW grosscapacity and are designed to be water cooled. Itis believed that water cooling, as opposed to aircooling will be required because <strong>of</strong> <strong>the</strong> highambient dry bulb temperatures encountered in <strong>the</strong>region.In order for a small project to be economic, it willbe necessary to adopt water well drilling practicesas opposed petroleum drilling practices.<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Potential marketAlthough extensive research has not beencompleted into available electrical loads that couldbe satisfied by geo<strong>the</strong>rmal electricity producedfrom <strong>the</strong> Hutton Sandstone, <strong>the</strong> project location isabout half way between <strong>the</strong> townships <strong>of</strong> Moombaand Innamincka, where it is known that <strong>the</strong>re is asignificant reliance on diesel and gas firedgeneration. In addition grazing homesteads arealso known to rely on diesel generation. Finally,<strong>the</strong>re are several gas plants and pipeline nodesrequiring energy, also representing a small localmarketAlthough <strong>the</strong> gas plants and pipeline node pointsare known, maps <strong>of</strong> <strong>the</strong>se have been removedfrom public access to prevent <strong>the</strong>m from beingtargets <strong>of</strong> a terrorist act. However, studying <strong>the</strong>pipeline network in Figure 7, one can indirectlyA 150mm diameter x 1,500m deep water welldrilled at Clifton Hills (outside <strong>the</strong> license area)flowed at approximately 155 kg/s under artesianpressure and had an overall cost <strong>of</strong> less than$1m. It is believed that similar technology couldbe utilized to drill to depths <strong>of</strong> 2-2500m for anoverall cost <strong>of</strong> less than $2m per well.MoombaHutton Sst > 2000m(red areas)210 0 mbsl2 0 0 mbs lGEL 220(black)Location and InfrastructureGEL 220 has been estimated to be host <strong>the</strong>hottest Hutton Sandstone in Panax’s geo<strong>the</strong>rmallicence portfolio. A strong candidate for <strong>the</strong> HuttonSandstone Geo<strong>the</strong>rmal Well is <strong>the</strong> south westernpart <strong>of</strong> GEL 220, as indicated in Figure 6. Thislocation is in a large area <strong>of</strong> deep Hutton, close toa road and outside <strong>the</strong> Innamincka RegionalReserve. There are Native Title agreementscovering this are as is <strong>the</strong> case for all <strong>of</strong> Panax’sgeo<strong>the</strong>rmal licences in Cooper Basin.Figure 7. Pipelines in Cooper Basin. Gas production plantsare inferred at end points <strong>of</strong> pipelines (blue) and nodes atintersection <strong>of</strong> pipelines .locate gas plants and pipeline nodes,representing small local electricity markets.Innamincka and Moomba townships are alsoannotated in this figure. It is interesting to note <strong>the</strong>huge number <strong>of</strong> wells that have been drilled in toCooper Basin, represented by black dots on thismap. Each <strong>of</strong> <strong>the</strong>se wells were preceded byintense studies <strong>of</strong> seismic, 2D and more recentlyalso 3D seismic. These data, available free <strong>of</strong>charge <strong>of</strong> PIRSA, represent a huge investmentand to Panax, a significant advantage inassessing <strong>the</strong> Hutton Sandstone, as has beenreviewed in previous sections.It is believed that a mini 3 phase power grid couldbe established to which users in <strong>the</strong> vicinity wouldhave access, ei<strong>the</strong>r with a 3 phase connection ora Single Wire Earth Return(WER)line.Figure 6: GEL 220 (black outline) with <strong>the</strong> areas whereHutton Sandstone is interpreted from regional data to bedeeper than 2000m (red areas). The estimate <strong>of</strong> <strong>the</strong> totalarea <strong>of</strong> Hutton Sandstone in excess <strong>of</strong> 2000 m is about 300km2. Light purple indicate pipe lines with Moomba gas Plantto <strong>the</strong> west <strong>of</strong> GEL 220.17Development Time FrameIt is envisaged that a small scale plant will be ableto be brought on line twelve to eighteen monthsafter <strong>the</strong> spudding <strong>of</strong> <strong>the</strong> production well.


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>PureCycle © units are built on a production line in<strong>the</strong> US and are shipped as a fully assembled skidand <strong>the</strong>refore a minimum amount <strong>of</strong> site work isrequired. A separate cooling system will need tobe engineered and installed.The production and injection wells are eachestimated to take about 3 weeks to drill.The overall project schedule is estimated to beabout 24 months.Cost estimates and assumptionsCapital costs have been estimated fromquotations received from plant suppliers anddrilling companies and from detailed in-houseestimates for balance <strong>of</strong> plant and o<strong>the</strong>rinfrastructure requirements.In respect <strong>of</strong> operating costs, a small plant <strong>of</strong> <strong>the</strong>type initially envisaged will not be permanentlymanned. Remote or automatic operation will berequired with routine maintenance performed onan as required basis. PureCycle plants are verysimple with plant overhauls required on a semiannualor longer interval basis.Modelling resultsThe investigation <strong>of</strong> various engineering scenariosfor using <strong>the</strong> Hutton Sandstones have focused onsmaller scale development (500kW – 1.5 MW)which could be used to replace existing diesel orgas fired generation in <strong>the</strong> adjacent oil fields,small settlements and pastoral leases.Even smaller sub-optimal developments can stillbe very attractive as small package plant can beused and parasitic pumping power is muchreduced because <strong>the</strong> artesian pressure toge<strong>the</strong>rwith <strong>the</strong>rmo siphon effects negates <strong>the</strong> need forproduction or reinjection pumps.PureCycle units as marketed by Pratt & WhitneyPower Systems could be ideal for this application.These are package units with a nominal rating <strong>of</strong>280 kW gross and multiple units could be installedor added to match electricity demand.Slim (150mm diameter), Deep (1,500m) waterwells drilled into <strong>the</strong> GAB have yielded significantartesian flow rates (155 l/s) at temperatures <strong>of</strong>about 100 deg C at surface. These wells can bedrilled very economically (


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>“Petroleum geology <strong>of</strong> South Australia, Volume 4:Cooper Basin, Department <strong>of</strong> Primary Industriesand Resources, South Australia, Report book,98/9. 1998.19


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Investment in common-use network infrastructure to triggerincremental expansion in geo<strong>the</strong>rmal energy generating capital stockAshok A. Kaniyal 1,3* , Jonathan J. Pincus 2 , Graham (Gus) J. Nathan 1,31 School <strong>of</strong> Mechanical Engineering, The University <strong>of</strong> Adelaide SA 50052 School <strong>of</strong> Economics, The University <strong>of</strong> Adelaide SA 50053 Centre for <strong>Energy</strong> Technology, The University <strong>of</strong> Adelaide SA 5005*Corresponding Author: Ashok A. Kaniyal, ashok.kaniyal@adelaide.edu.auThis paper analyses <strong>the</strong> potential <strong>of</strong> a novelapproach to avoid <strong>the</strong> cost <strong>of</strong> expensivetransmission infrastructure in connecting remotegeo<strong>the</strong>rmal power suppliers to market through acommunity <strong>of</strong> data centres. A strategy forinvestment in a common-use facility to triggerincremental growth in a complementarycommercial alliance is presented. The commercialalliance consists <strong>of</strong> investors in <strong>the</strong> ‘common-use’fibre-optic cable data network, a community <strong>of</strong>data centres, and geo<strong>the</strong>rmal energy resources.A real options approach to capital investmentdecision making is used to define <strong>the</strong> conditionsunder which investment in <strong>the</strong> common-usefacility (which in economics is a ‘local publicgood’), will be commercially justifiable.Excess capacity in <strong>the</strong> fibre-optic networkresource is what gives it <strong>the</strong> attributes <strong>of</strong> a ‘localpublic good’. A critical assessment shows thatinvestment in such infrastructure could play asignificant role in triggering <strong>the</strong> initial and lateradditions to installed geo<strong>the</strong>rmal energy capitalstock, to generate and supply power to a network<strong>of</strong> data centres in a remote area. Theinfrastructure needs <strong>of</strong> data centres are chosenfor this assessment because <strong>the</strong>se facilities canbe collocated with <strong>the</strong> geo<strong>the</strong>rmal resource, and<strong>the</strong>ir energy consumption is well suited to ademonstration-scale plant.The real options analysis <strong>of</strong> resource allocation inthis hypo<strong>the</strong>tical commercial setting isunderpinned by <strong>the</strong> stochastic representation <strong>of</strong><strong>the</strong> future growth in demand for energy from anetwork <strong>of</strong> data centres, in <strong>the</strong> micro-gridcommunity described. The results from thisanalysis provide an understanding <strong>of</strong> <strong>the</strong> criticalconditions under which investment in <strong>the</strong> fibreoptic network resource could take place.geo<strong>the</strong>rmal energy production capacity can bederived. This derivation provides an optimisedtime series pr<strong>of</strong>ile <strong>of</strong> incremental expansion incapital stock, to satisfy <strong>the</strong> discrete units <strong>of</strong>stochastic demand for energy in this micro-gridsetting. The benefits <strong>of</strong> this assessment thus lie in<strong>the</strong> ability to understand <strong>the</strong> likely time period overwhich significant economies <strong>of</strong> scale in generatingcapacity can be achieved. This hencefor<strong>the</strong>nables a characterisation <strong>of</strong> <strong>the</strong> point at whichinvestment in electricity grid infrastructure (or <strong>the</strong>like) may be justified. The process associated withthis stochastic approach to analysing investmentdecisions enables <strong>the</strong> consideration <strong>of</strong> <strong>the</strong>systematic risks in this much larger but end-goalinvestment horizon.Finally <strong>the</strong> study presents public policyrecommendations regarding State involvement inestablishing capacity in this network resource, toassist <strong>the</strong> development <strong>of</strong> <strong>the</strong> necessaryeconomies <strong>of</strong> scale in geo<strong>the</strong>rmal energyproduction over time.Keywords: Real options <strong>the</strong>ory, networkinfrastructure, local public good, geo<strong>the</strong>rmalenergy.ReferenceDixit, A., Pindyck, R.S., 1994. Investment underuncertainty. Princeton University Press, PrincetonNJ.The real options approach is an appropriate toolto assess investment strategy in this context,because it incorporates uncertainty in consumerdemand, and analyses <strong>the</strong> resultant flexibility in<strong>the</strong> timing <strong>of</strong> investment decisions. In contrast, <strong>the</strong>discounted cash flow method suggests that aninvestment decision is made only once, i.e. at <strong>the</strong>commencement <strong>of</strong> <strong>the</strong> discounting period.Once a commercially justifiable investmentpathway for <strong>the</strong> local public good is defined, apr<strong>of</strong>ile <strong>of</strong> incremental expansion in <strong>the</strong> installed20


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Ultra deep drilling technologies for geo<strong>the</strong>rmal energy productionDipl. Ing. Ivan Kočiš, PhD., Dipl. Ing. Tomáš Krišt<strong>of</strong>ič, Dipl. Ing. Igor KočišGeo<strong>the</strong>rmal AnywhereBratislava, Slovak republicAbstractSubstance <strong>of</strong> <strong>the</strong> presented research anddevelopment is <strong>the</strong> technology for realization <strong>of</strong>geo<strong>the</strong>rmal boreholes approximately 6 to 10 kmdeep. In such depths, rock temperature reaches200°C to 400°C practically all over <strong>the</strong> world. Inthis depth, <strong>the</strong>rmal capacity <strong>of</strong> 1 km 3 is about1017 J (when cooled down by 100°C); this iscomparable with annual demand <strong>of</strong> Slovakia. Withreal consumption <strong>of</strong> approximately 20 to 40 MW<strong>the</strong> capacity <strong>of</strong> <strong>the</strong> same borehole would besufficient for several hundreds <strong>of</strong> years. Deepgeo<strong>the</strong>rmal energy is available anywhere,represents <strong>the</strong> most serious candidate for a baseload 24/7 electricity production, <strong>the</strong>re are no CO 2emissions and is scalable according to <strong>the</strong> localneeds. The main obstacle for utilization <strong>of</strong> <strong>the</strong> vastenergy reserves is <strong>the</strong> price rising exponentiallyper 1 km <strong>of</strong> a borehole depth in present-daydrilling technologies. Costs <strong>of</strong> such boreholescannot be considered as a basis <strong>of</strong> repeatedprojects in most territories <strong>of</strong> <strong>the</strong> world. Thus,intense research and development <strong>of</strong> new deepdrilling technologies is necessary.There are more than 20 researched new drillingtechnologies, but none <strong>of</strong> <strong>the</strong>m gave at presentdesired economic and technical parameters for 6-10 km depths. The technology must becompatible with extreme conditions at such depth(pressure up to 1000 bar and temperatures morethan 400°C) and very hard rock like granite.Presented radically innovative concept <strong>of</strong> drillingand transport <strong>of</strong> material is protected by patentsand being a basis <strong>of</strong> a know-how based uponinnovative utilization <strong>of</strong> proven technologies. Themethod is suitable primarily for extreme pressureand temperature conditions, and has all prerequisitesto meet <strong>the</strong> basic requirement – linearprice growth with borehole depth. The conceptwas first time publicly presented during<strong>Conference</strong> <strong>of</strong> <strong>the</strong> 6th EU Framework Programmeproject "Engine", aimed at ultra-deep geo<strong>the</strong>rmalenergy and related research within future 7thFramework Program projects. The conceptaroused considerable attention and interest inparticipation in future projects.Keywords: Deep drilling, Bitless drilling, Noncontactdrilling, Pulsed plasma drilling, EGSIntroductionThe renowned MIT (USA) study "The Future <strong>of</strong>Geo<strong>the</strong>rmal <strong>Energy</strong> – Impact <strong>of</strong> EnhancedGeo<strong>the</strong>rmal Systems (EGS) on <strong>the</strong> United Statesin <strong>the</strong> 21st Century" (2006) points out <strong>the</strong>essential importance <strong>of</strong> <strong>the</strong> developing aneconomical deep geo<strong>the</strong>rmal drilling technology.With current drilling technologies, drilling pricebelow 3 km rises exponentially with depth. Thus,finding a drilling technology with which <strong>the</strong> drillingprice rise would be approximately linear withincreasing well depth is an important challenge.In his presentation, Jefferson Tester, a co-author<strong>of</strong> this study, characterizes <strong>the</strong> key requirementson new fast and ultra-deep drilling technology asfollows: <strong>the</strong> price <strong>of</strong> drilling rises linearly with depth, <strong>the</strong> possibility to make vertical or inclinedboreholes up to 20 km deep, casing formed on site in <strong>the</strong> well.There are under way more than 20 researchefforts solving innovative drilling technology suchas: laser, spallation, plasma, electron beam,pellets, enhanced rotary, electric spark anddischarge, electric arc, water jet erosion,ultrasonic, chemical, induction, nuclear, forcedflame explosive, turbine, high frequency,microwave, heating/cooling stress, electric currentand several o<strong>the</strong>r.No one from <strong>the</strong>se until now proved to beeffective in severe conditions and no one issolving <strong>the</strong> problem in complex including <strong>the</strong>energy and material transport from 6 to 10 kmtechnically and economically. We selected drillingapproach based on integration <strong>of</strong> pulsed electricalplasma with water jet assisted processes.What is different from current drillingtechnologies?Process <strong>of</strong> rock disintegration is <strong>the</strong> mostimportant activity when drilling ultra-deepborehole, but not <strong>the</strong> only one contributing to <strong>the</strong>exponential price rise. Therefore a completelynew approach should be considered. That is alsosubstantial difference between GA’s drillingconcept and mentioned drilling technologies.GA drilling approach is based on integration <strong>of</strong>pulsed electrically generated plasma with waterjet assisted processes. Advantages <strong>of</strong> <strong>the</strong> GA’stechnology are as follows:21


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>1. Controllability <strong>of</strong> <strong>the</strong> process <strong>of</strong> disintegrationand efficient generation <strong>of</strong> media fordisintegration2. Pulsed mode <strong>of</strong> <strong>the</strong> media towards <strong>the</strong>disintegrating rock3. High heat flow4. Pulsed power technologies - Timecompression5. Optimized cuttings6. Cuttings washout using <strong>the</strong>rmo lift and waterjet interaction7. Casing while drilling – vitrified rock8. Dynamic temperature stress on <strong>the</strong> rock9. Control and sensoric system in extremeconditions10. Restart <strong>of</strong> drilling process in extreme highpressure conditionsWe identified nine different physical processesused for disintegration <strong>of</strong> <strong>the</strong> rock. Under researchis a synergic exploitation <strong>of</strong> selected processes,also using supercritical fluids.Total energy costs <strong>of</strong> drilling represent only afraction <strong>of</strong> <strong>the</strong> total cost and our approach is tomelt <strong>the</strong> rock with a safe temperature tolerance.What is different compared tospallation technology?Spallation process is <strong>the</strong> closest technology, buthas several issues and drawbacks. We canmention small temperature interval in whichspallation process takes place, dependence <strong>of</strong> <strong>the</strong>interval from rocks and non-effective process <strong>of</strong>spallation in some types <strong>of</strong> rock.Total energy costs <strong>of</strong> drilling represent only afraction <strong>of</strong> <strong>the</strong> total cost. Our approach is to melt<strong>the</strong> rock and manage cuttings with optimized size.The presented drilling technology is based on aset <strong>of</strong> research project, development <strong>of</strong> criticalaggregates, proving correctness <strong>of</strong> <strong>the</strong> conceptand preparation for <strong>the</strong> industrial developmentstage which should serve <strong>the</strong> application aspect.In cooperation with several Universities andAcademy <strong>of</strong> Sciences teams are solved <strong>the</strong>difficult functional and material problems forextreme in-field conditions. The purpose <strong>of</strong> <strong>the</strong>project is to research all critical parts up to <strong>the</strong>level <strong>of</strong> functional laboratory samples. Sufficientbackground data for fur<strong>the</strong>r industrialdevelopment should be provided. On <strong>the</strong> basis <strong>of</strong><strong>the</strong> results obtained in technological parts <strong>of</strong> <strong>the</strong>solution, <strong>the</strong> project is assumed to givetechnological pro<strong>of</strong> <strong>of</strong> <strong>the</strong> whole concept.How is that possible?The innovation concept is able to integrate <strong>the</strong>proven technologies compatible with hightemperatures and pressures using <strong>the</strong>combination <strong>of</strong> electrical energy source for both –producing <strong>the</strong> needed form <strong>of</strong> <strong>the</strong> energy and forenabling <strong>the</strong> <strong>the</strong>rmal lift buoyancy effect fora cutting transport.The rock crushing technologies will be used ina synergy <strong>of</strong> electrical discharge, pulsed plasmaand water jet in appropriate alternatives which willbe <strong>the</strong> subject <strong>of</strong> research and experimental work.This radical innovative method avoids <strong>the</strong> inherentlimitations <strong>of</strong> conventional rotary drilling andmaterial transport.Complexity <strong>of</strong> <strong>the</strong> problem, harsh environment inwhich <strong>the</strong> targeted technology shall work, and <strong>the</strong>radical innovation concept requires gradualapproach to <strong>the</strong> research, development andrealization <strong>of</strong> <strong>the</strong> whole system.Ultra deep drilling technology -geo<strong>the</strong>rmal energy revolution enablerThe realization <strong>of</strong> <strong>the</strong> Ultra deep drillingtechnology will open <strong>the</strong> way to <strong>the</strong>rmal energyresources to be used for production <strong>of</strong> electricenergy without greenhouse gas emissions andwith zero operation costs <strong>of</strong> fuel. The currentstatus <strong>of</strong> electric energy production is based uponfossil fuel, it is not compatible with reduction <strong>of</strong>emissions, and, moreover, is not resistant againstincrease <strong>of</strong> prices <strong>of</strong> crude oil and gas in <strong>the</strong>world, and <strong>of</strong> those <strong>of</strong> <strong>the</strong> nuclear fuel, which arederived from <strong>the</strong>m.Deep geo<strong>the</strong>rmal systems open <strong>the</strong> way toreplacing coal and gas capacities by geo<strong>the</strong>rmalcapacities within <strong>the</strong> future 20 years.Figure 1: Extra and ordinary geo<strong>the</strong>rmal conditions –difference brings <strong>the</strong> ultra-deep drilling technology.Such resource <strong>of</strong> <strong>the</strong> energy will adequatelysatisfy <strong>the</strong> demand <strong>of</strong> energy, which has <strong>the</strong>following properties: It is local, stable, scalable upon need, with nolosses caused by long distance transfer. It does not produce any emissions, and issafe.22


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>No supply <strong>of</strong> energy carriers is needed, "fuel"costs are zero and unaffected by world pricesvariation, crisis developments and geopoliticalsituations.Creates numerous secondary applications,primarily for small and medium enterprises;moreover, creation <strong>of</strong> job opportunities isenhanced.ConclusionThe revolutionary patented concept <strong>of</strong> <strong>the</strong> ultradeepdrilling and transport <strong>of</strong> crushed rockmaterial upwards leads to new implementationpossibilities.It is a radical abandonment <strong>of</strong> <strong>the</strong> classic drillingtechnologies with connected tubes in long stringswith <strong>the</strong> inefficient energy transport to <strong>the</strong> drillingsite at <strong>the</strong> bottom <strong>of</strong> <strong>the</strong> well and complicated,inefficient pumping <strong>of</strong> <strong>the</strong> crushed material to <strong>the</strong>surface.This new drilling technology is a result <strong>of</strong> <strong>the</strong> longtime effort to solve <strong>the</strong> problem <strong>of</strong> <strong>the</strong>exponentially growing price in relation to <strong>the</strong>borehole depth and thus enabling <strong>the</strong> realexploitation <strong>of</strong> <strong>the</strong> geo<strong>the</strong>rmal energy for <strong>the</strong>electrical power generation.ReferencesTester, Jefferson W.; et. al. (2006), The Future <strong>of</strong>Geo<strong>the</strong>rmal <strong>Energy</strong>, Impact <strong>of</strong> EnhancedGeo<strong>the</strong>rmal Systems (EGS) on <strong>the</strong> United Statesin <strong>the</strong> 21st Century: ISBN 0-615-13438-6,http://geo<strong>the</strong>rmal.inel.gov/publications/future_<strong>of</strong>_geo<strong>the</strong>rmal_energy.pdfJefferson Tester et al., US Pat 5771984,“Continuous drilling <strong>of</strong> vertical boreholes by<strong>the</strong>rmal processes: rock spallation and fusion"Kobayashi et al., US Pat 6870128, “LASERBORING METHOD AND SYSTEM”Hirotoshi et al., 1999, "Pulsed Electric Breakdownand Destruction <strong>of</strong> Granite", published in Jpn. J.Appl. Phys. Vol.38 (1999), 6502-6505Dipl. Ing. Ivan Kočiš, PhD., Dipl. Ing. TomášKrišt<strong>of</strong>ič, Ultra deep drilling technologies forgeo<strong>the</strong>rmal energy production, InternationalGeo<strong>the</strong>rmal Days <strong>Conference</strong>, May 2009, CastaPapiernicka, Slovakia23


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>A Preliminary Study on Na-Cl-H 2 O-Rock Interactions <strong>of</strong> <strong>the</strong> HotFractured Rock Geo<strong>the</strong>rmal System in Cooper Basin, South AustraliaGideon B. Kuncoro 1 , Yung Ngothai 1* , Brian O’Neill 1 , Allan Pring 2 , Joël Brugger 21 The University <strong>of</strong> Adelaide, School <strong>of</strong> Chemical Engineering, North Terrace, Adelaide, SA, 50002 South <strong>Australian</strong> Museum, North Terrace, Adelaide, SA, 5000*Corresponding author: yung.ngothai@adelaide.edu.auA preliminary study was undertaken to observe<strong>the</strong> fluid-rock interaction in Na-Cl-H 2 O system.Samples <strong>of</strong> drill cuttings from a borehole 5 kmdeep from Habanero 3 well were contacted with250 ppm sodium chloride solution in a<strong>the</strong>rmosyphon induced loop reactor at 250 o C and40-50 bar. The experiments were carried out in aTitanium flow through cell for 1, 7, and 28 days at250 o C and 40 bars). The fluid was replaced every24 hours in order to accelerate <strong>the</strong> dilution rate toobserve which minerals are reactive (soluble) andto mimic a condition which uses fresh water ortreated water from a precipitation tank that isreinjected to <strong>the</strong> fracture. Fluid and rock sampleswere analysed prior to, and after circulation toobserve <strong>the</strong> dissolved minerals and mineralogy.Water analysis was performed using ICP-MS, androck analyses were conducted using an opticalmicroscope, SEM and XRD. The experimentalresults indicated that mineral dissolution wasmore rapid in <strong>the</strong> early stages <strong>of</strong> <strong>the</strong> experiment.This may be a consequence <strong>of</strong> <strong>the</strong> dissolution <strong>of</strong>finer rock particles. SEM observations showedevidence <strong>of</strong> etching <strong>of</strong> <strong>the</strong> mineral surfacesconsistent with partial dissolution. XRD resultsindicated that <strong>the</strong> feldspars (NaAlSi 3 O 8 andKAlSi 3 O 8 ) in <strong>the</strong> rock had completely dissolvedand small amount <strong>of</strong> quartz remained. ICP-MSanalysis on <strong>the</strong> water sample confirmed that somemineral dissolution has occurred. Theconcentrations <strong>of</strong> <strong>the</strong> elements increased withtime.Experiment running for 14 days is currently beingundertaken and <strong>the</strong> results will be used tocomplement this study. Future work will involvereaction path modelling to predict mineralprecipitation.Keywords: hot fractured rock, fluid-rockinteraction, Na-Cl-H 2 O system, geo<strong>the</strong>rmal,Cooper Basin, Habanero, <strong>the</strong>rmosyphonIntroductionA study <strong>of</strong> <strong>the</strong> interactions between rock andcirculating fluid is essential to determine <strong>the</strong>chemical changes and mineral alteration <strong>of</strong> ageo<strong>the</strong>rmal system. This study was undertaken toobserve mineral dissolution due to <strong>the</strong> interactionwith Na-Cl-H 2 O system. Existing reservoirgranites are currently in equilibrium with <strong>the</strong>surrounding ground water. The injection <strong>of</strong> freshwater to extract <strong>the</strong>rmal energy from <strong>the</strong> host rockwill alter <strong>the</strong> ground water chemistry and thus <strong>the</strong>fluid-rock equilibrium. While recirculating <strong>the</strong>brine, partial chemical dissolution or mineralspecies alteration may occur. This may potentiallyincrease <strong>the</strong> dissolved solids such as silica ando<strong>the</strong>r metals in <strong>the</strong> water. These dissolutionproducts <strong>of</strong> <strong>the</strong> components have differentequilibria, which will be a function <strong>of</strong> temperatureand pressure, thus precipitation or scaling <strong>of</strong> pipework and closure <strong>of</strong> fractures in <strong>the</strong> granite bodyare possible. The saturation <strong>of</strong> metals in fluid isvolume-dependent, where very small volumes <strong>of</strong>fluid may require slight under-cooling beforeprecipitation occurs. Clearly, characterization <strong>of</strong>fluid geochemistry is important in <strong>the</strong> evaluation <strong>of</strong><strong>the</strong> performance <strong>of</strong> geo<strong>the</strong>rmal systems (Grigsbyet al., 1989). Moreover, understanding <strong>the</strong>chemical interactions due to <strong>the</strong> injection <strong>of</strong> fluidinto hot granite is crucial for problems concerningclogging by precipitation and heat loss caused bydissolution (Azaroual and Fouillac, 1997).The study <strong>of</strong> fluid-rock interaction will allowdetermination <strong>of</strong> mineral alteration and dissolution<strong>of</strong> minerals due to <strong>the</strong> circulating water. To date,<strong>the</strong>re are a number <strong>of</strong> geochemical modellingcodes <strong>the</strong>refore <strong>the</strong>rmodynamic data bases areavailable and improved to predict equilibriumconditions and dissolution-precipitation rates(such as EQ3/6, TOUGH-REACT, SOLVEQ-CHILLER, SOLMINEQ, GWB, etc). However,fundamental processes associated with mineraldissolution and precipitation, pressuretemperaturegradient remain poorly understood(Marks et al., <strong>2010</strong>). Unfortunately, it is impossibleto generalize <strong>the</strong> actual field experience <strong>of</strong>mineral deposition in geo<strong>the</strong>rmal systems into oneconsistent <strong>the</strong>ory due to <strong>the</strong> vast chemical andoperational variation between field sites(Robinson, 1982). Therefore, although <strong>the</strong>re havebeen a number <strong>of</strong> studies on fluid-rockinteractions for different geo<strong>the</strong>rmal sites(Rimstidt and Barnes, 1980; Robinson, 1982;Posey-Dowty et al,. 1986; Savage et al., 1987;Grigsby et al., 1989; Savage et al., 1992;Azaroual and Fouillac, 1997; Yangisawa et al.,2005; Tarcan et al., 2005; Castro et al., 2006;Marks et al., <strong>2010</strong>), and studies <strong>of</strong> rock-chloridesolutions (Ellis, 1968; Dove and Crerar, 1990;Icenhower and Dowe, 2000) <strong>the</strong>se are probablynot directly applicable to <strong>the</strong> hot granite-basedgeo<strong>the</strong>rmal systems in <strong>the</strong> Cooper Basin.24


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>(a)(b)Figure 1: (a) Diagram <strong>of</strong> <strong>the</strong> flow through cell (b) Photograph <strong>of</strong> <strong>the</strong> geo<strong>the</strong>rmal flow through cellExperimentalSamples <strong>of</strong> drill cuttings from <strong>the</strong> Habanero 3 wellwere provided by Geodynamics. The sampleswere ultrasonically cleaned and analysedusing,<strong>the</strong> scanning electron microscope (SEM) at<strong>the</strong> Adelaide Microscopy Centre to observe bothsurface and cross-sectional area. Powder X-raydiffraction (XRD) analysis was carried out byAMDEL to observe <strong>the</strong> mineralogy. A preliminaryset <strong>of</strong> experiments to observe <strong>the</strong> fluid-rockinteraction were performed in batch mode. Thedrill cutting was used as <strong>the</strong> rock sample. Therock sample was crushed and sieved to give 100– 200 μm size fraction and approximately 0.7grams <strong>of</strong> rock were used in each batch. Thesample was enclosed in a pre-weighed wirebasket (approx. 50 μm mesh size) made fromstainless steel and placed in <strong>the</strong> sample holder <strong>of</strong><strong>the</strong> cell. The cell was filled through a valve in <strong>the</strong>base <strong>of</strong> <strong>the</strong> cell with 250 ppm sodium chloridesolution and 90 ml was drained from <strong>the</strong> cell toallow for fluid expansion upon heating. Thevelocity <strong>of</strong> <strong>the</strong> <strong>the</strong>rmosyphon circulating fluid isestimated to be approximately 0.1 m/s. The fluidrockinteraction periods were 1, 7, and 21 days. Atconclusion <strong>of</strong> this interaction period, <strong>the</strong> rocksample was dried (105 o C for 48 hours), cooled ina desiccator, and weighed to determine anyweight loss.The rock samples were analysed using SEM andXRD, and <strong>the</strong> water samples were stored andpreserved with 4% w/w <strong>of</strong> 1M nitric acid untilanalysis by ICP-MS to identify <strong>the</strong> dissolvedmetals. The silica content was quantified usingheteropoly blue method (HACH, 2009).Unfortunately, <strong>the</strong> anions were unable to be-analysed since <strong>the</strong> concentrations <strong>of</strong> HCO 3 andSO4 2- in <strong>the</strong> sample are lower than <strong>the</strong> detectionlimit <strong>of</strong> <strong>the</strong> current analysis.Results and DiscussionPreliminary results from <strong>the</strong> geo<strong>the</strong>rmal cellexperiment illustrate that <strong>the</strong> dissolution <strong>of</strong> <strong>the</strong>25


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Weight loss <strong>of</strong> rock (%)1<strong>2010</strong>080604020images are presented in Figure 3. The SEMimages <strong>of</strong> <strong>the</strong> rock sample surfaces <strong>of</strong> feldsparsbefore and after <strong>the</strong> experiments are shown inFigure 4. It can be seen that pitting has started tooccur in 1 day circulation period. At <strong>the</strong> conclusion<strong>of</strong> 7 days circulation, <strong>the</strong> surface <strong>of</strong> feldsparsexperienced severe pitting and breakage. By <strong>the</strong>end <strong>of</strong> 28 days circulation, <strong>the</strong> feldspar hascompletely dissolved and some quartz andundissolved minerals remain.00 5 10 15 20 25 30Time (d)H2ONaClFigure 2: Change in weight loss <strong>of</strong> rock (% w/w) versus timerock (% w/w) increases with time (Figure 2). Itshows that <strong>the</strong> dissolution appears more rapid in<strong>the</strong> early stages <strong>of</strong> <strong>the</strong> experiment. This isprobably due to <strong>the</strong> dissolution <strong>of</strong> <strong>the</strong> morereactive minerals (feldspars). It is seen that moreminerals dissolved in <strong>the</strong> Na-Cl-H 2 O systemcompared to pure water (reverse osmosis treatedwater). The presence <strong>of</strong> higher electrolyteconcentration (e.g., Cl - ) in Na-Cl-H 2 O systemincreases <strong>the</strong> dissolution rate <strong>of</strong> some mineralssuch as quartz (Dove and Crerar, 1990). Thelatter stage <strong>of</strong> <strong>the</strong> experiment approached anequilibrium state. However <strong>the</strong> fluid is notnecessarily saturated with minerals (feldspar), butdue to <strong>the</strong> exhaustion <strong>of</strong> <strong>the</strong> soluble phase(s) andslower dissolution rate <strong>of</strong> <strong>the</strong> remaining phase(s).Note that <strong>the</strong> circulating fluid is replaced every 24hours.Rock AnalysisMineralogical analysis was performed on <strong>the</strong> drillcuttings from Habanero 3 well using x-rayfluorescence (XRF) and x-ray diffraction (XRD).The major elements and <strong>the</strong>ir host minerals <strong>of</strong> <strong>the</strong>rock are quartz (SiO 2 ), albite (Na,Ca)AlSi 3 O 8 , andmicrocline (KAlSi 3 O 8 ) (Pring, pers. comm. 2009).The XRF analysis was carried out by <strong>the</strong> School<strong>of</strong> Earth and Environmental Sciences, AdelaideUniversity (Table 1). The XRD analysis wasperformed by AMDEL (given in %wt) andconverted to mg for better understanding. Theresults show clearly that rapid dissolution hasoccurred. Silicon internal standard was added toobserve any possible amorphous, unfortunately<strong>the</strong> amorphous content were unable to bequantified by Amdel. Hematite, magnetite,anatase, chlorite and goethite may be accessoryminerals due to corrosion <strong>of</strong> <strong>the</strong> stainless steelreservoirs and <strong>the</strong> stainless steel wire basketused in <strong>the</strong> experiment.SEM images <strong>of</strong> <strong>the</strong> surface particles wereobtained using <strong>the</strong> secondary electron detector(SE) <strong>of</strong> <strong>the</strong> XL30 in Adelaide Microscopy. TheTable 1 XRF analysis <strong>of</strong> <strong>the</strong> rock sampleStarting Sample % WeightSiO 2 77.27Al 2 O 3 10.62Fe 2 O 3 1.46MnO 0.08MgO 0.09CaO 0.60Na 2 O 2.54K 2 O 4.45TiO 2 0.07P 2 O 5 0.01SO 3 0.15LOI 2.10Total 99.44Table 2 XRD analysis <strong>of</strong> <strong>the</strong> rock sampleStartingsampleAfter 1dayAfter 7daysAfter 28daysMineral composition (mg)QuartzSiO 2 273.5 252.2 119.6 7.6Albite(Na,K,Ca)Al (1-2) Si (3-2) O 8 206.9 184.0 138.9 0.0K-FeldsparKAlSi 3 O 8 125.6 115.9 57.9 0.0Muscovite(Na,K,Ca) 2 (Al,Fe,Mg) 4-6(Al,Si) 8 O 20 (OH,F) 4 59.1 54.5 34.7 0.0PyroxeneXY(Si,Al) 2 O 6 14.8 13.6 0.0 0.0Silicon*Si 44.3 47.7 27.0 1.4Chalcopyrite and or CalciteCuFe 2 and or CaCO 3 7.4 6.8 3.9 0.0SideriteFeCO 3 7.4 6.8 0.0 0.0HematiteFe 2 O 3 0.0 0.0 0.0 3.7MagnetiteFe3O4 0.0 0.0 0.0 1.0AnataseTiO 2 0.0 0.0 0.0 0.4Chlorite(Mg,Fe) 3 (Si,Al) 4 O 10 (OH) 2 .(Mg,Fe) 3 (OH) 6 0.0 0.0 0.0 2.3GoethiteFeO(OH) 0.0 0.0 3.9 0.6Amorphous 0.0 0.0 0.0 2.5Total sample 739.1 681.5 385.7 19.4SEM analyses <strong>of</strong> <strong>the</strong> cross section <strong>of</strong> <strong>the</strong> rocksamples were also conducted. Results are given26


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>in Figure 4. These images were obtained using<strong>the</strong> backscattered electron detector (BSE) andanalysed using <strong>the</strong> energy dispersive x-rayspectrometer (EDAX). The results suggest thatalbite feldspar is <strong>the</strong> most reactive (soluble)mineral, followed by microcline and quartz. TheBSE image <strong>of</strong> <strong>the</strong> sample from 28 day circulation(Figure 4D) confirms that only quartz and o<strong>the</strong>raccessory minerals were observed, and n<strong>of</strong>eldspars were present.ABFigures 5 and 6 show <strong>the</strong> concentration <strong>of</strong>elements versus time from <strong>the</strong> ICP-MS analysis,and Figure 7 show <strong>the</strong> silica concentration on <strong>the</strong>circulating water after 1, 7, and 28 days <strong>of</strong> fluidrockinteractions.Cumulative Concentration(ppm)120.00100.0080.0060.0040.0020.000.000 5 10 15 20 25 30time (d)AlKFigure 5: Concentration <strong>of</strong> Al and K in experimental liquidversus time12000.00CFigure 3: SEM images <strong>of</strong> <strong>the</strong> rock sample surface (a) startingrock (b) after 1 day experiment (c) after 7 days experiment (d)after 28 day experimentDCumulative concentration(ppb)10000.008000.006000.004000.002000.000.000 5 10 15 20 25 30time (d)Fe Mg Mn Ca BaFigure 4: BSE images <strong>of</strong> <strong>the</strong> rock cross sectional area (a)starting rock (b) after 1 day experiment (c) after 7 daysexperiment (d) after 28 day experimentFigure 6: Concentration <strong>of</strong> Fe, Mg, Mn, Ca and Ba inexperimental liquid versus timeABAccumulativeConcentration (ppm)1800160014001200100080060040020000 5 10 15 20 25 30time (d)SiO2CWater AnalysisThe initial pH <strong>of</strong> <strong>the</strong> water was 5.5. This did notchange significantly in all batch experiments.DFigure 7: Concentration <strong>of</strong> SiO2 in experimental liquid versustimeWater analysis results showed that <strong>the</strong>re wasenhanced leaching <strong>of</strong> <strong>the</strong> minerals, indicated by<strong>the</strong> increased element concentration in <strong>the</strong> liquidphase. The rapid reaction is probably <strong>the</strong>27


consequence to <strong>the</strong> dissolution <strong>of</strong> more reactive(soluble) phases in <strong>the</strong> rock sample. It is seen thathigh concentration <strong>of</strong> silica, aluminium andpotassium were dissolved in <strong>the</strong> liquid due todissolution <strong>of</strong> albite, microcline and quartz.Unfortunately <strong>the</strong> sodium concentration could notbe analysed accurately due to <strong>the</strong> high initialconcentration <strong>of</strong> sodium in <strong>the</strong> circulating fluid(250 ppm NaCl).Mass BalanceA simple mass balance was undertaken toobserve <strong>the</strong> sample loss to <strong>the</strong> circulating fluid.Since <strong>the</strong> sodium cannot be analysed accuratelyat this stage, it was assumed that <strong>the</strong> dissolvedconcentration would be similar to <strong>the</strong> dissolution<strong>of</strong> Albite Feldspars in pure water. Table 3 shows<strong>the</strong> system mass balance. A short circulating timewould result in less sample loss. The sample lossmay be due to <strong>the</strong> replacement <strong>of</strong> circulating fluid,since at <strong>the</strong> time <strong>of</strong> reinjection, <strong>the</strong> liquid mustoverflow through <strong>the</strong> sample and exiting <strong>the</strong> cell toremove excess air (any air bubble may disrupt <strong>the</strong>flow in <strong>the</strong> <strong>the</strong>rmosyphon).Table 3 System mass balanceNot including <strong>the</strong> concentration <strong>of</strong> <strong>the</strong> anions mayalso be ano<strong>the</strong>r cause <strong>of</strong> <strong>the</strong> unclosed massbalance.ConclusionDissolved(calc),mgDissolved,(wateranalysis),mgThe mineralogical analysis showed that <strong>the</strong> majorcomposition <strong>of</strong> <strong>the</strong> rock is quartz, albite andmicrocline. The fluid-rock interaction experimentshowed that dissolution reactions occurpredominantly in <strong>the</strong> early stages (to 7 days) <strong>of</strong><strong>the</strong> experiment due to <strong>the</strong> dissolution <strong>of</strong> reactiveminerals (feldspars). The dissolution reactionbegins to decrease due to <strong>the</strong> exhaustion <strong>of</strong> <strong>the</strong>reactive mineral and proceeds with <strong>the</strong> dissolution<strong>of</strong> <strong>the</strong> less reactive phase. Results <strong>of</strong> XRDshowed that feldspar experienced a clearreduction with time, followed by quartz.Liquid analysis showed higher concentrations <strong>of</strong>Na, K, Si, and Al compared to o<strong>the</strong>r analysedelements. These results suggest that <strong>the</strong>dissolution reaction occurs primarily for <strong>the</strong>feldspars.The dissolution <strong>of</strong> feldspar would suggest <strong>the</strong>improvement <strong>of</strong> <strong>the</strong> permeability (however, notnecessarily improving <strong>the</strong> fracture where mineral<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>deposits occur) and also suggest <strong>of</strong> potentialsilica scaling (if circulating fluid is near neutralpH). The concentration <strong>of</strong> silica 1400 ppm (from0.7g rock sample) was released to <strong>the</strong> liquidphase throughout <strong>the</strong> experiment.Future WorktimeInitial,mgRemaining,mg% wt.Loss,mg1 745.2 681.5 63.7 8.55 41.30 22.407 734.4 385.7 348.7 47.48 271.00 77.7028 737.7 19.4 718.3 97.37 427.95 290.3528An experiment is currently being conducted for 14days period to obtain more understanding on <strong>the</strong>dissolution (Figure 2). Sodium concentrationwould need to be accurately analysed. Thecurrent work has used 250 ppm sodium chloridesolution for <strong>the</strong> fluid-rock interaction and does notquite represent <strong>the</strong> actual interaction.Experiments with Increased amount <strong>of</strong> rocksample (increasing <strong>the</strong> rock/water ratio) are beingcarried out to observe any changes in equilibriumor saturated condition. A dissolution andprecipitation model will be generated using <strong>the</strong>data from previous experiments (pure water) and<strong>the</strong> current study. The model will be used topredict <strong>the</strong> dissolution rate and precipitation rate<strong>of</strong> <strong>the</strong> actual fluid-rock interaction.AcknowledgmentsThe research described in this paper has beensupported by The Department <strong>of</strong> PrimaryIndustries and Resources <strong>of</strong> South Australia(PIRSA) and Geodynamics. Theauthor would like to thankGeodynamics for supplying <strong>the</strong> drillcuttings, and <strong>the</strong> South <strong>Australian</strong>Museum and Adelaide Microscopy for<strong>the</strong> equipment access. The authorswould like to thank John Stanley from<strong>the</strong> School <strong>of</strong> Earth and Environmental Sciences,Adelaide University, Benjamin Wade and AoifeMcFadden for assistance in ICP-MS analysis,Shaun Chan and Kevin Li for <strong>the</strong>ir assistance in<strong>the</strong> experiments.ReferencesAzaroual, M., and Fouillac, C., 1997,Experimental Study and Modelling <strong>of</strong> Granite-Distilled Water Interaction at 180 o C and 14 Bars:Applied Geochemistry, V. 12, pp. 55-73.Castro, M. R., Lopez, D. L., Reyes, J. A., Matus,A., Montalvo, F. E., Guerra, C. E., 2006, ExpectedSilica Scaling from Reinjection Waters AfterInstallation <strong>of</strong> a Binary Cycle Power Station atBerlin Geo<strong>the</strong>rmal Field, El Salvador, CentralAmerica: GRC Transactions, V. 30, pp. 487-492Dove, P. M., and Crerar, D. A., 1990, Kinetics <strong>of</strong>Quartz Dissolution in Electrolyte Solutions using aHydro<strong>the</strong>rmal Mixed Flow Reactor: Geochimica etCosmochimica Acta, V. 54, pp 955-969Ellis, A. J., 1968, Natural Hydro<strong>the</strong>rmal Systemsand Experimental Hot-Water/Rock Interaction:Reactions with NaCl solutions and trace metalextraction: Geochimica et Cosmochimica Acta, V.32, pp. 1356-1363


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Grigsby, C. O., Tester, J. W., Trujillo JR., P. E.,and Counce, D. A., 1989, Rock-Water Interactionsin <strong>the</strong> Fenton Hill, New Mexico, Hot Dry RockGeo<strong>the</strong>rmal Systems I, Fluid Mixing and ChemicalGeo<strong>the</strong>rmometry: Geo<strong>the</strong>rmics, V. 18, pp. 629-656.HACH, 2009, DR/<strong>2010</strong> PortableSpectrophotometer Procedures Manual.http://www.hach.com/fmmimghach?/CODE%3A4930022286|1, p 767 – 772, accessed September2008Icenhower, J. P., and Dove, P. M., 2000, TheDissolution Kinetics <strong>of</strong> Amorphous Silica intoSodium Chloride Solutions: Effects <strong>of</strong>Temperature and Ionic Strength: Geochimica etCosmochimica Acta, V. 64, pp. 4193-4203Posey-Dowty, J., Crerar, D., Hellerman, R., andClarence, D. C., 1986, Kinetics <strong>of</strong> Mineral-WaterReactions: Theory, Design, and Application <strong>of</strong>Circulating Hydro<strong>the</strong>rmal Equipment: AmericanMineralogist, V. 71, pp. 85-94.Pring, A., 2009, personal communication.Rimstidt, J. D., and Barnes, H. L., 1980, TheKinetics <strong>of</strong> Silica-Water Reactions: Geochimica etCosmochimica Acta, V. 44, pp. 1683-1700.Robinson, B. A., 1982, Quartz Dissolution andSilica Deposition in Hot Dry Rock Geo<strong>the</strong>rmalSystems, Thesis, Cambridge, MassachusettsInstitute <strong>of</strong> Technology.Savage, D., Cave, M. R., Milodowski, A. E., andGeorge I., 1987, Hydro<strong>the</strong>rmal Alteration <strong>of</strong>Granite by Meteoric Fluid: An Example from <strong>the</strong>Carnmenellis Granite, United Kingdom:Contributions to Mineralogy and Petrology, V. 96,pp. 391-405.Savage, D., Bateman, K., and Richards, H. G.,1992, Granite-Water Interactions in a FlowthroughExperimental System with Applications to<strong>the</strong> Hot Dry Rock Geo<strong>the</strong>rmal System atRosemanowes, Cornwall, U.K.: AppliedGeochemistry, V. 7, pp. 223-241.Tarcan, G., 2005, Mineral Saturation and ScalingTendencies <strong>of</strong> Waters Discharged from Wells(>150 o C) in Geo<strong>the</strong>rmal Areas <strong>of</strong> Turkey: Journal<strong>of</strong> Volcanology and Geo<strong>the</strong>rmal Research, V.142, pp. 263-283Yangisawa, N. Matsunaga, I., Sugita H., Sato, M.,and Okabe T., 2005, Scale Precipitation duringCirculation at <strong>the</strong> Hijiori HDR Test Field,Yamagata, Japan: <strong>Proceedings</strong> WorldGeo<strong>the</strong>rmal Congress 2005, Antalya, Turkey, 24-29 April 2005.29


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Geo<strong>the</strong>rmal <strong>Energy</strong> in <strong>the</strong> Perth Basin, AustraliaComparisons with <strong>the</strong> Rhine GrabenAdrian Larking 1 , Gary Meyer 21 & 2 Green Rock <strong>Energy</strong> Limited, 6/38 Colin Street, West Perth, Western Australia 6005, AustraliaAbstractUnlike <strong>the</strong> Rhine Graben where commercial scalegeo<strong>the</strong>rmal power and direct heat projects have beenoperating for some time, geo<strong>the</strong>rmal developments in<strong>the</strong> Perth Basin are only at <strong>the</strong> gestation stage. Over<strong>the</strong> next two years Green Rock <strong>Energy</strong> Limited plansto carry out a commercial demonstration project inPerth which is likely to be <strong>the</strong> first commercial scaledirect heat project <strong>of</strong> its type in Australia. This has onlybecome possible since July 2009 when Green Rock<strong>Energy</strong> along with <strong>the</strong> University <strong>of</strong> Western Australiawas awarded <strong>the</strong> first rights to explore for and producegeo<strong>the</strong>rmal energy in <strong>the</strong> state <strong>of</strong> Western Australia.This followed <strong>the</strong> introduction <strong>of</strong> <strong>the</strong> State’s firstgeo<strong>the</strong>rmal legislation in 2008 when <strong>the</strong> Petroleum Actwas amended to include geo<strong>the</strong>rmal energy.This direct heat project is designed to prove <strong>the</strong>concept <strong>of</strong> recoveering geo<strong>the</strong>rmal energy from hotsedimenary aquifers in <strong>the</strong> central Perth Basin todirectly cool and heat buildings in <strong>the</strong> PerthMetropolitan area. To assist <strong>the</strong> Company to achievethis objective in December 2009 <strong>the</strong> <strong>Australian</strong>Government announced that it was <strong>of</strong>fering GreenRock <strong>Energy</strong> Limited a grant <strong>of</strong> $7 million from itsGeo<strong>the</strong>rmal Drilling Program to assist <strong>the</strong> funding <strong>of</strong><strong>the</strong> Company‘s project to air-conditon <strong>the</strong> maincampus at University <strong>of</strong> Western Australia in <strong>the</strong> PerthMetropolitan area. The funding agreement was signedin September <strong>2010</strong>. One week later <strong>the</strong> Western<strong>Australian</strong> State Government announced that GreenRock <strong>Energy</strong> was to be <strong>of</strong>fered a fur<strong>the</strong>r grant <strong>of</strong> $5.4million for <strong>the</strong> same project. Funds from bothGovernments will be provided in stages and eachGovernment requires <strong>the</strong> Company to provide <strong>the</strong>balance <strong>of</strong> required funds from o<strong>the</strong>r sources.Financing <strong>of</strong> geo<strong>the</strong>rmal exploration projects inAustralia may differ from typical funding <strong>of</strong> projects inGermany. Most funds in Australia are obtained fromshareholders in companies listed on <strong>the</strong> <strong>Australian</strong>Securities Exchange.Both <strong>the</strong> Rhine and <strong>the</strong> Perth basins are favourablylocated near infrastructure. The Rhine Graben is <strong>the</strong>locus <strong>of</strong> a substantial portion <strong>of</strong> Germany’s populationand industrial muscle and is a major transport hub.The Perth Basin straddles Australia‘s south westerncoast where most <strong>of</strong> <strong>the</strong> State <strong>of</strong> Western Australia’spopulation <strong>of</strong> 2.3 million and power infrastructure arelocated. This favourable location close to marketstoge<strong>the</strong>r with Perth Basin’s geo<strong>the</strong>rmal energyresource potential presents <strong>the</strong> opportunity to supplyenergy for electricity production and direct heat useincluding air-conditioning and desalination <strong>of</strong> water.Both basins share one key thing in common: <strong>the</strong>irgeo<strong>the</strong>rmal systems have little surface expression at<strong>the</strong> surface hence drilling is required to map <strong>the</strong> subsurfaceheat resources. Knowlege <strong>of</strong> <strong>the</strong> extent anddistribution <strong>of</strong> geo<strong>the</strong>rmal energy in <strong>the</strong> Perth Basinand its exploration and development is only at an earlystage and may be 20 years behind <strong>the</strong> Rhine Graben.In both grabens <strong>the</strong> existing knowledge was mainlyderived from <strong>the</strong> petroleum industry where <strong>the</strong>re is ahistory <strong>of</strong> petroleum production. Petroleum explorationand production started much earlier in <strong>the</strong> Rhine, with<strong>the</strong> Forst-Weiher Field discovered between 1934 and1936. Production ceased <strong>the</strong>re by <strong>the</strong> 1960’s butcontinues at present in <strong>the</strong> Perth Basin. Petroleumdrilling commenced in <strong>the</strong> Perth Basin in <strong>the</strong> 1950sand resulted in <strong>the</strong> discovery <strong>of</strong> more than 13 oil andgas fields. Data derived from petroleum wells arera<strong>the</strong>r sparsely distributed and focused in limited areaswhere petroleum fields have been discovered, mainlyin <strong>the</strong> nor<strong>the</strong>rn Perth Basin. Only 250 petroleum wellshave been drilled and 23,985 km <strong>of</strong> 2D seismic and2,838 km 2 <strong>of</strong> 3D seismic acquired in <strong>the</strong> Perth Basin.In contrast, over 5,000 wells have been drilled in <strong>the</strong>Rhine but around 90% <strong>of</strong> <strong>the</strong>m were less than 600metres depth.Upper Rhine GrabenPerth BasinBoth <strong>the</strong> Rhine Graben and Perth Basins are N-Strending sediment filled extensional rifts. The Perthrifting is over 200Ma older and has a much thickersediment fill. The Perth Basin is a 1,000 km long rift orhalf graben containing a thick sequence <strong>of</strong> sedimentsin places up to 15 kilometres deep. This rifting30


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>produced <strong>the</strong> series <strong>of</strong> deep, north-south trendingbasins along <strong>the</strong> western margin <strong>of</strong> <strong>the</strong> Yilgarn Craton.Sediment deposition commenced with extensionduring <strong>the</strong> Permian (~290 Ma) and continued to <strong>the</strong>Early Cretaceous (~138 Ma). The Basin was upliftedduring <strong>the</strong> final separation <strong>of</strong> Western Australia andgreater India during <strong>the</strong> breakup <strong>of</strong> Gondwana.Rifting in <strong>the</strong> 300km long Rhine Graben commencedmuch later in <strong>the</strong> Middle Eocene. Graben sinking andshoulder lifting continues to this day with <strong>the</strong> maximumsediment fill being around 3.4km in <strong>the</strong> Upper RhineGraben.There are substantial geological differences between<strong>the</strong> Rhine Graben and Perth Basin, in particular <strong>the</strong>much younger age, shorter graben, thinnersedimentary pile thickness <strong>of</strong> <strong>the</strong> former and currenttensional and seismically active tectonic stress regime<strong>of</strong> <strong>the</strong> Rhine Graben compared to <strong>the</strong> compressionaland relatively seismically inactive regime <strong>of</strong> <strong>the</strong> PerthBasin. Even so <strong>the</strong>re are important similarities in <strong>the</strong>irstructural setting, extensional tectonic origins, thicksedimentary successions which overlie hot crystallinebasements, high heat flows and evidence <strong>of</strong> <strong>the</strong>existence <strong>of</strong> substantial geo<strong>the</strong>rmal energy resourcepotential.now overprinted by an essentially compressionalsetting as <strong>the</strong> <strong>Australian</strong> plate migrates NW with arotational component at <strong>the</strong> relatively fast geologicalrate <strong>of</strong> nearly 7 cm per year. The contemporary stressregime for <strong>the</strong> Perth Basin has been interpreted to bea transitional reverse to strike-slip faulting stressregime with an approximate east-west maximumhorizontal compression direction. Stress field data for<strong>the</strong> Perth Basin are derived mainly from petroleum wellborehole breakouts and drilling-induced tensilefractures from 34 measurements as shown in <strong>the</strong>World Stress Map. This is important for targetting wellsto tap critically stressed faults and fracture directions.Perth Basin Stratigraphy &Tectonic stagesFinal breakup <strong>of</strong> Gondwanaleading to dextral strike-slipdeformation (transfer zones)& basin inversionGeological MapsFrom Song & Cawood, 1999From Thomas & Brown 1983Both basins have vertical structural asymetry with <strong>the</strong>sedimentary fill being geater in <strong>the</strong> eastern flank than<strong>the</strong> western flank and higher graben shoulders on <strong>the</strong>east flank in <strong>the</strong> case <strong>of</strong> <strong>the</strong> Rhine. This is consideredto have important influences on regional ground waterflow in <strong>the</strong> Rhine. Similarly <strong>the</strong> hills marking <strong>the</strong> NStrending Darling Fault forms <strong>the</strong> eastern boundary fault<strong>of</strong> <strong>the</strong> Perth Basin and is also expected to have aninfluence on ground water flow.In <strong>the</strong> Rhine <strong>the</strong> current stress regime is strike slip with<strong>the</strong> maximum horizontal stress being orientedapproximately NW/SE. In contrast to <strong>the</strong> Rhine, <strong>the</strong>early extensional tectonic regime <strong>of</strong> <strong>the</strong> Perth Basin isGeo<strong>the</strong>rmal energy has been recovered to powerelectricity generation from both sediments and granitesin <strong>the</strong> Rhine Graben at Soultz sous Forêts andLandau. Heat flows <strong>of</strong> up to 150mW/m 2 have beenrecorded in both grabens. Thermal anomalies occuralong <strong>the</strong> western rim <strong>of</strong> <strong>the</strong> Rhine Graben. This is hasbeen attributed to enhancement <strong>of</strong> a conductive basalheat flow <strong>of</strong> 70-80mW/m 2 by convection. Some <strong>of</strong><strong>the</strong>se sites were mapped as early as 1929 where atemperature <strong>of</strong> 50ºC at depth <strong>of</strong> 400 metres wasknown at Soultz.At Landau convective hot spots have temperatures <strong>of</strong>55°C at a depth <strong>of</strong> 500m & 98°C at a depth <strong>of</strong>1,000m. There is considerable evidence for convectivewater flows in <strong>the</strong> Rhine Graben, particularly in <strong>the</strong>western flank where a pattern <strong>of</strong> adjacent hot and coldspots was found. This is generally considered to be <strong>the</strong>surface expression <strong>of</strong> deep convective geo<strong>the</strong>rmalsystems. At Soultz <strong>the</strong>re is a large reservoir with asimilar fluid chemistry. The same geo<strong>the</strong>rmal fluid isfound in different wells and in different lithologiesincluding sediments and granite basement.Geo<strong>the</strong>rmal water at Soultz has salinities <strong>of</strong> around100g/l and pH <strong>of</strong> 5.31


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>sequences in <strong>the</strong> Perth Basin. It is not known if thisreflects any deeper convection.In <strong>the</strong> Rhine Graben in recent years <strong>the</strong> emphasis hasshifted from targeting temperatures <strong>of</strong> around 200ºC atdepths <strong>of</strong> 5,000 metres where natural flow rates fromfracture permeability have proven to be inadequate totargetting shallower depths <strong>of</strong> 2,500m to 3,500 metreswhere tempertures <strong>of</strong> 150ºC to 160ºC and substantiallyhigher flow rates can be expected from natural faultsand fractures.With its thick sequences <strong>of</strong> sandstones, <strong>the</strong> presence<strong>of</strong> <strong>the</strong>rmal insulating shales and coals and high heatflows <strong>the</strong> Perth Basin has potential to housegeo<strong>the</strong>rmal energy resources in <strong>the</strong> form <strong>of</strong> hotsedimentary aquifers (HSA) and hot rocks. The source<strong>of</strong> <strong>the</strong> heat flows in <strong>the</strong> Perth Basin may be radioactivebasement rocks and radiogenic sedimentary horizons.The Perth Basin contains some <strong>of</strong> <strong>the</strong> worlds largestmineral sands deposits many <strong>of</strong> which are rich inradiogenic thorium minerals at shallow depths.Source: From Schwarz 2005 & Lichen 2005The highest known heat flows in <strong>the</strong> Perth Basin havebeen determined from petroleum wells in or nearproducing oil and gas fields in <strong>the</strong> nor<strong>the</strong>rn PerthBasin. Green Rock holds nine Geo<strong>the</strong>rmal ExplorationPermits in this region near high voltage power gridsconnected to Perth’s major power markets. Heat flowsexceed 100mW/m 2 within <strong>the</strong>se Permits.Temperatures <strong>of</strong> around 160°C are expected in hotsedimentary aquifers at depths less than 4,000mwhich is sufficient to generate electricity commerciallyat this location provided that sufficient geo<strong>the</strong>rmalwater flow rates can be achieved.Unlike Germany, electricity generated from geo<strong>the</strong>rmalenergy in Australia does not benefit from any feed intariff arragement and retail electricity prices in Australiaare substantially lower than Gemany‘s. In general thismeans that higher recovered temperatures or flowrates are required in Westen Australia to ensurecommercial viability. However generators <strong>of</strong> renewableenergy including geo<strong>the</strong>rmal energy are entitled underFederal legislation to sell Renewable <strong>Energy</strong>Certificates (REC’s) in addition to selling <strong>the</strong> electricity<strong>the</strong>y generate. In <strong>the</strong> absence <strong>of</strong> feed in tariffs inWestern Australia electricity is sold to utilities viapower purchase agreements.Landau: Temperatures at 1000m (°C)Grid in kms (Gauss-KrügerSource: Charissé 2007It is early days yet but evidence is emerging <strong>of</strong>convective flows in <strong>the</strong> shallow sedimentaryWithin Green Rock‘s permits in <strong>the</strong> North Perth Basinpetroleum wells have proven good primary waterpermeabilities in sandstone reservoirs down to depths<strong>of</strong> around 2,700 metres but <strong>the</strong>re is some limitedevidence <strong>of</strong> substantially lower permeabilities atgreater depths where temperatures above 150ºCwould be expected. Much less is known about <strong>the</strong>potential for good water flows from natural fault or32


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>fracture permeability as this has not been targetted by<strong>the</strong> petroleum industry <strong>the</strong>re.Drilling Water Well in Perth for Heating Aquatic CentresSource: Hot Dry Rocks Pty Ltd 2008In <strong>the</strong> central Perth Basin near <strong>the</strong> city <strong>of</strong> Perth heatflows are lower and temperatures expected at depthare likely to be insufficient for commercial generation<strong>of</strong> electricity but should be adequate for direct heatuses such as purification <strong>of</strong> water by distillation and forair-conditioning <strong>of</strong> buildings. Viability depends onattaining sufficient permeabilities from <strong>the</strong> aquifers.Within <strong>the</strong> Perth city area, where petroleum wells anddeep seismic data are lacking, most <strong>of</strong> <strong>the</strong> usefultemperature and permeability data have come fromdeep water bores, <strong>the</strong> deepest <strong>of</strong> which extend to onlyabout 1000 metres but have sufficiently high water flowrates from natural matrix or granular permeability. On<strong>the</strong> basis <strong>of</strong> petroleum wells outside <strong>the</strong> Perth Permitareas good permeabilities are expected in Perth atleast down to depths <strong>of</strong> 2,500 metres.Geo<strong>the</strong>rmal energy has been recovered from aquifersbeween 750 and 1,000 metres deep in Green Rock’sPermit GEP1 in metropolitan Perth. This geo<strong>the</strong>rmalwater is used to heat a number <strong>of</strong> major swimmingcentres including <strong>the</strong> Challenge Stadium AquaticCentre where <strong>the</strong> World Swimming Championshipshave been held twice in <strong>the</strong> past decade.To develop opportunities in GEP1, Green Rock<strong>Energy</strong>, plans to carry out a commercial demonstrationproject to recover geo<strong>the</strong>rmal energy from hotsedimentary aquifers beneath <strong>the</strong> main Perth campusat <strong>the</strong> University <strong>of</strong> Western Australia (UWA). Thisproject will be <strong>the</strong> first stepping stone to largercommercial developments in Perth.The demonstration project is designed to replace asignificant portion <strong>of</strong> <strong>the</strong> UWA’s electrical powered airconditioningwith geo<strong>the</strong>rmal powered absorptionchillers for its air-conditioning and heating needs.Absorption chillers, like <strong>the</strong> one shown below, arecommercially available in Australia.Commercial viability <strong>of</strong> this project at <strong>the</strong> UWA campuswill depend on obtaining adequate geo<strong>the</strong>rmaltemperatures and water flow rates from <strong>the</strong> sandstoneaquifers at depth. Geo<strong>the</strong>rmal water temperatures <strong>of</strong>between 80⁰C and 100⁰C are required for commercialoperation <strong>of</strong> <strong>the</strong> absorption chillers which will providechilled water for <strong>the</strong> campus. Expected temperaturesat <strong>the</strong> target depths <strong>of</strong> 2.5km to 3km in Perth should beadequate as indicated by estimated heat flowsdetermined from temperature pr<strong>of</strong>iles measured indeep water bores and petroleum wells.33


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>ReferencesAbsorption ChillerFor this first project at <strong>the</strong> UWA campus, oneproduction and one injection well will be drilled toaround 2.5 to 3 kilometres deep to recover geo<strong>the</strong>rmalenergy from sandstone aquifers in <strong>the</strong> fluvialYarragadee Formation and Cattamarra CoalMeasures. Drilling wells to <strong>the</strong>se depths should notpresent any particular difficulty as <strong>the</strong>re is abundanthistory <strong>of</strong> petroleum wells drilled without significantproblems in <strong>the</strong> Perth Basin. Preparatory site work andwell design is underway to enable this drilling to becarried out in 2011. Seismic acquisition will becompleted to optimise well design and orientation priorto drilling.Chopra P.N. and Holgate, F. (Earthinsite Pty Ltd):Geo<strong>the</strong>rmal <strong>Energy</strong> Potential in Selected areas <strong>of</strong>Western Australia, a Report commissioned by Western<strong>Australian</strong> Department <strong>of</strong> Industry and Resources2007; and also – A GIS Analysis <strong>of</strong> Temperature in <strong>the</strong><strong>Australian</strong> Crust; <strong>Proceedings</strong> <strong>of</strong> World Geo<strong>the</strong>rmalCongress, Antalya, Turkey 2005, pp 7.Clauser, C and Villinger, H, Analysis <strong>of</strong> conductive andconvective heat transfer in a sedimentary basindemonstrated for <strong>the</strong> Rheingraben, Geophys. J 100,393-414, 1990Davidson, W.A... Hydrogeology and groundwaterresources <strong>of</strong> <strong>the</strong> Perth Region, Western Australia:Western Australia Geological Survey, Bulletin 142, 257pp, 1995Freeman, M.J., and Donaldson, M.J.: Geology <strong>of</strong> <strong>the</strong>sou<strong>the</strong>rn Perth Basin and Margaret River wine district,southwestern Western Australia – a field guide:Western Australia Geological Survey, Record 2006/20,2006Genter, A., Baumgärtner, J., Cuenot, N., Graff, J J.,Kolbel, T., Sanjuan, B. The EGS Soultz Case Study:Lessons Learnt After Two Decades <strong>of</strong> Geo<strong>the</strong>rmalResearches. Second European Geo<strong>the</strong>rmal Review,<strong>Proceedings</strong>, Mainz June 21-23, <strong>2010</strong>Gori, K.A.R.: Perth Basin’s Geo<strong>the</strong>rmal Resources,<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong> <strong>Conference</strong> 2008,Extended Abstract. Geological Survey, Department <strong>of</strong>Industry and Resources, 2008Hot Dry Rocks Pty Ltd: Geo<strong>the</strong>rmal <strong>Energy</strong> Potential inSelected Areas <strong>of</strong> Western Australia, Perth Basin, pp270, 2008Hot Dry Rocks Pty Ltd: Western Perth Geo<strong>the</strong>rmalproject, Geo<strong>the</strong>rmal Exploration Stage 2, unpublishedreport for Green Rock <strong>Energy</strong> Limited, pp28, 2009,Mory, A.J., Haig, D.W., Mcloughlin, S., and Hocking,R.M.: Geology <strong>of</strong> <strong>the</strong> nor<strong>the</strong>rn Perth Basin, WesternAustralia – a field guide: Western Australia GeologicalSurvey, Record 2005/9, 2005Mory, R.J, and Lasky, R.P.: Stratigraphy and Structure<strong>of</strong> <strong>the</strong> Onshore Nor<strong>the</strong>rn Perth Basin, Report 46,Geological Survey <strong>of</strong> Western Australia pp 126, 1996Regenauer-Lieb, Pr<strong>of</strong>. K, Horowitz Dr F, The PerthBasin Geo<strong>the</strong>rmal Opportunity, The University <strong>of</strong>Western Australia & CSIRO, p42-44, April 2007Schwarz M, Henk, A, Evolution and structure <strong>of</strong> <strong>the</strong>Upper Rhine Graben: insights from three-dimensional<strong>the</strong>rmomechanical modeling, Int J Earth Sci (GeolRundsch), 94: 732-750, 2005.34


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Australia’s Geo<strong>the</strong>rmal Research ActivitiesA.D. Long 1* , A.R. Budd 2 , H. Gurgenci 3 , M. Hand 4 , C. Huddlestone-Holmes 5 , B. Moghtaderi 6 andRegenauer-Lieb, K. 71 Primary Industries & Resources SA, GPO Box 1671, Adelaide, South Australia, 5001.2 Geoscience Australia, GPO Box 378, Canberra, <strong>Australian</strong> Capital Territory, 2601.3 QGECE, The University <strong>of</strong> Queensland, Brisbane, Queensland, 4072.4 SACGER, IMER, The University <strong>of</strong> Adelaide, South Australia, 5005.5 CSIRO, PO Box 883, Kenmore, Queensland, 4069.6 ATC, The University <strong>of</strong> Newcastle, Callaghan, NSW, 2308.7 WAGCOE, ARRC, 26 Dick Perry Avenue, Kensington, 6151.*Corresponding author: alexandra.long@sa.gov.auThe challenges and technology needs <strong>of</strong>Australia’s geo<strong>the</strong>rmal energy industry aresignificant yet achievable. The sector is organisedand has a clear pathway through <strong>the</strong> stages <strong>of</strong>project development defined in <strong>the</strong> DevelopmentFramework and Technology Roadmap (DRET,2008). Collaboration is facilitated by <strong>the</strong> <strong>Australian</strong>Geo<strong>the</strong>rmal <strong>Energy</strong> Group and its TechnicalInterest Groups, where research needs areprioritised by <strong>the</strong> industry and researchers. Thecapacity and capability to undertake <strong>the</strong> muchneeded research work will be met by geo<strong>the</strong>rmalresearch centres which work competitively yetcollaboratively, with complementary programs, toachieve research outcomes most efficiently. Thispaper will provide a guide to <strong>the</strong> researchactivities in Australia, outlining <strong>the</strong> programs andareas <strong>of</strong> expertise <strong>of</strong> <strong>the</strong> key research groupsworking in <strong>the</strong> geo<strong>the</strong>rmal arena; a summary <strong>of</strong>current projects; and how to find out moreinformation.Keywords: Geo<strong>the</strong>rmal, research, technologydevelopment.Centres <strong>of</strong> expertiseThe desire to develop Australia’s geo<strong>the</strong>rmalenergy resources to supply secure andenvironmentally sustainable energy has led to <strong>the</strong>impressive growth <strong>of</strong> <strong>the</strong> <strong>Australian</strong> geo<strong>the</strong>rmalsector. The challenges facing <strong>the</strong> sector areknown, and <strong>the</strong> research and development needs<strong>of</strong> <strong>the</strong> industry as <strong>the</strong>y strive to commercialise <strong>the</strong>resources are being met by a growing capacity atdedicated research centres, universities andresearch groups.Centres for geo<strong>the</strong>rmal energy research haveformed: at <strong>the</strong> University <strong>of</strong> Queensland, with <strong>the</strong>Queensland Geo<strong>the</strong>rmal <strong>Energy</strong> Centre <strong>of</strong>Excellence (QGECE); in a joint venture <strong>of</strong> <strong>the</strong>University <strong>of</strong> Western Australia, Curtin Universityand <strong>the</strong> CSIRO, <strong>the</strong> Western <strong>Australian</strong>Geo<strong>the</strong>rmal Centre <strong>of</strong> Excellence (WAGCOE);and at <strong>the</strong> University <strong>of</strong> Adelaide, <strong>the</strong> South<strong>Australian</strong> Centre for Geo<strong>the</strong>rmal <strong>Energy</strong>Research (SACGER). Geo<strong>the</strong>rmal energyresearch is also being supported at manyuniversities around Australia, GeoscienceAustralia and at <strong>the</strong> CSIRO. The followingsections will describe each <strong>of</strong> <strong>the</strong>se centres andresearch groups and <strong>the</strong>ir capability.Geoscience AustraliaThe <strong>Australian</strong> Government announced <strong>the</strong>AU$58.9M Onshore <strong>Energy</strong> Security Initiative inAugust 2006, and as part <strong>of</strong> this, GeoscienceAustralia established a geo<strong>the</strong>rmal energy project.The project aims to improve <strong>the</strong> existingknowledge about <strong>the</strong> type and location <strong>of</strong>geo<strong>the</strong>rmal resources in Australia on a nationalscale. It also aims to encourage investment,exploration and exploitation <strong>of</strong> this energy sourcethrough provision <strong>of</strong> pre-competitive geosciencedatasets relevant to geo<strong>the</strong>rmal energy.To achieve <strong>the</strong>se objectives, <strong>the</strong> geo<strong>the</strong>rmalproject:collects new heat flow data across Australiato better define and locate geo<strong>the</strong>rmalresources; uses (heat) source and (<strong>the</strong>rmal) trapmodelling to identify potential Hot Rock andHot Sedimentary Aquifer systems;works to compile national datasets which maybe useful to <strong>the</strong> geo<strong>the</strong>rmal industry includinggroundwater temperatures, boreholetemperatures, rock <strong>the</strong>rmal conductivities andgranite and sediment chemistry;uses <strong>the</strong>se new datasets to produce a revisedestimate <strong>of</strong> Australia's total containedgeo<strong>the</strong>rmal resource; andprovides advice to government on geo<strong>the</strong>rmalresource issues, including <strong>the</strong> AU$50MGeo<strong>the</strong>rmal Drilling Program.For more information see www.ga.gov.auor contact <strong>the</strong> geo<strong>the</strong>rmal energy team:geo<strong>the</strong>rmal@ga.gov.au.Queensland Geo<strong>the</strong>rmal <strong>Energy</strong> Centre <strong>of</strong>Excellence - QGECEThe Queensland Geo<strong>the</strong>rmal <strong>Energy</strong> Centre <strong>of</strong>Excellence is based at <strong>the</strong> University <strong>of</strong>Queensland and was established with anAU$15M grant from <strong>the</strong> Queensland Governmentand AU$3.3M <strong>of</strong> in-kind support from <strong>the</strong>university. The centre commenced operations in35


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>January 2009 with a 5 year program. The centre’sresearch programs were developed to fill gaps in<strong>the</strong> national and international geo<strong>the</strong>rmalresearch effort and have a focus on above groundtechnologies with <strong>the</strong> aim <strong>of</strong> quickening <strong>the</strong> pace<strong>of</strong> large-scale utilisation <strong>of</strong> hot rocks geo<strong>the</strong>rmalenergy in Australia. QGECE has four researchprograms: Power Conversion: developing technologiesto enable production <strong>of</strong> 50% more electricityfrom binary plants using <strong>the</strong> same subsurfaceinvestment;Heat Exchangers: development <strong>of</strong> naturaldraft dry cooling towers and o<strong>the</strong>r coolingsolutions to increase by up to 15% <strong>the</strong> netoutput <strong>of</strong> geo<strong>the</strong>rmal plants that use aircooledcondensers; Reservoir Geology: establish ageochemical/isotopic and geochronologicaldatabase and improve understanding <strong>of</strong>geo<strong>the</strong>rmal resources in Queensland anddevelop routine exploration tools for hot rockgeo<strong>the</strong>rmal systems; and,Transmission: research in to electricity gridinteraction with an emphasis on remotegeneration infrastructure.The current major projects include: Design and development <strong>of</strong> small (5-kWe)supercritical turbines for testing in <strong>the</strong>QGECE laboratory.Construction <strong>of</strong> a 100-kWe mobile geo<strong>the</strong>rmaltest plant with high-pressure capability to trysupercritical turbines. Characterisation <strong>of</strong> <strong>the</strong> heat-producinggranites in Queensland. The effect <strong>of</strong> ambient dust on air-cooledcondenser performance and design againstdust.Investigation <strong>of</strong> options for connecting remotegeo<strong>the</strong>rmal power generation to <strong>the</strong>Queensland grid.See also www.uq.edu.au/geo<strong>the</strong>rmalor contact <strong>the</strong> centre Director, Pr<strong>of</strong>essor HalGurgenci: h.gurgenci@uq.edu.au.Western <strong>Australian</strong> Geo<strong>the</strong>rmal Centre <strong>of</strong>Excellence - WAGCOEThe Western <strong>Australian</strong> Geo<strong>the</strong>rmal Centre <strong>of</strong>Excellence is an unincorporated joint venturebetween <strong>the</strong> Commonwealth Science andIndustry Research Organisation (CSIRO), <strong>the</strong>University <strong>of</strong> Western Australia, and CurtinUniversity. The centre was established inFebruary 2009 with an AU$2.3M grant over threeyears from <strong>the</strong> Western <strong>Australian</strong> governmentand substantial in-kind and cash contributionsfrom <strong>the</strong> centres’ members. The centre isproviding a scientific focus to <strong>the</strong> development <strong>of</strong><strong>the</strong> geo<strong>the</strong>rmal industry in Western Australia,concentrating on <strong>the</strong> Perth basin, and buildingeducational programs around geo<strong>the</strong>rmal energy.The centre’s research focus is on HotSedimentary Aquifers and direct use <strong>of</strong> <strong>the</strong> heatproduced from <strong>the</strong>se resources, as summarised in<strong>the</strong> centre’s vision statement “To providegeo<strong>the</strong>rmal zero-emission desalinated water, airconditioningand power to our cities”.WAGCOE has three research programs: Perth Basin Assessment: Develop a rigorousscientific understanding <strong>of</strong> <strong>the</strong> geo<strong>the</strong>rmalresource in <strong>the</strong> Perth Basin;Above Ground Technologies: Identify anddemonstrate innovative applications <strong>of</strong> HSAgeo<strong>the</strong>rmal energy; and, Deep Resources: Provide a scientificframework for <strong>the</strong> potential exploitation <strong>of</strong>deep geo<strong>the</strong>rmal resources.Current major projects include: Research and development activitiesassociated with <strong>the</strong> direct use geo<strong>the</strong>rmalpowered supercomputer cooling system thatis part <strong>of</strong> CSIRO’s Sustainable <strong>Energy</strong> forSKA project (see below). This system targetshot sedimentary aquifers <strong>of</strong> <strong>the</strong> Perth Basin.Design <strong>of</strong> an additional sensor equipped deepresearch and monitoring well at <strong>the</strong> same sitefor research, education, training and longterm monitoring. Research and development activitiesassociated with <strong>the</strong> direct geo<strong>the</strong>rmally drivenMW th scale campus cooling project at UWArun by <strong>the</strong> leaseholders Green Rock <strong>Energy</strong>and UWA. Development <strong>of</strong> a novel desalinationtechnology with 30% yield boost from lowgrade geo<strong>the</strong>rmal waters <strong>of</strong> 65C and less. Acontainerised m 3 /day first generationprototype is sponsored by <strong>the</strong> <strong>Australian</strong>Government National Centre <strong>of</strong> Excellence inDesalination located at Murdoch University.For more information see www.geo<strong>the</strong>rmal.orgor contact <strong>the</strong> centre business manager, SeanWebb: sean.webb@geo<strong>the</strong>rmal.org.au.South <strong>Australian</strong> Centre for Geo<strong>the</strong>rmal<strong>Energy</strong> Research - SACGERThe South <strong>Australian</strong> Centre for Geo<strong>the</strong>rmal<strong>Energy</strong> Research is based at <strong>the</strong> University <strong>of</strong>Adelaide within <strong>the</strong> Institute for Minerals and<strong>Energy</strong> Resources, www.adelaide.edu.au/imer.The centre was announced by <strong>the</strong> South<strong>Australian</strong> Government as <strong>the</strong> first project to befunded from <strong>the</strong> South <strong>Australian</strong> Renewable<strong>Energy</strong> Fund, established with a grant <strong>of</strong>36


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>AU$1.6M over two years from 1 July 2009. TheUniversity <strong>of</strong> Adelaide is providing AU$400,000over <strong>the</strong> same period.The SACGER research program will focus onsubsurface factors in Hot Rock and EGSresources such as reservoir characterisation andmodelling. This is complementary to <strong>the</strong> researchprograms <strong>of</strong> o<strong>the</strong>r centres. The research programis under development and will be designed inconsultation with <strong>the</strong> sector.Current projects at <strong>the</strong> centre include those whichwere funded by tied grants from PIRSA:Geophysical mapping and monitoring <strong>of</strong> anenhanced geo<strong>the</strong>rmal system usingmagnetotellurics.Rock fracture characterisation for hot dry rockenhanced geo<strong>the</strong>rmal systems. Building a regional <strong>the</strong>rmal model for <strong>the</strong>Adelaide rift complex. Experimental verification <strong>of</strong> undergroundcooling for efficient <strong>the</strong>rmal cycles. Optimisation <strong>of</strong> geo<strong>the</strong>rmal energyinvestments. Investigate low temperature <strong>the</strong>rmalprocessing using geo<strong>the</strong>rmal energy. Reconnaissance <strong>the</strong>rmal mapping foruranium and geo<strong>the</strong>rmal exploration.For more information seewww.adelaide.edu.au/geo<strong>the</strong>rmal/or contact <strong>the</strong> centre: imer@adelaide.edu.au.CSIROCSIRO’s research capabilities in <strong>the</strong> geo<strong>the</strong>rmalarena are broad, due to <strong>the</strong> organisation’sresearch diversity and ability to integratemultidisciplinary skills. The primary focus <strong>of</strong>CSIRO’s activities in geo<strong>the</strong>rmal has beenthrough its contribution to WAGCOE. CSIRO’scontributions to <strong>the</strong> centre are mainly in <strong>the</strong>geological, geophysical, ground water, andreservoir engineering aspects <strong>of</strong> <strong>the</strong> Perth BasinAssessment research program. CSIRO is alsodeploying its research expertise in hydraulicfracturing, reservoir engineering, well borestability, rock petrophysics and microseismicmonitoring to geo<strong>the</strong>rmal projectsFunding from <strong>the</strong> Education Investment Fund forCSIRO’s Sustainable <strong>Energy</strong> for SKA project wasrecently announced. A significant component <strong>of</strong>this project is a 10 MW th direct use geo<strong>the</strong>rmalcooling system for <strong>the</strong> Pawsey High PerformanceComputing Centre in Perth. The construction <strong>of</strong>this system will start with <strong>the</strong> drilling <strong>of</strong> aresearch/monitoring well, followed by a productionand injection doublet. The heat produced will beused in an adsorption chiller to provide cooling for<strong>the</strong> supercomputer. CSIRO will work closely withWAGCOE during <strong>the</strong> development <strong>of</strong> this project.The geo<strong>the</strong>rmal component <strong>of</strong> <strong>the</strong> project is led byCSIRO Earth Science and Resource Engineeringin collaboration with <strong>the</strong> leaseholder, Geo<strong>the</strong>rmalPower Pty Ltd.O<strong>the</strong>r projects include: Development <strong>of</strong> numerical modelling toolsthat couple <strong>the</strong>rmal and poro-elasticprocesses for <strong>the</strong> assessment <strong>of</strong> well stability. Development <strong>of</strong> numerical modelling toolsand procedures for hydraulic stimulation athigh pressures and temperatures.Development <strong>of</strong> numerical modelling tools forfluid flow in fractures. Evaluating <strong>the</strong> application <strong>of</strong> petrophysicallogging techniques to <strong>the</strong> assessment <strong>of</strong><strong>the</strong>rmal conductivity;Assessment <strong>of</strong> waveform characterisationtechniques for <strong>the</strong> interpretation <strong>of</strong>microseismic monitoring data throughlaboratory based studies (high pressure hightemperature triaxial cell with acousticemissions monitoring) and <strong>the</strong> analysis <strong>of</strong>field data.For more information seewww.csiro.au/org/geo<strong>the</strong>rmalor contact <strong>the</strong> CSIRO: geo<strong>the</strong>rmal@csiro.au.University <strong>of</strong> Newcastle (Priority ResearchCentre for <strong>Energy</strong> – PRCfE)Located at <strong>the</strong> University <strong>of</strong> Newcastle, <strong>the</strong>Priority Research Centre for <strong>Energy</strong> has beenworking on geo<strong>the</strong>rmal energy research projectsfor a number <strong>of</strong> years through <strong>the</strong> researchprogram on Renewable <strong>Energy</strong> Systems. TheUniversity <strong>of</strong> Newcastle has received AU$30Mfrom <strong>the</strong> Federal Government through <strong>the</strong>Education Investment Fund and AU$30Mmatching funding from o<strong>the</strong>r sources to establish<strong>the</strong> Newcastle Institute for <strong>Energy</strong> & Resources(NIER). As part <strong>of</strong> this initiative, significant fundinghas been allocated for geo<strong>the</strong>rmal research, inparticular for <strong>the</strong> establishment <strong>of</strong> a state <strong>of</strong> <strong>the</strong>art facility for pilot-scale experimental research.The focus <strong>of</strong> geo<strong>the</strong>rmal research at <strong>the</strong>University <strong>of</strong> Newcastle is on novel powergeneration cycles and <strong>the</strong> concept <strong>of</strong> a CO 2<strong>the</strong>rmo siphon for EGS. The study <strong>of</strong> powercycles is regarded as one <strong>of</strong> <strong>the</strong> key areas formajor technological improvements since many <strong>of</strong><strong>the</strong> problems associated with power generationfrom geo<strong>the</strong>rmal sources are underpinned byinefficient and <strong>of</strong>ten unsuitable heat exchangeprocesses within power cycles. In recognition <strong>of</strong><strong>the</strong>se shortcomings, <strong>the</strong> University <strong>of</strong> Newcastleinitiated a joint R&D program with Granite PowerLtd in 2006 with <strong>the</strong> goal <strong>of</strong> establishingalternative and potentially more efficient ways <strong>of</strong>generating power from geo<strong>the</strong>rmal and o<strong>the</strong>r low-37


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>grade heat sources, such as industrial waste heat.The result was <strong>the</strong> creation <strong>of</strong> <strong>the</strong> GRANEXRegenerative Supercritical Power Cycle which isnow being commercialised.For more information seewww.newcastle.edu.au/research-centre/energyor contact <strong>the</strong> Renewable <strong>Energy</strong> SystemsProgram leader, Pr<strong>of</strong>essor Behdad Moghtaderi:Behdad.Moghtaderi@newcastle.edu.au.Melbourne <strong>Energy</strong> InstituteThe Melbourne <strong>Energy</strong> Institute is located at <strong>the</strong>University <strong>of</strong> Melbourne and has a number <strong>of</strong>geo<strong>the</strong>rmal projects including <strong>the</strong> VictorianGeo<strong>the</strong>rmal Assessment Report, which intends toaddress critical issues for <strong>the</strong> successfuldevelopment <strong>of</strong> geo<strong>the</strong>rmal power capability inVictoria.For more information see energy.unimelb.edu.auor contact <strong>the</strong> institute: mei-info@unimelb.edu.auRMITA significant project linking geo<strong>the</strong>rmal energyand desalination is underway at RMIT inpartnership with Greenearth <strong>Energy</strong>.The project involves <strong>the</strong> development <strong>of</strong> aprototype system that combines fresh waterproduction with electricity generation usingentirely renewable sources. The project issupported by an <strong>Australian</strong> Research CouncilLinkage grant and Greenearth <strong>Energy</strong>.For more information on this project contact MarkMiller, Managing Director <strong>of</strong> Greenearth <strong>Energy</strong>,via email markm@greenear<strong>the</strong>nergy.com.au ortelephone 03 9620 1566.For <strong>the</strong> RMIT website see www.rmit.edu.auAGEG Technical Interest GroupsCollaboration amongst all participants in <strong>the</strong>sector is enabled through <strong>the</strong> <strong>Australian</strong>Geo<strong>the</strong>rmal <strong>Energy</strong> Group (AGEG) and <strong>the</strong>AGEG Technical Interest Groups (TIGs).Through linkages to <strong>the</strong> AGEG and its TIGs,Australia is a member <strong>of</strong> and contributes to <strong>the</strong>work <strong>of</strong> both <strong>the</strong> International <strong>Energy</strong> AgencyGeo<strong>the</strong>rmal Implementing Agreement (IEA-GIA)and <strong>the</strong> International Partnership for Geo<strong>the</strong>rmalTechnologies (IPGT). The 105 organisations thatare members <strong>of</strong> <strong>the</strong> AGEG have nominatedresearch topics <strong>of</strong> <strong>the</strong> highest priority to <strong>the</strong>industry, which are closely aligned with <strong>the</strong>priorities <strong>of</strong> both <strong>the</strong> GIA and <strong>the</strong> IPGT.The 12 TIGs are named in Table 1, and describedin more detail in <strong>the</strong> following section. For moreinformation or to join any <strong>of</strong> <strong>the</strong> TIGs: see <strong>the</strong>AGEG website, ,go to AGEG, Technical Interest Groups; orcontact <strong>the</strong> TIG leader. Contact details for all TIGleaders are also provided on <strong>the</strong> website.Table 1. AGEG Technical Interest GroupsTIGTopic1 Water management & environmental sustainability2 Reserves and resources3 Induced seismicity4 Outreach5 Economic modelling and novel use6 Power plants7 Direct use8 Information and data9 Reservoir development and engineering10 Exploration and well log technologies11 Drilling and well construction12 EducationTIG 1 water management and environmentalsustainabilityFollowing discussions and a decision made at <strong>the</strong>AGEG AGM in February, <strong>the</strong> name and focus <strong>of</strong>TIG 1 has been redefined as water managementand environmental sustainability. The scope <strong>of</strong> <strong>the</strong>TIG and definition <strong>of</strong> outputs from <strong>the</strong> TIG will bedeveloped by <strong>the</strong> members and will be availableon <strong>the</strong> TIG webpage. The TIG leader is StevenKennedy from <strong>the</strong> Victorian Department <strong>of</strong>Primary Industries.TIG 2 reserves and resourcesThe reserves and resources technical interestgroup is predominantly to provide a forum forAGEG members to contribute to discussion on <strong>the</strong><strong>Australian</strong> Geo<strong>the</strong>rmal Reporting Code. The codeis developed and reviewed by <strong>the</strong> joint AGEG andAGEA <strong>Australian</strong> Geo<strong>the</strong>rmal Reporting CodeCommittee, chaired by Peter Reid fromPetra<strong>the</strong>rm. Peter is also <strong>the</strong> TIG 2 leader,allowing feedback to <strong>the</strong> committee. The<strong>Australian</strong> Code for Reporting <strong>of</strong> ExplorationResults, Geo<strong>the</strong>rmal Resources and Geo<strong>the</strong>rmalReserves, The Geo<strong>the</strong>rmal Reporting Code(AGRCC, 2008), was launched in August 2008 at<strong>the</strong> AGEG and AGEA <strong>Australian</strong> Geo<strong>the</strong>rmal<strong>Energy</strong> <strong>Conference</strong>.TIG 3 induced seismicityHighlighting <strong>the</strong> importance <strong>of</strong> this topic and <strong>the</strong>need for research in this area, a new technicalinterest group has been created to focus oninduced seismicity. Led by Michael Malavazosand Barry Goldstein from PIRSA, this TIG willbuild on <strong>the</strong> work done under <strong>the</strong> previous TIG 1,which included <strong>the</strong> release <strong>of</strong> two reports, CooperBasin HDR hazard evaluation: predictivemodelling <strong>of</strong> local stress changes due to HFRgeo<strong>the</strong>rmal energy operations in South Australia(Hunt and Morelli, 2006) and Analysis andmanagement <strong>of</strong> seismic risks associated wi<strong>the</strong>ngineered geo<strong>the</strong>rmal system operations inSouth Australia (Morelli, 2009).38


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>TIG 4 outreachThe scope <strong>of</strong> TIG 4 is to assist <strong>the</strong> development<strong>of</strong> <strong>the</strong> <strong>Australian</strong> geo<strong>the</strong>rmal industry throughcoordinated geo<strong>the</strong>rmal training courses (inconjunction with IGA) an annual conference (inconjunction with AGEA), improvingcommunications through provision <strong>of</strong> a dedicatedwebsite that provides linkages to geo<strong>the</strong>rmalresource material and informing <strong>the</strong> publicthrough <strong>the</strong> provision <strong>of</strong> accessible information.TIG 4 is led by Betina Bendall from PIRSA.TIG 5 economic modelling and novel useTIG 5 has been modified to now cover economicmodelling as well as novel use applications forgeo<strong>the</strong>rmal energy including hybrid systems.Stephen Hinchliffe from SKM is <strong>the</strong> TIG leader.TIG 6 power plantsThe aim <strong>of</strong> TIG 6 is to achieve substantialimprovements in geo<strong>the</strong>rmal power plantefficiency through improvements in, for example,<strong>the</strong> cycle type, cycle fluids, heat exchangerefficiencies and more efficient cooling processes.Currently <strong>the</strong> focus is on <strong>the</strong> following areas:New cycles and cycle fluidsDry cooling Supercritical CO 2 geo<strong>the</strong>rmal siphonThe work <strong>of</strong> this TIG mirrors <strong>the</strong> IEA Geo<strong>the</strong>rmalResearch Annex VI. Hal Gurgenci from <strong>the</strong>QGECE and Behdad Moghtaderi from <strong>the</strong>University <strong>of</strong> Newcastle are co-leaders <strong>of</strong> TIG 6.TIG 7 direct useDirect use geo<strong>the</strong>rmal applications include bothcirculating hot water & geo<strong>the</strong>rmal heat pumps.Direct use geo<strong>the</strong>rmal is being pursued throughwork in this TIG as a highly desirable substitutefor electricity use due to:Widespread occurrenceShallow depths (i.e. lower cost)High efficiency (no energy conversion) Utilisation <strong>of</strong> conventional plant andequipment Relatively easy set up Can be small to industrial scaleThe TIG for direct use is led by Klaus Regenauer-Lieb from <strong>the</strong> WAGCOE and Donald Payne from<strong>the</strong> University <strong>of</strong> Melbourne.TIG 8 data managementTIG 8, led by Anthony Budd from GeoscienceAustralia, aims to assist <strong>the</strong> development <strong>of</strong> <strong>the</strong><strong>Australian</strong> geo<strong>the</strong>rmal industry by simplifying dataavailability, usefulness and exchange throughstandards, database design, content, ongoingenhancements and development <strong>of</strong> manipulationand interpretive tools. Some initiatives alreadycompleted through <strong>the</strong> TIG include <strong>the</strong>development <strong>of</strong> an extension to 3D GeoModellerto enable prediction <strong>of</strong> 3D temperature and heatflow from inputs <strong>of</strong> heat production and <strong>the</strong>rmalconductivity. Future projects planned are topopulate a heat flow database with new data,liaise with international parties working ongeo<strong>the</strong>rmal data management for webinteroperability standards and to build a datasystem within <strong>the</strong> Onshore <strong>Energy</strong> and MineralsDivision <strong>of</strong> Geoscience Australia.TIG 9 geo<strong>the</strong>rmal reservoir characterisation andengineeringAgreed terms <strong>of</strong> reference for this TIG are t<strong>of</strong>acilitate collaboration and information exchangeon topics including, but not limited to, Reservoir characterisation and modellingincluding 3D stochastic modelling and <strong>the</strong>simulation <strong>of</strong> fracture networksFracture stimulation with emphasis on designand modellingGeochemistry, corrosion and scaling coveringboth <strong>the</strong> geo<strong>the</strong>rmal plant and equipment and<strong>the</strong> rock-fluid interaction in <strong>the</strong> reservoir.Some projects planned by <strong>the</strong> TIG include tocompile and evaluate a list <strong>of</strong> available numericalmodels (algorithms) for fracture characterisation,scan for pre-existing geo<strong>the</strong>rmal data handbooksand build up to include information learnt fromoverseas projects and to date from <strong>Australian</strong>projects, promote international collaborationthrough exchanges and develop 3D stochasticmodelling and simulation <strong>of</strong> fracture networks andfracture propagation in crystalline rocks. PeterDowd from <strong>the</strong> University <strong>of</strong> Adelaide is <strong>the</strong> leader<strong>of</strong> this TIG.TIG 10 exploration technologiesTIG 10 aims to cooperate in studies to advancegeo<strong>the</strong>rmal methods and technologies: including<strong>the</strong> indirect detection <strong>of</strong> subsurface properties todelineate prospective trends; to develop, collect,improve and disseminate geo<strong>the</strong>rmal-relatedinformation; to identify opportunities to facilitate<strong>the</strong> efficient advancement <strong>of</strong> geo<strong>the</strong>rmal energyprojects; and to disseminate information ongeo<strong>the</strong>rmal energy in Australia and internationallyby way <strong>of</strong> workshops, and open interchange <strong>of</strong>experiences and ideas generated within <strong>the</strong><strong>Australian</strong> community. The group have held anumber <strong>of</strong> successful workshops and have beenactively defining <strong>the</strong> research focus <strong>of</strong> <strong>the</strong> TIG. Afew topics that are <strong>the</strong> focus <strong>of</strong> <strong>the</strong> group include: geophysical and geological methods toreduce exploration risks prior to deep drilling39


investigating <strong>the</strong> possible use <strong>of</strong> satellite andairborne systems to measure surfaceradiation to detect high heat producinggranites in <strong>the</strong> sub-surface <strong>the</strong> use <strong>of</strong> magneto-telluric survey data toidentify and locate conductive fluids infractured rocks collection and processing <strong>of</strong> micro-seismicdata around geo<strong>the</strong>rmal projects.Des Fitzgerald from Intrepid Geophysics leadsTIG 10.TIG 11 drilling and well constructionTIG 11 has been very active and has regularmeetings to advance <strong>the</strong> group’s objectives.Topics in scope for <strong>the</strong> TIG include, but are notlimited to:Lower Cost Drilling: Investigate techniquesand new technologies which may lead to areduction in costs to drill geo<strong>the</strong>rmal wells. Zonal Isolation and Packers: Isolationtechniques and equipment need to bedeveloped to isolate zones <strong>of</strong> interest, atextremely high temperatures and possiblypressures, to allow both stimulation andproduction through different zones.Temporary Sealing <strong>of</strong> Fractures: Develop anon-damaging means <strong>of</strong> isolating fractureswhere multiple fractures/ loss zones may beencountered.Cutting Exploration Drilling Costs: A number<strong>of</strong> mechanisms can be developed to reducecosts, such as improving ROP, utilisingsmaller rigs, smaller hole sizes, correctselection <strong>of</strong> materials.The two projects that will be <strong>the</strong> focus for <strong>the</strong>coming year are to progress <strong>the</strong> slimhole drillinggroup and organise a drilling workshop. TIG 11 isled by Dean Hindle and Melanie Von<strong>the</strong>th<strong>of</strong>f fromGeodynamics.TIG 12 educationTIG 12 was recently formed to work on <strong>the</strong> topics<strong>of</strong> education for <strong>the</strong> geo<strong>the</strong>rmal sector andencompasses topics such as defining <strong>the</strong>education needs for <strong>the</strong> industry, <strong>the</strong> development<strong>of</strong> courses ei<strong>the</strong>r at tertiary or postgraduate levelor short courses for industry. The TIG wouldcoordinate with aligned international programsand facilitate <strong>the</strong> initiation & promotion <strong>of</strong>occasional society lunches with guest speakers.<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>ReferencesDepartment <strong>of</strong> Resources, <strong>Energy</strong> and Tourism(DRET), 2008, <strong>Australian</strong> Geo<strong>the</strong>rmal IndustryDevelopment Framework, and, <strong>Australian</strong>Geo<strong>the</strong>rmal Industry Technology Roadmap,Commonwealth <strong>of</strong> Australia, Canberra.<strong>Australian</strong> Geo<strong>the</strong>rmal Reporting CodeCommittee (AGRCC), 2008, The Geo<strong>the</strong>rmalReporting Code. <strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong>Group, Adelaide.Hunt, S.P. and Morelli C.P, 2006, Cooper BasinHDR hazard evaluation: predictive modelling <strong>of</strong>local stress changes due to HFR geo<strong>the</strong>rmalenergy operations in South Australia. Report Book2006/16. Department <strong>of</strong> Primary Industries andResources South Australia, Adelaide.Morelli, C.P., 2009, Analysis and management <strong>of</strong>seismic risks associated with engineeredgeo<strong>the</strong>rmal system operations in South Australia.Report Book 2009/11. Department <strong>of</strong> PrimaryIndustries and Resources South Australia,Adelaide.For more information about any <strong>of</strong> <strong>the</strong> TechnicalInterest Groups please see:www.geo<strong>the</strong>rmal.pir.sa.gov.au/agegor contact pirsa.ageg@sa.gov.au.40


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Comparative petrology & geochemistry <strong>of</strong> high heat-producinggranites in Australia & EuropeV Marshall* 1,2 , J Van Zyl 1,2 , SE Bryan 3 , T Uysal 1,2 , M Gasparon 1,21. Queensland Geo<strong>the</strong>rmal <strong>Energy</strong> Centre <strong>of</strong> Excellence, The University <strong>of</strong> Queensland, St Lucia, QLD 40722. School <strong>of</strong> Earth Sciences, The University <strong>of</strong> Queensland, St Lucia, QLD 40723. Queensland University <strong>of</strong> Technology, Biogeoscience, GPO Box 2434, Brisbane, QLD 4001To better understand <strong>the</strong> origin, tectonic settingand generation <strong>of</strong> high heat-producing granites(HHPG) and provide target criteria for <strong>the</strong>exploration <strong>of</strong> granite-hosted EnhancedGeo<strong>the</strong>rmal Systems (EGS), <strong>Australian</strong> examplesare being studied and compared with betterknown European analogues that are being reexamined.Three areas <strong>of</strong> long-standing interest for EGS inEurope are Cornwall, UK; Soultz-sous-Forêts,France; and <strong>the</strong> Erzgebirge, Germany. Theseareas have higher than average heat flow (atsurface and depth), and concentrations <strong>of</strong> <strong>the</strong>main heat-producing elements Uranium (U),Thorium (Th) and Potassium (K) in granitic rocks.The Big Lake granite suite <strong>of</strong> <strong>the</strong> central<strong>Australian</strong> Cooper Basin (Gatehouse et al., 1995),is a pre-eminent HHPG target for EGSdevelopment in Australia. The Big Lake Suitegranites are Australia’s hottest with temperatures<strong>of</strong> >250ºC at ~4km depth (Habanero 1, (Baisch etal., 2006). The Soultz-sous-Forêts and CooperBasin systems have in common an insulatingsediment cover <strong>of</strong> several kilometres.Keywords: high heat-producing granites (HHPG),Cooper Basin, Cornwall, Soultz-sous-Forêts,Erzgebirge, Uranium, Thorium, Permo-Carboniferous, intraplate.BackgroundThe development <strong>of</strong> EGS in <strong>the</strong> Cooper Basinwas started by Geodynamics Ltd in 2002 with <strong>the</strong>aim to be <strong>the</strong> first <strong>Australian</strong> Company producingelectricity from EGS sources. Their firstgeo<strong>the</strong>rmal well (Habanero 1) encounteredgranite at depth. The granite (Big Lake Suite) issituated in <strong>the</strong> Nappamerrie trough (Meixner etal., 2000; Sun, 1997) and intruded into <strong>the</strong>Cambrian – Ordovician Warburton Basin(Gatehouse et al., 1995). The Big Lake SuiteGranite is covered by a ~3km thick sedimentarypackage consisting <strong>of</strong> <strong>the</strong> Cooper (LateCarboniferous – Middle Triassic), Eromanga(Early Jurassic) and Lake Eyre (Early Tertiary -Holocene) Basins. U/Pb series dating <strong>of</strong> zircon <strong>of</strong>granite intersected at depth in two wellsestablished a Permo-Carboniferous age rangingbetween 323±5 Ma and 298±4 (Gatehouse et al.,1995).The Cornubian batholith in Cornwall (SWEngland; Fig. 1) is comprised <strong>of</strong> six plutonsranging in age from 293.1±1.3 Ma to 274.5±1.4Ma, based on U/Pb dating <strong>of</strong> magmatic monazites(Chen et al., 1993). Two plutons <strong>of</strong> interest are<strong>the</strong> Carnmenellis and Land’s End granites (Fig. 2)as <strong>the</strong>y contain <strong>the</strong> highest levels <strong>of</strong> U and Th(Table 1). During <strong>the</strong> 1970’s and 1980’s <strong>the</strong>Rosemanowes area <strong>of</strong> <strong>the</strong> Carnmenellis granitewas a test site for <strong>the</strong> Department <strong>of</strong> <strong>Energy</strong>,European Commission and Cambourne School <strong>of</strong>Mines investigation into EGS technology as it has<strong>the</strong> highest heat flow in England, over 120 mW/m 2(Tenzer, 2001).Soultz-sous-Forêts (Fig. 1) has been <strong>the</strong>European test site for EGS since 1987, withtemperatures <strong>of</strong> 200°C at 5 km depth (Antics andSanner, 2007).The granites <strong>of</strong> <strong>the</strong> Erzgebirge region (Fig. 1), likeCornwall, are associated with Tin (Sn), Tungsten(W), Lead (Pb), Zinc (Zn), Fluorine (F), Barium(Ba) and U mineralisation, with <strong>the</strong> high U and Thcontents and crustal heat flow values givingadded prospectivity as a clean energy resource.Tectonic HistoryLAURASIA200 kmFigure 1: Location <strong>of</strong> <strong>the</strong> Hercynian/ Variscan mountainchains in <strong>the</strong> middle <strong>of</strong> <strong>the</strong> Carboniferous period. Red linesare sutures. Yellow line is subduction zone (triangles point indirection <strong>of</strong> subduction) (Scotese, 2001). Adapted from Matte(2001) and Zeigler (1990).Regionally, <strong>the</strong> European granites were emplacedin an extensional environment between 334-270Ma following collision <strong>of</strong> Laurasia and Gondwanato form <strong>the</strong> supercontinent Pangaea (Willis-Richards and Jackson, 1989). This collisionalevent, known as <strong>the</strong> Variscan (Hercynian)orogeny, resulted in an extensive rift systemwithin <strong>the</strong> nor<strong>the</strong>rn foreland <strong>of</strong> <strong>the</strong> Variscan41


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>orogenic belt following termination <strong>of</strong> orogenicactivity (Wilson et al., 2004).LAND’S ENDCornwallCARNMENELLISFigure 2: Heat flow map <strong>of</strong> Cornwall, UK, showing <strong>the</strong>location <strong>of</strong> <strong>the</strong> Carnmenellis and Land’s End plutons. Heatflow <strong>of</strong> >120 mW/m 2 (deep red), to 60-70 mW/m 2 (green).Adapted from British Geological Survey GIS heat flow map,<strong>2010</strong>.The Cornubian batholith was emplaced at <strong>the</strong> end<strong>of</strong> <strong>the</strong> Variscan orogeny terminating a period <strong>of</strong>regional, back-arc continental extension during<strong>the</strong> Devonian and Early Carboniferous,(Darbyshire and Shepherd, 1985).This orogenic event caused crustal thickening(Willis-Richards and Jackson, 1989) and hasbeen suspected to have caused anatectic melting(Clark et al., 1993).Figure 1 shows that at <strong>the</strong> time <strong>of</strong> emplacement<strong>the</strong> Cornubian granites were over 1350 km awayfrom <strong>the</strong> nearest active plate margin (bounding<strong>the</strong> Neo-Tethys), suggesting <strong>the</strong>y are notsubduction related.Soultz-sous-ForêtsThe Soultz-sous-Forêts granites lie within <strong>the</strong>Upper Rhine Graben, a tectonically reactivatedregion associated with Oligocene crustalextension and thinning (Genter et al., 2003).These granites were emplaced slightly prior tothose in Cornwall following <strong>the</strong> Variscan orogeny,from 334 +3.8/-3.5 Ma (U/Pb monzogranite) to319.8±0.6 Ma ( 40 Ar/ 39 Ar), (Cocherie et al., 2004and Stussi et al., 2002).ErzgebirgeThe Erzgebirge granites were also intruded from<strong>the</strong> Late Carboniferous to Early Permian duringlarge-scale extension following orogenic collapse(Förster et al., 1999b). In addition, wrenching wasassociated with granite emplacement (Edel et al.,2007).Förster and Förster (2000) concluded that peakorogenic metamorphism occurred 350-340 Ma,followed by rapid uplift and cooling between 340and 326 Ma with <strong>the</strong> oldest, post-collisional,granites intruded to a depth <strong>of</strong> 3-6 km at 325 Ma(Förster et al., 1999b).Table 1 is a summary <strong>of</strong> relevant information for<strong>the</strong>se areas <strong>of</strong> HHPG.Granite PetrographyCooper BasinThe samples studied from <strong>the</strong> Big Lake Suitehave varying degrees <strong>of</strong> alteration, with alterationincreasing with decreasing depth. Unalteredsamples consist <strong>of</strong> quartz (31%), K-feldspar(31%) and plagioclase (31%), with minor biotite(5%) and accessory phases (2%). Accessoryphases indentified are magnetite, apatite,thorite/huttonite, zircon, monazite and xenotimewith some fluorite.The altered samples show varying degrees <strong>of</strong>sericitisation, ranging from minor replacement <strong>of</strong><strong>the</strong> feldspars to complete replacement and <strong>the</strong>formation <strong>of</strong> illite. Biotite has altered to chlorite,after which chlorite is replaced by illite. Freshbiotite still exists in <strong>the</strong> altered samples, but isrestricted to small inclusions in quartz. The illitefrom <strong>the</strong> Big Lake Suite alteration assemblageoccurs as two main textures: 1) pseudomorphicand 2) cryptocrystalline.AbAnorthoclaseSanidineOrAlbiteOligoclaseAndesineLabradorite BytowniteAnorthiteAnFigure 3: Feldspar classification diagram showing <strong>the</strong>feldspar composition. Cooper Basin (•) and Soultz–sous–Forêts (■) (Komninou and Yardley, 1997; Stussi et al.,2002).Electron Probe Microanalysis (EPMA) data showsno compositional differences between <strong>the</strong>different illite textural types. Although illite doesnot show compositonal differences between <strong>the</strong>textural types, <strong>the</strong>re are two compositionallydistinct illites - <strong>the</strong> first is a pure illite with low(


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>undulose extinction, with some grains exhibitingplanar deformation features.Figure 4: Photomicrographs <strong>of</strong> two illite textures (top), andplanar deformation features in quartz (bottom) in Big LakeSuite granites.CornwallThe Carnmenellis granites generally containaround 34% quartz, 32% K-feldspar, 22%plagioclase, 6% biotite, 4% muscovite, 1%tourmaline and 1% accessory phases includingandalusite, cordierite, ilmenite, zircon, monaziteand uraninite (Charoy, 1985; Chappell and Hine,2006).The radioactive mineral assemblageimportant for hosting Th and U are predominantlymonazite, apatite, xenotime, zircon and uraninite(hosting ~90% <strong>of</strong> total U) (Jefferies, 1984; Martelet al., 1990), all <strong>of</strong> which are commonlyassociated with apatite and ilmenite (Jefferies,1984).Soultz-sous-ForêtsThese granites have a normative composition <strong>of</strong>around 43% plagioclase (37% albite, 6%anorthite), 25% K-feldspar, 22% quartz, 6%biotite, 2% hornblende, and


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>confirmed Tammemagi and Smith’s (1975)observations <strong>of</strong> abundant K-feldspar megacrystsin places. Some plutons have subhorizontal flowfabrics (e.g., St Austell granite) suggesting somegranitic magma emplacement in sill-like orlaccolithic bodies, and mineralogical and agevariations indicate <strong>the</strong> batholith has beenincrementally built.Soultz-sous-ForêtsThe Soultz-sous-Forêts granites have beenclassified as S-type according to tectonicdiscrimination diagrams (Fig. 6), however <strong>the</strong>y arenoted to have hornblende (Stussi et al., 2002) andoxidised K-feldspar, suggesting possible I- or A-type classification. They are also peraluminousand porphyritic, with K-feldspar megacrysts up to80 mm in diameter. These granites are thought tohave originated from ei<strong>the</strong>r crustal partial melting<strong>of</strong> enriched metamorphic greywacke, granuliteand amphibolite, or meta-igneous rocks <strong>of</strong>appropriate composition; however, a minor mantlecontribution can’t be excluded due to <strong>the</strong> negativeεNd values (Stussi et al., 2002). Subhorizontalmagma fabric oriented to <strong>the</strong> NE was also notedsuggesting ei<strong>the</strong>r a laccolithic body or <strong>the</strong> ro<strong>of</strong> <strong>of</strong>a diapir-like intrusion, in association with postmagmaticfracturing (Stussi et al., 2002).ErzgebirgeThe Erzgebirge granites are more varied, withmildly peraluminous transitional I- to S-types andstrongly peraluminous S-types both present(Förster et al., 1999b, Fig. 5).Förster et al. (1999b) also noted some graniteshave peraluminous A-type chemical affinities,consistent with <strong>the</strong> intraplate setting <strong>of</strong> thismagmatism.Förster and Förster (2000) recognised that <strong>the</strong>surface heat flow is higher where <strong>the</strong> granitesoccur, contributing 70-90 mW/m 2 to <strong>the</strong> surfaceheat flow - two to four times higher than would beestimated from <strong>the</strong> average composition <strong>of</strong> <strong>the</strong>continental bulk crust.Table 1: Compositions <strong>of</strong> targeted HHPG for EGS. Sources: Charoy (1985), Chappell and Hine (2006), Jefferies (1984), Martelet al. (1990), Tammemagi and Smith (1975), Willis-Richards and Jackson (1989), Chen et al. (1993), Müller et al. (2006), FörsterH.J. (1999), Förster and Förster (2000), Förster et al. (1999a), Förster et al. (1999b), Hooijkaas et al. (2006), Stussi et al. (2002),Uysal and van Zyl (unpubl. data), and Taylor and McLennan, (1985).EGSTARGETEDGRANITESCarnmenellisCornwall, UKLand’s EndCornwall, UKSoultz-sous-ForêtsUpper RhineGraben, FranceErzgebirge,GermanyCooper Basin,AustraliaUpperContinentalCrustAGE(Ma)LITHOLOGY295-270 Megacrystic biotite and two-micagranitesSiO2(wt%)K2O(wt%)U(ppm)70-76 4-4.3 4.3-35(12.1mean)Th(ppm)11-25(19.3mean)277-274.5 Early megacrystic biotite granites, 66-73 3.5-6 6.9-38 4.4-46.2younger Li-siderophyllite granites334-319 Porphyritic monzogranite 67-69 3.8-4 6.2-14.1 23-37325-315 Transitional I-, S- and A- type biotitegranites, two-mica granites and S- andA- type Li-mica granites323-298 Coarse grained two feldspar biotitegranite, moderately wea<strong>the</strong>red67-77(biotite)71-76(two-mica)3.8-5.4 9-30.9 10.4-34.373-76(Li-mica)- - 11 - 27 17 - 11766 3.4 2.7 10.744


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>ANK3.02.8 Metaluminous Peraluminous2.62.42.22.01.81.61.41.21.00.8Peralkaline0.60.40.5 1.0 1.5 2.0ACNKFigure 5: ASI index for granites classification plot accordingto Shand (1927), Cooper Basin (); Cocherie et al. (2004),Soultz-sous-Forêts (•); Chappell and Hine (2006) andMüller et al. (2006), Cornwall (•); and Förster et al. (1999b)Erzgebirge (X).100090040080307210Cooper BasinLa Ce Pr Nd Sm Eu Gd Tb Dy Ho Er Tm Yb Lu100WPGNb10VAG+Syn-COLGORG11 10 100 10002000Figure 6: Tectonic discrimination diagram comparing <strong>the</strong>studied granite suites (Pearce et al., 1984).300Y900.0400.0Erzgebirge80.0FeO/MgO20FG30.07.02.0OGT150 600Zr+Nb+Ce+Y0.60.1La Ce Pr Nd Sm Eu Gd Tb Dy Ho Er Tm Yb LuFigure 7: Granite discrimination plot from Whalen et al.(1987) OGT - O<strong>the</strong>r Granite Types (I-, M-, S- type), FG –Fractionated Felsic Granites.Figure 8: REE Spider plots for <strong>the</strong> four granite intrusions.Normalisation was performed using McDonough and Sun(1995).45


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Discussion and Comparison Both European and <strong>Australian</strong> examples <strong>of</strong>HHPG are Late Carboniferous to EarlyPermian in age. All HHPG in this study were emplaced well inboard from active plate margins. TheEuropean granites are post-collisional andextension-related, whereas <strong>the</strong> Cooper Basingranites are also within-plate but may be(temporally) related to intraplate deformation. The Cooper Basin, Soultz-sous-Forêts and<strong>the</strong> Erzgebirge show similar abundances <strong>of</strong>quartz, plagioclase and K-feldspar, withplagioclase being <strong>the</strong> more abundant phasein Soultz-sous-Forêts. The Cooper Basin andErzgebirge are equigranular, whereas Soultzsous-Forêtsand <strong>the</strong> Carnmenellis aredistinctly megacrystic granites. It is difficult to use <strong>the</strong> I- and S- typeclassification for fractionated granites, but thisstudy suggests all <strong>the</strong> granites areperaluminous, with <strong>the</strong> European granitesdominantly S-type, but Cooper Basin andErzgebirge also showing I- and A- typeaffinities suggesting that crustal sourcecomposition may not be a prime control onHHPG generation. Literature and field observations indicate thatat least part <strong>of</strong> <strong>the</strong> Cornubian and Soultzsous-Forêtsgranites have sill-like intrusivecomponents but importantly, that all <strong>the</strong>batholiths discussed here have beenincrementally built by a number <strong>of</strong> intrusions. Trace element geochemistry and rare ear<strong>the</strong>lement abundances <strong>of</strong> <strong>the</strong> Cooper Basingranites show a range from less fractionatedto highly fractionated (Eu/Eu* =0.04 to 0.17),whereas Soultz-sous-Forêts show moreuniform REE patterns, and a wide range <strong>of</strong>REE patterns have been described for <strong>the</strong>Erzgebirge granites. The Carnmenellis has anarrower range in REE than <strong>the</strong> Erzgebirge.The Cooper Basin, Carnmenellis andErzgebirge all show strong Eu anomaliesindicating fractional crystallisation wasimportant in <strong>the</strong> production <strong>of</strong> <strong>the</strong>se granites(Fig. 7). Isotope data suggests that all examples havecrustal signatures. The Cooper Basin granites are more enrichedin Th, but <strong>the</strong>re is similar U enrichment for allexamples. Currently, <strong>the</strong> reason for U and Thenrichment is unknown, except for <strong>the</strong> normalfractional crystallisation processes.The current conclusion from this study is that <strong>the</strong>peraluminous, highly fractionated chemistrieshave promoted <strong>the</strong> U and Th enrichment <strong>of</strong>HHPG.ReferencesAntics, M., and Sanner, B., 2007, Status <strong>of</strong>geo<strong>the</strong>rmal energy use and resources in Europe,<strong>Proceedings</strong> European Geo<strong>the</strong>rmal Congress, 2Baisch, S., Weidler, R., Vörös, R., Wyborn, D. andde Graaf, L., 2006. Induced Seismicity during <strong>the</strong>Stimulation <strong>of</strong> a Geo<strong>the</strong>rmal HFR Reservoir in <strong>the</strong>Cooper Basin, Australia. Bulletin <strong>of</strong> <strong>the</strong>Seismological Society <strong>of</strong> America, 96(6): 15.Bartier, D. et al., 2008. Hydro<strong>the</strong>rmal alteration <strong>of</strong><strong>the</strong> Soultz-sous-Forêts granite (Hot FracturedRock geo<strong>the</strong>rmal exchanger) into a tosudite andillite assemblage. European Journal <strong>of</strong>Mineralogy, 20: 12Charoy, B., 1985, The genesis <strong>of</strong> <strong>the</strong> CornubianBatholith (south-west England): <strong>the</strong> example <strong>of</strong><strong>the</strong> Carnmenellis Pluton, Journal <strong>of</strong> Petrology, 27,Part 3, 571-604Chappel, B.W. and Hine, 2006, The CornubianBatholith: An Example <strong>of</strong> Magmatic Fractionationon Crustal Scale, Resource Geology, 56, 203-244Chappell, B.W. and White, A.J.R., 2001. TwoContrasting granite types: 25 years later.<strong>Australian</strong> Journal <strong>of</strong> Earth Sciences, 48: 12.Chen Y., Clark, A.H., Farrar, E., Wasteneys,H.A.H.P., Hodgson, M.J. and Bromley, A.V.,1993, Diachronous and independent histories <strong>of</strong>plutonism and mineralisation in <strong>the</strong> CornubianBatholith, southwest England, Journal <strong>of</strong> <strong>the</strong>Geological Society, 150, 1183-1191Clark, A.H., Chen,Y., Farrar, E., Wasteneys,H.A.H.P, Stimac, J.A., Hodgson, M.J., Willis-Richards, J., and Bromley, A.V., 1993, TheCornubian Sn-Cu (-As, W) metallogeneticprovince: product <strong>of</strong> a 30 M.Y. history <strong>of</strong> discreteand concomitant anatectic, intrusive andhydro<strong>the</strong>rmal events, <strong>Proceedings</strong> <strong>of</strong> <strong>the</strong> UssherSociety, 8, 112-116Cocherie, A., Guerrot, C., Fanning, C.M. andGenter, A., 2004, Datation U-Pb des deux facièsdu granite de Soultz (Fossé rhénan, France),Géochimie (Géochronologie), 336, 775-787Darbyshire, D.P.F., and Shepherd, T.J., 1985,Chronology <strong>of</strong> granite magmatism and associatedmineralisation, SW England, Journal <strong>of</strong> <strong>the</strong>Geological Society, 142, 1159-1177Edel, J.B., Schulmann, K. and Rotstein, Y., 2007,The Variscan tectonic inheritance <strong>of</strong> <strong>the</strong> UpperRhine Graben: evidence <strong>of</strong> reactivations in <strong>the</strong>Lias, Late Eocene-Oligocene up to <strong>the</strong> recent,International Journal <strong>of</strong> Earth Science, 96, 305-325Förster H.J., 1999, The chemical composition <strong>of</strong>uraninite in Variscan granites <strong>of</strong> <strong>the</strong> Erzgebirge,Germany, Mineralogical Magazine, 63, 2, 239-25246


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Förster, H.J., Davis, J.C., Tischendorf, G., andSeltmann, R., 1999a, Multivariate analyses <strong>of</strong>Erzgebirge granite and rhyolite composition:implications for classification <strong>of</strong> granites and <strong>the</strong>irgenetic relations, Computers and Geosciences,25, 533-546Förster H.J.,Tischendorf, R.B., Trumbull, R.B. andGottesmann, B., 1999b, Late-collisional granitesin <strong>the</strong> Variscan Erzgebirge, Germany, Journal <strong>of</strong>Petrology, 40, 11, 1613-1645Förster, A. and Förster H.J., 2000, Crustalcomposition and mantle heat flow: Implicationsfrom surface heat flow and radiogenic heatproduction in <strong>the</strong> Variscan Erzgebirge (Germany),Journal <strong>of</strong> Geophysical Research, 105, B12,27,917-27,938Gatehouse, C.G., Fanning, C.M. and Flint, R.B.,1995. Geochronology <strong>of</strong> <strong>the</strong> Big Lake Suite,Warburton Basin, nor<strong>the</strong>astern South Australia. .Quarterly Geological Notes <strong>of</strong> <strong>the</strong> GeologicalSurvey <strong>of</strong> South Australia, 128: 7.Genter, A., Guillou-Frottier, L., Feybesse, J-L.,Nicol, N., Dezayes, C. and Schwartz, S., 2003,Typology <strong>of</strong> potential hot fractured rock resourcesin Europe, Geo<strong>the</strong>rmics, 32, 701-710Ghosh, P.K., 1934, The Carnmenellis Granite: itspetrology, metamorphism and tectonics, QuarterlyJournal <strong>of</strong> <strong>the</strong> Geological Society, 90, 240-273Hooijkaas, G.R., Genter, A. and Dezayes, C.,2006, Deep-seated geology <strong>of</strong> <strong>the</strong> graniteintrusions at <strong>the</strong> Soultz EGS site based on datafrom 5 km-deep boreholes, Geo<strong>the</strong>rmics, 35, 484-506Komninou, A. and Yardley, B.W.D., 1997. Fluidrockinteractions in <strong>the</strong> Rhine Graben: A<strong>the</strong>rmodynamic model <strong>of</strong> <strong>the</strong> hydro<strong>the</strong>rmalalteration observed in deep drilling. Geochimica etCosmochimica Acta, 61(3): 17Jefferies, N.L., 1984, The radioactive mineralassemblage <strong>of</strong> <strong>the</strong> Carnmenellis Granite,Cornwall, <strong>Proceedings</strong> <strong>of</strong> <strong>the</strong> Ussher Society, 6,35-40Martel, D.J., O’Nions, R.K., Hilton, D.R. andOxburgh, E.R., 1990, The role <strong>of</strong> elementdistribution in production and release <strong>of</strong>radiogenic helium: <strong>the</strong> Carnmenellis Granite,southwest England, Chemical Geology, 88, 207-221Matte, P., 2001, The Variscan collage andorogeny (480 – 290 Ma) and <strong>the</strong> tectonicdefinition <strong>of</strong> <strong>the</strong> Armorica microplate; a review,Terra Nova, 13, 122-128McLaren, S. and Dunlap, W.J., 2006. Use <strong>of</strong>40Ar/39Ar K-Feldspar <strong>the</strong>rmochronology in <strong>the</strong>basin <strong>the</strong>rmal history reconstruction: an examplefrom <strong>the</strong> Big Lake Suite Granites, WarburtonBasin, South Australia. Basin Research, 18: 15.Meixner, T.J. et al., 2000. The Nature <strong>of</strong> <strong>the</strong>Basement to <strong>the</strong> Cooper Basin region, SouthAustralia. Exploration Geophysics, 31: 9.Müller, A., Seltmann, R., Halls, C., Siebel, W.,Dulski, P., Jeffries, T., Spratt, J. and Kronz, A.,2006, The magmatic evolution <strong>of</strong> <strong>the</strong> Land’s Endpluton, Cornwall, and associated pre-enrichment<strong>of</strong> metals, Ore Geology Reviews, 28, 329-367Pearce, J.A., Harris, N.B.W. and Tindle, A.G.,1984. Trace Element Discrimination Diagrams for<strong>the</strong> Tectonic Interpretation <strong>of</strong> Granitic Rocks.Journal <strong>of</strong> Petrology, 25(4): 28.Scotese, C.R., 2001, Late Carboniferous: Atlas <strong>of</strong>Earth History, 1, Paleogeography, PALEOMAPProject, 52Stussi, J.M., Cheilletz, A., Royer, J.J.,Chevremont, P. and Feraud, G., 2002. TheHidden monzogranite <strong>of</strong> Soultz-sous- Forêts(Rhine Graben, France). Géologie de laFrance(1): 19.Sun, X., 1997. Structural style <strong>of</strong> <strong>the</strong> WarburtonBasin and control on <strong>the</strong> Cooper and EromangaBasins, South Australia. Exploration Geophysics,28: 6Tammemagi, H,Y. and Smith, N.L., 1975, Aradiogeologic study <strong>of</strong> <strong>the</strong> granites <strong>of</strong> SW.England, Journal <strong>of</strong> <strong>the</strong> Geological Society, 131.415-427Taylor, S.R. and McLennan, S.M., 1985, TheContinental Crust: its Composition and Evolution,Blackwell Scientific Publications, 46Tenzer, H., 2001, Development <strong>of</strong> hot dry rocktechnology, GHC Bulletin, 18Whalen, J.B., Currie, K.L. and Chappell, B.W.,1987. A-Type granites: Geochemicalcharacterisitcs, discrimination and pretrogenesis.Contributions to Mineralogy and Petrology, 95: 13Willis-Richards, J. and Jackson, N.J., 1989,Evolution <strong>of</strong> <strong>the</strong> Cornubian ore field, southwestEngland: Part I. Batholith modelling and oredistribution, Economic Geology, 84, 1078-1100Wilson, M., Neumann, E. R., Davies, G. R.,Timmerman, M. J., Heeremans, M., and Larsen,B. T., 2004, Permo-Carboniferous magmatismand rifting in Europe: introduction, The GeologicalSociety, London, Special Publication, 223, 1-10Veevers, J.J., 2009, Mid-Carboniferous Centralianuplift linked by U-Pb zircon chronology to <strong>the</strong>onset <strong>of</strong> <strong>Australian</strong> glaciation and glacio-eustasy,<strong>Australian</strong> Journal <strong>of</strong> Earth Sciences, 56, 711–717.Zeigler, P.A., 1990, Geological Atlas <strong>of</strong> Westernand Central Europe, Shell International PetroleumMaatschappij BV (2 nd edition)47


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Geo<strong>the</strong>rmal Prospection Using Existing Groundwater Geochemicaland Thermal Datasets: Identifying Regions <strong>of</strong> Interest in Queenslandfrom Government Well and Bore Data* +Craig McClarren 1,2 , Massimo Gasparon 1,2,3 , and I. Tonguç Uysal 1,21 School <strong>of</strong> Earth Sciences, The University <strong>of</strong> Queensland, Brisbane, QLD. 40722 Queensland Geo<strong>the</strong>rmal <strong>Energy</strong> Centre <strong>of</strong> Excellence, The University <strong>of</strong> Queensland, Brisbane, QLD. 40723 National Centre for Groundwater Research and Training, The University <strong>of</strong> Queensland, Brisbane, QLD. 4072Geochemical analysis <strong>of</strong> well and bore waters has<strong>the</strong> potential to provide valuable clues inidentifying regions <strong>of</strong> high geo<strong>the</strong>rmal potential.Chemical and isotopic markers indicative <strong>of</strong> <strong>the</strong>presence <strong>of</strong> high heat producing granites or o<strong>the</strong>rheat producing bodies may be mobilized byflowing groundwater and may make <strong>the</strong>ir way todeep wells and bores. Though likely highlydiluted, <strong>the</strong>se markers may also be detectable inshallow wells and bores in some regionsdepending on local geological and hydrologicalconditions. A significant quantity <strong>of</strong> data <strong>of</strong> thistype already exists in publicly availablegovernment databases. These data are <strong>of</strong>tencoarse and <strong>of</strong> frequently unknown quality, butmay prove to be a useful tool in first-order largescalegeo<strong>the</strong>rmal prospection. We have obtainedsuch a dataset from <strong>the</strong> Queensland Department<strong>of</strong> Environment and Resource Management, andhave extensively analysed <strong>the</strong> data with <strong>the</strong> aim<strong>of</strong> identifying potential areas <strong>of</strong> interest ingeo<strong>the</strong>rmal prospection. This research represents<strong>the</strong> first stage <strong>of</strong> a large multi-stage project ingroundwater geochemistry aimed at geo<strong>the</strong>rmalprospection.Keywords: Geo<strong>the</strong>rmal exploration, bore water,trace element, isotope, QueenslandThe Potential for GroundwaterGeochemistry in Geo<strong>the</strong>rmalProspectingGeochemical analysis <strong>of</strong> groundwater may holdsignificant potential for identification <strong>of</strong>unrecognized regions <strong>of</strong> high geo<strong>the</strong>rmalpotential. Geo<strong>the</strong>rmal source rocks, whe<strong>the</strong>rsedimentary, radiogenic igneous, or youngigneous, produce mineralogical, chemical, andisotopic markers which can be used to identify<strong>the</strong>m (Marini, L.). Many <strong>of</strong> <strong>the</strong>se markers arewater soluble and can thus be moved from depthtoward <strong>the</strong> surface (Barbier, et. al, 1983). During<strong>the</strong> process, <strong>the</strong>se markers may suffer significantdilution, but may still be detectable in groundwatersamples taken at or near <strong>the</strong>se <strong>the</strong>rmallysignificant regions (Smedley, P., 1991) .Thousands <strong>of</strong> ground water samples from acrossQueensland have already been taken andanalysed for a limited range <strong>of</strong> water qualityparameters; this data can be obtained from <strong>the</strong>State Government for research purposes. Byproviding chemical analysis results from almost28,000 water wells and bores across <strong>the</strong> state,<strong>the</strong> Queensland Department <strong>of</strong> Environment andResource Management (DERM) water boreholedatabase is a locally unparalleled resource forconducting a large-scale first-order typeinvestigation and identification <strong>of</strong> geo<strong>the</strong>rmallyprospective regions within <strong>the</strong> state.Geochemical toolsWhile <strong>the</strong>re are dozens <strong>of</strong> mineralogical,chemical, and isotopic markers that can be usedto identify potential geo<strong>the</strong>rmal targets, in using<strong>the</strong> data available from <strong>the</strong> DERM water boreholedatabase, one is restricted to <strong>the</strong> limited set <strong>of</strong>parameters measured. The quality andcompleteness <strong>of</strong> <strong>the</strong> chemical data can bedescribed as highly variable, with results collectedand analysed by many different parties usingunknown procedures over <strong>the</strong> course <strong>of</strong> severaldecades. Moreover, <strong>the</strong> results <strong>the</strong>mselves areinconsistent between analyses, withmeasurements for elements such as boron andphosphorous making occasional appearanceswhile largely remaining absent from <strong>the</strong> rest <strong>of</strong> <strong>the</strong>dataset.While <strong>the</strong> quality <strong>of</strong> measurements may be calledinto question, <strong>the</strong> abundance <strong>of</strong> analyses, as wellas <strong>the</strong>ir geographic population density in manyregions, suggests that <strong>the</strong> data may still becautiously used on a large scale (typically a fewthousand square kilometres at best) to identifysources <strong>of</strong> heat at depth. From <strong>the</strong> database,initially a large number <strong>of</strong> known indicators <strong>of</strong>geo<strong>the</strong>rmal potential, used extensivelyinternationally, were selected. These include <strong>the</strong>elements and compounds Na, K, Cl, F, Cu, SO 4 ,Zn, PO 4 , and B. While it was readilyacknowledged that many <strong>of</strong> <strong>the</strong>se elements maybe associated to non-geo<strong>the</strong>rmally indicativesources, <strong>the</strong> rationale for this analysis is thatwhere a large number <strong>of</strong> notably highconcentration values for <strong>the</strong>se elementsoverlapped, <strong>the</strong>se areas would be most worthy <strong>of</strong>fur<strong>the</strong>r investigation.48


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Figure 1: Early map <strong>of</strong> regions to contain potentialgeo<strong>the</strong>rmal resources based on unfiltered geochemical data.The image was composed by colouring regions with <strong>the</strong>highest potential for each selected element or compound and<strong>the</strong>n overlaying all <strong>of</strong> <strong>the</strong> layers. Diagonal hashes indicateslightly promising regions while boxed X’s are <strong>the</strong> mostpromising regions based on this early analysis.Refining <strong>the</strong> dataWith this preliminary analysis <strong>of</strong> data completed,maps <strong>of</strong> individual elements were more closelystudied to assess <strong>the</strong>ir suitability as potentialindicators <strong>of</strong> associated geo<strong>the</strong>rmal systems . Naand K were first discarded because <strong>of</strong> <strong>the</strong>tremendous abundance <strong>of</strong> possible alternativesources. Cl was next discarded because <strong>of</strong> itsclose relationship with K and Na. PO 4 was nextremoved as data on this element throughout <strong>the</strong>dataset was extremely sparse and because <strong>the</strong>highest values tended to be in wetter, moretropical, parts <strong>of</strong> Queensland which may simplyreflect <strong>the</strong> infiltration <strong>of</strong> organic phosphate from<strong>the</strong> surface into a shallow watertable. Zn wasremoved both for its scarcity <strong>of</strong> data as well as fornot showing any distinguishable trends or patternswhen concentrations were mapped. While Cuconcentration showed possibly promising results,again <strong>the</strong> data was relatively sparse. SO 4 did notshow clear trends and has many possiblesources, so it was initially removed. One potentialsource <strong>of</strong> sulphate, however, are coal measureswhich are known to be effective cap units togeo<strong>the</strong>rmal reservoirs. Thus, sulphate data maybe revisited in <strong>the</strong> future to analyse <strong>the</strong> suitability<strong>of</strong> a geo<strong>the</strong>rmally interesting site to futureexploitation.It was finally decided to focus primarily on boron(B) and fluoride (F - ), which are both relativelysoluble and abundant in felsic igneous bodies.Boron data, though somewhat sparse, showseasily distinguished trends (non-randomgeographical and/or geological distributions) whenmapped. Fluoride data is abundant and alsoshows easily distinguished trends when mapped.It was additionally decided that F - would be mostindicative <strong>of</strong> buried high heat producing granites(HHPGs) at depth, as <strong>the</strong>re are fewer likelyalternative sources for F - than for B.Filtering <strong>the</strong> dataThe aim <strong>of</strong> this research is two-fold. First, it is toidentify potential regions <strong>of</strong> geo<strong>the</strong>rmal interestand secondly to identify regions on which to focusfuture sampling work for later stages <strong>of</strong> thisresearch project (<strong>the</strong> details <strong>of</strong> which will bediscussed elsewhere). The first filter applied was<strong>the</strong> most fundamental: many <strong>of</strong> <strong>the</strong> bores in <strong>the</strong>database were no longer existing, but werecategorized as “Abandoned and Destroyed.”These entries were removed as <strong>the</strong>y were <strong>of</strong> nopractical use to us, in that <strong>the</strong> results could not beverified by future sampling. Wells that wereclassified as “Existing” or “Abandoned butUseable” were left in <strong>the</strong> set. The next filterapplied was for F - concentration; after someconsultation and discussion within <strong>the</strong> group, avalue <strong>of</strong> 1.4 ppm was decided upon as a lowerlimit for water chemistries we deemed“interesting”. The choice <strong>of</strong> this value significantlyreduced <strong>the</strong> dataset, but left behind more than3500 values showing easily distinguishable trendsand patterns when mapped across Queensland.High values around known igneous regions, suchas <strong>the</strong> Stanthorpe Granite Belt and <strong>the</strong> morerecently active Cairns region, strongly suggeststhat this could be an extremely valuable tool inidentifying igneous bodies at depth elsewhere.High values in regions not already known tocontain intrusive bodies will be investigated.The next filter applied was depth as it is likely thatwith greater depth comes a lower likelihood <strong>of</strong>significant dilution <strong>of</strong> circulating or simply flowinggroundwater by local and relatively recentmeteoric waters. Entries with bore depths <strong>of</strong> lessthan 10 meters were removed; however, becausemany entries do not have a recorded depth (andthus receive a value <strong>of</strong> zero through intermediateprocessing steps), values <strong>of</strong> zero were left so thatwells <strong>of</strong> unrecorded depth, <strong>of</strong> which <strong>the</strong>re aremany, would remain. Next, because at or nearHHPGs we expect to find elevated Bconcentrations in groundwaters, <strong>the</strong> sites with <strong>the</strong>lowest B values were removed from <strong>the</strong> remainingdataset. A cut-<strong>of</strong>f <strong>of</strong> 0.3 ppm B was chosen to49


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>remove <strong>the</strong> sites least likely to show evidence <strong>of</strong> anearby HHPG; similar to <strong>the</strong> filter for depth,values <strong>of</strong> zero were left as most <strong>of</strong> <strong>the</strong> sitessampled for F - content unfortunately do not showB results.Finally, with purely <strong>the</strong> aim <strong>of</strong> sample access inmind <strong>the</strong> category <strong>of</strong> “owner” needed to befiltered. Location and ownership information isprovided with <strong>the</strong> data; however access to <strong>the</strong>monitoring bores is restricted to DERM staff. With<strong>the</strong>se data filtered out, most <strong>of</strong> <strong>the</strong> prospectivesampling sites along coastal Queensland areremoved; <strong>the</strong> majority <strong>of</strong> <strong>the</strong> inland bores, whichare usually privately owned, remain, allowing usto extensively investigate most <strong>of</strong> <strong>the</strong>geochemically interesting regions within <strong>the</strong> state.Coastal regions, with close proximity to populationcentres, however, are <strong>the</strong>reby restricted.prove useful when considered toge<strong>the</strong>r withgeochemical data in <strong>the</strong> future.In addition to water bore and well data fromDERM, <strong>the</strong>re are also publically available datafrom exploratory coal, oil, and gas drilling in <strong>the</strong>Queensland Petroleum Exploration Database(QPED) from <strong>the</strong> Queensland Department <strong>of</strong>Mines and <strong>Energy</strong> (DME). These data includetemperature results as well as geochemicalanalyses; because <strong>of</strong> <strong>the</strong>ir extremely limitedgeographic distribution, however, this dataset isunsuitable to state-wide geo<strong>the</strong>rmal prospection.A high concentration <strong>of</strong> data points in <strong>the</strong> GreatArtesian Basin in Queensland’s Southwest cornermay prove useful to individuals or groupsinvestigating this known region <strong>of</strong> high geo<strong>the</strong>rmalpotential. In a far more local context, QPED wellcompletion reports may prove valuable as anearly investigatory step in areas where suchdrilling has been conducted.Figure 2: Water well and bore data across Queenslandfiltered for Fluorine and Boron content, depth, and “owner”.The colour scale is for Fluorine content in ppm.Hydro<strong>the</strong>rmal Data and Results fromO<strong>the</strong>r DatasetsAs well as geochemical analyses <strong>of</strong> water boresthroughout <strong>the</strong> state, <strong>the</strong> DERM dataset alsocontains water temperature data from many <strong>of</strong><strong>the</strong>se same bores. These data, however, are <strong>of</strong>limited value due to <strong>the</strong> limitations <strong>of</strong> bore depth;water temperatures are low throughout coastalQueensland and rise ra<strong>the</strong>r predictably withdistance inland, likely reflecting <strong>the</strong> increasingdepth to <strong>the</strong> water table ra<strong>the</strong>r than a significantgeo<strong>the</strong>rmal gradient. These data, however, mayFigure 3: Unfiltered water well and bore <strong>the</strong>rmal data acrossQueensland. The map shows maximum temperaturesrecorded at each site; <strong>the</strong> colour scale is for watertemperature in degrees Celsius.SummaryAn extensive dataset comprising <strong>the</strong>rmal andgeochemical analyses <strong>of</strong> public and privatelyowned water wells and bores from across <strong>the</strong>state <strong>of</strong> Queensland is publicly available from <strong>the</strong>Queensland Department <strong>of</strong> Environment andResource Management. While <strong>the</strong> <strong>the</strong>rmal datahave limited potential in geo<strong>the</strong>rmal prospectiondue to <strong>the</strong> depth-dependent nature <strong>of</strong> <strong>the</strong>measurements, <strong>the</strong> geochemical dataset may be50


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong><strong>of</strong> tremendous value. Chemical markers indicative<strong>of</strong> HHPGs or o<strong>the</strong>r heat producing bodies may bemobilized by flowing groundwater, making <strong>the</strong>irway to deep wells and bores. Though likelydiluted, <strong>the</strong>se markers may also be detectable inshallow wells and bores depending on localgeological and hydrological conditions.We have analysed <strong>the</strong> available dataset, choosingto focus primarily on fluoride and boronconcentrations, as a first-order exploratory tool toidentify regions potentially containing geo<strong>the</strong>rmalresources and to identify sites and regions forfuture sampling and geochemical analysistowards that end. Several filters were put in place,reducing <strong>the</strong> extensive dataset to a moremanageable and consistent and size and nature.The Queensland Petroleum and ExplorationDatabase publically available from <strong>the</strong>Department <strong>of</strong> Mines and <strong>Energy</strong> is not suitablefor state-wide geo<strong>the</strong>rmal prospection due to <strong>the</strong>geographic distribution <strong>of</strong> sampling sites, but maybe <strong>of</strong> significant local value in SouthwestQueensland.(including accuracy, reliability, completeness orsuitability) and accepts no liability (includingwithout limitation, liability in negligence) for anyloss, damage or costs (including consequentialdamage) relating to any use <strong>of</strong> <strong>the</strong> dataReferencesBarbier, E., Fanelli, M., Gonfiantini, R.,1983,Isotopes in Geo<strong>the</strong>rmal <strong>Energy</strong> Exploration, IAEABulletin, v. 25, no. 2, pp. 31-36Marini, L., Geochemical Techniques for <strong>the</strong>Exploration and Exploitation <strong>of</strong> Geo<strong>the</strong>rmal<strong>Energy</strong>, Dipartimento per lo Studio del Territorio edelle sue Risorse, Università degli Studi diGenova, Genova, ItalySmedley, P., 1991, The Geochemistry <strong>of</strong> RareEarth Elements in Groundwater from <strong>the</strong>Carnmenellis Area, Southwest England,Geochimica et Cosmochimica Acta, v. 55, pp.2767-2779* Based on or contains data provided by <strong>the</strong> State<strong>of</strong> Queensland (Department <strong>of</strong> Environment andResource Management) [2009]. In consideration<strong>of</strong> <strong>the</strong> State permitting use <strong>of</strong> this data youacknowledge and agree that <strong>the</strong> State gives nowarranty in relation to <strong>the</strong> data (includingaccuracy, reliability, completeness, currency orsuitability) and accepts no liability (includingwithout limitation, liability in negligence) for anyloss, damage or costs (including consequentialdamage) relating to any use <strong>of</strong> <strong>the</strong> data. Datamust not be used for direct marketing or be usedin breach <strong>of</strong> <strong>the</strong> privacy laws.+Based on or contains data provided by <strong>the</strong> State<strong>of</strong> Queensland (Department <strong>of</strong> Employment,Economic Development and Innovation) [2009]which gives no warranty in relation to <strong>the</strong> data51


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Genie Impact DrillsSynopsis <strong>of</strong> a New Hard Rock Drilling DevelopmentMalcolm B McInnes FIEAust. CPEng MESc BE ARMIT Mech Eng MAIE SPESpecialised Drilling Services Australia Pty LtdPO BOX 297, Fullarton, South Australia 5063, Australia.AbstractIn 2004, a lean new <strong>Australian</strong> company wasestablished to independently focus on <strong>the</strong>development and commercialisation <strong>of</strong> newdrilling technology for <strong>the</strong> geo<strong>the</strong>rmal, petroleum& scientific industries. It began with assetsincluding know-how, intellectual property,documentation and some equipment retainedfrom pioneering work undertaken in <strong>the</strong> parentcompany between 1992 and 2002. It hasproduced a new commercial product, <strong>the</strong> Genie185, a drilling liquid powered impact drill, <strong>the</strong> firstin a range <strong>of</strong> new, high performance tools which<strong>of</strong>fer higher Rates Of Penetration and simpler,lighter drill strings for hard formation drilling.PurposeTo build a pr<strong>of</strong>itable commercial enterprise basedon <strong>the</strong> development and provision <strong>of</strong> superiorquality drilling services & products to <strong>the</strong>petroleum, geo<strong>the</strong>rmal and scientific industries.Geo<strong>the</strong>rmal power market<strong>Australian</strong> geo<strong>the</strong>rmal wells are being drilled todepths <strong>of</strong> around 4,500m but financial viability <strong>of</strong>hard fractured rock reservoirs is threatened by lowRates Of Penetration and problems associatedwith traditional rotary drilling systems in <strong>the</strong>seenvironments.TechnologyHigh ROP, drilling liquid powered impact drillingsystems for harder formations.ProductRented, on-site supported, fully serviced &equipped Genie impact drills and bit sales. .Genie impact drillConceived and designed as a flexibly sized tool tocreate a range ra<strong>the</strong>r than a series <strong>of</strong> successiveindividually designed tools. The design isdisciplined and imbedded in <strong>the</strong> drawings <strong>of</strong> <strong>the</strong>definitive, mid-range Genie 185 (for bits between8-1/2" & 9-7/8"). See Fig. 1. There are fewer partsthan in predecessor tools as well as enhanced bitalignment, new hard surface designs andtreatments, corrosion protection, simple andsecure jet nozzle mounting, longer tong grip zoneand new assembly system for easy, fast and safemaintenance and set-up. A general ma<strong>the</strong>maticalmodel generates hydraulic & dynamicperformance simulations which are used with awell model for application checks & set-up.FIG. 1 – TALISMAN ENERGY INC WITH GENIE 185 ONNABORS RIG – BC, CANADAGeneral design & manufacturingPart designs are geometrically and parametricallylinked to each o<strong>the</strong>r and to a single scalingparameter which sets tool size. This savesrepletion and improves drafting quality. The midrangeGenie 185 has a scaling parameter <strong>of</strong> 1.Each Genie model has an associated range <strong>of</strong> bitsizes. Bit head design geometry is linked to asecond independent scaling parameter, <strong>the</strong> bitgauge diameter. A custom bit <strong>of</strong> any size between<strong>the</strong> specified minimum and maximum size can beproduced. Design changes are more easilymanaged. Manufacturing is more flexible andsimpler with improved quality and lead time as <strong>the</strong>result <strong>of</strong> feature commonality through <strong>the</strong> range.Model selection & model numberThe housing diameter in each Genie model ismatched to BHA collar sizes whilst keeping <strong>the</strong>target bit gauge within range. The tool housingdiameter in mm (rounded to nearest 5) provides<strong>the</strong> model number. The model number is notlinked to any particular bit size and bit size rangescan overlap between some models.Size & transportGenie tools were designed with consideration forcarrying in pick-ups and helicopters. They havean integral twin check valve. The Genie 185 is52


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>under 2m long, including <strong>the</strong> integral jet sub andis half <strong>the</strong> size and weight <strong>of</strong> predecessor tools.Connecting threadsGenie tools have pin down API female topthreads for protection during handling and forreduced length & mass. Genie bits are retained ina “pin up”, splined drive sub (chuck) which screwsinto <strong>the</strong> Genie tool using a new design thread.Model rangeCurrent planned models include Genie130 (6” to6⅞” bits), 160 (7½” to 8⅝”), 185, 200 (9⅜” to 11”),260 (12” to 14¼”) & 320 (14⅝” to 17½”). The 320& 260 are next to be made. Smaller tools involvemore manufacturing challenges and are expectedto follow <strong>the</strong> bigger tools. A Genie 100 coring toolhas been considered.HydraulicsThe flow rate <strong>of</strong> fluid to power a new Genie toolover its operating range is generally lower than<strong>the</strong> flow rate used to clean <strong>the</strong> hole. The Genietool <strong>the</strong>refore has an integral jet sub with a dualcheck valve. It enables jet nozzles to be fitted asmay be required to provide for any additional flowrate at <strong>the</strong> same differential pressure. As adynamic mechanism, <strong>the</strong> tool will be subject togradual wear through its life at a rate dependingon <strong>the</strong> amount <strong>of</strong> sand or o<strong>the</strong>r abrasive materialsin <strong>the</strong> drilling fluid. It is important for economicreasons to keep <strong>the</strong> drilling fluid as free <strong>of</strong> cuttingsas practically possible. Wear may becompensated for by increasing <strong>the</strong> pump rate. It isrecommended that a working flow rate range beprovided to maximise tool operating flexibilitythrough its life. The Genie tool stops impactcycling when lifted <strong>of</strong>f bottom and additional flowpaths open within <strong>the</strong> tool to provide a more directand lower flow resistant passage through <strong>the</strong>exhaust ports in <strong>the</strong> bit face. This enables higherflow rate bottoms-up circulation at lowerdifferential pressure. It also facilitates passage <strong>of</strong>LCM. Fluid can become more abrasive under lostcirculation control conditions.Differential pressure & flow rateThe flow rate to run <strong>the</strong> tool from low to highpower, and <strong>the</strong> resulting differential pressure,depend on <strong>the</strong> fluid. As an example and using adrilling fluid <strong>of</strong> 1.05 SG with a Newtoniankinematic viscosity <strong>of</strong> 5.55 mm²/s (~35 secondMarsh funnel), <strong>the</strong> flow rate is approximately 0.61to 0.87 m³/min for a new tool and about 0.89 to1.33 m³/min for a half-worn tool. Thecorresponding range <strong>of</strong> differential pressure isabout 6.21 to 11.03 MPa. This is much lower than12.76 to 17.24 MPa <strong>of</strong> <strong>the</strong> predecessor tools.Weight On Bit (WOB)A low WOB <strong>of</strong> 1.1 to 4.5 kdaN is required for <strong>the</strong>Genie 185 with an 8½” (215.9 mm) drill bit. TheWOB for a rotary drilling system <strong>of</strong> <strong>the</strong> same sizemay exceed 20 tonnes for hard formations. WOBoutside <strong>the</strong> Genie limits will cause a reduction inimpact energy delivered to <strong>the</strong> bit face, a loss <strong>of</strong>ROP and an increase in drill string torque.Bottom Hole Assembly (BHA)A for ease <strong>of</strong> control, <strong>the</strong> lower BHA is isolatedfrom <strong>the</strong> rest <strong>of</strong> <strong>the</strong> drill string by a fully pressurebalancedheave compensator type stroke sub.The applied WOB is thus limited to <strong>the</strong> weight <strong>of</strong><strong>the</strong> items below it. See Fig. 2 for an example.TARGET WOB = 1.1 to 4.5 kdaNLengths & weights in example estimatedonly. Detailed drill string & BHA design toachieve target WOB is <strong>the</strong> responsibility<strong>of</strong> <strong>the</strong> client.StabilizerUnder gauge, roller reamerrecommended. Spiral stabilizer moreprone to getting hooked on ledges.X-OverFully pressure balanced stroke subUpper partTelescopic joint (only items below thisjoint apply WOB)eg: Smiths HE 6½” Hydra-Stroke AEBBfully pressure balanced, or equivalentNOT A THRUSTER.Lower partPony collar or CollarGenie 185 integral jet sub & checkvalve systemGenie 185Genie 185 bitFIG. 2 – GENIE 185 BOTTOM HOLE ASSEMBLY53


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Project statusApproaching sign-<strong>of</strong>f on <strong>the</strong> Genie 185 tool withits hard surfacing developments.Relevance to Geo<strong>the</strong>rmal projects SUITABLE for HARD formations(metalliferous mining origins) HIGH TEMPERATURE RATING – 204Cstandard & 260C high temp. version HIGH ROP – up to 3 times <strong>of</strong>fset rotary LOW WOB (1.1 to 4.5 kdaN for 8½” hole) LOW rotational speed (typically 25 rpm) LOW DRILL STRING STRESS LIGHT BHA – faster trips with less rig power API top thread & housing suits collar size LOW VIBRATION NO SEALED BEARINGS SIMPLE – only 3 moving parts plus bit ONE PART CUSTOMISED to mud DIRECTIONALLY STABLE EASY TO USE – manual or auto drill LOWER OFF–BOTTOM CIRCULATIONPRESSURE RELIABLE – has always started on bottom RISK MANAGEMENT – no fishing & no bitslost on bottom (since 1993 start) AVAILABLE – designed & manufactured inAustralia & based in Adelaide COST EFFECTIVE – cheaper drill string, nomud motor, less string wear, light & compactfor transport, integral check valve & jet sub,potential to complete drilling in less than50% <strong>of</strong> rotary drilling time for earlyproduction.Abbreviated development chronology1992 A system was conceived by Fred Moir,founder <strong>of</strong> S.D.S. Pty Ltd to drill 5¼" blast holes <strong>of</strong>20 m depth in hard metalliferous mines usingcoaxial drill rods and a down-hole hammerpowered by clean, high pressure, recirculatedwater. He sought <strong>the</strong> benefits <strong>of</strong> top-holehydraulic hammers, down-hole air hammers and abenign, dustless drilling fluid. Used water returnedto <strong>the</strong> surface in drill rods for re-use. A controlledportion was exhausted through <strong>the</strong> bit for holecleaning. Malcolm McInnes was contracted toundertake system R&D. Trialled in undergroundmines with Western Mining and Pasminco withspeed and dust suppression advantages.1993 Performance diminished with depth dueto “water hammer” vibration, <strong>the</strong> result <strong>of</strong> unevencyclic flow resistance. Novel down-hole hydraulicaccumulator systems had limited success.Managing <strong>the</strong> effect was replaced with managing<strong>the</strong> cause. A new concept impact drill (see Fig. 3)with progressive, staged pistons, cyclic flowresistance levelling, anti-cavitation impact facesand a new constant-exhaust bit was invented anddesigned by Malcolm McInnes who <strong>the</strong>n won a$500,000 competitive Government R&D grant andcompleted <strong>the</strong> project to budget. Extensivema<strong>the</strong>matical system modelling was undertaken.FIG. 3 – 1993 HYDRAULIC PERCUSSIVE DRILLThe compact new, patented design providedsmoo<strong>the</strong>r, more powerful operation (see Fig 4)independently <strong>of</strong> depth. Recirculation through drillrods was abandoned for hole cleaning.FIG. 4 – WATER HAMMER PROTOTYPE TESTING WITHGRANITE & UNDERGROUND1994 Fur<strong>the</strong>r underground testing with Mt.IsaMines. Total distance drilled 1000m.1995 Attracted to petroleum industry with moresuitable pump & fluid infrastructure and morecommercial potential. Developed tool coatings forcontaminated fluids. Sub project to accommodate54


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>denser drilling fluids put on hold. Mixed results inoil field trial with partner Santos. Partly related tocontrol & instrumentation issues and a packer.casing. Development progressed in <strong>of</strong>fshore trialswith <strong>the</strong> ODP and sea water drilling fluid.1996 Breakthrough field trial <strong>of</strong> 6" WaterHammer with Shell in Canadian Rockies foothillswith water. Drilled in a pipe stand in an 8½” holeat ~4.5 times ROP <strong>of</strong> roller cone using manualand automatic drilling.FIG. 7 – FLUID HAMMER 260 WITH ODPFIG. 5 – FRED MOIR & MALCOLM McINNES AT WATERHAMMER RUN, CANADA 1996.1998 Ran 12¼" tool <strong>of</strong>f shore from jack-up rigthrough short hard layer with ARCO Indonesia(see Fig. 8). Tool put in at 1,350 m & drilled 11hours at higher than <strong>of</strong>fset ROP (up to 5 x). Thiswas despite some damage incurred to <strong>the</strong> bit dueto tungsten carbide inserts left in <strong>the</strong> hole by <strong>the</strong>preceding roller cone.Began development <strong>of</strong> Water Hammer for 12¼"bit to suit same commercial application (water).FIG. 8 – WATER HAMMER & ARCO INDONESIAFIG. 6 – CLUSTER WATER HAMMERDeveloped and successfully trialled 32” holecluster drilling tool based on 4 water hammers forJ C McDermott & Sons. See Fig. 6. Potential for26” conductors & sub-sea anchorages.Manufacturing & drafting moved from SDS Pty Ltdin Adelaide to SDS Digger Tools in WA.1997 New 12¼" hole size water hammerdesigned & made. Immediately worked inCanada. 30 hour running time with new hardcoating technology and flock water.Developed case-while-drilling systems for OceanDrilling Program. Achieved fast, unsupportedspudding on hard, smooth, 30° sloping granite.Quarry tested CWD insertion and retrieval <strong>of</strong>Continued drilling 650 m surface holes with 14¼"bits with Talisman <strong>Energy</strong> Inc at ROP consistently2 to 3 times faster than conventional rock bits inhard formations. See Figs. 9 & 10. A majordownturn in <strong>the</strong> international mining industrythreatens <strong>the</strong> internally funded project.FIG. 9 – WATER HAMMER – CHERT CUTTINGS55


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Depth (m)SDS FLUID HAMMER 260 - CASE STUDIES in <strong>the</strong> CANADIAN ROCKIES FOOTHILLSTime (days)0 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 240Black = Air hammer drills100Red = Roller cone bitsBlue = SDS Fluid Hammer200300400500SDS Corporation Ltd commissions anindependent technical review <strong>of</strong> <strong>the</strong> design. Theengineering and technology is validated.2000 Drilled with PDVSA in Venezuela at 4,355m depth (2 to 3 x <strong>of</strong>fset instantaneous ROP) withSDS water hammer 260 (12-1/4" bit). The fluidwas a mineral oil <strong>of</strong> about 1.03 SG. WOB difficultto control. See Fg. 13.600700Talisman E/A Highhat d-78-K/93-P-5 Phillips Sukunka c-54-F/93-P-5 PC Gwillim B-78-H/93-P-5OEI Petrorep Sukunka a-39-F/93-P-5 Talisman Sukunka A-18-K/93-P-5 Talisman Sukunka B-11-L/93-P-5Shell Esso Gwillim a-51-H/93-P-5 Talisman POCO Highhat a-54-K/93-P-5 Talisman Highhat d-83-L/93-P-5FIG. 10 – COMPARATIVE PERFORMANCEShoreline approach hole opening job at StatoilMongstad refinery, Norway with 12¼” holeopening bit on slope rig run by Halliburton. Fig 11.FIG. 14 STEERING HYDRA 185. FIG. 13 PDVSAFirst steering run using unfinished prototypeHydra 185 (8½”) at Sperry-Sun Nisku test facility.The tool built a turn <strong>of</strong> 5° using a 1° bent sub and9°using a 1.5° bent sub, in 18.3 m <strong>of</strong> concretewhich it drilled at 100 m/hr (Fig. 14). Successfullydemonstrated steering and operation in a wellwith Measurement While Drilling System (Hydra185 not developed for fluid SG over about 1.05).FIG. 11 – WATER HAMMER 260 & STATOIL1999 Began development <strong>of</strong> new 8½” hole toolwith fewer parts, new features and for range <strong>of</strong>drilling fluids (not completed), as new series basemodel. Performance testing undertaken in OrangeGrove quarry, WA. See Fig. 12. Drilling with 12¼”tool with Northstar energy - Recorded continuousROP 4-7 Mt/Hr Vs 2 Mt/Hr tricone. Hammer lifeincreased to 40 hours.2001 May. Controlled surface benchmarktesting <strong>of</strong> SDS Fluid Hammer 185 at TerraTektesting facility (see Fig. 15) in Salt Lake City,Utah, USA, separately and in conjunction withconsortium lead by US Department <strong>of</strong> <strong>Energy</strong>.Facility simulates deep, overbalanced drilling withstandard rock samples and drilling muds. Despitetool not being designed for 1.2 and 1.8 SG muds,Extensive testing confirmed <strong>the</strong> soundness <strong>of</strong> <strong>the</strong>concept, verified operating characteristics andinspired development to suit denser fluids andexpand application versatility.FIG. 12 – QUARRY TEST 8½” PROTOTYPESFIG. 15 – TERRATEK & FLUID HAMMER 18556


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Fluid Hammer 260 tool (12¼” bit) was trialled withPDVSA in well MCA-2X in Venezuela at 1,498 m.A new drilling technique had been developed in<strong>the</strong>ory and was successfully used to control <strong>the</strong>tool and Weight On Bit for optimum ROP, a majorbreakthrough that also protected <strong>the</strong> bit. Workeddespite failure <strong>of</strong> hook feed indicator. Aninstantaneous ROP 2 to 3 times <strong>of</strong>f-set roller conewas demonstrated. Project investment andfinance options were pursued for <strong>the</strong> board.2002 June. Verification field tested prototypeSDS Fluid Hammer 185 (9⅞” bit) with Talisman<strong>Energy</strong> Inc. & Precision Drilling. See Fig. 16.Used new design Bottom Hole Assembly. BHAprovided required low Weight On Bit. Identifiedtorque as a key WOB maximum & minimumindicator. System worked and overcame majorhurdles in applying <strong>the</strong> technology commercially.FIG. 17 – FLUID HAMMER 260 & CWD & IODP JOIDESRESOLUTION2005 Successfully completed IODP jobJanuary, 2005. 2 tools ran a total <strong>of</strong> over 92 hrs insea water without significant performance loss.The revenue supported <strong>the</strong> Genie project for <strong>the</strong>first 18 months. See Fig. 18.FIG. 18 – IODP RE-ENTRY CONE ON FLUID HAMMER 260& CWD INSERTED CASINGFIG. 16 – PROTOTYPE 185 & BHA. TALISMAN ENERGYINC & PRECISION DRILLINGFluid Hammer project suspended.2004 Project and its assets moved from SDSDigger Tools into new Adelaide based entityIMPACT DRILLING INTERNATIONAL Pty Ltd. t<strong>of</strong>ocus on development and commercialisation <strong>of</strong><strong>the</strong> technology for <strong>the</strong> petroleum & geo<strong>the</strong>rmalindustries. Genie project announced. New design,engineering, manufacturing and supply, testing,operations, quality systems, branding and fundingto develop new range <strong>of</strong> tools for industry drillingfluids and with lower operating differentialpressure to maximise versatility. Managed byMalcolm McInnes. Concurrently with new tooldevelopment, <strong>the</strong> company won a commercialcontract with Integrated Ocean Drilling Program touse two 1997 design 260 tools with IODP HardRock Re-entry Systems (up to 15” bits) to insertcasing with re-entry cones 30m into AtlanticOcean floor, (1.5 to 2.5 km depth) north <strong>of</strong> <strong>the</strong>Azores, without a template. See Figures 17 & 18.Designed & built in-house, impact drilldynamometer test rig for new Genie range R&D(see Fig. 19) with mud cooling, mixing,instrumentation, prime pump & twin HT400pumps. Many components were reclaimed scrap.FIG. 19 – IDI GENIE DYNAMOMETER TEST RIGSuccessfully tested two different prototypes (seeFig 20) on water and standard muds 1.2 & 1.8 SG(as used in USA benchmark testing), withoutsignificant hydraulic vibration and at lowerdifferential pressures. Different valvessuccessfully used for different fluids. The partssupplier was late and <strong>the</strong> order incomplete.Enough parts provided for 2 complete Genieprototypes and one spare set <strong>of</strong> internals.57


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>FIG. 20 – A PROTOTYPE GENIE 185All part drawings parametrically linked and alldrawings <strong>of</strong> <strong>the</strong> models in <strong>the</strong> product rangelinked to simplify and speed-up drafting, improvequality, simplify and standardise manufacturing,reduce lead times & costs. Check valve systemredesigned for high solids mud. Safer, easier &faster assembly procedure and tools developed.2006 SDS Corporation Limited sold to SandvikMining & Construction, Adelaide.IMPACT DRILLING INTERNATIONAL Pty Ltdacquired by Fred Moir & minor shareholders.2007 Prototype Genie 185 design &manufacturing completed. Business namechanged to SPECIALISED DRILLING SERVICESAUSTRALIA Pty Ltd.2008 Prototype Genie 185 tools run with fieldtrial partner Talisman <strong>Energy</strong> Inc in CanadianRockies foothills, 5 to 9 January 2008. Fig. 21.The new Genie 185 system demonstrated: Directional stability. Deviation no more than ¾° Low rig mechanical & hydraulic vibration. High ROP, average 3 times <strong>of</strong>fset tool ROP. Easy auto & manual drilling control. Reliable & predictable starting & operation. Automatically regulated, low WOB withlightweight BHA. Different but easy to learn to use. Can pass loss control material.R&D program to increase durability. Prototypesdid not employ hard overlays as used inpredecessor tools. Accelerated wear wasobserved during lost circulation management dueto increased sand level in drilling fluid. Newdesign features, materials and pioneeringmanufacturing processes developed andincorporated into <strong>the</strong> Genie tools. A new dualcheck valve system was developed.FIG. 21 – GENIE 185 TRIAL WELL, CANADA2009 R&D and prototype manufacture <strong>of</strong> newhard overlaid tools completed in second half <strong>of</strong>year. New production systems developed for highvolumes and low lead time. Additional field trialpartners sought after follow-up drilling programdelay in Canada due to financial crisis in USA.Local opportunity provided with contract won inlate 2009.<strong>2010</strong> Tools mobilized to rig. Returned unusedafter anticipated hard formation was notencountered. Tools on stand-by for new project.Contract won for trial managed pressure drillingrun in Asian project during last quarter <strong>of</strong> year.Development <strong>of</strong> below-<strong>the</strong>-hook lifting systems,maintenance procedures, manuals, drawings ando<strong>the</strong>r documentation continues.ManagementChairman <strong>of</strong> <strong>the</strong> Board <strong>of</strong> Directors and principalshareholder is Mr Fred Moir. Fred is aninternational business leader with extensivedrilling, service provision and manufacturingexperience in <strong>the</strong> mining industry. Fred wasfounder <strong>of</strong> SDS Pty Ltd and instigated <strong>the</strong> originalproject to develop a water powered percussiondrilling tool in 1992. Impact Drilling InternationalPty Ltd was established under his Chairmanship.The business is managed by Malcolm McInnes,FIEAust. CPEng MESc BE ARMIT Mech Eng MAIE SPE withover 30 years experience in manufacturing,product development, R&D, marketing, sales &management and has run his own business since1992. He is <strong>the</strong> designer and inventor <strong>of</strong> <strong>the</strong>Genie tools and inventor <strong>of</strong> <strong>the</strong> <strong>of</strong> <strong>the</strong>internationally patented SDS water/fluid hammerin 1993. Malcolm has 17 years experience in <strong>the</strong>drilling industry and became an employee andshareholder <strong>of</strong> SDSA in 2006.ReferencesMcInnes, M.B. - Internal reports & photographs &company documents & photographs 1992 - <strong>2010</strong>.The Author acknowledges <strong>the</strong> contributions <strong>of</strong> allpeople involved in <strong>the</strong> project since its inception58


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Hydro<strong>the</strong>rmal alteration aspects <strong>of</strong> high heat producing granites inAustralia & EuropeAlexander W. Middleton* 1 , I. Tonguç Uysal 1 , Massimo Gasparon 2 , and Scott Bryan 3Queensland Geo<strong>the</strong>rmal <strong>Energy</strong> Centre <strong>of</strong> Excellence, The University <strong>of</strong> Queensland, Brisbane, QLD. 4072* 1School <strong>of</strong> Earth Sciences, The University <strong>of</strong> Queensland, Brisbane, QLD. 4072 2Queensland University <strong>of</strong> Technology, BiogeoScience, GPO Box 2434, Brisbane, QLD. 4001 3In order to fully understand <strong>the</strong> relativelyunstudied high heat producing granites (HHPG) <strong>of</strong><strong>the</strong> <strong>Australian</strong> continent, this project has studied<strong>the</strong> European analogues <strong>of</strong> Cornwall, (UnitedKingdom), Soultz-sous-Forêts (France) and <strong>the</strong>Erzgebirge (Germany). HHPGs are characterisedby <strong>the</strong>ir anomalous radiogenic element (U, Th andK) contents (Table 1), which is higher thanaverage continental crust values. The Big LakeSuite in <strong>the</strong> Cooper Basin is <strong>the</strong> most investigated<strong>Australian</strong> enhanced geo<strong>the</strong>rmal system (EGS);Gatehouse et al., 1995).Alteration mineralogy is a widely used feature toexplore for potential ore deposits; however, thismethod has not yet been deployed for identifyingand characterising EGS. In <strong>the</strong> current project, weare investigating alteration mineralogy <strong>of</strong> HHPG,with particular emphasis on trace element andstable isotope geochemistry. If successful, thiscan <strong>of</strong>fer an additional approach to geo<strong>the</strong>rmalexploration and resource characterisation.phase disequilibrium with <strong>the</strong> fluid. The alterationassemblage produced depends on factors suchas wall-rock and fluid composition, temperature,salinity and water/rock ratio. The variation inalteration assemblage may control <strong>the</strong>concentration <strong>of</strong> incompatible elements, including<strong>the</strong> radiogenic elements as certain alterationreactions are associated with ei<strong>the</strong>r enrichment ordepletion <strong>of</strong> <strong>the</strong>se elements. A pertinent example<strong>of</strong> this was noted to have occurred in someCarnmenellis (Cornwall, UK) monazites(Poitrasson et al., 1996), whereby Th wasenriched through brabantitic (Förster, 1998) cationexchange during chloritisation <strong>of</strong> biotites:2REE 3+ Th 4+ + Ca 2+Incompatible elements (HFSE, REE, LILE, and Betc., including <strong>the</strong> radiogenic elements) have alow partition coefficient (K D ) (White, 2007), andhence will preferentially stay in fluid phases duringTable 1: Typical compositions for high heat producing granites for EGS. Sourced from T Uysal, J Van Zyl, S Bryan, unpubl.data; Charoy, 1986; Stussi et al., 2002; Forster et al., 1999; Chappell & Hine, 2006EGS Target Composition Age SiO 2 K 2 O U (ppm) Th (ppm)(Ma) (wt%) (wt%)Cooper Basin granites Biotite granites ~Mid-Carb.- - 10.0-30 28-144Carnmenellis granites(Cornwall, UK)K-feldspar megacrysticbiotite granites293-27469-76 4.6- 13-20 15-205.9 (4-38) (5-45)Soultz-sous-Forêts(Rhine Graben, France)Erzgebirge (Germany)Keywords: Geo<strong>the</strong>rmal, alteration mineralogy,Cooper Basin, stable isotopes, REE, Soultz-sous-ForêtsBackgroundK-feldspar porphyriticmonzograniteBiotite, 2 mica & LimicagranitesDuring emplacement <strong>of</strong> granitic bodies, advectiveheat flow can occur due to hydro<strong>the</strong>rmalcirculation <strong>of</strong> surrounding waters. Several studieshave noted that igneous rocks enriched inradioactive elements such as U, Th and K canhave a similar effect and promote hydro<strong>the</strong>rmalcirculation long after <strong>the</strong> intrusion has cooled(Allman-Ward, 1985, Pirajno, 2005). Oncirculation <strong>of</strong> <strong>the</strong>se hydro<strong>the</strong>rmal fluids, variablealteration products will result from original mineral~330 67-69 ~4.5 6.2-14.1 24-37325-31870-77 4.5-5.3crystallisation <strong>of</strong> melt and hydro<strong>the</strong>rmal fluidmovement. .Hydro<strong>the</strong>rmal fluids affecting surrounding wallrockscan be classified (based on <strong>the</strong>ir origin), intometeoric, magmatic, marine or connate. Oneaspect <strong>of</strong> this project is to deduce <strong>the</strong> origin andevolution <strong>of</strong> <strong>the</strong> hydro<strong>the</strong>rmal fluids involved in <strong>the</strong>alteration <strong>of</strong> HHPG and surrounding sedimentaryrocks.Analytical Work8.0-30 15-37The project results will be attained viamultifaceted petrographic, geochemical andgeochronological analyses. The geochronologywill use Rb-Sr isochron dating <strong>of</strong> alteration-relatedillitic clay minerals, whereas <strong>the</strong> geochemicaltechniques will include both stable isotope59


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>analysis (δ18O and δD) for hydro<strong>the</strong>rmal fluidevolution and ICP-MS analysis for trace elementquantification.Qualitative and quantitative petrographic analyseswill be achieved with transmitted and reflectivemicroscopy, as well as EDS (via JEOL XL 30SEM) and EPMA. The EPMA will be used todetermine quantitatively which mineral phasesencompass <strong>the</strong> elements <strong>of</strong> interest; such asincompatibles and radiogenics.Queensland EGS targets and CooperBasinQueenslandFollowing estimated subcrustal temperaturemapping and <strong>the</strong> increasing need for renewableenergy sources, Queensland has been targetedby <strong>the</strong> state government as a prospective area forgeo<strong>the</strong>rmal energy. The principal areas <strong>of</strong> interestfor EGS are <strong>the</strong> Galilee Basin, Innot Hot Springsregion, Hodgkinson Province, Styx Basin,Maryborough Basin and North d’Aguillar Block,Wandilla Province. These targeted areas havebeen based on <strong>the</strong> presence or likely presence <strong>of</strong>HHPG at depth ranging in age from <strong>the</strong> LateDevonian to Cretaceous. Many <strong>of</strong> <strong>the</strong> granitebodies emplaced within Queensland are linked toan extensional tectonic origin (Glen, 2005).Analysis <strong>of</strong> <strong>the</strong> intrusions, overlying sedimentsand <strong>the</strong>ir associated alteration zones will beperformed as part <strong>of</strong> this project.Cooper BasinThe Carboniferous Big Lake Suite granite in <strong>the</strong>Cooper Basin’ represents one <strong>of</strong> <strong>the</strong> world’shottest EGS (Gatehouse et al., 1996). Accordingto our recently acquired ICP-MS trace elementdata, U and Th contents in <strong>the</strong>se granites reachlevels <strong>of</strong> up to 144ppm, reflecting enrichmentlevels up to 13 times that <strong>of</strong> <strong>the</strong> upper continentalcrust (UCC( McLennan, 2001)). Cores taken from<strong>the</strong> granite and overlying sediments show varyingdegrees <strong>of</strong> alteration, with a range <strong>of</strong> incompatibleelement enrichment, such as U and Th. Thehighly altered zones have a predominant greisenstylesericite (illite) and re-precipitated quartzassemblage. We believe that this alteration maywell have caused <strong>the</strong> localised enrichment inradiogenic element-bearing minerals such as illite,K-feldspar, and some accessory minerals (e.g.,thorite ).The fluid history <strong>of</strong> <strong>the</strong> Cooper Basin can bededuced with <strong>the</strong> use <strong>of</strong> both crystallinity andstable isotope analyses <strong>of</strong> <strong>the</strong> illite. Illitecrystallinity is a useful indicator <strong>of</strong> <strong>the</strong> temperaturegradient in active geo<strong>the</strong>rmal systems and forlocating fossil hydro<strong>the</strong>rmal systems associatedwith ore deposition (Ji and Browne, 2000).Depth500100015002000250030003500400045000.2 0.4 0.6 0.8 1Illite Crystallinity Δ2θMB 1graniteBL 1 graniteMcL 1 graniteJol graniteHab 1 graniteMB 1‐2‐7 sedimentBL 1‐2‐31‐57 sedimentMcL 1 sedimentTW 1sedimentWT 1sedimentFig 1: Graph <strong>of</strong> illite crystallinity against depth from CooperBasin coresIllite crystallinity is controlled by crystallisationtemperature, water/rock ratio, and time availablefor crystallization (Arkai, 2002; Ji and Browne,2000; Merrriman and Frey, 1999). Betterdevelopedcrystalline illites show narrower 001basal illite peaks and have lower IC values. Suchillites were formed at higher temperatures orduring prolonged heating events. Higher ICvalues (wider peaks), on <strong>the</strong> o<strong>the</strong>r hand, indicatelower crystallisation temperatures and/or rapidprecipitation during hydro<strong>the</strong>rmal processes. Illitecrystallinities are seen to progressively increasewith increasing core depth, suggesting a highercrystallisation temperature and hencehydro<strong>the</strong>rmal fluid temperature at depth. Thegranite intersected in Jolokia and McLeod 1seems to have experienced highest reservoirtemperatures.According to our present isotopic studies <strong>of</strong>alteration-related illite within <strong>the</strong> granite andsedimentary cover, oxygen and hydrogen isotopecompositions range from δ18O = -1.8‰ to+2.7‰;δD = -99‰ to -121‰ and δ18O = +2.3‰to +9.7‰, δD = -78‰ to -119‰, respectively.Such values are much lower than those reportedfor many deeply buried sedimentary basins(Clauer and Chaudhuri, 1995). The calculatedoxygen and hydrogen isotope compositions <strong>of</strong>60


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>fluids in equilibrium with <strong>the</strong> illites are depleted in18 O and deuterium, comparable to those <strong>of</strong> watersreported for most high-latitude sedimentarybasins. Hence, stable isotope data <strong>of</strong> alterationminerals in <strong>the</strong> granite and <strong>the</strong> overlyingsedimentary rocks suggest <strong>the</strong> operation <strong>of</strong> ahydro<strong>the</strong>rmal system involving high latitudemeteoric waters during Permo-Carboniferousextensional tectonism in <strong>the</strong> Cooper Basin region.EuropeThe European HHPG examples have all beenconsidered to be approximately syn-genetic wi<strong>the</strong>xtension following <strong>the</strong> late PalaeozoicHercynian/Variscan orogeny between Gondwanaand Laurasia.extension (Schleicher, 1998). Petrographicstudies <strong>of</strong> alteration mineralogy by Bartier et al.(2008) identified intense propylitically alteredgranite with newly equilibrated mineralassemblages <strong>of</strong> tosudite (chlorite-smectite), illite,chlorite and carbonates, whilst K-feldspar appearsto be largely preserved.Following fur<strong>the</strong>r transmitted and scanningelectronmicroscopy performed at The University<strong>of</strong> Queensland, we identified several keyalteration-related mineral phases. Altered sphene,for example, found in sample K177 (2000m –EPS1), is acting as a principal mineral phase thatcontains various rare earth elements (REE).Estimations <strong>of</strong> composition from semi-quantitativeEDS have detected Ce, Y, Nd, La, Th and Ca withpossible PO 4 or SiO 4 anion complexes.***Sphene*Cornwall*Soultz-sous-Forêts*Erzgebirge064Fig 2: Possible tectonic suture configuration <strong>of</strong> Hercynianorogeny from Matte (2001)Erzgebirge, GermanyLocated at <strong>the</strong> north-western edge <strong>of</strong> <strong>the</strong>Bohemian Massif (Förster and Förster, 2000), <strong>the</strong>Erzgebirge consist <strong>of</strong> highly-evolved voluminousgranites intruded into highly crystallinemetamorphic rocks (Tischendorf et al., 1965).These granites are highly enriched in U and Th(Table 1) with principal radiogenic mineral phases<strong>of</strong> uraninite, U-bearing micas, xenotime,monazite-(Ce)-brabantite solid solution seriesminerals, and thorite (Förster, 1998).As <strong>of</strong> yet, our analyses (Rb – Sr dating and stableisotope) have not been undertaken on Erzgebirgesamples, but samples will be analysed incollaboration with Dr. Hans-Jurgen Förster(Potsdam, GeoForschungsZentrum).Soultz-sous-Forêts, FranceLocated south-west <strong>of</strong> <strong>the</strong> Erzgebirge outcrops,Soultz-sous-Forêts was emplaced debatablyei<strong>the</strong>r as an I-type subduction-related or latestageextensional granite body (Flötmann andOncken, 1992). Hydro<strong>the</strong>rmal fluid circulation andalteration was promoted by E-W lithosphericFig 3: Altered sphene compassing several REE-elementbearingmineral phases30 µmThis may indicate a potentially high fluid/rock ratioallowing for incompatible element transport duringalteration <strong>of</strong> <strong>the</strong> granitic protolith. Monazite hasalso been found proximal to subhedral hematitegrains. A possible mechanism for this mineralassociation can be traced back to <strong>the</strong> formation <strong>of</strong>a redox interface with co-precipitation <strong>of</strong> U 4+ andFe 3+ .Counts0642700Ca Ti2400210018001500CeCe1200 OYLaLa CeY Th TiCe Ce 900C Ce Si Th CaLaYLa600 Fe Al Th KLa Fe30000.00 1.00 2.00 3.00 4.00 5.00 6.00 7.00 8.00 9.00keVFig 6: EDS for altered sphene found in sample K177exhibiting intense propylitic alteration.Cornwall, United KingdomCornwall marks <strong>the</strong> far western district <strong>of</strong> <strong>the</strong>Euro-Hercynian granites with 5 major outcrops;Dartmoor, Bodmin Moor, St. Austell, Carnmenellis61


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>and Lands End. Multiple studies by Ball et al.,(1979) and Charoy (1986) have found <strong>the</strong>Cornwall granites to be similarly enriched inradiogenic elements (Fig. 1) as <strong>the</strong> middle-European examples. Alteration systematics are <strong>of</strong>great importance within this system as <strong>the</strong>y havebeen directly linked to <strong>the</strong> leaching andmineralisation <strong>of</strong> uranium. Allman-Ward (1985)noted 4 predominant alteration styles affecting <strong>the</strong>St. Austell granite; greisenisation,tourmalinisation, kaolinisation and haematisation.Uranium is likely to be transported in solutionduring hydro<strong>the</strong>rmal alteration, as oxidising fluidswill cause a loss <strong>of</strong> electrons (U 4+ to U 6+ ) andhence increase mobility. The most likely location<strong>of</strong> <strong>the</strong> displaced uranium will be in a distalalteration zone possibly accompanied byhaematite mineralisation. An example <strong>of</strong> this canbe seen in Wheal Remfry where quartz-haematiteveins show uranium values <strong>of</strong> up to 50ppm(Allman-Ward, 1985).SummaryHighly altered granites in <strong>the</strong> Cooper Basin aresubstantially enriched in lithophile elements,particularly in Cs, Rb, Be, Th, U relative to <strong>the</strong>upper continental crust. U and Th contents are 10and 13 times higher than those <strong>of</strong> <strong>the</strong> UCC. Someenrichment <strong>of</strong> heat-producing elements waspromoted by a regional hydro<strong>the</strong>rmal eventleading to <strong>the</strong> precipitation <strong>of</strong> U and Th- bearingminerals such as illite, K-feldspar and accessoryminerals (o<strong>the</strong>r than zircon). Oxygen andhydrogen isotope compositions <strong>of</strong> fluids aredepleted in 18 O and deuterium, comparable tothose <strong>of</strong> waters reported for most high-latitudesedimentary basins. European examples <strong>of</strong>enhanced geo<strong>the</strong>rmal systems show similarredistribution and enrichment patterns <strong>of</strong> rareearth and radiogenic elements as a result <strong>of</strong>hydro<strong>the</strong>rmal alteration. This can be seen inmonazites proximal to chloritised biotites in <strong>the</strong>Carnmenellis granite <strong>of</strong> Cornwall. Unlike <strong>the</strong>Cooper Basin, stable isotope data has not yetbeen acquired from European samples. Howeveronce performed, hydro<strong>the</strong>rmal fluid origin andevolution can be deduced for <strong>the</strong>se EGS.Alteration mineralogy and geochemistry <strong>of</strong>relatively shallow sedimentary sections is apotentially valuable tool to evaluate <strong>the</strong> presence<strong>of</strong> a concealed geo<strong>the</strong>rmal heat source in <strong>the</strong>basement <strong>of</strong> sedimentary basins.ReferencesAllman-Ward, P., 1985. Distribution <strong>of</strong> uraniumand thorium in <strong>the</strong> western lobe <strong>of</strong> <strong>the</strong> St. Austellgranite and <strong>the</strong> effects <strong>of</strong> alteration processes,High heat production granites, hydro<strong>the</strong>rmalcirculation and ore genesis conference, TheInstitute <strong>of</strong> Mining and Metallurgy, 437-458.Aquilina, L., Pauwels, H., Genter, A., and Fouillac,C., 1997. Water-Rock interaction processes in <strong>the</strong>Triassic sandstone and granitic basement <strong>of</strong> <strong>the</strong>Rhine Graben : Geochemical investigation <strong>of</strong> ageo<strong>the</strong>rmal resevoir. Geochimica etCosmochimica Acta, 6, 4281-4295.Arkai, P., 2002. Phyllosilicates in very low-grademetamorphism: Transformation to micas. Micas:Crystal Chemistry and Metamorphic Petrology,46: 463-478.Bartier, D. et al., 2008. Hydro<strong>the</strong>rmal alteration <strong>of</strong><strong>the</strong> Soultz-sous-Forêts granite (Hot FracturedRock geo<strong>the</strong>rmal exchanger) into tosudite andillite assemblage. European Journal <strong>of</strong>Mineralogy, 20, 131-142.Bryan, S. E., Holcombe, R. J. and Fielding, C. R,2001. Yarrol Terrane <strong>of</strong> <strong>the</strong> nor<strong>the</strong>n New EnglandFold Belt: forearc or backarc? <strong>Australian</strong> Journal<strong>of</strong> Earth Sciences, 48 296-316Clauer, N. and Chaudhuri, S., 1995. Clays inCrustal Environments. Isotope Dating andTracing. Springer Verlag, Heidelberg, 359.Flötmann, T. and Oncken, O., 1992. Constraintson <strong>the</strong> evolution <strong>of</strong> <strong>the</strong> Mid Crystalline Rise –astudy <strong>of</strong> outcrops west <strong>of</strong> <strong>the</strong> river Rhine.Geologische Rundschau, 81, 2, 515-543.Förster, H-J., 1998. The chemical composition <strong>of</strong>REE-Y-Th-U-rich accesspry minerals inperalumnous granites <strong>of</strong> <strong>the</strong> Erzgebirge-Fichtelgebirge region, Germany, Part 1: Theminazite-(Ce)-brabantite solid solution series.American Mineralogist, 83, 259-272.Förster, H-J., 1998. 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<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Merrriman, R.J. and Frey, M., 1999. Patterns <strong>of</strong>very low-grade metamorphism in metapeliticrocks. In: M. Frey and D. Robinson (Editors), LowGrade Metamorphism. Blackwell Science,Cambridge, pp. 61-107.Murray, C. G., 2003. Granites <strong>of</strong> <strong>the</strong> New EnglandOrogen., from: Blevin, P. L., Jones, M. andChappell, B., Magmas to Mineralisation: TheIshihara Symposium. Geoscience AustraliaRecord, 2003/14, 101-108.Pirajno, F., 2005. Hydro<strong>the</strong>rmal Processes andMineral Systems. Springer Link, GeologicalSurvey <strong>of</strong> Australia, 73-157, 990-995.Schleicher, A. M., Warr, L. N., Kober, B., Laverret,E. and Clauer, N., 2006. Episodic mineralisation<strong>of</strong> hydro<strong>the</strong>rmal illite in <strong>the</strong> Soultz-sous-Forêtsgranite (Upper Rhine Graben, France). ContribMineral Petrol, 152, 349-364.Stussi, J-M. et al., 2002. The hiddenmonzogranite <strong>of</strong> Soultz-sous-Forêts (RhineGraben, France): Mineralogy, petrology andgenesis. Géologie de la France, 1, 45-64.Taylor, H. P., 1997. Oxygen and HydrogenIsotope Relationships in Hydor<strong>the</strong>rmal MineralDeposits, from: Barnes, H. L., 1997.Geochemistry <strong>of</strong> Hydro<strong>the</strong>rmal Ore Deposits.John Wiley and Sons, Inc, 229-288.White, W. M., 2007. Geochemistry: TraceElements in Igneous Process. John HopkinsUniversity Press, 258-312.63


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>A Geo<strong>the</strong>rmal Web Catalog Service for <strong>the</strong> Perth BasinThomas Poulet 1,2,3 , Soazig Corbel 1,2 , Michael Stegherr 1,41CSIRO Earth Science and Resource Engineering, P.O. Box 1130, Bentley, WA 6102, Australia.2Western <strong>Australian</strong> Geo<strong>the</strong>rmal Centre <strong>of</strong> Excellence, P.O. Box 1130, Bentley, WA 6102, Australia.3The School <strong>of</strong> Earth and Environment, University <strong>of</strong> Western Australia, WA 6009, Australia.4 School <strong>of</strong> Science, Curtin University, GPO Box U1987, Perth, WA 6845, AustraliaThe Western <strong>Australian</strong> Geo<strong>the</strong>rmal Centre <strong>of</strong>Excellence (WAGCOE) is a science collaborationbetween Western Australia’s leading innovativeresearch institutions – CSIRO, The University <strong>of</strong>Western Australia and Curtin University <strong>of</strong>Technology. One <strong>of</strong> its key research initiatives isto assess geological and geophysical data from<strong>the</strong> Perth Basin to identify geo<strong>the</strong>rmal targets.This geo<strong>the</strong>rmal exploration task involves <strong>the</strong>collection and analysis <strong>of</strong> all datasets available,which can be a challenging and sometimesdaunting exercise. This paper addresses <strong>the</strong>difficulties encountered in ga<strong>the</strong>ring data forgeo<strong>the</strong>rmal exploration and presents our webcatalog service, <strong>the</strong> application we use to manageour spatially referenced resources.Keywords: Western Australia, Perth Basin,geo<strong>the</strong>rmal exploration, GeoNetwork opensourceFinding and using geo-referenced dataGeo<strong>the</strong>rmal exploration is a data intensive activitywhich requires access to all relevant informationavailable in <strong>the</strong> region <strong>of</strong> interest, such asstratigraphic sections and horizons, downholetemperature measurements, rock properties, andhydrogeologic parameters including water quality.Because so many types <strong>of</strong> sciences are involved(geophysics, geology, geochemistry...), data maybe derived from many different potential sourcessuch as seismic surveys, petroleum well logs,mechanical property laboratories, or groundwatermineralogical assays. Data really is anindispensable element for exploration and yet it isstill so difficult and expensive to discover, search,access and use; those four simple steps cansometimes represent a real obstacle course forany first-time user. Although most public datasetsare nowadays accessible through companies’ orgovernmental agencies’ websites, any potentialuser still needs to know all key data holders in <strong>the</strong>area in order to access essential information.Once <strong>the</strong> appropriate data custodian for aparticular type <strong>of</strong> data is identified, <strong>the</strong> secondtask is usually to search for data relevant to <strong>the</strong>location <strong>of</strong> interest, only to discover that datasetsare rarely fully searchable. The third step is <strong>the</strong>nto access this data, which can sometimes involvegoing physically to an organisation to copyseveral computer hard drives. The last step isgenerally to understand <strong>the</strong> format used, whichmay be non-standard and can lead to <strong>the</strong> mostsignificant inefficiencies in a given project. Datamanipulation can include for example largeamounts <strong>of</strong> preliminary data conversion,deciphering any implicit assumption about units <strong>of</strong>measures and geographical references, or eventrying to infer <strong>the</strong> creation process <strong>of</strong> <strong>the</strong> data inorder to obtain one piece <strong>of</strong> missing information. Ifdata is interrelated, this investigative process canloop on itself, creating workflow problems. Anyuser who has spent a long time going through thisprocess can indeed wonder legitimately if newerdata is now available. Our web catalog service isan attempt to eliminate <strong>the</strong> painful aspects <strong>of</strong>Perth Basin data discovery.Using GeoNetwork opensourceGeoNetwork opensource 1 is a discovery serviceand catalog application, which is useful formanaging spatially referenced resources andspecially built to facilitate <strong>the</strong> connection betweenspatial information communities and <strong>the</strong>ir data. Itis a Standardised Geospatial InformationManagement System based on internationalstandards, with a large community <strong>of</strong> severalhundreds <strong>of</strong> users and developers participatingactively to its growth. A more complete descriptioncan be found in Ticheler & Hielkema (2007). Incollaboration with AuScope Grid (Woodcock2008) we decided to use GeoNetwork as ourcatalog application since it addresses mostpotential problems mentioned above, <strong>of</strong> datadiscovery, search, access and usage.GeoNetwork is accessible to users through a webinterface and <strong>the</strong>refore only requires a webbrowser on any computer platform. Its searchfunctionalities make data easily discoverable andFigure 1: Workflow diagram showing <strong>the</strong> architecture <strong>of</strong>WAGCOE’s geo<strong>the</strong>rmal catalog, using GeoNetwork as <strong>the</strong>catalog application linking to a petabyte datastore holding <strong>the</strong>corresponding data. Both components use iVEC’sinfrastructure and provide an efficient and secure system thatcan connect to o<strong>the</strong>r web services1 http://geonetwork-opensource.org64


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>searchable. Since we are using GeoNetwork as acataloguing application, <strong>the</strong> granularity <strong>of</strong> <strong>the</strong>search is limited to <strong>the</strong> metadata and not <strong>the</strong> datacontent itself. This library function is different froma web portal connected to a full database whichwould make <strong>the</strong> entire data fully searchable.However, <strong>the</strong> search facility allows users to findinformation easily and access <strong>the</strong> correspondingmetadata, including a link to download <strong>the</strong>associated data itself from a Petabyte store.Figure presents <strong>the</strong> workflow <strong>of</strong> any useraccessing WAGCOE’s web catalog service. Both<strong>the</strong> web service and Petabyte store are hosted atiVEC 2 , <strong>the</strong> hub <strong>of</strong> advanced computing inWestern Australia, and all connections aresecure. The web catalog service points directly to<strong>the</strong> data store, and can also be connected too<strong>the</strong>r web catalog services from o<strong>the</strong>r institutions.Using that data is also greatly facilitated asGeoNetwork organises, documents and publishesdata collections in a standardised and consistentway, both at <strong>the</strong> metadata and data levels,following international standards from <strong>the</strong> OpenGeospatial Consortium 3 . This fully descriptivemetadata in XML format improves accessibilityand removes any possibility <strong>of</strong> datamisinterpretation based on assumptions.As Ticheler & Hielkema (2007) point out,GeoNetwork has also been developed using Web2.0 techniques to allow for more interactive andintuitive use <strong>of</strong> <strong>the</strong> system and to <strong>of</strong>fer buildingblocks for future web services. This interactionwith o<strong>the</strong>r web services is a central feature to helpreduce duplication and working towards a singlepoint <strong>of</strong> truth paradigm. It is an essentialcomponent <strong>of</strong> WAGCOE’s data strategy to link toall data custodians’ databases as defined by <strong>the</strong><strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong> Group (AGEG)Technical Interest Group focusing on datamanagement. Such a framework can definitelyimprove geo-referenced data sharing within andbetween organisations, hence developing bettercollaboration. It can also open opportunities fordata comparisons which can empower consumersFigure 2: screenshot <strong>of</strong> WAGCOE’s GeoNetwork web interface. All data are searchable through metadata, including keywordsand geographical location. Results are displayed with all corresponding metadata including links for download <strong>of</strong> <strong>the</strong> underlyingreal data.2 http://www.ivec.org3 http://www.opengeospatial.org65


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>(Rezabakhsh et al., 2006). In our case <strong>the</strong> firstexternal web service we are planning tointerconnect is <strong>the</strong> web interface to CSIRO’sPressurePlot 4 , a query tool linked to <strong>the</strong>PressureDB database. That database containsrock properties such as porosity, permeability and<strong>the</strong>rmal conductivity measurements, as well asstratigraphic and downhole pressure data formore than 1700 wells across Australia.WAGCOE’s web catalog serviceFigure shows a screenshot <strong>of</strong> WAGCOE’sGeoNetwork web interface 5 with three entriesvisible. Each entry is represented by its title andabstract, as well as two small pictures. Athumbnail on <strong>the</strong> right hand side represents <strong>the</strong>corresponding data and a logo on <strong>the</strong> left handside indicates visually <strong>the</strong> origin <strong>of</strong> <strong>the</strong> data. Allcurrent entries appear with WAGCOE’s logo asGeoNetwork is not connected to any o<strong>the</strong>rexternal service yet. Part <strong>of</strong> <strong>the</strong> data we store wasproduced by WAGCOE and includesmeasurements (see Figure ) as well as resultsfrom numerical models. Most <strong>of</strong> <strong>the</strong> underlyingdata however was not originally created byWAGCOE and comes from o<strong>the</strong>r organisationssuch as <strong>the</strong> Western <strong>Australian</strong> Department <strong>of</strong>Mines and Petroleum, Geoscience Australia, oro<strong>the</strong>r private companies, research andgovernmental organisations. This local hostingdemonstrates <strong>the</strong> temporary nature <strong>of</strong> thoseentries as we are working toward <strong>the</strong> single point<strong>of</strong> truth principle enunciated previously. We areonly hosting o<strong>the</strong>r organisations’ data with <strong>the</strong>irpermission as <strong>the</strong>y agree for us to do whilebuilding <strong>the</strong>ir own web services. We are alsoplanning to host data for geo<strong>the</strong>rmal companieswho choose to use our system to manage part <strong>of</strong><strong>the</strong>ir data.As shown on Figure , our infrastructure isdeployed at iVEC and benefits <strong>the</strong>refore from <strong>the</strong>irpr<strong>of</strong>essional services. All connections toGeoNetwork are encrypted and secure. A customgroup management function <strong>the</strong>n provides <strong>the</strong>granularity required to open some data to <strong>the</strong>public while restricting <strong>the</strong> access to protectedcompany data, for example.The data stored in our catalog covers all majorscientific areas relevant to geo<strong>the</strong>rmal explorationand GeoNetwork’s advanced options allow usersto search for entries using <strong>the</strong> following two levels<strong>of</strong> categories and sub-categories:• remote sensing: <strong>the</strong>rmal infra-red, landsat,spots, light detection and ranging (LIDAR),Figure 3: Example <strong>of</strong> data accessible through our catalog web service. This map shows Bouguer gravity from regionalGeoscience Australia data combined with new survey data acquired by WA Geo<strong>the</strong>rmal Centre <strong>of</strong> Excellence.4 http://www.pressureplot.com5 https://wagcoe.ivec.org/geonetwork66


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>• geophysics: seismic, velocities, magnetics,gravity, electomagnetics, radiometrics,geophysical logs, stress measurements,seismology data, magnetotellurics,• geology: geological maps, palynology data,sedimentology data, thin sections, grainsizeanalysis,• hydrogeology: hydraulic heads, water levels,water flows, rainfall, evapotranspiration data,recharge data, specific yield, storativity,• geochemistry: water quality, rock geochemistry,<strong>the</strong>rmochronology,• rock physics: permeability, porosity, <strong>the</strong>rmalconductivities, heat flux.While all mechanisms have been implemented forus to manage <strong>the</strong>se data types, populating <strong>the</strong>catalog with data references is a work in progress;not all sub-categories have data available yet.WAGCOE’s catalog management toolsWe have developed a suite <strong>of</strong> administrative toolsin order to build and manage our system asshown in Figure . We can <strong>the</strong>refore easily enforceconsistency between <strong>the</strong> metadata onGeoNetwork and <strong>the</strong> corresponding data on <strong>the</strong>petabyte store. The user’s group management inboth places is also greatly simplified, although notcompletely automatic. The main feature <strong>of</strong> ouradministrative toolbox is a converter betweenGeoNetworks’ metadata XML file format and anin-house extension <strong>of</strong> it allowing us to handlespecific metadata information which is notsupported in GeoNetwork by default and is notpart <strong>of</strong> our customised version yet.Figure presents a workflow diagram <strong>of</strong> allconversions occurring, between our WAGCOEmetadata XML file format and GeoNetwork’soriginal one, through an internal Python structurewhich allows easy data handling and processing,including checking validity, updating time stampsor creating unique identifiers. We can <strong>the</strong>n storeour extended metadata along with <strong>the</strong> originaldata and still retain <strong>the</strong> ability to efficiently evolveFigure 4: workflow diagram describing WAGCOE’s metadatamanagementour GeoNetwork implementation through <strong>of</strong>ficialupdates or in-house customisations. All metadatainformation is stored in <strong>the</strong> most appropriateformat for <strong>the</strong> particular data type, even though<strong>the</strong> additional information is displayed currentlyonly as part <strong>of</strong> a “supplemental information”paragraph for each entry. Any future enhanceddisplay handling in GeoNetwork can be easilyaccommodated with a script updating allGeoNetwork entries from our original extendedmetadata files.Future workWAGCOE’s geo<strong>the</strong>rmal catalog is currently underdevelopment and even though nearly all majortools have been developed, some major work stillremains to populate <strong>the</strong> catalog. The last majorupgrade to our administrative tools remains aGraphical User Interface (GUI) to enter metadatamore easily, as shown on Figure , instead <strong>of</strong>directly editing metadata files or internal Pythonstructures. There are also several featuresplanned for <strong>the</strong> future which will come fromWAGCOE’s strong collaboration with <strong>the</strong>AuScope Grid project (Woodcock 2008). The firstmajor enhancement will be to connect our catalogto o<strong>the</strong>r web services, starting with CSIRO’sPressurePlot web service. This linkage willprovide access to a real pressure andtemperature database allowing full contentsearches (whereas current searches on ourcatalog are limited to metadata). We are alsoplanning to register our data collection to <strong>the</strong><strong>Australian</strong> National Data Service (ANDS) RegisterMy Data service 6 which will <strong>the</strong>n automaticallyharvest all metadata and provide greaterexposure to our public entries. Finally, we aremonitoring closely <strong>the</strong> AuScope Grid portaldevelopment as it could provide an even moreuser friendly interface to our catalog. Van Oort(2009) pointed <strong>the</strong> cost <strong>of</strong> building such a portal,which only emphasises <strong>the</strong> importance <strong>of</strong>AuScope Grid’s generic and open source toolsdevelopment.ConclusionIn <strong>the</strong> last few years, web services such asGeoNetwork have redefined <strong>the</strong> way users candiscover, search, access and use geo-referenceddata. This powerful tool is currently seeing amajor uptake as it allows a dramatic change <strong>of</strong>practise for users who can now spend <strong>the</strong>ir timeusing data ra<strong>the</strong>r than searching for it.WAGCOE’s GeoNetwork catalog brings thisenormous advantage to <strong>the</strong> geo<strong>the</strong>rmalexploration industry and provides an easy,remote, and secure access to various geo<strong>the</strong>rmaldata sources through an intuitive web interface. I<strong>the</strong>lps to reduce <strong>the</strong> risk for geo<strong>the</strong>rmal explorationin <strong>the</strong> Perth Basin and could also help some6 http://ands.org.au/services/register-my-data.html67


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>companies to store and access <strong>the</strong>ir data. We arehoping to connect it as soon as possible to o<strong>the</strong>rweb services from various geological surveys,companies, research and governmentalorganisations, thanks to some <strong>of</strong> <strong>the</strong> technologydeveloped by <strong>the</strong> AuScope Grid projectReferencesvan Oort, P.; Kuyper, M.; Bregt, A. & Crompvoets,J. (2009), Geoportals: An Internet MarketingPerspective. Data Science Journal, 8, 162-181.Rezabakhsh, B., Bornemann, D., Hansen, U., &Schrader, U. (2006), Consumer Power: AComparison <strong>of</strong> <strong>the</strong> Old Economy and <strong>the</strong> InternetEconomy. Journal <strong>of</strong> Consumer Policy V29, 3-36.Ticheler, J. & Hielkema, J. U. (2007), GeoNetworkopensource, OSGeo Journal vol. 2, sep 2007.Woodcock, R., (2008), AuScope: <strong>Australian</strong> EarthScience Research Information Infrastructure,Geological Society <strong>of</strong> Australia and <strong>the</strong> <strong>Australian</strong>Institute <strong>of</strong> Geoscientists. <strong>Australian</strong> EarthSceinces Convention (AESC) 2008. NewGeneration Advances in Geoscience. AbstractsNo 89 <strong>of</strong> <strong>the</strong> 19 th <strong>Australian</strong> GeologicalConverntion, Perth Convention and ExhibitionCentre, Perth WA, Australia. July 20-24, 276pages.68


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Flow and heat modelling <strong>of</strong> a Hot Sedimentary Aquifer (HSA) fordirect-use geo<strong>the</strong>rmal heat production in <strong>the</strong> Perth urban area,Western Australia (WA)Martin Pujol 1* , Grant Bolton 1 and Fabrice Golfier 2 .1 Rockwater Pty Ltd. 76 Jersey Street, Jolimont WA2 Laboratoire Environnement Géomécanique et Ouvrages. Nancy Universités, Rue du doyen Marcel Roubault,Vandoeuvre-lès-Nancy BP40, 54501FRANCE* Corresponding author: mpujol@rockwater.com.auThe deep confined aquifers <strong>of</strong> <strong>the</strong> Perth basinhave been explored for water supply and heatproduction since <strong>the</strong> beginning <strong>of</strong> <strong>the</strong> 20thcentury. The availability <strong>of</strong> warm water was anadditional asset and was very popular withlaundries and bathing services. Currently, sixgeo<strong>the</strong>rmal bores use warm water from <strong>the</strong>Yarragadee confined aquifer for heatingswimming pools and buildings and several newbores are proposed to be drilled. The cooledformation groundwater is injected into <strong>the</strong> sameaquifer for environmental reasons.Following <strong>the</strong> recent success <strong>of</strong> <strong>the</strong> release <strong>of</strong>geo<strong>the</strong>rmal acreage for geo<strong>the</strong>rmal exploration inWA, HSA direct-use is getting more recognitionand support, and <strong>the</strong> number <strong>of</strong> projects is likelyto increase because <strong>the</strong> technology is now moreadvanced, low-risk, and has relatively low C0 2emissions and at low cost. Typical savings after20 years <strong>of</strong> production can be as high as$6,000,000, with payback in about 5 years andC0 2 savings <strong>of</strong> up to 800 tonnes/annum.A key concern for HSA future development inPerth is sustainability and management. This willbe achieved through a more comprehensiveassessment <strong>of</strong> HSA geo<strong>the</strong>rmal resources. Thelatter will also require a good estimation <strong>of</strong> <strong>the</strong>longevity <strong>of</strong> existing and future direct-use HSAsystems.In this paper we discuss how simple numericalmodelling <strong>of</strong> temperature and fluid flow usingSEAWAT s<strong>of</strong>tware and <strong>the</strong> “equivalent solute”approach allows for more accurate evaluations <strong>of</strong>geo<strong>the</strong>rmal resources and sustainability. This isan interesting management tool for existing andfuture HSA projects in Perth and is an alternativeapproach compared to <strong>the</strong> classical interpolation<strong>of</strong> measured temperatures between bores. Aboveall, <strong>the</strong> scope <strong>of</strong> this paper is to raise questionsand discuss <strong>the</strong> future management <strong>of</strong> existinggeo<strong>the</strong>rmal bores in <strong>the</strong> Perth area and to assistgeo<strong>the</strong>rmal explorers to develop shallow HSAdirect-use projects in <strong>the</strong> Perth area.Keywords: Western Australia, Perth, HotSedimentary Aquifer, HSA, geo<strong>the</strong>rmal, injection,direct-use, heat transport modelling, SEAWAT.HSA direct-use in <strong>the</strong> central PerthbasinGeological settingThe Perth urban area is located on <strong>the</strong> SwanCoastal Plain and is underlain by <strong>the</strong> Perthsedimentary Basin. The basin is comprised <strong>of</strong> aseries <strong>of</strong> sub-basins, troughs, shelves and ridgescontaining predominantly Early Permian to LateCretaceous sedimentary sequences that are up to15 km thick.The central Perth basin comprises a thicksequence <strong>of</strong> sedimentary rock, <strong>of</strong> which <strong>the</strong> upper3,000 m <strong>of</strong> Quaternary to Jurassic age arerelevant for geo<strong>the</strong>rmal projects targeting lowtemperature HSA systems.Existing geo<strong>the</strong>rmal bores have been drilled todepths up to 1,000 m in Perth; which havetargeted aquifers within <strong>the</strong> YarragadeeFormation and/or <strong>the</strong> overlying Gage Formation.The Yarragadee Formation consists <strong>of</strong> laterallydiscontinuous interbedded sandstones, siltstonesand shales and is inferred to be about 1,350 to1,500 m thick in <strong>the</strong> Perth urban area.HydrogeologyThe interbedded sandstones <strong>of</strong> <strong>the</strong> YarragadeeFormation form <strong>the</strong> Yarragadee confined aquiferand are hydraulically connected with interbeddedsandstone aquifers <strong>of</strong> <strong>the</strong> Gage Formation.The hydraulic properties <strong>of</strong> <strong>the</strong> Yarragadeeaquifer vary with location. In <strong>the</strong> study area, <strong>the</strong>discontinuous nature <strong>of</strong> <strong>the</strong> sandstone beds haslowered <strong>the</strong> average horizontal hydraulicconductivity to about 3 m/day. Hydraulicconductivity can locally be higher as indicated bypumping tests.The average rate <strong>of</strong> groundwater flow through <strong>the</strong>Yarragadee aquifer is about 0.9 m/year,confirming <strong>the</strong> very slow rate <strong>of</strong> flow indicated by<strong>the</strong> 14 C dating <strong>of</strong> <strong>the</strong> groundwater (Thorpe andDavidson, 1991). It is likely that most <strong>of</strong> <strong>the</strong>groundwater flow occurs in <strong>the</strong> top part <strong>of</strong> <strong>the</strong>aquifer, in about <strong>the</strong> top 500 m. Beneath thisdepth, <strong>the</strong> groundwater flow is likely to be loweras indicated by higher salinities (Davidson andYu, 2005).69


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>HSA Resource Assessment: Temperature,Heat in Place, Bore Deliverability andRecoverable HeatUsing a typical “stored heat” method as applied byBeardsmore et al (2009), <strong>the</strong> HSA geo<strong>the</strong>rmalresource for a specific direct-use application canbe estimated. However, <strong>the</strong> authors <strong>of</strong> this paperemphasize that <strong>the</strong> Stored Heat calculated belowis given as an element <strong>of</strong> comparison and is not tobe used for o<strong>the</strong>r purposes.For <strong>the</strong> purpose <strong>of</strong> reservoir volume estimations,we assume a minimum cut-<strong>of</strong>f temperature <strong>of</strong>40°C for direct-use projects, and an injectiontemperature <strong>of</strong> 30°C. The base <strong>of</strong> <strong>the</strong> Yarragadeeaquifer is inferred to be at about 70.6°C. Thisyields a reservoir volume <strong>of</strong> 126 km 3 below <strong>the</strong>100km 2 modelled area where most <strong>of</strong> <strong>the</strong>geo<strong>the</strong>rmal bores operate. The average reservoirtemperature is 55.3°C. Using calculated values <strong>of</strong>heat capacity for <strong>the</strong> fluid and solid, an averageporosity <strong>of</strong> 0.15, we estimate 7,926 PetaJoules(PJ=10 15 Joules) <strong>of</strong> heat in <strong>the</strong> modelledreservoir. Should o<strong>the</strong>r uses be considered, <strong>the</strong>cut-<strong>of</strong>f temperature, injection temperature andinferred resource may differ.The deliverable <strong>the</strong>rmal energy for a typical directusegeo<strong>the</strong>rmal bore is a function <strong>of</strong> sourcetemperature, heat exchanger efficiency, flow-rateand injection temperature. Typical values <strong>of</strong> 25L/s and 12°C temperature drop can provide adeliverable <strong>the</strong>rmal power <strong>of</strong> 1,113 kilowatt (kW th )and recoverable heat energy <strong>of</strong> 0.04 PJ/annum or9747 Megawatts hours/annum (MWh th ).Hence, in first estimation, <strong>the</strong> Yarragadee aquiferappears to be able to sustain a generalised use <strong>of</strong>HSA for heating buildings and swimming poolsamong o<strong>the</strong>r uses in <strong>the</strong> Perth urban area formany years. However, this may only be possible if<strong>the</strong>re is no (or very little) <strong>the</strong>rmal contaminationbetween <strong>the</strong> geo<strong>the</strong>rmal and injection bores. Thiscan be predicted using a numerical model <strong>of</strong>groundwater flow and heat transport. This is <strong>the</strong>general purpose <strong>of</strong> this study.HSA modelling: Initial temperaturedistribution in <strong>the</strong> aquifer (Conductivemodel)3D structural model <strong>of</strong> a selected area <strong>of</strong> <strong>the</strong>Perth basinData from Davidson and Yu (2005), andproprietary data from Rockwater Pty Ltd havebeen used to create a detailed structural model <strong>of</strong>an area <strong>of</strong> about 100 km 2 <strong>of</strong> <strong>the</strong> central PerthBasin where most <strong>of</strong> <strong>the</strong> geo<strong>the</strong>rmal boresoperate. The model comprises seven geologicalformations: superficial sediments (TQ), Tertiaryalluvial (Tk), Cretaceous sediments (Kco, Kwl,Kws and Kwg) and Jurassic sediments (Jy).Geostatistical methods have been used to inferformation top and bottom surfaces. Additionally,formation coverages specifying <strong>the</strong> extent <strong>of</strong> eachgeological formation (derived from contours inDavidson and Yu (2005) and modified in areaswhere new data had become available) havebeen used to constrain <strong>the</strong> model.Purely conductive heat flow 1D modellingA common practice in <strong>the</strong> geo<strong>the</strong>rmal industry,when modelling steady state temperatureconditions <strong>of</strong> HSA geo<strong>the</strong>rmal reservoirs, is toassume purely conductive heat transfer andconstant heat conductivity within each <strong>of</strong> <strong>the</strong>geological layers. This is referred as conductiveheat flow 1D modelling and is considered moreaccurate than <strong>the</strong> classical approach <strong>of</strong> averagegradient as it accounts for <strong>the</strong>rmal resistancevariations within <strong>the</strong> lithological column. This hasbeen demonstrated in several studies includingCooper and Beardsmore (1998).The conductive heat flow 1D assumption failswhen heat convection occurs such as in areas <strong>of</strong>high groundwater velocity such as faults, bores orwhen significant heterogeneity occurs. However,purely conductive models have proven tosatisfactorily represent temperature conditions in<strong>the</strong> Perth Basin and will be used to provide initialtemperatures for a more comprehensiveconductive and convective numerical model.In a conductive heat regime <strong>the</strong> temperature (T)at <strong>the</strong> bottom <strong>of</strong> a geological layer, is equal to <strong>the</strong>temperature at <strong>the</strong> top <strong>of</strong> <strong>the</strong> layer (T 0 ) plus <strong>the</strong>product <strong>of</strong> Heat Flow (Q) and <strong>the</strong>rmal resistance<strong>of</strong> <strong>the</strong> geological layer (R) (where <strong>the</strong> <strong>the</strong>rmalresistance equals <strong>the</strong> thickness <strong>of</strong> <strong>the</strong> layerdivided by <strong>the</strong> average <strong>the</strong>rmal conductivity).Consequently, <strong>the</strong> occurrence <strong>of</strong> prospectivegeo<strong>the</strong>rmally warmed groundwater in sedimentaryaquifers results from sufficiently low conductivity(high <strong>the</strong>rmal resistance) <strong>of</strong> <strong>the</strong> sedimentary covercombined with high flow <strong>of</strong> heat from <strong>the</strong> centre <strong>of</strong><strong>the</strong> Earth. Heat Flow (Q) is a function <strong>of</strong> <strong>the</strong> heatgenerated within <strong>the</strong> crust by <strong>the</strong> decay <strong>of</strong>radiogenic minerals plus heat conducted from <strong>the</strong>mantle. A commonly accepted value, derived fromnearby temperature logs for <strong>the</strong> modelled area is74 mW/m 2 .Conceptual modelIn order to represent <strong>the</strong> temperature distributionin <strong>the</strong> basin, several physical properties andboundary conditions have to be estimated and aso called conceptual model must be constructed.For each modelled stratigraphic layer, it isassumed that <strong>the</strong> lithology and physical propertiesare <strong>the</strong> same throughout. Measured <strong>the</strong>rmalconductivities are available for <strong>the</strong> formations <strong>of</strong><strong>the</strong> Perth basin (Chopra and Holgate, 2008) andhave been modified for <strong>the</strong> purpose <strong>of</strong> <strong>the</strong>numerical model by a classical trial and error70


method during <strong>the</strong> calibration <strong>of</strong> <strong>the</strong> model. Formost <strong>of</strong> <strong>the</strong> geological formations, <strong>the</strong> modelledvalue is close to <strong>the</strong> calculated value. However,modelled and measured heat conductivity valueswere found to differ for some geologicalformations. It is believed that it is due tolithological variations within those formations andvariation <strong>of</strong> <strong>the</strong> physical properties with depth.Table 1: Heat conductivity values (W/mC) <strong>of</strong> geologicalformations in <strong>the</strong> Perth BasinGeological Formation Modelled Measuredat 30°CTQ 1.5 1.42Tk 2.20 No dataKco 2.30 to 2.50 No dataKwl 1.70 to 2.50 2.56Kws 1.50 1.71 to 1.72Kwg 2.55 to 2.60 1.71 to 2.20Jy 3.05 to 3.20 2.30 to 4.31Method and boundary conditionsThe thickness <strong>of</strong> each geological formation atgiven coordinates have been extracted and usedtoge<strong>the</strong>r with heat conductivity properties for<strong>the</strong>se layers, to calculate <strong>the</strong>rmal resistances.Assuming a constant surface temperature <strong>of</strong>19.5°C at <strong>the</strong> upper boundary (taken as real meanair value measured at <strong>the</strong> Perth airport plus 1 Cto account for <strong>the</strong>rmal insulation <strong>of</strong> rocks) andusing <strong>the</strong> <strong>the</strong>rmal resistance values calculatedabove and <strong>the</strong> assumed constant heat flow <strong>of</strong> 74mW/m 2 , it was possible to predict <strong>the</strong> temperaturedistribution within <strong>the</strong> Yarragadee aquifer.Fig. 1: simplified 3D structural model <strong>of</strong> <strong>the</strong> modelled areawith geological formations considered in this study andapproximate locations <strong>of</strong> geo<strong>the</strong>rmal production boresCS: Challenge Stadium; TOC:Town Of Claremont;CCGS: ChristChurch Grammar School;SHG: St Hilda Geo<strong>the</strong>rmal, BPC: Bicton Polo Club.<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>HSA modelling: Initial temperaturedistribution in <strong>the</strong> aquifer (uncoupledConductive and Convective model)3D structural model <strong>of</strong> a selected area <strong>of</strong> <strong>the</strong>Perth basinThe same data as before are used but <strong>the</strong>structural model is limited to <strong>the</strong> Yarragadeeaquifer (Fig. 1).All layers overlying <strong>the</strong> Gage Formation are notmodelled, apart from <strong>the</strong> portion <strong>of</strong> Kings ParkFormation that has eroded <strong>the</strong> Gage andYarragadee Formations and which is likely toinfluence groundwater flow and heat transport.Heat transport modelling using <strong>the</strong>“equivalent solute” approach and <strong>the</strong>numerical code SEAWATSEAWAT is a standard finite-difference solutecode included in <strong>the</strong> state-<strong>of</strong>-<strong>the</strong>-art modellings<strong>of</strong>tware Visual Modflow Pro.Due to <strong>the</strong> similarities between heat and solutetransport, standard solute codes such asSEAWAT can be used to represent heat transportand variables for SEAWAT solute transportsimulator can be reinterpreted for heat transport.This has been demonstrated in several studiesincluding Langevin et al (2008). More detailedinformation on using solute transport simulationfor heat transport modelling can be found inHecht-Mendez et al (2009). Additional informationspecific to <strong>the</strong> use <strong>of</strong> <strong>the</strong> SEAWAT code for heattransport is available in Ma and Zheng (<strong>2010</strong>).In addition, for this study, SEAWAT has beenevaluated against analytical results developed forgeo<strong>the</strong>rmal and injection bores (doublet) and <strong>the</strong>results were comparable. The analytical solutionhas been developed by Gringarten and Sauty(1976) to predict <strong>the</strong> temperature evolution atHSA geo<strong>the</strong>rmal production bores used forgeo<strong>the</strong>rmal urban heating in <strong>the</strong> Paris basin.Conceptual modelAs groundwater flow needs to be consideredwhen undertaking conductive and convectivegeo<strong>the</strong>rmal modelling, a numerical code had to beused. For <strong>the</strong> present work, SEAWAT is used.The previously created 3D structural model isimported into SEAWAT and extrapolated to afinite difference 3D grid where <strong>the</strong> flow and heattransport equations are solved.Horizontal cell size varies from 140 m to 5 m near<strong>the</strong> bores and is about 25 m in vertical. Attentionhas been given to keep aspect ratio (ratiobetween cell size along x and z and y and zrespectively) less than 6.The calibrated <strong>the</strong>rmal conductivity for KingsPark, Gage and Yarragadee Formations areassigned to <strong>the</strong> corresponding cells and setconstant for each formation.71


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Hydrogeological parameters are available for <strong>the</strong>formations <strong>of</strong> <strong>the</strong> Perth basin (Davidson and Yu(2005) and proprietary data from Rockwater PtyLtd) and have been modified for <strong>the</strong> purpose <strong>of</strong><strong>the</strong> numerical model by a classical trial and errormethod during <strong>the</strong> calibration <strong>of</strong> <strong>the</strong> model.Table 2: Modelled hydrogeological parameters <strong>of</strong> geologicalformations in <strong>the</strong> Perth BasinGeological Kh Kh/Kv SFm. (m/day) (-)(-)Tk


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>borehead has been recorded since <strong>the</strong> bore wascommissioned. Considering <strong>the</strong> aboveassumptions, run 2 (Fig. 3) shows an acceptableagreement with pumped temperature increasingby 0.1°C after 10 years.Note that a more accurate evolution <strong>of</strong>temperature at <strong>the</strong> bore could be obtained using alocal model with a higher spatial resolution and anexplicit numerical solution for advection.Fig. 3: CCGS1 modelled pumped temperaturesIn addition, steady state modelled drawdown is10.3 m and agrees with <strong>the</strong> aquifer losses <strong>of</strong> 8 mmeasured at <strong>the</strong> end <strong>of</strong> <strong>the</strong> 48 hours constant-ratepumping test.Results: environmental impact <strong>of</strong> <strong>the</strong> injectionFollowing <strong>the</strong> calibration, <strong>the</strong> model was run fromJanuary 2000 to January 2050 to predict <strong>the</strong>evolution <strong>of</strong> temperatures within <strong>the</strong> basin.The model aims are (i) to determine <strong>the</strong> generalevolution <strong>of</strong> temperature <strong>of</strong> <strong>the</strong> Yarragadeeaquifer, (ii) to give a first estimation <strong>of</strong> <strong>the</strong> lifetime<strong>of</strong> existing geo<strong>the</strong>rmal installations and (iii) toidentify areas where <strong>the</strong>re is an impact <strong>of</strong> injectedwater on aquifer temperatures.almost 50 years <strong>of</strong> continuous operation as shownin Fig. 4.The modelled temperature decline at CCGS1 inJanuary 2050 is 0.39°C after 48 years, and0.12°C at TOC 1 after 45 years whereas <strong>the</strong>temperature at SHG1 has increased by 0.14°Cafter 40 years. This is likely to have little impacton <strong>the</strong> geo<strong>the</strong>rmal installation efficiencies andsubsequently <strong>the</strong> lifetime <strong>of</strong> all three geo<strong>the</strong>rmalinstallations; estimated to be more than 40 years.DiscussionFor all three bores, <strong>the</strong> temperature evolution canbe described as follows:• Stage 1: Increased temperature <strong>of</strong> <strong>the</strong>pumped water (increase is higher when flow-rateis higher) provoked by <strong>the</strong> inflow <strong>of</strong> deeper andwarmer groundwater in <strong>the</strong> bores. This is fur<strong>the</strong>rfacilitated by <strong>the</strong> presence <strong>of</strong> upward heads.• Stage 2: As <strong>the</strong> cooled groundwater isinjected and travels through <strong>the</strong> aquifer in <strong>the</strong>direction <strong>of</strong> <strong>the</strong> production bore, <strong>the</strong> rate <strong>of</strong>temperature increase diminishes and eventuallystabilises (this happens earlier when <strong>the</strong> verticaldistance between injection and productionscreened section is small).• Stage 3: Pumped temperatures startdeclining and eventually decline at a linear rate. Itis calculated that bores CCGS1 and TOC1 willreach Stage 3 in year 2050 because <strong>of</strong> <strong>the</strong>smaller vertical separation between productionand injection screened sections, whereas SHG1is likely to still be in Stage 2.Fig. 4: Predicted evolution <strong>of</strong> temperature at CCGS1, TOC1and SHG1The initial observation is that <strong>the</strong>re is littletemperature decline at <strong>the</strong> production bores afterFig. 5: Calculated temperature distribution (°C) in selectedlayers: layer 6 from -520 to -676 m AHD and layer 9 from -651 to -767m AHDThe modelled results show that <strong>the</strong> cooler injectedwater has a limited impact on <strong>the</strong> pumpedgroundwater temperature because <strong>of</strong> <strong>the</strong>moderately low vertical hydraulic conductivities,upward heads in <strong>the</strong> deeper geo<strong>the</strong>rmal bores,and <strong>the</strong> vertical distances between production andinjection bore screens.73


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>The cooled groundwater plume is calculated toextend 850 m in a circular pattern from TOC1(Claremont AC) by 2050 (Fig. 5) indicating thatnatural groundwater flow has little influence on <strong>the</strong>shape <strong>of</strong> <strong>the</strong> groundwater plume. Conversely, <strong>the</strong>groundwater plume generated by CS1 (ChallengeStadium) has a very distinctive tear-drop pattern(Fig. 5, layer 9) indicating that a portion <strong>of</strong> <strong>the</strong>injected water is recirculated and that <strong>the</strong>rmalcontamination is occurring.Conclusion: HSA direct-usesustainability and future researchobjectivesAlthough <strong>the</strong> presented simulation is decoupled(water density is independent <strong>of</strong> temperature) andmay not be accurate where density effectsdominate, <strong>the</strong> results show that pumpedgroundwater temperatures are unlikely to changesignificantly over <strong>the</strong> next 40 years. This supports<strong>the</strong> notion that HSA direct-use is a cost-effectivesolution (payback is about 5 years) for heatingbuildings or swimming pools for example.However, temperature depletion seems to extendhorizontally and although no visible interferencebetween bores has been recorded, it is advisableto avoid pumping from <strong>the</strong> same depth as water isinjected. Therefore, it is recommended that futureproduction bores should be sited at least 500 mfrom one ano<strong>the</strong>r and at different depths (i.e. 100to 150 m deeper than <strong>the</strong> nearest injectionscreens).To increase <strong>the</strong> accuracy <strong>of</strong> <strong>the</strong> model and to beable to guarantee <strong>the</strong> sustainability <strong>of</strong> HSA directuseprojects, additional work could be performed:• Create local, high resolution models foreach geo<strong>the</strong>rmal installation.• Perform temperature logging periodically.• Model heterogeneity patterns <strong>of</strong> <strong>the</strong>Yarragadee aquifer.• Refine <strong>the</strong> structural model byconsidering geological members within <strong>the</strong>Osborne and Leederville formations.• Refine <strong>the</strong> calibration <strong>of</strong> <strong>the</strong> model usinga transient constant-rate pumping test.• Perform hydraulic head versus depthmeasurements.• Correlate <strong>the</strong> stratigraphy (siltstone andsandstone beds) between production andinjection bores to increase vertical accuracy.• Monitor geo<strong>the</strong>rmal installationsperiodically to obtain monthly data <strong>of</strong> injectiontemperatures, pumped water temperatures, flowratesand injection pressures.• Evaluate <strong>the</strong> impact <strong>of</strong> density forces(forces driving <strong>the</strong> formation <strong>of</strong> convection cells)on initial temperature distribution.• Consider heat flow variations over <strong>the</strong>modelled domain.• Refine <strong>the</strong> calibration using recenttemperature logs <strong>of</strong> artesian monitoring bores.ReferencesBeardsmore, G. R., et al, 2009, Statement <strong>of</strong>estimated Geo<strong>the</strong>rmal Resources MetropolitanPerth Geo<strong>the</strong>rmal Play, 31/07-8 GEP, 27 July2009.Chopra, P.N, and F., Holgate., 2008, Geo<strong>the</strong>rmalenergy potential in selected areas <strong>of</strong> WesternAustralia; a consultancy report by Hot Dry RocksPty Ltd for Geological Survey <strong>of</strong> WesternAustralia: Geological Survey <strong>of</strong> Western Australia,G31888 A2.Cooper, G. T., and Beardsmore, G. R.,Geo<strong>the</strong>rmal systems assessment: understandingrisks in geo<strong>the</strong>rmal exploration in Australia: PESAEastern Australasian Basins Symposium IIISydney, 14–17 September, 2008.Davidson, W.A., and Yu, X., 2005. Perth regionalaquifer modelling system (PRAMS) modeldevelopment: Hydrogeology and groundwatermodelling : Western Australia Department <strong>of</strong>Water, Hydrogeological record series HG 20.Gringarten, A.C., and Sauty, J.P., 1976, Theeffect <strong>of</strong> reinjection on <strong>the</strong> temperature <strong>of</strong> ageo<strong>the</strong>rmal reservoir used for urban heating:BRGM, Orleans. 12p.Hecht-Mendez, J. et al., 2009, EvaluatingMT3DMS for Heat Transport Simulation <strong>of</strong> ClosedGeo<strong>the</strong>rmal Systems: Wiley-Blackwell. 16p.Langevin, C.D., Thorne, D.T. Jr., Dausman, A.M.,Sukop, M.C, and Guo, Weixing, 2008, SEAWATVersion 4: A Computer Program for Simulation <strong>of</strong>Multi-Species Solute and Head Transport: U.S.Geological Survey Techniques and Methods Book6, Chapter A22, 39 p.Loague, K., and R.E., Green, 1991, Statistical andgraphical methods for evaluating solute transportmodels: Overview and application: Journal <strong>of</strong>Contaminant Hydrology 7, no. 1–2: 51–73.Ma, R., and Zheng, C., <strong>2010</strong>, Effects <strong>of</strong> densityand viscosity in modelling heat as a groundwatertracer: Groundwater, Volume 48 Issue3, pp. 380-389.Thorpe, P.M., and Davidson, W.A., 1991,Groundwater age and hydrodynamics <strong>of</strong> <strong>the</strong>confined aquifers, Perth, Western Australia:<strong>Proceedings</strong> <strong>of</strong> <strong>the</strong> International <strong>Conference</strong> onGroundwater in Large Sedimentary Basins, Perth,Western Australia, 1990. <strong>Australian</strong> WaterResources Council Series, no. 20, p. 420-436.74


In most Precambrian terrains including India,moderate-to-low temperature hot spring systemsrepresent <strong>the</strong> potential conventional geo<strong>the</strong>rmalenergy resources. This scenario is in contrast togeo<strong>the</strong>rmal fields under production in o<strong>the</strong>r parts<strong>of</strong> <strong>the</strong> world, which are located in Quaternaryvolcanic / magmatic settings (Gupta and Roy,2006). This paper outlines (i) <strong>the</strong> major hot springoccurrences in India, (ii) <strong>the</strong> exploration effortsundertaken so far, (iii) possible geo<strong>the</strong>rmalmodels in <strong>the</strong> light <strong>of</strong> regional heat flow and heatproduction datasets, (iv) a few critical informationgaps that need to be covered to make realisticassessment <strong>of</strong> <strong>the</strong> geo<strong>the</strong>rmal energy potential,and (v) perspectives for development andutilisation <strong>of</strong> geo<strong>the</strong>rmal energy in <strong>the</strong> country,both for electric power generation as well as fordirect uses.Geo<strong>the</strong>rmal Exploration in IndiaSukanta RoyNational Geophysical Research Institute(Council <strong>of</strong> Scientific and Industrial Research)Uppal Road, Hyderabad 500 606, IndiaCorresponding author: sukantaroy@yahoo.com<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Keywords: India, geo<strong>the</strong>rmal energy, heat flow,radiogenic heat productionExploration <strong>of</strong> Geo<strong>the</strong>rmal <strong>Energy</strong>ResourcesThe major groups <strong>of</strong> hot springs in India occur inManikaran, Puga-Chhumathang valley andTapoban in <strong>the</strong> Himalaya, a near N-S trendinglinear belt in <strong>the</strong> west coast <strong>of</strong> Maharashtra, <strong>the</strong>Son-Narmada-Tapti lineament zone in centralIndia, Tattapani in Chattisgarh, and Rajgir-Monghyr, Surajkund and Bakreshwar in easternIndia. The distribution <strong>of</strong> major groups <strong>of</strong> hotsprings is shown in Figure 1. Rao (1997) providesa brief summary <strong>of</strong> <strong>the</strong> historical development <strong>of</strong>studies on <strong>the</strong> Indian geo<strong>the</strong>rmal resources,starting with <strong>the</strong> first compilations <strong>of</strong> 99 hotsprings in India and <strong>the</strong> adjacent countries bySchlagintweit (1865). The locations, geologicalsettings and temperatures <strong>of</strong> hot springs locatedin different geologic provinces in India have beencompiled by previous workers (for example,Oldham, 1882; Ghosh, 1954; Gupta, 1974; Guha,1986; GSI, 1991, 2002 and o<strong>the</strong>rs). A number <strong>of</strong>those geo<strong>the</strong>rmal springs have been used forbalneological purposes. However, India is yet toproduce electric power from a geo<strong>the</strong>rmal field.Among <strong>the</strong> most notable achievements during <strong>the</strong>past five decades have been <strong>the</strong> assessment <strong>of</strong>geo<strong>the</strong>rmal fields by <strong>the</strong> Government <strong>of</strong> India in1966 and publication <strong>of</strong> a comprehensive report in1968 recommending preliminary prospecting <strong>of</strong>Figure 1. Outline <strong>of</strong> India showing <strong>the</strong> distribution <strong>of</strong> majorgroups <strong>of</strong> warm and hot springs (modified after Krishnaswamy,1975). Temperatures <strong>of</strong> <strong>the</strong> hot spring waters are indicatedusing symbols (see legend). Shaded regions (exaggeratedscale) show <strong>the</strong> major clusters <strong>of</strong> hot springs.<strong>the</strong> Puga and Manikaran geo<strong>the</strong>rmal fields in <strong>the</strong>Himalaya (Hot Springs Committee, 1968). Amajor, systematic, multi-disciplinary, multi-Institutional programme (including drilling up to385 m) covering <strong>the</strong> Puga-Chumathang field inLadakh was mounted during 1972-74 under <strong>the</strong>stewardship <strong>of</strong> V.S. Krishnaswamy <strong>of</strong> <strong>the</strong>Geological Survey <strong>of</strong> India (GSI). The subsurfacefeatures were delineated in considerable detailand <strong>the</strong> results were presented at <strong>the</strong> SecondUnited Nations Symposium on <strong>the</strong> Developmentand Use <strong>of</strong> Geo<strong>the</strong>rmal Resources in 1975. Themost significant outcome <strong>of</strong> <strong>the</strong> effort was aproposal to set up a 1 MWe binary-cycle powerplant on a pilot scale basis, which has not beenimplemented so far. Attempts to revisit <strong>the</strong>geo<strong>the</strong>rmal exploration in <strong>the</strong> area include anumber <strong>of</strong> geochemical studies (GSI, 1996) andrecent magnetotelluric studies (Abdul Azeez andHarinarayana, 2007). An expert group set up in2008 by <strong>the</strong> Ministry <strong>of</strong> New and Renewable<strong>Energy</strong>, Government <strong>of</strong> India made strongrecommendations to install pilot-scale plant by75


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>drilling exploration cum demonstration wells in <strong>the</strong>area (MNRE, 2008). This would be useful not onlyfor monitoring <strong>the</strong> hot water discharge andtemperatures over a period <strong>of</strong> time but alsostudying <strong>the</strong> shallow reservoir characteristics.Ano<strong>the</strong>r major initiative, directed towards <strong>the</strong> hotsprings <strong>of</strong> <strong>the</strong> West Coast belt and <strong>the</strong> Son-Narmada-Tapti belt was taken up by <strong>the</strong> GSI withUNDP assistance during 1976-77, and wasextended for a few years on its own, includingdeep drilling up to depth <strong>of</strong> 500 m. The resultswere published in <strong>the</strong> Records <strong>of</strong> <strong>the</strong> GSI (1987).The Tattapani hot springs <strong>of</strong> Chattisgarh districtwas identified for trials with regard to powerproduction using a 300 KW e binary-cycle powerplant. Summaries <strong>of</strong> various explorationprogrammes undertaken in <strong>the</strong> country during <strong>the</strong>period 1970-1990 are given in Gupta et al. (1973,1974); Shanker et al. (1976); Singh et al. (1983);Krishnaswamy and Ravi Shanker (1980); GSI(1983, 1991, 1996, 2002); Thussu et al. (1987);Moon and Dharam (1988) and Gupta (1992). Thesalient results in <strong>the</strong> case <strong>of</strong> <strong>the</strong> two potentialgeo<strong>the</strong>rmal fields, Puga and Tattapani, aresummarized below.Puga Valley Hot SpringsIn <strong>the</strong> case <strong>of</strong> Puga valley springs, geo<strong>the</strong>rmalevidence ga<strong>the</strong>red so far and geochemicalindicators including <strong>the</strong> occurrence <strong>of</strong> cesiumdeposits around <strong>the</strong> springs have suggested <strong>the</strong>possibility <strong>of</strong> high temperature hydro<strong>the</strong>rmalcirculation in <strong>the</strong> subsurface (Absar et al., 1996).A shallow reservoir in <strong>the</strong> top few hundred meterswas inferred from geophysical and geo<strong>the</strong>rmalinvestigations carried out during <strong>the</strong> 1970s.Recent magnetotelluric studies indicate <strong>the</strong>presence <strong>of</strong> an anomalous conductive feature (~5Ohm m) below a depth <strong>of</strong> ~2 km in <strong>the</strong> area <strong>of</strong> <strong>the</strong><strong>the</strong>rmal manifestations (Harinarayana et al., 2006;Abdul Azeez and Harinarayana, 2007). Althoughbroad correlations between high electricalconductivity and high temperatures have beenobserved in some geo<strong>the</strong>rmal areas, <strong>the</strong>calibration <strong>of</strong> electrical conductivity anomalies totemperature anomalies at depth is notestablished. Fur<strong>the</strong>r efforts are necessary to fillexisting gaps in knowledge and verify <strong>the</strong>hypo<strong>the</strong>sis regarding <strong>the</strong> occurrence <strong>of</strong>subsurface magma chambers or young intrusivegranites in <strong>the</strong> region. Such heat sources alonecan sustain power generation on a reasonablescale (Rao et al., 2003). Determination <strong>of</strong>background heat flow outside <strong>the</strong> hot springszone, helium-isotopic measurements on <strong>the</strong><strong>the</strong>rmal waters, detailed petrographic andgeochronological studies on young graniteintrusives, and tritium dating <strong>of</strong> <strong>the</strong> waters wouldbe useful for testing a magmatic heat source.Tattapani Hot SpringsIn <strong>the</strong> case <strong>of</strong> <strong>the</strong> Tattapani hot springs, <strong>the</strong>temperatures <strong>of</strong> <strong>the</strong> issuing waters is ~110 o C, <strong>the</strong>highest recorded so far in <strong>the</strong> shield. The springwaters are meteoric in origin as indicated byoxygen and helium isotopic data, and <strong>the</strong> age <strong>of</strong><strong>the</strong>se waters indicated by tritium dating is ~40years (Thussu et al., 1987; Sharma et al., 1996;Minnisale et al., 2000). Repeat well testing carriedout by GSI in 1995 and 1999 indicate nosignificant fall in temperatures and pressuresduring <strong>the</strong> intervening period (Sarolkar andSharma, 2002). Recent magnetotelluric studies in<strong>the</strong> area have delineated a deep, anomalousconductive zone possibly indicating <strong>the</strong>subsurface extent <strong>of</strong> <strong>the</strong> reservoir (Harinarayanaet al., 2004). Lack <strong>of</strong> evidence for Quaternarymagmatism in <strong>the</strong> region as well as <strong>the</strong> meteoricnature <strong>of</strong> <strong>the</strong> hot spring waters indicate that <strong>the</strong>hot springs are controlled by forced convectiondue to peizometric gradient existing between <strong>the</strong>recharge area and <strong>the</strong> hot springs, and that <strong>the</strong>springs could be simply “mining” <strong>the</strong> normal heatflow (Roy and Rao, 1996; Rao et al., 2003).However, no heat flow measurements outside <strong>the</strong>localized hot springs zone have been made.There is <strong>the</strong>refore a clear need to establish <strong>the</strong>regional <strong>the</strong>rmal conditions by systematicgeo<strong>the</strong>rmal measurements because <strong>the</strong>y wouldcontain information about subsurface flow andlocation <strong>of</strong> recharge area also (Lachenbruch etal., 1976).O<strong>the</strong>r areasA large number <strong>of</strong> warm to hot springs occur inwestern, central and eastern parts <strong>of</strong> <strong>the</strong> Indianshield. The temperatures <strong>of</strong> <strong>the</strong>se springs arelower than those at Tattapani and vary between35 o and 80 o C. It is likely that a geo<strong>the</strong>rmal modelsimilar to that at Tattapani could explain <strong>the</strong>occurrence <strong>of</strong> <strong>the</strong>se hot springs.Heat Flow and Heat ProductionHeat flow determinations made through precisetemperature measurements in boreholes and<strong>the</strong>rmal conductivity measurements onrepresentative rock formations have been <strong>the</strong>central <strong>the</strong>me <strong>of</strong> <strong>the</strong> heat flow studies programmeat <strong>the</strong> National Geophysical Research Institutesince its inception in 1961. Although boreholes <strong>of</strong>opportunity have been used for <strong>the</strong> majority <strong>of</strong>measurements, a selection has been made on <strong>the</strong>following criteria to make <strong>the</strong> heat flowdeterminations useful for characterizion <strong>of</strong> <strong>the</strong><strong>the</strong>rmal state <strong>of</strong> <strong>the</strong> lithosphere: (1) depths greaterthan 150 m in hard rock areas and severalhundred metres in sedimentary basins (2) sitesaway from hot spring manifestations, tectonicallyactive regions, and rugged topography (3)temperature pr<strong>of</strong>iles with no characteristicperturbations such as those <strong>of</strong> heat refraction andgroundwater movement. The principal constraintin <strong>the</strong> data acquisition programme has been <strong>the</strong>availability <strong>of</strong> suitable boreholes for making76


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>temperature measurements. This constraint hasbeen addressed, to some extent, through <strong>the</strong>drilling <strong>of</strong> 14 dedicated “heat flow” boreholes todepths <strong>of</strong> up to 500 m at carefully chosen sites insouth India. The careful siting <strong>of</strong> <strong>the</strong> boreholes inareas <strong>of</strong> relative lithological homogeneity and lowgroundwater yields facilitated <strong>the</strong> acquisition <strong>of</strong>undisturbed temperature-depth pr<strong>of</strong>iles fromwhich gradients could be estimated with a greatdegree <strong>of</strong> confidence. In geologic provinces <strong>of</strong>nor<strong>the</strong>rn Indian shield, <strong>the</strong> heat flow coverage isvariable and several gaps exist over largesegments. In <strong>the</strong> Himalaya, regional heat flowdata are not available. Borehole temperaturemeasurements in close proximity <strong>of</strong> hot springsexist at a few locations only. However, <strong>the</strong>semeasurements are affected by convection due tohydro<strong>the</strong>rmal circulation in <strong>the</strong> near surface zoneand are not representative <strong>of</strong> deep crustalconditions. Thermal conductivity data for all majorrock formations in <strong>the</strong> sou<strong>the</strong>rn Indian shield andseveral rock formations from o<strong>the</strong>r parts <strong>of</strong> Indiaconstitute a very extensive database for modelling<strong>the</strong> <strong>the</strong>rmal structure in <strong>the</strong> upper few kilometres<strong>of</strong> <strong>the</strong> crust.Heat Flow and Geo<strong>the</strong>rmal GradientsFigure 2. Heat flow map <strong>of</strong> <strong>the</strong> Indian Shield. Heat flow sitesare shown by filled triangles. Heat flow determinations havebeen made on <strong>the</strong> basis <strong>of</strong> temperature measurements inboreholes and <strong>the</strong>rmal conductivity <strong>of</strong> rock formations. Overlarge regions in nor<strong>the</strong>rn India which are not covered with heatflow measurements, <strong>the</strong> contours should be treated withcaution. [Sources <strong>of</strong> data: Roy and Rao (2000) and originalreferences <strong>the</strong>rein; Ray et al. (2003); Rao et al. (2003); Roy(2008); Roy et al. (2008)].A heat flow map for <strong>the</strong> Indian shield is shown inFigure 2. Heat flow data are now available frommeasurements made in ~210 boreholesdistributed over <strong>the</strong> major geological provinces in<strong>the</strong> shield. The dataset shown here is confined tosites where complete information on geo<strong>the</strong>rmalgradient and <strong>the</strong>rmal conductivity are available.Heat flow determined using o<strong>the</strong>r techniques suchas chemical composition <strong>of</strong> water, andcorrelations with P-wave velocity and age, areexcluded. A detailed discussion <strong>of</strong> heat flowcharacteristics <strong>of</strong> different provinces is given in<strong>the</strong> papers by Roy and Rao (2000) and Rao et al.(2003). The salient features <strong>of</strong> <strong>the</strong> heat flowspectrum in <strong>the</strong> Indian shield are brieflymentioned below.1. The sou<strong>the</strong>rn Indian shield comprising <strong>the</strong>Archaean Dharwar greenstone-granitegneissprovince and gneiss-granuliteprovince, is characterized by low heat flow,generally ranging from 25 to 50 mW m -2 .Geo<strong>the</strong>rmal gradients measured in <strong>the</strong> topfew hundred meters in boreholes and up to2150 m in a deep mine are in <strong>the</strong> range 12--115 mK m .2. The low heat flow regime <strong>of</strong> south Indiaextends northward beneath <strong>the</strong> DeccanTraps in central India, which indicate <strong>the</strong>absence <strong>of</strong> <strong>the</strong>rmal transients related to <strong>the</strong>~65 Ma Deccan volcanism in <strong>the</strong> present-dayheat flow. Measurements at several localitiesdistributed in Deccan Traps province indicatean average gradient <strong>of</strong> ~25 mK m -1 .However, beneath <strong>the</strong> Traps which rangefrom a few meters in <strong>the</strong> east to 2-3 km in <strong>the</strong>west, <strong>the</strong> gradient in <strong>the</strong> Precambrian graniticbasement drops to ~15 mK m -1 due to higher<strong>the</strong>rmal conductivity <strong>of</strong> granitic rocks relativeto basalts.3. The Precambrian provinces in nor<strong>the</strong>rnIndian shield show a contrasting heat flowregime, with values ranging from 50 to 96mW m -2 . Previous studies have attributed <strong>the</strong>enhanced heat flow to high levels <strong>of</strong>radiogenic heat production in <strong>the</strong> upper crust.Temperature gradients vary between 12 and-130 mK m across different rock formations.4. The Gondwana sedimentary basins (UpperCarboniferous to Lower Cretaceous) have agenerally high but variable heat flow in <strong>the</strong>range 46 to 107 mW m -2 . Temperaturegradients show large variability, and reachpeak values <strong>of</strong> up to ~50 o Ckm -1 in <strong>the</strong>o -1Damodar Valley basins and ~40 Ckm inGodavari Valley basin.5. The Cambay sedimentary basin <strong>of</strong> Tertiaryage in western India shows consistent highheat flow, 75-96 mW m -2 in <strong>the</strong> nor<strong>the</strong>rn partsand a lower heat flow, 55-67 mW m -2 , in <strong>the</strong>sou<strong>the</strong>rn parts. Very high gradients in <strong>the</strong>range 37 to 56 o C km -1 were computed fromtemperature measurements to depths >1000m in <strong>the</strong> nor<strong>the</strong>rn part.77


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Radiogenic Heat ProductionHeat production due to radioactive decay <strong>of</strong> longlivedisotopes <strong>of</strong> U, Th and K (namely, 235 U, 238 U,232 Th, and 40 K) in rock formations constituting <strong>the</strong>continental crust plays a key role in interpretation<strong>of</strong> heat flow data. With this primary objective, alow-level counting gamma-ray spectrometricfacility using a single-channel analyser wasestablished at <strong>the</strong> NGRI for analysis <strong>of</strong> rocks forradioelements U and Th (at ppm levels) and K(Rao, 1974; Rao and Rao, 1979). The facility hasbeen progressively upgraded using a multichannelanalyser and later, a PC-based multichannelanalysing card that provides spectrumstabilization (Roy and Rao, 1999, 2003). Severalhundred samples covering major rock types in <strong>the</strong>Indian shield have been analysed for U, Th and K.The salient features <strong>of</strong> <strong>the</strong> dataset are describedin Roy (2008).Over <strong>the</strong> last two decades, laboratory analyseshave been complemented by in-situ gamma-rayspectrometric analysis in several areas in <strong>the</strong>Indian shield (Roy, 1997; Roy and Rao, 2000,2003; Ray et al., 2003, 2008). A field-portable,four-channel, spectrum stabilized, gamma-rayspectrometer and a large crystal (6” high and 4”diameter) detector have been used. Analysis forU, Th and K are made by placing <strong>the</strong> detectordirectly over fresh rock outcrops. In this case, <strong>the</strong>detector senses a much larger volume <strong>of</strong> rockmass, typically a circle <strong>of</strong> investigation <strong>of</strong> ~40 cmand a depth <strong>of</strong> ~12 cm, compared to <strong>the</strong>laboratory method. In areas abounding with freshoutcrops, this method results in faster coverage.Significant observations include delineation <strong>of</strong>pockets <strong>of</strong> very high heat production in graniticrocks, for example in Tattapani area, and younggranite intrusives in northwestern parts <strong>of</strong> India,detection <strong>of</strong> granulite facies rocks with lowest heatproduction reported in literature, and a range <strong>of</strong>rock formations with intermediate heat productionvalues.Perspectives for Development <strong>of</strong>Geo<strong>the</strong>rmal <strong>Energy</strong>Re-assessment <strong>of</strong> <strong>Energy</strong> Potential <strong>of</strong>Conventional Geo<strong>the</strong>rmal ResourcesIn view <strong>of</strong> growing energy demands and <strong>the</strong>emphasis on renewable energy in India, a reassessment<strong>of</strong> geo<strong>the</strong>rmal energy potential <strong>of</strong>Puga Valley hot springs in Ladakh and Tattapanihot springs in Chatttisgarh should be carried outby covering some critical gaps in informationthrough acquisition <strong>of</strong> new data, combinedinterpretation <strong>of</strong> geo<strong>the</strong>rmal datasets and existinggeological, hydrological, geochemical andgeophysical datasets to throw light on <strong>the</strong> nature<strong>of</strong> <strong>the</strong> heat source <strong>of</strong> <strong>the</strong> hot springs and <strong>the</strong>irsustainability for power production, undertakingdrilling and setting up <strong>of</strong> pilot-scale binary-cyclepower plants.Geo<strong>the</strong>rmal resources vary widely from onelocation to ano<strong>the</strong>r, depending on <strong>the</strong> temperatureand depth <strong>of</strong> <strong>the</strong> resource, <strong>the</strong> rock chemistry,and <strong>the</strong> abundance <strong>of</strong> groundwater. The type <strong>of</strong>geo<strong>the</strong>rmal resource determines <strong>the</strong> method <strong>of</strong> itsutilization. Variants <strong>of</strong> binary cycles appropriate tooptimum utilization <strong>of</strong> geo<strong>the</strong>rmal heat from hotsprings in non-volcanic settings such as those inIndia need to be developed.Direct Heat UsesThe heat extracted from warm-to-hot watersemerging from o<strong>the</strong>r hot spring systems in <strong>the</strong>country can be gainfully employed for a number <strong>of</strong>direct uses such as development <strong>of</strong> tourist spasfor bathing, swimming and balneology,greenhouse cultivation in cold climates, extraction<strong>of</strong> borax and rare materials such as cesium, andagricultural product processing. The significanteconomic and environmental benefits <strong>of</strong> usingmoderate-to-low enthalpy geo<strong>the</strong>rmal waters toreplace even small quantities <strong>of</strong> conventionalfuels for direct uses cannot be ignored today inview <strong>of</strong> <strong>the</strong> steep increase in costs <strong>of</strong> fossil fuelsand associated greenhouse gas emissions.Exploration for Enhanced Geo<strong>the</strong>rmalSystemsA second category <strong>of</strong> geo<strong>the</strong>rmal resourcetraditionally referred to as “hot dry rock” and morerecently as “enhanced geo<strong>the</strong>rmal systemsEGS)”, has not yet been explored in India. Theprimary requirement for such a resource is <strong>the</strong>occurrence <strong>of</strong> high temperatures (typicallyupwards <strong>of</strong> 150 o C) at economically viable depths(typically <strong>the</strong> top 1-4 km <strong>of</strong> <strong>the</strong> Earth’s crust).Areas <strong>of</strong> anomalous high heat flow, high-heatproducinggranites and o<strong>the</strong>r silicic igneousintrusives having a depth extent <strong>of</strong> a fewkilometers, could be possible targets <strong>of</strong> futureexploration efforts in <strong>the</strong> country (Roy, 2008).These considerations reinforce <strong>the</strong> need forcarrying out systematic heat flow as well asradiogenic heat production investigations on acountry-wide scale.Geo<strong>the</strong>rmal Heat PumpsThe viability <strong>of</strong> geo<strong>the</strong>rmal heat pumps for heatinginside buildings should be explored in <strong>the</strong> states<strong>of</strong> Jammu and Kashmir, Himachal Pradesh andparts <strong>of</strong> Uttarakhand which experience severewinter conditions for long periods. Space coolingrequirements in most parts <strong>of</strong> India have grownseveral fold in <strong>the</strong> recent years with <strong>the</strong> growth ineconomy. There is enormous scope fordeveloping <strong>the</strong> capabilities in geo<strong>the</strong>rmal cooling<strong>of</strong> buildings by modifying existing technologies tosuit Indian conditions. A proper assessment <strong>of</strong> <strong>the</strong>technology for application to different climaticenvironments existing in <strong>the</strong> region, and its78


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>exploitation by integrating it with building designsshould be encouraged.SummaryModerate-to-low enthalpy hot spring systemsprimarily represent <strong>the</strong> known geo<strong>the</strong>rmal energyresources in India. These resources aredistributed in diverse physiographic and tectonicsettings, viz., <strong>the</strong> Himalayan belt and <strong>the</strong>Precambrian shield. Detailed geological andgeochemical exploration followed by limitedgeophysical exploration and shallow drillinginvestigations up to a few hundred meters haveresulted in first-order geo<strong>the</strong>rmal models for <strong>the</strong>major hot spring zones in <strong>the</strong> country. However,development <strong>of</strong> <strong>the</strong> geo<strong>the</strong>rmal resources hasremained at a very low level mainly due toinadequate characterization <strong>of</strong> <strong>the</strong> deeper <strong>the</strong>rmalregime leading to low confidence in proposedreservoir models and sustainability <strong>of</strong> <strong>the</strong> heatsource. There is <strong>the</strong>refore an urgent need to carryout a reassessment <strong>of</strong> <strong>the</strong> geo<strong>the</strong>rmal energypotential <strong>of</strong> hot springs by employing newgeophysical probing tools and computationaltechniques available today, both for electric powergeneration as well as for direct uses. Efficientexploitation technologies appropriate to nonvolcanicareas need to be developed. Systematicheat flow and heat production investigations needto be carried out for <strong>the</strong> identification <strong>of</strong> areaswhere high temperatures in <strong>the</strong> top few kilometersbelow <strong>the</strong> ground surface indicate potential for“hot sedimentary aquifers” as well as “enhancedgeo<strong>the</strong>rmal systems”. The vast potential forgeo<strong>the</strong>rmal heat pumps is yet to be tapped. 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India Memoir, v. 53, p.347-391.Rao, R.U.M., 1974, Gamma-ray spectrometricset-up at NGRI for analysis <strong>of</strong> U, Th and K inrocks : Geophys. Res. Bull., v.12, p.91-101.Rao, R.U.M., and Rao, G.V., 1979, Radiogeologicstudies at NGRI – A Review : Geophys. Res.Bull., v. 17, p. 163-173.Rao, R.U.M., 1997, Book review – Geo<strong>the</strong>rmalenergy in India, Pitale, U.L. and Padhi, R.N., eds.: J. Geol. Soc. India, v.49, p.746–748Roy, S., 2008, Heat Flow Studies in India during<strong>the</strong> past five decades: Geological Society <strong>of</strong> IndiaMemoir 68, p. 89-122. .Roy, S. and Rao, R.U.M., 1996, Regional heatflow and <strong>the</strong> perspective for <strong>the</strong> origin <strong>of</strong> hotsprings in <strong>the</strong> Indian shield, in Pitale, U.L., Padhi,R.N., eds., Geo<strong>the</strong>rmal <strong>Energy</strong> in India:Geological Survey <strong>of</strong> India, Special Publication45, p. 39–40.Roy, S. and Rao, R.U.M., 2000, Heat flow in <strong>the</strong>Indian shield: J. Geophys. Res., v.105, p.25,587-25,604.Roy, S. and Rao, R.U.M., 2003, Towards a crustal<strong>the</strong>rmal model for <strong>the</strong> Archaean Dharwar Craton,sou<strong>the</strong>rn India: Physics and Chemistry <strong>of</strong> <strong>the</strong>Earth, v.28, p.361-373.Roy, S., Ray L., Kumar, P.S., Reddy, G.K., andSrinivasan, R., 2003, Heat Flow and HeatProduction in <strong>the</strong> Precambrian Gneiss-GranuliteProvince <strong>of</strong> Sou<strong>the</strong>rn India, in M. Ramakrishnan,ed., Tectonics <strong>of</strong> Sou<strong>the</strong>rn Granulite Terrain –Kuppam-Palani Geotransect: Geological Society<strong>of</strong> India, Memoir 50, p.177-191.Roy, S., Ray, L., Bhattacharya, and Srinivasan,R., 2008, Heat flow and crustal <strong>the</strong>rmal structurein <strong>the</strong> Late Archaean Closepet Granite batholith,south India : Int. J. Earth Sci., v.97, doi:10.1007/s00531-007-0239-2, p.245-256.Sarolkar, P.B., and Sharma, S.K., 2002,Geo<strong>the</strong>rmal well testing at Tattapani geo<strong>the</strong>rmalfield, district Surguja, India: 27th Workshop onGeo<strong>the</strong>rmal Reservoir Engineering, StanfordUniversity, Stanford, California, Abstracts, SGP-TR-171Schlagintweit, R. de., 1865, Enumeration <strong>of</strong> HotSprings <strong>of</strong> India and High Asia : Journal <strong>of</strong> <strong>the</strong>Asiatic Society <strong>of</strong> Bengal, v. 33 (2), p. 51-73.Shanker R., Padhi, R.N., Arora, C.L., Prakash, G.,Thussu, J.L., and Dua, K.J.S., 1976, Geo<strong>the</strong>rmalexploration <strong>of</strong> Puga and Chumathang geo<strong>the</strong>rmalfields, Ladakh, India : Second U.N. Symposiumon <strong>the</strong> development and use <strong>of</strong> geo<strong>the</strong>rmalresources, San Francisco, Abstracts, p. 245-258.Sharma S., Nair, A.R., Kulkarni, U., Navada, S.V.,and Pitale, U.L., 1996, Isotope and geochemicalstudies in Tattapani geo<strong>the</strong>rmal area, districtSurguja, Madhya Pradesh, in Pitale UL and PadhiRN, eds, Geo<strong>the</strong>rmal <strong>Energy</strong> in India: GeologicalSurvey <strong>of</strong> India , Special Publication 45, p. 233-242.Singh, S.B., Drolia, R.K., Sharma, S.R., andGupta, M.L., 1983, Application <strong>of</strong> resistivitysurveying to geo<strong>the</strong>rmal exploration in <strong>the</strong> Pugavalley, India: Geoexploration, v. 21, p. 1-11.Thussu, J.L., Rao, S.M., Prasad, J.M., Navada,S.V., and Kulkarni, U., 1987, Isotope composition<strong>of</strong> <strong>the</strong>rmal and non-<strong>the</strong>rmal waters <strong>of</strong> Tattapanihot spring area, district Surguja, Madhya Pradesh:Geological Survey <strong>of</strong> India, Records, v.115, Pt.6,p. 56-65.80


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Queensland Coastal Geo<strong>the</strong>rmal <strong>Energy</strong> Initiative – An Approach to aRegional AssessmentBehnam Talebi 1 *, Mark Maxwell 1 , Sarah Sargent 1 and Steven Bowden 11 Mines and <strong>Energy</strong>, 80 Meiers Road, Indooroopilly QLD 4068.*Corresponding author: behnam.talebi@deedi.qld.gov.auThe best-known potential geo<strong>the</strong>rmal resources inQueensland are located beneath <strong>the</strong> Cooper-Eromanga Basins in <strong>the</strong> south-west <strong>of</strong> <strong>the</strong> state.The depth to <strong>the</strong> resources, and <strong>the</strong>ir distancefrom potential markets and <strong>the</strong> existing nationalelectricity grid, are <strong>the</strong> main challenges for <strong>the</strong>irdevelopment for power generation in <strong>the</strong> nearterm. The $5 million Coastal Geo<strong>the</strong>rmal <strong>Energy</strong>Initiative (CGEI) is <strong>the</strong> Queensland Government’sprogram to implement <strong>the</strong> commitment made in<strong>the</strong> ClimateSmart 2050 strategy through <strong>the</strong>Queensland Renewable <strong>Energy</strong> Fund toinvestigate additional sources <strong>of</strong> hot rocks forgeo<strong>the</strong>rmal energy close to existing transmissionlines and potential markets. The initiative is acooperative project between Office <strong>of</strong> Clean<strong>Energy</strong> and Geological Survey <strong>of</strong> Queensland(GSQ) and comprises a structured drillingprogram <strong>of</strong> shallow boreholes for <strong>the</strong> collection <strong>of</strong>new datasets to identify heat-flow anomaliesalong <strong>the</strong> east coast <strong>of</strong> Queensland. Target areashave been identified based on geological andgeophysical characteristics and have been rankedbased on <strong>the</strong>ir potential for a geo<strong>the</strong>rmalresource. The CGEI will reduce exploration risksand assist potential explorers to explore for anddevelop this source <strong>of</strong> clean energy inQueensland.Keywords: Queensland, geo<strong>the</strong>rmal exploration,drilling, heat flow, inversion modelling.ObjectivesThe main objectives <strong>of</strong> <strong>the</strong> CGEI are to identifyprospective areas along <strong>the</strong> east coast <strong>of</strong>Queensland and collect additional datasetsthrough a shallow drilling program. The purpose<strong>of</strong> this is firstly to increase knowledge <strong>of</strong> <strong>the</strong>crustal temperatures along <strong>the</strong> coast andsecondly to provide an enhanced assessment <strong>of</strong>geo<strong>the</strong>rmal resource potential by generating basicdatasets. This new data should assist geo<strong>the</strong>rmalexploration and development programs inQueensland.Heat Flow InvestigationA precise crustal heat-flow determination is <strong>the</strong>preferred method <strong>of</strong> identifying <strong>the</strong> geo<strong>the</strong>rmalprospectivity <strong>of</strong> a target area. Heat flow is <strong>the</strong>product <strong>of</strong> <strong>the</strong> temperature gradient and <strong>the</strong><strong>the</strong>rmal conductivity <strong>of</strong> rocks in <strong>the</strong> earth’s crust,and can be determined through <strong>the</strong> sampling andlogging <strong>of</strong> cored drill holes. A heat-flowinvestigation program has been planned as part <strong>of</strong><strong>the</strong> CGEI to evaluate <strong>the</strong> geo<strong>the</strong>rmal prospectivity<strong>of</strong> selected geological provinces along <strong>the</strong> eastcoast <strong>of</strong> Queensland.Drill Target SelectionThe potential occurrence <strong>of</strong> suitable heat sourceswithin basement was evaluated, based onavailable geophysical datasets and regionalgeological knowledge for each area. The maingeo<strong>the</strong>rmal source/reservoir targets are felsiccrystalline basement rocks such as granitoids andrhyolite with high <strong>the</strong>rmal conductivity values(generally greater than 4 Watt per meter Kelvin(W/mK)) and high radiogenic heat productionability (greater than 5 micro Watt per cubic meter(μW/m 3 )).Figure 1a: Location <strong>of</strong> CGEI drill targets in Central andSou<strong>the</strong>rn Queensland81


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Priority in <strong>the</strong> CGEI was given to geologicalprovinces where geo<strong>the</strong>rmal source/reservoirunits are overlain by a thick succession <strong>of</strong> <strong>the</strong>rmalblanketing sediments with harmonic mean <strong>the</strong>rmalconductivity values generally less than 3 W/mK.The assessment process involved a desktopanalysis <strong>of</strong> each geological province. Theprovinces were selected as <strong>the</strong>y were consideredlikely to have a high heat-flow or evidence <strong>of</strong>previous elevated temperatures. Existingtemperature data from available petroleum wellsin or adjacent to each geological province wereconsidered to infer subsurface temperaturegradients. The main obstacle to this approach hasbeen <strong>the</strong> variable data quality and availability ineastern Queensland where petroleum drilling isrelatively rare. The temperature gradients wereintegrated with <strong>the</strong> available geological andgeophysical data with <strong>the</strong> aim <strong>of</strong> identifyingpossible sources <strong>of</strong> heat at depth. Specifictargets were <strong>the</strong>n identified that would test <strong>the</strong>interpretation that this part <strong>of</strong> <strong>the</strong> geologicalprovince has geo<strong>the</strong>rmal potential.To date, forty-seven targets generally within100km <strong>of</strong> <strong>the</strong> existing national electricity grid havebeen identified with thirty-two being selected fordrilling. These targets are located from nearCairns in <strong>the</strong> north to <strong>the</strong> border <strong>of</strong> New SouthWales (Figures 1a, b).Figure 1b: Location <strong>of</strong> CGEI drill targets in Nor<strong>the</strong>rnQueenslandTechnical criteria were used to rank targets inorder <strong>of</strong> likelihood <strong>of</strong> <strong>the</strong> identification <strong>of</strong> ageo<strong>the</strong>rmal resource. The criteria were based on<strong>the</strong> nature <strong>of</strong> <strong>the</strong> basement and <strong>the</strong> <strong>the</strong>rmalblanketing sedimentary cover. All targets wereranked against <strong>the</strong>se criteria in order to establisha drilling priority. The final location <strong>of</strong> each drillhole was determined after consultation withlandholders and consideration <strong>of</strong> terrain condition,environmental and cultural heritage issues. Thespatial distribution <strong>of</strong> <strong>the</strong> holes effectively requireseach site to be considered as a drilling project inits own entity. Consequently, a substantialamount <strong>of</strong> extra work has been required to obtain<strong>the</strong> necessary clearances. Phase 1 drilling <strong>of</strong> <strong>the</strong>10 highest priority targets is scheduled tocommence in late <strong>2010</strong> (pending contractconfirmation).Geological SettingTraditionally, rifting margins have been identifiedas more prospective for geo<strong>the</strong>rmal energyexploitation. However, preliminary geologicalassessment <strong>of</strong> <strong>the</strong> geo<strong>the</strong>rmal potential <strong>of</strong> coastalQueensland shows a variety <strong>of</strong> tectonic settingsmay host high heat producing (HHP) granitesunder insulating cover sequences. Theassessment process resulted in <strong>the</strong> identification<strong>of</strong> five different geological settings which aresummarised in Table 1.Table 1: Geological Setting <strong>of</strong> CGEI TargetsAGE Geological Setting No. <strong>of</strong> CGEITargetsProterozoic Intercontinental rifting 5Ordovician-Silurian Thomson Orogen 4Early Carboniferous– Tasman Orogenic Zone 13Early PermianLate Permian – Mid Hunter Bowen Orogen 7TriassicLate Cretaceous -TertiaryCretaceous Rifting 3Intercontinental Rifting: The Proterozoic was atime <strong>of</strong> elevated heat flow causing <strong>the</strong>emplacement <strong>of</strong> voluminous granites andassociated volcanics in nor<strong>the</strong>rn Queensland(McLaren et al, 2003). These granites wereemplaced during multi-stage intracratonic riftingevents and in some areas <strong>the</strong>y are overlain bysedimentary basins which include <strong>the</strong> MillungeraBasin (no younger than Triassic, Figure 2) and <strong>the</strong>Jurassic - Late Cretaceous Carpentaria Basin.The heat production values <strong>of</strong> 5-9 µW/m 3 (GSQGeochemistry database, <strong>2010</strong>) from intrusives <strong>of</strong><strong>the</strong> Croydon Province and <strong>the</strong> Georgetown andMt Isa Inliers (including <strong>the</strong> Esmeralda, Forsaythand Williams Supersuites) delineate a prospectiveheat source at depth in <strong>the</strong>se areas. A number <strong>of</strong>geophysical tools including gravity, magnetic,magnetotelluric and radiometric ternary images aswell as sporadic drilling data were used to identify82


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>five targets which are considered worthy <strong>of</strong> fur<strong>the</strong>rinvestigation. These targets are found beneath<strong>the</strong> insulating units <strong>of</strong> <strong>the</strong> Karumba, Carpentariaand Millungera Basins and <strong>the</strong> Georgetown Inlier(Figure 1b).Figure 2: Millungera Basin CGEI rationale, showing gravityresponse (Bouguer), location and extent <strong>of</strong> outcroppingProterozoic intrusives and high heat producing rocksThomson Orogen: Ano<strong>the</strong>r region <strong>of</strong> outcroppingpotentially HHP granites is located within <strong>the</strong>basement packages <strong>of</strong> <strong>the</strong> Ordovician-SilurianThomson Orogen. The heat production values <strong>of</strong>I-type and S-type granites are generally greaterthan 5 µW/m 3 . If properly insulated, <strong>the</strong>se graniteswould provide a geo<strong>the</strong>rmal heat source at depth.A geophysical and geological assessmentidentified <strong>the</strong> western and sou<strong>the</strong>rn Bowen Basin,eastern Drummond Basin,and <strong>the</strong> Burdekin Basin,as target areas, as inferred HHP granites arepresent in <strong>the</strong> basement complexes <strong>of</strong> <strong>the</strong>sebasins with Tertiary volcanics, which couldindicate an additional, younger contributing heatsource.Tasman Orogenic Zone: The Carboniferous-Permian intrusions <strong>of</strong> <strong>the</strong> Tasman Orogenic Zone(which encompasses <strong>the</strong> Nor<strong>the</strong>rn TasmanOrogenic Zone and <strong>the</strong> New England Orogen)contain medium to high concentrations <strong>of</strong> <strong>the</strong>radiogenic elements uranium, thorium andpotassium and should be prospective forgeo<strong>the</strong>rmal energy potential. Within <strong>the</strong> Nor<strong>the</strong>rnTasman Orogenic Zone, <strong>the</strong> Carboniferous–Permian Wypalla Supersuite and <strong>the</strong> PurkinGranite have heat production values between 3.5-8.55 µW/m 3 (GSQ Geochemistry database,<strong>2010</strong>). The heat production potential <strong>of</strong> <strong>the</strong>seintrusive units at depth in conjunction with a goodinsulating capacity and thickness <strong>of</strong> overlyingcover sequences have identified three targetswithin <strong>the</strong> Hodgkinson Province, nor<strong>the</strong>rnEromanga Basin and Camel Creek Province. Theexistence <strong>of</strong> anomalous heat flow within <strong>the</strong>Hodgkinson Province in particular can be inferredby <strong>the</strong> Innot hot spring which has a surfacetemperature <strong>of</strong> 71°C (Lottermoser & Cleverley,2007). This spring is located in <strong>the</strong> sou<strong>the</strong>rn part<strong>of</strong> <strong>the</strong> province.The New England Orogen contains numerous I-type and S-type intrusions and associated felsicvolcanics. Whole rock geochemical analyses <strong>of</strong><strong>the</strong>se units indicate medium concentrations <strong>of</strong>potassium, thorium and uranium. As a result <strong>the</strong>geological and geophysical assessmentsundertaken delineated where <strong>the</strong>se intrusivesextend at depth underneath insulating basins. Theoverlying insulating sedimentary packages includeoil shale units <strong>of</strong> <strong>the</strong> Duaringa Basin andextensive coal measures <strong>of</strong> <strong>the</strong> Bowen, Clarence-Moreton and Styx Basins. Nine sites wereselected for heat flow determinations including <strong>the</strong>Bulgonnuna Volcanics, Lizzie Creek Volcanics,Bowen Basin, Roma Granite, Styx Basin,Duaringa Basin, western Clarence Moreton Basin(Jandowae) and Inglewood (Figure 1a).Hunter Bowen Orogen: The onset <strong>of</strong> <strong>the</strong> Permian-Triassic Hunter Bowen Orogen initiated <strong>the</strong>widespread emplacement <strong>of</strong> granites along <strong>the</strong>New England Fold Belt. Elevated heat is likely as<strong>the</strong> granitic outcrops generally have heatproduction values greater than 5 µW/m 3 . Gravity,seismic and magnetotelluric datasets suggest<strong>the</strong>se potentially HHP granites extend at depthunderneath <strong>the</strong> cover <strong>of</strong> <strong>the</strong> Tarong, Mulgildie,Clarence-Moreton, Galilee and MaryboroughBasins, which all contain coal measures. A moredetailed geological and geophysical assessment<strong>of</strong> <strong>the</strong>se basins identified seven target sites asprospective for elevated heat flow namely <strong>the</strong>Thunderbolt Granite, Tarong Basin, easternClarence-Moreton Basin, Mulgildie Basin,Stanthorpe Granite, Barcaldine and nor<strong>the</strong>rnMaryborough Basin (Figures 1a and 3).Cretaceous Rifting: The Cretaceous saw <strong>the</strong>cessation <strong>of</strong> <strong>the</strong> active convergent margin along<strong>the</strong> east <strong>of</strong> <strong>the</strong> <strong>Australian</strong> continent and <strong>the</strong>initiation <strong>of</strong> rifting <strong>of</strong> <strong>the</strong> Tasman and Coral Seas.Cretaceous granites lining <strong>the</strong> western edge <strong>of</strong><strong>the</strong> Maryborough Basin (Figure 3) may be aprospective geo<strong>the</strong>rmal target. The sedimentthickness <strong>of</strong> <strong>the</strong> overlying Maryborough Basin isup to 3400m with two significant coal sequences,Tiaro Coal Measures and Burrum Coal Measures,forming an excellent insulator to any potentialheat producing intrusive at depth.The Hillsborough Basin (Figure 4) and NarrowsGraben sites primarily target <strong>the</strong> more nor<strong>the</strong>rnCretaceous intrusions. These two sites may alsobenefit from additional heat sources associatedwith intrusions and related volcanics <strong>of</strong> <strong>the</strong> Late83


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Cretaceous Whitsunday Large Igneous Province.In addition, volcanics resulting from Tertiary riftingand intraplate volcanism suggest that <strong>the</strong>re stillmay be significant heat production in this area.The insulating capacity <strong>of</strong> <strong>the</strong> Hillsborough Basinand Narrows Graben sequences is considered tobe good due to <strong>the</strong> presence <strong>of</strong> significantintervals <strong>of</strong> oil shale.Sampling is to be undertaken at <strong>the</strong> drill siteimmediately after <strong>the</strong> core has been logged.Each sample is enclosed in plastic wrap topreserve <strong>the</strong>ir in-situ fluid saturation levels prior todispatch to a laboratory. Visual assessment <strong>of</strong> <strong>the</strong>downhole geology (lithological log) against <strong>the</strong>temperature log will also be used as a tool forfur<strong>the</strong>r sampling in case additional <strong>the</strong>rmalconductivity analyses are required at a later stage(Figure 5).Figure 3: Maryborough Basin CGEI rationale, showinggravity response (Bouguer), location and extent <strong>of</strong> Jurassic-Cretaceous and Permian-Triassic outcropping intrusivesDrilling Program and Data CollectionAn effective heat-flow determination processrequires a shallow (300–500m) drill hole, suitablycompleted to enable a temperature log to beacquired that accurately records <strong>the</strong> temperaturein lithological units intersected. In order to get anaccurate temperature log <strong>the</strong> hole needs toremain undisturbed for sufficient time (typically 5–8 weeks) to minimise any remaining drillinginducedtemperature disturbances and essentiallyensure that <strong>the</strong> downhole temperature isadequately re-equilibrated. Each well is <strong>the</strong>n<strong>the</strong>rmally logged from <strong>the</strong> surface to <strong>the</strong> bottom <strong>of</strong><strong>the</strong> hole by measuring a temperature at specificintervals (typically every 1 meter). From <strong>the</strong>semeasurements, temperature gradients can becalculated for <strong>the</strong> corresponding intervals down<strong>the</strong> hole.The hole should also be continuously cored from<strong>the</strong> base <strong>of</strong> unconsolidated units to total depth(~320m) to recover at least 200-250 meters <strong>of</strong>continuous core enabling samples to be takenand analysed for <strong>the</strong>rmal conductivity propertiesin order to establish a <strong>the</strong>rmal conductivity pr<strong>of</strong>ilefor <strong>the</strong> hole. Core samples are usually taken atregular intervals, typically every 10 metres.Figure 4: Hillsborough Basin CGEI rationale, showing gravityresponse (Bouguer), ternary radiometric image, location andextent <strong>of</strong> outcropping Carboniferous and CretaceousintrusivesThe CGEI drilling program is likely to consist <strong>of</strong> upto 32 HQ size shallow boreholes to a nominaldepth <strong>of</strong> ~320 metres cased with continuous PVC.The hole design and completion have been84


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>optimised to ensure that a high quality datacollection process is attained throughout <strong>the</strong>program (Figure 6). A call for tender was releasedin June <strong>2010</strong> for <strong>the</strong> selection <strong>of</strong> drillingcontractors. Geophysical downhole logs such asResistivity, Spontaneous Potential (SP) andGamma Ray are being run on an “as–required”basis with <strong>the</strong> aim <strong>of</strong> determining possible aquiferleakage into <strong>the</strong> hole that may interfere with <strong>the</strong>temperature pr<strong>of</strong>ile and also for data qualitychecking purposes.a purely conductive regime and <strong>the</strong>refore aconstant heat flow across all lithological unitsintersected. From <strong>the</strong> global heat-flow database,<strong>the</strong> mean surface heat flow <strong>of</strong> <strong>the</strong> <strong>Australian</strong>continent is approximately 65 mW/m 2 , so areaswith heat-flow values greater than this mayindicate promising areas for fur<strong>the</strong>r geo<strong>the</strong>rmalinvestigation and exploration activities providedthat <strong>the</strong> <strong>the</strong>rmal resistance <strong>of</strong> <strong>the</strong> overlyinglithological units is sufficient to support presence<strong>of</strong> economical temperature at depth.Considering <strong>the</strong> spatial coverage <strong>of</strong> <strong>the</strong> CGEI,one dimensional inversion modelling <strong>of</strong> <strong>the</strong>conductive heat-flow regime in <strong>the</strong> vicinity <strong>of</strong> eachborehole is to be undertaken using <strong>the</strong> newtemperature and <strong>the</strong>rmal conductivity datasetscollected (Figure 7). Modelled data will <strong>the</strong>n beextrapolated to 5 km, <strong>the</strong> economic drilling depthfor most geo<strong>the</strong>rmal resources, to predicttemperatures at this depth range. Generally,temperatures <strong>of</strong> greater than 200°C are expectedat such depths for Engineered Geo<strong>the</strong>rmalSystem (EGS) to be commercially viable forelectricity generation.Figure 5: Example <strong>of</strong> a temperature log versus lithological logHeat-Flow ModellingMa<strong>the</strong>matically, <strong>the</strong> average vertical conductiveheat flow at <strong>the</strong> earth’s surface, q (in W/m 2 ), canbe calculated using <strong>the</strong> Fourier expression:q k.dTdzWhere (k) is <strong>the</strong> rock <strong>the</strong>rmal conductivity (inW/mK) at depth z, and (dT/dz) is <strong>the</strong>corresponding vertical temperature gradient (inK/m) over <strong>the</strong> same interval. As shown by <strong>the</strong>equation, <strong>the</strong> temperature gradient has an inverserelationship with <strong>the</strong>rmal conductivity (onedecreases as <strong>the</strong> o<strong>the</strong>r increases). This assumesFigure 6: Schematic borehole designIn addition, depth predictions <strong>of</strong> <strong>the</strong> 100, 150 and200°C iso<strong>the</strong>rms may be approached dependingon data availability for estimating <strong>the</strong> formationsintersected at those iso<strong>the</strong>rm depths. This willassist in <strong>the</strong> assessment <strong>of</strong> <strong>the</strong> prospectivity <strong>of</strong>each target area for ei<strong>the</strong>r Hot SedimentaryAquifer (HSA) or Engineered Geo<strong>the</strong>rmal System(EGS) development in <strong>the</strong> future.CollaborationCollaboration with o<strong>the</strong>r government agencies,research centres and industry is an important part85


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong><strong>of</strong> this initiative. In this respect, GeoscienceAustralia will provide technical support to <strong>the</strong>CGEI by providing down-hole temperature loggingand laboratory analysis services through anagreement under <strong>the</strong> National GeoscienceAccord. Fur<strong>the</strong>rmore, additional research over <strong>the</strong>CGEI target areas has been discussed throughcollaboration with <strong>the</strong> Queensland Geo<strong>the</strong>rmal<strong>Energy</strong> Centre <strong>of</strong> Excellence (QGECE) based at<strong>the</strong> University <strong>of</strong> Queensland through postgraduateresearch studies.Figure 7: Example <strong>of</strong> 1D inversion heat flow modellingFuture WorkFuture work that would contribute to a betterunderstanding <strong>of</strong> geo<strong>the</strong>rmal prospectivity ineastern Queensland would include <strong>the</strong> collection<strong>of</strong> new heat-flow data at a closer spacing forprospective areas identified from <strong>the</strong> CGEI. Anassessment <strong>of</strong> current regional and local in-situstress fields in those areas could also beundertaken to evaluate <strong>the</strong> susceptibility <strong>of</strong>potential reservoir rock to <strong>the</strong> artificial permeabilityenhancement process.SummaryThe Coastal Geo<strong>the</strong>rmal <strong>Energy</strong> Initiative is <strong>the</strong>Queensland Government’s program for identifyingsources <strong>of</strong> hot rocks for geo<strong>the</strong>rmal energy closeto existing national electricity grid and potentialmarkets along <strong>the</strong> east coast <strong>of</strong> Queensland. Theinitiative will be implemented through a structureddrilling program <strong>of</strong> up to 32 shallow boreholes witha nominal depth <strong>of</strong> ~320 metres to collect newtemperature and heat-flow datasets. The majoraim <strong>of</strong> <strong>the</strong> initiative will be to increase knowledge<strong>of</strong> <strong>the</strong> crustal temperatures in selected geologicalsettings along <strong>the</strong> coast and provide backgrounddata for industry that would consequentlystimulate exploration activities for geo<strong>the</strong>rmalenergy in Queensland. It is anticipated that finalresults <strong>of</strong> <strong>the</strong> initiative will be publically availableby <strong>the</strong> middle <strong>of</strong> year 2012.AcknowledgementsThe authors wish to acknowledge staff from o<strong>the</strong>rGSQ units who are strongly supporting <strong>the</strong>implementation <strong>of</strong> <strong>the</strong> Coastal Geo<strong>the</strong>rmal <strong>Energy</strong>Initiative by any means and in every aspect.ReferencesBeardsmore, G. R., and Cull, J. P., 2001, CrustalHeat Flow: A Guide to Measurement andModelling, Cambridge University Press, 324pp.Cull, J. P. and Beardsmore, G. R., 1992,Statistical methods for estimates <strong>of</strong> heat flow inAustralia, Journal <strong>of</strong> Exploration Geophysics 23,p. 83-86.Denaro, T. and Dhnaram, C. (Compilers), 2009,Queensland Minerals 2009. A Summary <strong>of</strong> majormineral resources, mines and projects.Department <strong>of</strong> Mines and <strong>Energy</strong>, 87pp.Fitzell, M., Hamilton, S., Beeston, J., Cranfield, L.,Nelson, K., Xavier, C. and Green P., 2009,Approaches for identifying geo<strong>the</strong>rmal energyresources in coastal Queensland, <strong>Proceedings</strong> <strong>of</strong><strong>the</strong> 2009 <strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong><strong>Conference</strong>, 6pp.McLaren, S., Sandiford, M., hand, M., Neumann,N., Wyborn, L. and Bastrakova, I., 2003, The hotsou<strong>the</strong>rn continent: heat flow and heat productionin <strong>Australian</strong> Proterozoic terranes, In: Hillis R.R. &Müller R.D. eds. Evolution and Dynamics <strong>of</strong> <strong>the</strong><strong>Australian</strong> Plate, Geological Society <strong>of</strong> AustraliaSpecial Publication 22.Murray, C., 2003. Granites <strong>of</strong> <strong>the</strong> nor<strong>the</strong>rn NewEngland Orogen, in BLEVIN, P., JONES, M., &CHAPPELL, B., editors, Magmas toMineralisation: The Ishihara Symposium,Geoscience Australia, Record 2003/14, 19-24.Rybach, L., 1989, Heat flow techniques ingeo<strong>the</strong>rmal exploration, First Break Vol. 7, No.1,p. 9-16.Somerville, M., Wyborn, D., Chopra, P., Rahman,S., Estrella, D. and Van der Meulen, T., 1994, HotDry Rocks Feasibility Study, <strong>Energy</strong> Researchand Development Corporation, Report 243,133pp.Webb, A. W. and McDougall, Ian, 1968, Thegeochronology <strong>of</strong> <strong>the</strong> igneous rocks <strong>of</strong> EasternQueensland, <strong>Australian</strong> Journal <strong>of</strong> EarthSciences, 15: 2, 313 — 346.86


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Geo<strong>the</strong>rmal Exploration in Victoria, AustraliaDavid H Taylor, Ben Harrison, Michelle Ayling, Kate BassanoGeoScience Victoria, GPO Box 4440, Melbourne, Victoria, AustraliaCorresponding author: david.taylor@dpi.vic.gov.auGeo<strong>the</strong>rmal energy is keenly sought as asustainable, low emissions energy source forVictoria. Exploration companies have been activesince 2006 looking for geo<strong>the</strong>rmal systems wheretemperatures <strong>of</strong> greater than 150 C would allowelectricity generation. Initial exploration waslargely guided by legacy temperature data ingroundwater and petroleum bores but lots <strong>of</strong>dedicated heat flow data is now being acquired,including a State-wide program by <strong>the</strong>government. Active volcanic systems are notpresent but <strong>the</strong>re is good potential for hotsedimentary aquifers already known from <strong>the</strong>legacy data. O<strong>the</strong>r heat sources such asPalaeozoic radioactive granites or residualmagmatic heat from recent basaltic volcanism arepossible but data is very limited. As explorationprogresses, a number <strong>of</strong> different geo<strong>the</strong>rmal playtypes across <strong>the</strong> various heat sources are beinginvestigated. A number <strong>of</strong> inferred resourceshave already been declared, in preparation fordeep appraisal drilling.Keywords: Hot Sedimentary Aquifer, Heat Flow,geo<strong>the</strong>rmalVictorian geo<strong>the</strong>rmal backgroundThe oil shocks <strong>of</strong> <strong>the</strong> 1970’s piqued interest intoalternate energy sources. Town water suppliesbeing drawn from thick Cretaceous-Tertiarybasins along <strong>the</strong> Victorian coast at that time,showed temperatures <strong>of</strong> about 50-90 C at 1-2 kmdepth. The potential <strong>of</strong> direct use <strong>of</strong> this hot waterwas investigated (King et al., 1987). Petroleumexploration in <strong>the</strong> same area also occasionallyintersected deeper basin aquifers withtemperatures <strong>of</strong> about 130-150 C at 3.5-4 kmdepth (Woollands and Wong, 2001).Low oil prices throughout <strong>the</strong> 1990’s suppressedinterest in alternate energy sources but <strong>the</strong> return<strong>of</strong> higher prices and concerns around greenhousegas emissions have again sparked interest ingeo<strong>the</strong>rmal energy. Dedicated legislation was putin place in 2005 and a grid <strong>of</strong> large explorationpermit blocks was established across <strong>the</strong> State.Exploration companies took up many <strong>of</strong> <strong>the</strong>permits in two rounds <strong>of</strong> tenders over 2006 and2008. About two thirds <strong>of</strong> <strong>the</strong> State is now underexploration for <strong>the</strong> next 3-4 years by sevencompanies with work plan commitments <strong>of</strong>approximately $365M.Victorian Geo<strong>the</strong>rmal DataTo support <strong>the</strong> tender bidding process for permits,a preliminary review <strong>of</strong> geo<strong>the</strong>rmal prospectivitywas published by <strong>the</strong> State government geologyorganisation (Driscoll, 2006). This report includeda compilation <strong>of</strong> about 300 temperature datapoints from pre-existing groundwater andpetroleum bores but <strong>the</strong> accuracy and precision <strong>of</strong>much <strong>of</strong> <strong>the</strong> petroleum temperature data forgeo<strong>the</strong>rmal assessments is questionable.A handful <strong>of</strong> heat flow calculations from precisiontemperature logging and rock conductivityanalysis already existed as a result <strong>of</strong> academicstudies since <strong>the</strong> 1970s. Many <strong>of</strong> <strong>the</strong> geo<strong>the</strong>rmalexploration companies have started collectingmuch more <strong>of</strong> this dedicated type <strong>of</strong> geo<strong>the</strong>rmaldata. To accelerate this type <strong>of</strong> work <strong>the</strong> Stategovernment has undertaken a data collectionprogram for heat flow.The Victorian Heat Flow MapIn 2009-10 <strong>the</strong> State government commissioned aone year $500,000 project to generate a Statewideheat flow map. Over <strong>the</strong> year, this projecthas compiled <strong>the</strong> existing academic and companydata, plus collected new data, to generate over100 heat flow measurements that give goodcoverage over much <strong>of</strong> <strong>the</strong> State. Data points aregenerally close enough toge<strong>the</strong>r (ideally closertoge<strong>the</strong>r than <strong>the</strong> crust is thick: about 40 km) sothat interpolation <strong>of</strong> <strong>the</strong> point data into a mapshould still have regional scale meaning.GeoScience Victoria directly collected boreholetemperature pr<strong>of</strong>iles in <strong>the</strong> sou<strong>the</strong>rn Murray Basinand across <strong>the</strong> Otway Basin using its owntemperature logging unit. As part <strong>of</strong> <strong>the</strong> NationalGeo<strong>the</strong>rmal <strong>Energy</strong> Project (Budd et al., 2009)GeoScience Australia collected temperature datafrom <strong>the</strong> nor<strong>the</strong>rn Murray Basin using <strong>the</strong>irtemperature logging unit. GeoScience Victoria isalso working collaboratively with MelbourneUniversity who have collect data from <strong>the</strong>Gippsland basin. The exploration companies in<strong>the</strong> Gippsland Basin have also collected a fairamount <strong>of</strong> new temperature data in that regionand made it available. Several recentunpublished honours <strong>the</strong>sis and some additionaltemperature logging for GeoScience Victoriaundertaken by Hot Dry Rocks add fur<strong>the</strong>r data to<strong>the</strong> previous handful <strong>of</strong> heatflow measurementsthat was all that was available several years ago.87


About 200 conductivity analyses have beenperformed by Hot Dry Rocks on samples from <strong>the</strong>boreholes measured for temperature. This dataallows reasonably precise heat flow calculationsto be generated. Heat flow modelling for datafrom completely new holes was undertaken byHot Dry Rocks. The various pre-existing honours<strong>the</strong>sis and company work was remodelled byGeoScience Victoria using consistently appliedmethodology and better informed conductivitiesstemming from <strong>the</strong> new sampling.This regional scale appraisal <strong>of</strong> heat flow, whencombined with analysis <strong>of</strong> thickness <strong>of</strong> basincover, will help show ‘where it is hot and where itis not’. The map will help companies direct <strong>the</strong>irpermit scale efforts, as well as informinggovernment policy on geo<strong>the</strong>rmal resourcepotential.This work is still in progress and thus currentassessments <strong>of</strong> Victoria’s geo<strong>the</strong>rmal potentialstill rely on looking at geological factors.<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Geological Framework for geo<strong>the</strong>rmalpotentialGeo<strong>the</strong>rmal potential depends on <strong>the</strong> interaction<strong>of</strong> a number <strong>of</strong> geological factors. The bestresources are likely to exist in regions where highheat flow passes through rocks <strong>of</strong> low conductivity(good insulation) to create high temperature atshallow depth (Duffield & Sass, 2003).The recent publication <strong>of</strong> a more completegeo<strong>the</strong>rmal systems assessment framework(Cooper & Beardsmore, 2008) outlines that inaddition to (1) <strong>the</strong> heat producing basement (2) aninsulating blanket; <strong>the</strong>re needs to be (3) a fluidavailable to extract and move <strong>the</strong> heat; and (4) areservoir to accommodate <strong>the</strong> fluid.Applying this four factor analysis to <strong>the</strong> majorgeological provinces <strong>of</strong> Victoria gives some idea<strong>of</strong> <strong>the</strong>ir relative geo<strong>the</strong>rmal prospectivity. Thebroad diversity in <strong>the</strong> age and types <strong>of</strong> rocksacross Victoria (Figure 1) gives some potential forall three types <strong>of</strong> geo<strong>the</strong>rmal systems: Hot Rock;Hot Sedimentary Aquifer; and Magmatic.Figure 1: Geological geo<strong>the</strong>rmal province map88


Three broad geological/geo<strong>the</strong>rmal provinces canbe delineated across Victoria: (1) The Palaeozoicbedrock (2) <strong>the</strong> onshore Otway and GippslandBasins and (3) <strong>the</strong> Murray Basin.The Palaeozoic bedrock consists predominantly<strong>of</strong> Cambrian to Devonian deep marine muddysiliciclastics that have been tightly folded andcleaved at various times in <strong>the</strong> Palaeozoic (blues,browns and purples <strong>of</strong> Figure 1). This bedrockalso underlies <strong>the</strong> o<strong>the</strong>r provinces and thus givesgood insight into <strong>the</strong> potential <strong>of</strong> <strong>the</strong>ir heatproducing basement. Numerous granites intrudethis bedrock (red blobs on Figure 1). In west andcentral Victoria some <strong>of</strong> <strong>the</strong>m have felsic,fractionated geochemistry with mild enrichment inheat producing elements, so Hot Rock plays maybe possible where granites lie buried within <strong>the</strong>bedrock or beneath <strong>the</strong> adjacent basins. In <strong>the</strong>southwest, an extensive province <strong>of</strong> youngbasalts has erupted onto <strong>the</strong> bedrock in <strong>the</strong> lastfew million to tens <strong>of</strong> thousands <strong>of</strong> years (<strong>the</strong> lightpink in Figure 1). Teleseismic data suggests amantle hot spot still underlies this recentvolcanism (Graeber et al., 2002). In addition to anincreased mantle heat flow contribution acrossthis region, <strong>the</strong>re may be some residual magmaticheat in <strong>the</strong> crust from <strong>the</strong> volcanic activity to allowMagmatic geo<strong>the</strong>rmal plays.The Onshore Otway and Gippsland Basins areCretaceous rift basins associated with Gondwanabreak-up (greens and yellow along coast in Figure1). These basins are well characterised thanks toa long history <strong>of</strong> petroleum exploration with manydeep wells. They contain several kilometres <strong>of</strong>muddy sediments overlying a coarser grainedbasal unit. This basal unit provides a naturalreservoir already charged with hot water beneathan insulating blanket to create an attractivefairway for Hot Sedimentary Aquifer plays. In <strong>the</strong>Otways this basal unit has been intersected upon<strong>the</strong> basin floor but in <strong>the</strong> Gippsland basin this unithas yet to be tested away from <strong>the</strong> margins, at <strong>the</strong>depths necessary for a geo<strong>the</strong>rmal play. Beneath<strong>the</strong>se basins <strong>the</strong>re is also potential for Hot Rockplays in places where <strong>the</strong>y are floored by granites.The Murray Basin is a Tertiary intracratonic sagbasin (light greens and yellow inland in Figure 1).It generally contains only a few hundred metres <strong>of</strong>sandy marly cover. This is insufficient cover toact as a heat blanket but in some places deepertroughs – such as <strong>the</strong> Wentworth, Ne<strong>the</strong>rby,Numurkah and Ovens - exist and can contain upto a couple <strong>of</strong> kilometres <strong>of</strong> sediment that is poorlyknown since <strong>the</strong>re has been limited petroleumexploration here. Alignment <strong>of</strong> favourable factorsover <strong>the</strong> deeper troughs may allow Hot Rock orHot Sedimentary Aquifer plays but <strong>the</strong>favourability <strong>of</strong> <strong>the</strong> geo<strong>the</strong>rmal factors in thisprovince has yet to be validated.<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Pathways to Resource DevelopmentIn <strong>the</strong> absence <strong>of</strong> detailed, dedicated geo<strong>the</strong>rmaldata, most <strong>of</strong> Victoria can be viewed as ‘blue sky’or perhaps ‘green fields’ at best, in those areaswhere some legacy petroleum data exists. Thenew heat flow map and better characterisation <strong>of</strong>rock <strong>the</strong>rmal insulation (conductivities) will providea new level <strong>of</strong> interpretation on prospectivity.Most <strong>of</strong> <strong>the</strong> Victorian geo<strong>the</strong>rmal explorers aresmall companies with limited amounts <strong>of</strong> capitaland cash-flow to fund <strong>the</strong>ir 5 year explorationprograms. Ideally, as <strong>the</strong>se companies collectinformation and decrease risks and unknowns,<strong>the</strong>y could call for more capital through ei<strong>the</strong>r debtor equity raisings until it becomes probable that amajor backer would farm-in for development. TheGlobal Financial Crisis has badly affected thistraditional venture capital pathway through toresource development.At <strong>the</strong> national level <strong>the</strong> Federal government hascommitted a significant amount <strong>of</strong> funds into ageoscience investigation program and also put upmoney for co-funding deep appraisal drilling. If<strong>the</strong>se drilling appraisals lead to early success,<strong>the</strong>n perceived risks around geo<strong>the</strong>rmal energymay be reduced and allow easier funding for <strong>the</strong>whole industry from <strong>the</strong> more traditional pathway.The State government has also <strong>of</strong>feredsubstantial funds towards industry assistance forshallow and deep drilling plus contingent moneyfor demonstration power plants.Company announcements around InferredResources and/or conceptual targets suggest thatseveral thousand MW <strong>of</strong> electricity generationmay be possible but it is still early days for <strong>the</strong>geo<strong>the</strong>rmal industry in Victoria.ReferencesBudd, A.R., Holgate, F.L., Gerner, E.J., Ayling,B.F. & Barnicoat, A.C., 2009, Pre-competitivegeoscience for geo<strong>the</strong>rmal exploration anddevelopment in Australia: GeoscienceAustralia's Onshore <strong>Energy</strong> Security Program.<strong>Proceedings</strong>, <strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong><strong>Conference</strong>, Brisbane, Australia.Cooper, G.T. & Beardsmore, G.R., 2008,Geo<strong>the</strong>rmal systems assessment:understanding <strong>the</strong> risks in geo<strong>the</strong>rmalexploration in Australia. <strong>Proceedings</strong>, Eastern<strong>Australian</strong> Basins Symposium III, Sydney,Australia.Driscoll, J., 2006, Geo<strong>the</strong>rmal propsectivity <strong>of</strong>onshore Victoria, Australia. VIMP Report 85.GeoScience Victoria.Duffield, W.A. & Sass, J.H., 2003, Geo<strong>the</strong>rmalenergy: Clean power from <strong>the</strong> earth's heat.Circular, U. S. Geological Survey 1249.Graeber, F.M., Houseman, G.A. & Greenhalgh,S.A., 2002, Regional teleseismic tomography<strong>of</strong> <strong>the</strong> western Lachlan Orogen and <strong>the</strong> Newer89


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Volcanic Province, sou<strong>the</strong>ast Australia.Geophysical Journal International, v. 149,249-266.King, R.L., Ford A.J., Stanley, D.R., Kenley, P.R.,& Cecil, M.K., 1987, Geo<strong>the</strong>rmal Resources <strong>of</strong>Victoria, Department <strong>of</strong> Industry, Technologyand Resources and Victorian Solar <strong>Energy</strong>Council, Melbourne.Woollands, M.A., & Wong, D., (eds.) 2001,Petroleum Atlas <strong>of</strong> Victoria, Australia,Department <strong>of</strong> Natural Resources andEnvironment.90


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Geochemistry <strong>of</strong> silica rocks in <strong>the</strong> Drummond Basin as a record <strong>of</strong>geo<strong>the</strong>rmal potentialI. Tonguç Uysal* 1 , Alexander W. Middleton 1 , Robert Bolhar 2 , and Massimo Gasparon 2Queensland Geo<strong>the</strong>rmal <strong>Energy</strong> Centre <strong>of</strong> Excellence, The University <strong>of</strong> Queensland, Brisbane, QLD. 4072* 1Department <strong>of</strong> Earth Sciences, The University <strong>of</strong> Queensland, Brisbane, QLD. 4072 2Silica is <strong>the</strong> most abundant mineral in <strong>the</strong> Earth’supper crust; yet its trace element composition hasnot been utilised routinely in <strong>the</strong> exploration <strong>of</strong>natural resources. Siliceous sinters are pristinerocks that precipitate at <strong>the</strong> surface from springwaters heated by deep-seated magma chambers.They can be useful indicators <strong>of</strong> hot radioactivemagmatic basements in sedimentary basins.However, distinguishing silica sinters from o<strong>the</strong>rsiliceous lithologies is <strong>of</strong>ten ambiguous becausesiliceous lithologies <strong>of</strong> various origins occurubiquitously on <strong>the</strong> ground surface as rock chipsor soil material eroded from deeper geologicalunits. In this study, we characterise trace elementcompositions <strong>of</strong> silica sinters to providegeochemical criteria for exploration <strong>of</strong> geo<strong>the</strong>rmalenergy sources. We investigated silica sinters and<strong>the</strong> associated hydro<strong>the</strong>rmal quartz veins,volcanic rocks, silicified hydro<strong>the</strong>rmal breccias,alteration minerals, and some soil samples from<strong>the</strong> Paleozoic Drummond Basin, Australia by ICP-MS trace element analysis.Keywords: Sinter, quartz, geochemistry,geo<strong>the</strong>rmal, Drummond Basin, Galilee BasinSamplingSamples for this study were collected from <strong>the</strong>Twin Hills area hosting high-grade epi<strong>the</strong>rmal goldresource, 309 and Lone Sister (BMA componyreport). Location 309 mine is a fault-boundedarea characterised by <strong>the</strong> occurrence <strong>of</strong> a silicifiedbreccia system capped by sinter deposits,whereas Lone Sister represents a rhyolite dome.The textual features <strong>of</strong> <strong>the</strong> sinters at 309 are verysimilar to those <strong>of</strong> sinters from o<strong>the</strong>r locations in<strong>the</strong> Drummond Basin (Cunneen and Sillitoe,1989; White et al., 1989). They are welllaminated(from white through gray to orangebrown),consisting <strong>of</strong> dense and vitreouschalcedony.Results and implicationsThe Drummond Basin sinters and quartz veinsare unique in having anomalously enrichedincompatible element (Cs, Li, Be, W, U, Th andrare earth elements) concentrations incomparison to hydro<strong>the</strong>rmal quartz veins fromvarious granitic-pegmatitic systems elsewhere in<strong>the</strong> world (Figure 1). Bonding factors such as ionicsize and charge are <strong>the</strong> main factors controlling<strong>the</strong> distribution <strong>of</strong> elements in precipitatingcrystals. Large-ion lithophile elements (LILE, e.g.Rb, Cs), large highly charged cations (e.g. W 6+ ,U 4+ ) and small variable charged cations (e.g. Be,Li ) are usually prevented from being incorporatedinto crystalline phases during early magmaticprocesses (Strong, 1981). Hence <strong>the</strong>seincompatible elements tend to concentrate inresidual melts with high concentrations <strong>of</strong> fluidsand volatiles, which commonly occurs duringpegmatitic stages <strong>of</strong> granite magmatism. It haslong been recognised that that Cs, Li, Rb, Be (<strong>the</strong>alkali and alkaline earth elements) can be quitemobile during water/rock interaction (Nesbitt andMarkovics, 1997; Nesbitt and Young, 1989).Tracing such elements can thus be used as ageochemical tool for locating areas <strong>of</strong>hydro<strong>the</strong>rmal convection cells interacting withdeep heat-producing granitic rocks. Alkali mobileelement concentrations are divided byconcentration <strong>of</strong> most immobile elements such asLu to compare alkali element mobility (Fig. 2). Themajority <strong>of</strong> sinter and quartz samples within ornear <strong>the</strong> highly mineralised area (309 mine) aresignificantly more mobile for Cs, Li, Rb and Bethan <strong>the</strong> sinters and silica deposits from areasdistal to 309 (except <strong>the</strong> quartz vein from OffLimits) and <strong>the</strong> volcanic rocks (Fig. 2). Plotting alldata set, a good correlation (R 2 =0.70, powerregression) is evident between Cs/Lu and Be/Lu,with <strong>the</strong> highest ratios being for sinter samplesfrom 309 (Fig. 2A). Considering only silicadeposits in Fig. 8A (black filled symbols) asignificantly better correlation (R 2 =0.79, powerregression) would be obtained. Sinter and quartzsamples from 309 have also high Rb/Lu and Li/Luratios, (Fig. 2B). A well-developed correlation (R 2=0.77) between Rb/Lu and Li/Lu is evident amongsilica samples from <strong>the</strong> entire Twin Hills area (Fig.2B). The interaction <strong>of</strong> hydro<strong>the</strong>rmal waters with<strong>the</strong> late Carboniferous alkaline igneous rocksresulted in <strong>the</strong> breakdown <strong>of</strong> K-Feldspar releasingalkali elements, which were subsequentlymobilised in <strong>the</strong>se fluids. This process led to <strong>the</strong>generation <strong>of</strong> an evolved, fertile hydro<strong>the</strong>rmal fluidsystem that carried precious metals (Au, Ag) aswas <strong>the</strong> case at 309 and Lone Sister in <strong>the</strong> TwinHills area.U and Th content <strong>of</strong> silica and clay samples from<strong>the</strong> surface can also be used in evaluating hot dryrock geo<strong>the</strong>rmal potential <strong>of</strong> <strong>the</strong> igneous rockassociation buried by heat-insulating sediments inadjacent sedimentary basins. Compared topegmatite quartz compiled from <strong>the</strong> literature(Götze et al., 2004), U and Th concentrations in91


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Figure 1: Upper continental crust (UCC) –normalised trace element concentration <strong>of</strong> <strong>the</strong> silica deposits from <strong>the</strong> DrummondBasin (Twin Hills area) in comparison to quartz from various granitic/pegmatitic environments.sinter and quartz deposits from <strong>the</strong> DrummondBasin are significantly elevated (Fig. 3A-B). U andTh contents <strong>of</strong> <strong>the</strong> illitic clay minerals that formedin response to <strong>the</strong> interaction <strong>of</strong> hydro<strong>the</strong>rmalfluids with host rocks are similarly high as thosefrom <strong>the</strong> Cooper Basin. The latter represent aradiometric heat production from <strong>the</strong> basementgranite (Middleton, 1979), whereas <strong>the</strong> clayconcentrations for <strong>the</strong> Bowen Basin inQueensland and Paris Basin in Europe are similarto those <strong>of</strong> <strong>the</strong> upper continental crust (Fig. 6A-B).Geo<strong>the</strong>rmal potential in <strong>the</strong> Galilee BasinIgneous rocks <strong>of</strong> <strong>the</strong> Drummond Basin occur as<strong>the</strong> basement <strong>of</strong> <strong>the</strong> adjacent Galilee Basin <strong>of</strong>Upper Carboniferous to Middle Triassic age(Evans, 1980). The late Permian coal depositsand carbonaceous pelitic rocks in <strong>the</strong> GalileeBasin are ideal heat insulating sediments (Nunand Li, 2002) that would store <strong>the</strong> radioactive heatgeneration in <strong>the</strong> basement. Indeed,temperatures <strong>of</strong> about 80C at 1000 m weremeasured in coal seam gas drilling boreholes in<strong>the</strong> Galilee Basin (pers. commun. with severalcoal seam gas companies) that indicate high heatflux from <strong>the</strong> basement. Fur<strong>the</strong>rmore, <strong>the</strong> vitrinitereflectance values measured on <strong>the</strong> coal coresthroughout most <strong>of</strong> <strong>the</strong> Galilee Basin rangebetween 0.63 and 0.73 %R o max (Holland andApplegate, 2008), translating into reservoirtemperatures <strong>of</strong> about 95C - 110C (Barker andPawlewicz, 1986).Figure 2. Alkali element mobility in <strong>the</strong> Twin Hills area.92


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Figure 3. U – Th abundances <strong>of</strong> sinter and clay deposits from<strong>the</strong> Drummond Basin in comparison to those <strong>of</strong> o<strong>the</strong>rsedimentary basins. Pegmatite quartz from Götze et al.(2004).ConclusionThe results <strong>of</strong> <strong>the</strong> pilot study suggest that traceelement geochemistry <strong>of</strong> silica samples and <strong>the</strong>associated clay alteration can serve as a powerfultool in 1) discriminating between sinter and quartzveins from hydro<strong>the</strong>rmal systems driven bygranitic heat sources and o<strong>the</strong>r siliceous rocktypes (barren quartz/silica deposits) and 2) to beused in reconnaissance soil sampling to identifyhydro<strong>the</strong>rmal alteration zones associated withheat-producing granite plutons. Fur<strong>the</strong>r workaimed at investigating similar samples fromvarious settings with different ages will expandexisting knowledge <strong>of</strong> how <strong>the</strong>se techniques canbe used to effectively discriminate areas with highgeo<strong>the</strong>rmal potential from barren systems on aroutine basis.Evans, P.R., 1980. Geology <strong>of</strong> <strong>the</strong> Galilee Basin.In: R.A. Henderson and P.J. Stephensen(Editors), Geology and Geophysics <strong>of</strong>Nor<strong>the</strong>astern Australia. Geological Society <strong>of</strong>Australia, Queensland Division, pp. 299–305.Götze, J., Plotze, M., Graupner, T., Hallbauer,D.K. and Bray, C.J., 2004. Trace elementincorporation into quartz: A combined study byICP-MS, electron spin resonance,cathodoluminescence, capillary ion analysis, andgas chromatography. Geochimica EtCosmochimica Acta, 68(18): 3741-3759Holland, J.R. and Applegate, J.K., 2008. RecentCoalbed Methane Exploration in <strong>the</strong> GalileeBasin, Queensland, Australia. 2008 InternationalCoalbved & Shale Gas Symposium.Middleton, M.F., 1979. Heat flow in <strong>the</strong> Moomba,Big lake gas fields <strong>of</strong> <strong>the</strong> Cooper Basin andimplications for hydrocarbon maturation. Bulletin<strong>of</strong> <strong>the</strong> <strong>Australian</strong> Society <strong>of</strong> ExplorationGeophysics, 10: 149-155.Nesbitt, H.W. and Markovics, G., 1997.Wea<strong>the</strong>ring <strong>of</strong> granodioritic crust, long-termstorage <strong>of</strong> elements in wea<strong>the</strong>ring pr<strong>of</strong>iles, andpetrogenesis <strong>of</strong> siliciclastic sediments.Geochimica Et Cosmochimica Acta, 61(8): 1653-1670.Nesbitt, H.W. and Young, G.M., 1989. Formationand diagenesis <strong>of</strong> wea<strong>the</strong>ring pr<strong>of</strong>iles. Journal <strong>of</strong>Geology, 97(2): 129-147.Nunn, J.A. and Lin, G., 2002. Insulating effect <strong>of</strong>coals and organic rich shales: implications fortopography-driven fluid flow, heat transport, andgenesis <strong>of</strong> ore deposits in <strong>the</strong> Arkoma Basin andOzark Plateau. Basin Research(14): 129-145.Strong, D.F., 1981. Ore deposit models – 5. Amodel for Granophile mineral deposits. GeoscieCanada, 8: 155–161White, N.C., Wood, D.G. and Lee, M.C., 1989.Epi<strong>the</strong>rmal sinters <strong>of</strong> Paleozoic age in northQueensland, Australia. Geology, 17(8): 718-722.ReferencesBarker, C.E., Pawlewicz, 1986. The correlation <strong>of</strong>vitrinite reflectance with maximum temperature inhumic organic matter. In: Buntebarth, G. andStegena, L. (Eds.), Paleogeo<strong>the</strong>rmics, New York,Springer-Verlag, p. 79-83.Cunneen, R. and Sillitoe, R.H., 1989. Paleozoichot-spring sinter in <strong>the</strong> Drummond Basin,Queensland, Australia. Economic Geology, 84(1):135-142.93


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Estimates <strong>of</strong> <strong>the</strong> magnitude <strong>of</strong> topographical effects on surface heatflow from finite element modellingGordon Webb 1 * and Ben Harrison 21 Nor<strong>the</strong>rn Territory Geological Survey, PO Box 8760, Alice Springs NT 0871, Australia2 School <strong>of</strong> Earth Sciences, The University <strong>of</strong> Melbourne, Victoria 3010, Australia* Corresponding author: gordon.webb@nt.gov.auIntroductionSurface heat flow calculations are employed bygeo<strong>the</strong>rmal exploration companies to estimate <strong>the</strong>geo<strong>the</strong>rmal gradient down to depths <strong>of</strong> 3 km to6 km. Surface heat flow is typically calculatedfrom coincident <strong>the</strong>rmal conductivity data orestimates, and temperatures obtained by drilling aslim-line hole down to depths <strong>of</strong> 300 m to 1000 m.At such shallow depths <strong>the</strong> effect <strong>of</strong> a variablesurface topography needs to be considered whenperforming temperature extrapolations to greaterdepth. This is because, for a given crustal volumewith an undulating surface, heat will tend to flowtowards topographic lows and away fromtopographic highs as it migrates from <strong>the</strong> base to<strong>the</strong> ground surface. A linear approximationmethod was developed by Lees (1910) to correctfor topography under idealised geometricmountain ranges.This study presents results from a series <strong>of</strong> finiteelement method (FEM) models that predict <strong>the</strong>magnitude <strong>of</strong> variation <strong>of</strong> surface heat flow at <strong>the</strong>surface <strong>of</strong> a homogenous two-dimensional slice <strong>of</strong>crust with a uniformly curved surface. The resultsfrom this simple geometry are <strong>the</strong>n compared toirregular topographic surfaces derived from realworld examples.The main advantage <strong>of</strong> using <strong>the</strong> FEM method,described in this study, - ra<strong>the</strong>r than <strong>the</strong> methoddescribed by Lees (1910) - is that any regular orirregular surface topography may be used.Keywords: surface heat flow, temperature,numerical modelling, topography.Model ParametersA series <strong>of</strong> two-dimensional model geometrieswere constructed with a flat base and sides and asinusoidal top edge representing <strong>the</strong> topographicsurface (Figure 1). The models were all 10 kmdeep (measured from <strong>the</strong> midway point <strong>of</strong> <strong>the</strong>surface curvature to <strong>the</strong> base) to minimise nearfieldeffects in fixed boundary conditions. Thesurface topography has a sinusoidal form with awavelength denoted by λ and maximum elevationdifference denoted Δh.The width <strong>of</strong> <strong>the</strong> models was scaled with respectto <strong>the</strong> x-axis to generate different values for <strong>the</strong>ratio Δh/λ. Fifteen model geometries wereconstructed with values <strong>of</strong> Δh/λ varying between0.01 (representing subdued, long wavelengthtopography) and 0.9 (representing steep, shortwavelength topography). Δh had a constant value<strong>of</strong> 412 m for each <strong>of</strong> <strong>the</strong> models. The lower Δh/λvalues might represent <strong>the</strong> gently undulatingterrains encountered in areas such as <strong>the</strong> DarlingRanges near Perth, while Δh/λ values <strong>of</strong> about0.07 might represent areas <strong>of</strong> moderatetopographic expression, such as <strong>the</strong> FlindersRanges and Mt L<strong>of</strong>ty Ranges in South Australia.The model volume was defined as “nonradiogenicgranite” with an isotropic <strong>the</strong>rmalconductivity (k) <strong>of</strong> 3.2 W.m -1 .K -1 , a heat capacity(C) <strong>of</strong> 8500 J.kg -1 .K -1 and a density (ρ) <strong>of</strong>2600 kg.m -3 .Figure 1: Diagram showing <strong>the</strong> generic geometry <strong>of</strong> <strong>the</strong>models.A constant temperature <strong>of</strong> 20 degrees Celsiuswas maintained at <strong>the</strong> top surface <strong>of</strong> <strong>the</strong> models.The sides <strong>of</strong> <strong>the</strong> model were defined to besymmetrical and reflective to remove edgeeffects.A uniform heat flux (Q) was applied to <strong>the</strong> bottomsurface <strong>of</strong> each model. A basal heat flux <strong>of</strong>60 mW.m -2 was applied to each <strong>of</strong> <strong>the</strong> 15 models.Ten additional models were run with a basal heatflux <strong>of</strong> 80 mW.m -2 for comparison. The modelswere meshed with a uniform Lagrange linearmesh with greater than 10,000 nodes per modelspace. The models were solved iteratively using<strong>the</strong> time-varying relationship,until <strong>the</strong> model residuals approach zero and asteady-state solution was attained.ResultsFigure 2 shows <strong>the</strong> percentage decrease orincrease in <strong>the</strong> modelled surface heat flow with94


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>respect to basal heat flux at <strong>the</strong> highest andlowest topographic points, respectively. Forrelatively short wavelength topography (Δh/λ >0.2) <strong>the</strong> modelled surface heat flow differs from<strong>the</strong> basal heat flux by greater than 50%. Themodelled surface heat flow is within 5% <strong>of</strong> <strong>the</strong>basal heat flux value for very long wavelength,subdued topography (Δh/λ < 0.02).wavelength - low relief topography <strong>the</strong> observeddifference will be less but may still be significant.These models also predict that <strong>the</strong> depth <strong>of</strong><strong>the</strong>rmal perturbation is related to <strong>the</strong> ratio <strong>of</strong> <strong>the</strong>relief height and <strong>the</strong> wavelength <strong>of</strong> surfacetopography and that this relationship is not linear.Figure 2: Plot <strong>of</strong> <strong>the</strong> percentage difference between <strong>the</strong>modelled surface heat flow with respect to <strong>the</strong> basal heat fluxmeasured at <strong>the</strong> highest (peak; negative change) and lowest(valley; positive change) points on <strong>the</strong> surface topography.Curves were generated below <strong>the</strong> highest andlowest topographic points that describe <strong>the</strong>vertical variation between <strong>the</strong> modelled surfaceheat flow and <strong>the</strong> basal heat flux (figure 3). Eachpair <strong>of</strong> curves is a characteristic <strong>of</strong> <strong>the</strong> specificgeometry <strong>of</strong> <strong>the</strong> model surface. An arbitrary pointat which <strong>the</strong> curves have decayed to within 5% <strong>of</strong><strong>the</strong> basal heat flux value can be usefullycompared in each model to assess <strong>the</strong> depth atwhich <strong>the</strong> <strong>the</strong>rmal perturbation is significantlydiminished (figure 4). The depth <strong>of</strong> <strong>the</strong> <strong>the</strong>rmalperturbation gradually increases with increasingwavelength (decreasing Δh/λ) until a maximumpenetration is reached at a Δh/λ value <strong>of</strong> ~0.04(figure 4).DiscussionThe model solutions presented here represent aninitial attempt to assess <strong>the</strong> magnitude <strong>of</strong> <strong>the</strong>variation <strong>of</strong> surface heat flow measurements withrespect to regional heat flux due to <strong>the</strong> effect <strong>of</strong>topography using <strong>the</strong> finite element method. Anumber <strong>of</strong> o<strong>the</strong>r factors also affect surface heatflow measurement including (but not limited to)internal heat production, ground water flux,altitude/climate effects, and lateral <strong>the</strong>rmalconductivity contrasts (Beardsmore and Cull,2001 and references <strong>the</strong>rein). The approachtaken in this study deliberately ignores <strong>the</strong>se o<strong>the</strong>reffects to specifically investigate <strong>the</strong> effect <strong>of</strong>topography in isolation.These models predict that, for relatively shortwavelength - high relief topography, surface heatflow measurements, will be significantly differentfrom <strong>the</strong> regional, “deep” heat flux. For longerFigure 3: Pr<strong>of</strong>ile <strong>of</strong> <strong>the</strong> modelled vertical heat flux below <strong>the</strong>peak (highest surface elevation) and <strong>the</strong> valley (lowestsurface elevation) for model hft010 (Δh/λ = 0.082, λ = 5 km,Δh = 412 m). The decay <strong>of</strong> <strong>the</strong> <strong>the</strong>rmal perturbationincreases with depth until <strong>the</strong> basal heat flux value isreached. The 5% cut-<strong>of</strong>f values used to generate figure 4 areshown.Figure 4: Plot <strong>of</strong> <strong>the</strong> depth at which <strong>the</strong> model heat flow iswithin 5% <strong>of</strong> <strong>the</strong> basal heat flux measured below <strong>the</strong> highest(peak) and lowest (valley) points on <strong>the</strong> surface topography.Note that <strong>the</strong> depth <strong>of</strong> perturbation attains a maximum valueand <strong>the</strong>n diminishes as a function <strong>of</strong> Δh/λ.This study highlights a potentially significantsource <strong>of</strong> uncertainty that must be factoredin/corrected for when extrapolating heat flow datato depths <strong>of</strong> 3 km to 6 km. Fur<strong>the</strong>rmore, <strong>the</strong>results <strong>of</strong> this study suggest that <strong>the</strong> practice <strong>of</strong>estimating resource temperatures by calculatingone-dimensional <strong>the</strong>rmal models may only bevalid for areas where surface topography isrelatively subdued. In most o<strong>the</strong>r cases it ispreferable to construct well parameterised twoand/orthree dimensional <strong>the</strong>rmal models.95


ReferencesBeardsmore, G. R. & Cull, J. P. 2001 Crustal heatflow: a guide to measurement and modelling.Cambridge University Press.Lees, C. H. (1910) On <strong>the</strong> Shapes <strong>of</strong> <strong>the</strong>Isogeo<strong>the</strong>rms under Mountain Ranges in Radio-Active Districts. <strong>Proceedings</strong> <strong>of</strong> <strong>the</strong> Royal Society<strong>of</strong> London. Vol. 83, No. 563, pp. 339-346<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>96


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>The next <strong>Australian</strong> EGS Reservoir – Jolokia 1 stimulationDoone Wyborn*, Robert Hogarth, Delton Chen and Michel RosenerGeodynamics Limited.PO Box 2046, Milton, Queensland, 4064AbstractGeodynamics drilled <strong>the</strong> Jolokia 1 well in 2008 toa depth <strong>of</strong> 4,911m in <strong>the</strong> Innamincka granite at alocation 9.5km west <strong>of</strong> <strong>the</strong> Habanero EGS field innorth eastern South Australia. The reservoirstimulation program was delayed until <strong>2010</strong>.Initially <strong>the</strong> delay was related to <strong>the</strong> need toundertake fur<strong>the</strong>r evaluation <strong>of</strong> <strong>the</strong> well andimplementation <strong>of</strong> a technical solution to allowmulti-fracture stimulation. The stimulation wasfur<strong>the</strong>r delayed when <strong>the</strong> casing in Habanero 3well failed in April 2009.The aims <strong>of</strong> <strong>the</strong> stimulation are to:(i) Confirm <strong>the</strong> capacity to create heatexchange reservoirs at locationsspread across <strong>the</strong> Innamincka graniteresource.(ii) Develop two separate reservoirs in <strong>the</strong>one well, both deeper and hotter than<strong>the</strong> reservoir operated at <strong>the</strong>Habanero field(iii) Demonstrate injectivity increasescompared to <strong>the</strong> Habanero field.Prior to <strong>the</strong> stimulation <strong>the</strong> well is to be loggedwith a high temperature imaging tool andcompleted with a liner, tubing and packer. Thestimulation consists <strong>of</strong> injecting more than 20,000cubic metres <strong>of</strong> clean water into <strong>the</strong> well atpressures up to 69MPa. A conservative benignchemical tracer is included in <strong>the</strong> injected water. Itis expected that a single reservoir will be createdat a depth below <strong>the</strong> liner set to 4,350m. Thereservoir development is monitored by amicroseismic network <strong>of</strong> seven triaxial geophonestations up to 5 km from <strong>the</strong> well and 100 to 200mdeep. The stimulation will be carried out over aperiod <strong>of</strong> 10 days. A pumping regime has beendetermined based on (i) <strong>the</strong> understanding thathas come from <strong>the</strong> stimulations <strong>of</strong> <strong>the</strong> Habaner<strong>of</strong>ield, and (ii) <strong>the</strong> best information frominternational experts who have carried out suchoperations in o<strong>the</strong>r projects. Currently <strong>the</strong>operation is due to take place in August <strong>2010</strong>. Acomprehensive site-specific microseismic riskanalysis was needed before <strong>the</strong> South <strong>Australian</strong>regulators could give approval to proceed.Existing understanding <strong>of</strong> <strong>the</strong> stimulation processindicates that once a fracture zone begins tostimulate its transmissibility increases by orders <strong>of</strong>magnitude so that that zone dominates <strong>the</strong>continuance <strong>of</strong> reservoir growth with time. At <strong>the</strong>Habanero field <strong>the</strong> reservoir grew outwards at arelatively constant rate <strong>of</strong> 1 km 2 for every 12,000m 3 <strong>of</strong> water pumped after an initially more rapidgrowth within 200m radius <strong>of</strong> <strong>the</strong> wellbore. Basedon transient well-test analyses <strong>the</strong> transmissibility<strong>of</strong> <strong>the</strong> Habanero reservoir increased from a prestimulated50 milliDarcy metres to a poststimulation 2000 milliDarcy metres. This increaseis less than has been observed in <strong>the</strong> lower stressconditions <strong>of</strong> o<strong>the</strong>r projects. The increase isconsidered permanent because <strong>the</strong> roughness <strong>of</strong><strong>the</strong> fracture surface gives rise to self-propping <strong>of</strong><strong>the</strong> fracture once it has slipped by an amount in<strong>the</strong> order <strong>of</strong> <strong>the</strong> dimensions <strong>of</strong> <strong>the</strong> grain size <strong>of</strong> <strong>the</strong>rock. This permanency was vindicated atHabanero since stimulation in 2005 proceededaerially beyond what had been achieved by <strong>the</strong>first stimulation in 2003, with virtually no overlap indevelopment within 1 km <strong>of</strong> <strong>the</strong> injection well.Only one reservoir can be developed at a time.Given <strong>the</strong> stress conditions <strong>of</strong> <strong>the</strong> Innaminckagranite determined at <strong>the</strong> Habanero field <strong>the</strong>re isample potential for <strong>the</strong> stacking <strong>of</strong> multiplereservoirs in a vertical interval <strong>of</strong> well-boreprovided <strong>the</strong>se can be grown separately. TheJolokia reservoir program envisages one reservoirbuilt from Jolokia 1 and a second built from a laterwell Jolokia 2 at a different depth interval. Futureuse <strong>of</strong> open hole high temperature packers shouldallow for such multiple reservoir development tobe achieved in a single well.The Jolokia 1 stimulation is to be carried out inAugust <strong>2010</strong> and measurement <strong>of</strong> injectivity andmapping <strong>of</strong> reservoir growth based onmicroseismic returns will allow comparisons with<strong>the</strong> Habanero reservoir. The stimulation programincludes pressure transient fall-<strong>of</strong>f analysis usingdown-hole gauges and pressure-temperaturespinnerlogs to evaluate <strong>the</strong> distribution <strong>of</strong>permeable fractures.This paper reports on <strong>the</strong> results <strong>of</strong> <strong>the</strong> Jolokia 1stimulation and <strong>the</strong> implications for fur<strong>the</strong>rdevelopment <strong>of</strong> <strong>the</strong> vast Innamincka granitegeo<strong>the</strong>rmal resource. The Jolokia stimulation is<strong>the</strong> key to proving that EGS development can beeffected at virtually any location in granite bodies.The prize <strong>of</strong> large scale economic production <strong>of</strong>zero-emission EGS electricity will <strong>the</strong>n depend onachieving increased heat extraction rates andreduced development costs.Keywords:Stimulation, EGS, microseismic monitoring, multifracturereservoir97


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Optimised Fracture Network Model for Habanero ReservoirChaoshui Xu*, School <strong>of</strong> Civil, Environmental and Mining Engineering, University <strong>of</strong> AdelaidePeter Dowd, Faculty <strong>of</strong> Engineering, Computer and Ma<strong>the</strong>matical Sciences, University <strong>of</strong> AdelaideDoone Wyborn, Geodynamics LimitedAbstract:Fracture networks and <strong>the</strong>ir connectivity are <strong>the</strong>principal factors affecting fluid flow in hot dry rock(HDR) geo<strong>the</strong>rmal reservoirs. Largely because <strong>of</strong><strong>the</strong> complexity <strong>of</strong> <strong>the</strong> problem models <strong>of</strong> HDRreservoirs tend to be over-simplified using ei<strong>the</strong>r avery limited number <strong>of</strong> fractures or an equivalentporous media approach. This paper describes aMarkov Chain Monte Carlo (MCMC) conditioningtechnique for reservoir fracture modelling bytaking into account <strong>the</strong> seismic events collectedduring <strong>the</strong> fracture stimulation process. Using <strong>the</strong>technique, <strong>the</strong> fracture model “evolves” during <strong>the</strong>simulation process and eventually converges to apredefined optimal criterion. The proposedmethod is tested using seismic data collectedduring <strong>the</strong> hydraulic fracture stimulationprocesses <strong>of</strong> <strong>the</strong> Habanero wells in Geodynamics’Cooper Basin project.Keywords: Fracture network, seismic events,Markov chain Monte Carlo.IntroductionThe technical and commercial viability <strong>of</strong> HDRgeo<strong>the</strong>rmal energy depends on <strong>the</strong> creation <strong>of</strong>artificial reservoirs, or Enhanced Geo<strong>the</strong>rmalSystems (EGS), in <strong>the</strong> rock mass by stimulatingand creating fractures (generally by hydr<strong>of</strong>racturing)to enable geo<strong>the</strong>rmal flow. Theartificial reservoir forms <strong>the</strong> critical component inan EGS: <strong>the</strong> fracture network that connects <strong>the</strong>injection and production wells and acts as <strong>the</strong>heat exchange chamber for <strong>the</strong> system. HDRproductivity depends crucially on <strong>the</strong>connectivity/permeability <strong>of</strong> <strong>the</strong> reservoir fracturenetwork and a realistic fracture model, such asthat described in this paper, is <strong>the</strong> key toassessing reservoir performance and designing asuitable heat exchange chamber for <strong>the</strong> EGS.The characterisation <strong>of</strong> rock fracture networks is avery difficult problem not least because accuratefield measurement <strong>of</strong> a single fracture is difficultand measurement <strong>of</strong> all fractures is impossible.Thus, in practice, <strong>the</strong> whole fracture system is notobservable on any meaningful scale and <strong>the</strong> onlyrealistic approach is via a stochastic modelinformed by sparse data and/or by analogues. InHDR applications, a realistic solution is even moredifficult as <strong>the</strong> only reference data related to <strong>the</strong>fracture system are ei<strong>the</strong>r from geophysicalborehole logs and/or sparse seismic eventskilometres beneath <strong>the</strong> surface and detectedduring <strong>the</strong> hydraulic stimulation process. For<strong>the</strong>se reasons current models <strong>of</strong> fracture systemsused for HDR flow modelling are oversimplifiedrepresentations <strong>of</strong> reality. They ei<strong>the</strong>r use anequivalent porous media approach (e.g., Xing etal. 2009), single fracture representation (e.g.,Zhang et al., 2009) or a combination <strong>of</strong> both.Stochastic fracture modelling is <strong>the</strong> generalapproach in which locations, size, orientation ando<strong>the</strong>r properties <strong>of</strong> fractures are treated asrandom variables with inferred probabilitydistributions. In <strong>the</strong> simplest case, once <strong>the</strong>parameters <strong>of</strong> <strong>the</strong> distributions are inferred, <strong>the</strong>rock fracture model is constructed by Monte Carlosimulation. First, <strong>the</strong> fracture locations aregenerated, usually by a Poisson distribution inwhich fracture intensity for a particular area isei<strong>the</strong>r assumed to be constant or is derived fromgeostatistical estimation or simulation. Secondly,<strong>the</strong> orientation <strong>of</strong> each fracture is generated, mostcommonly from a Fisher distribution. Finally, <strong>the</strong>size <strong>of</strong> each fracture is generated from a specifieddistribution, <strong>the</strong> most common being exponential,lognormal or gamma. O<strong>the</strong>r fracture properties,such as aperture width and fracture strength, can<strong>the</strong>n be added into <strong>the</strong> network by additionalMonte Carlo steps. Options for fractureintersections and fracture termination can also beincorporated. Simulated fracture models areusually validated by sampling <strong>the</strong> model (usingscan lines or areas) and assessing <strong>the</strong> extent towhich <strong>the</strong> sampled values conform to <strong>the</strong>statistical models specified (Kulatilake et al.2003). Such models are certainly very useful indescribing <strong>the</strong> statistical behaviours <strong>of</strong> <strong>the</strong> fracturesystem. However, in order to make <strong>the</strong> generatedmodels more realistic, some forms <strong>of</strong> dataconditioning must be built into <strong>the</strong> fracturegeneration process. Data conditioning in twodimensionalfracture trace simulation is generallyconsidered a simple matter but, probably because<strong>of</strong> <strong>the</strong> complexity involved, <strong>the</strong>re are very fewpublications <strong>of</strong> algorithms and methods for dataconditioning in three-dimensional stochasticfracture modelling. Mardia et. al (2007) describedan attempt to condition a fracture model byborehole intersection data using Markov ChainMonte Carlo (MCMC) simulation. In this paper,however, <strong>the</strong> conditioning data are <strong>the</strong> seismicevents observed during <strong>the</strong> fracture stimulationprocess <strong>of</strong> <strong>the</strong> HDR reservoir and <strong>the</strong>y are not,<strong>the</strong>refore, confined to any known order (e.g.,boreholes).During hydraulic stimulation, fractureslips/initiations/propagations produce micro-98


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>seismic events that can be monitored by anetwork <strong>of</strong> geophones and analysed to obtain <strong>the</strong>event locations. To date, <strong>the</strong>se “point cloud” datahave been used to estimate <strong>the</strong> volume <strong>of</strong> areservoir that is connected by wells. We believe<strong>the</strong>se micro-seismic events not only identify <strong>the</strong>locations <strong>of</strong> fracture slip, initiation and/orpropagation but also contain vital informationabout <strong>the</strong> structure <strong>of</strong> existing fractures andfracture networks. Successful extraction <strong>of</strong> thisinformation will significantly improve <strong>the</strong> reliability<strong>of</strong> fracture models so that a more realistic fracturerepresentation <strong>of</strong> <strong>the</strong> HDR reservoir can beobtained. Moriya et al. (2002) use microseismicmultiplet analysis to derive <strong>the</strong> fracture plane on<strong>the</strong> assumption that seismic events from <strong>the</strong> samefracture will produce similar microseismicities.This approach, however, only accounts for a smallproportion <strong>of</strong> <strong>the</strong> total seismic events (17% inMoriya et al. 2002) and <strong>the</strong> fundamentalassumption behind <strong>the</strong> approach is questionable.AssumptionIt is generally acknowledged that during <strong>the</strong>hydraulic fracture stimulation process, <strong>the</strong>effective normal compressive stress acting acrosstwo fracture planes <strong>of</strong> a fracture is reduced due to<strong>the</strong> hydraulic pressure and that will cause <strong>the</strong> twoplanes to slip against each o<strong>the</strong>r. This isgenerally considered to be <strong>the</strong> key mechanism increating a permeable HDR reservoir as shearslipswill result in mis-alignment <strong>of</strong> fracturesurface topographies which will cause a lateraldilation and <strong>the</strong>reby enhance fracture aperturesand significantly increase <strong>the</strong> permeability <strong>of</strong> <strong>the</strong>fracture network. The shear slips betweenfracture planes will produce small-scale seismicitywhose seismic waves can be captured andanalysed by a network <strong>of</strong> geophones to derive <strong>the</strong>location <strong>of</strong> <strong>the</strong> event (Baisch et al. 2006). Theeffect <strong>of</strong> hydraulic pressure also makes it possiblefor existing fractures to propagate in <strong>the</strong> reservoirand new fractures to be initiated. The finaloutcome <strong>of</strong> <strong>the</strong> process will be a permeablereservoir connected to <strong>the</strong> wells through acomplex fracture network.Based on this conceptual description <strong>of</strong> <strong>the</strong>fracture stimulation process, it is reasonable toassume that seismic events only occur on fractureplanes. The criterion <strong>of</strong> a realistic fracture modelis <strong>the</strong>n directly related to <strong>the</strong> overall closeness <strong>of</strong><strong>the</strong> seismic events to fracture planes fitted in <strong>the</strong>model. In this context, fracture simulationessentially becomes a stochastic geometryreconstruction problem given a set <strong>of</strong> pointclouds. Reconstruction <strong>of</strong> a surface from randompoint clouds is computationally and algorithmicallychallenging and is an active research area incomputer and ma<strong>the</strong>matical sciences (Bercovieret al. 2002). The success <strong>of</strong> current practice,however, depends critically on close samplingpoints on <strong>the</strong> surface, which is usually not anissue as <strong>the</strong> point clouds are generally obtainedfrom laser scanning or some form <strong>of</strong> digitizing.For seismic point clouds in geo<strong>the</strong>rmalapplications, however, samples are very sparse.For a given fracture, only a few points areavailable, which indicate ei<strong>the</strong>r <strong>the</strong> propagationfront <strong>of</strong> <strong>the</strong> fracture or a point on <strong>the</strong> fracturesurface where shear slip occurs at <strong>the</strong> time <strong>the</strong>events are detected. Current methodology is thusnot directly applicable to fracture modelling.The most common approach in stochastic fracturemodelling is to use a 3D plane to represent afracture, which could be bounded (e.g., ellipticalplane, polygonal plane) or unbounded (e.g.,Poisson plane). The fracture model (network)<strong>the</strong>n becomes a series <strong>of</strong> connected fractureplanes, F i , i=1,2…n, where n is <strong>the</strong> total number<strong>of</strong> fractures. A seismic event point, P j , j=1,2..m (mis <strong>the</strong> total number <strong>of</strong> seismic event points) can<strong>the</strong>n be associated with a fracture F i with distanced j:i .m2d j : ij1can <strong>the</strong>n be used as a simplecriterion to quantify <strong>the</strong> goodness <strong>of</strong> fit <strong>of</strong> <strong>the</strong> fittedfracture model.MCMC modelPlanar polygons are used to represent fractures inthis research. For each fracture polygon F i , <strong>the</strong>location is described by <strong>the</strong> coordinates <strong>of</strong> itscentre point (x i , y i , z i ), <strong>the</strong> orientations aredescribed by three angles: dip direction i , dipangle i and rotation angle i and <strong>the</strong> sizes <strong>of</strong> <strong>the</strong>fractures are described by a major axis a i and aminor axis b i <strong>of</strong> an ellipse containing <strong>the</strong> polygon(Xu & Dowd, <strong>2010</strong>). In o<strong>the</strong>r words, weparameterize fracture planes with parameters (x i ,y i , z i , i , i , i , a i , b i ), i=1,2…n. Fracture plane F ican also be expressed in functional form as x y z ( i)( i)( i)( i)x y z( i)( i)( i)x, y, z)( whereis <strong>the</strong> unit vector normal to <strong>the</strong>fracture plane and can be calculated from ( i , i , i ). Given a point P j (x j , y j , z j ), not necessarilylying on <strong>the</strong> plane, <strong>the</strong> signed orthogonal distanceto fracture F i is defined by:dj:iwhereii( ) x ( ) yx( FP ijjyo<strong>the</strong>rwise)ji ( ) zzji ()ifP( Fi )j F(1)is <strong>the</strong> projection point <strong>of</strong> P j onfracture plane F i . A matching function(j){1,2,…,n} is used to associate each point P jwith one and only one fracture polygon. We shalli99


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>impose a simple criterion <strong>of</strong> minimum distance forthis association and <strong>the</strong>refore by writing d j:i wemean point P j is associated with fracture polygonF i as its distance calculated by Equation (1) is <strong>the</strong>minimum when compared with distances to anyo<strong>the</strong>r fracture plane.d={d j:i }j is <strong>the</strong>n <strong>the</strong> complete set <strong>of</strong> projectiondistances. Since seismic event points that lie on<strong>the</strong> same fracture will not be exactly co-planar, wemust allow for statistical variation and treat afracture as a distorted version <strong>of</strong> an idealizedplane. A simple Gaussian noise model can <strong>the</strong>nbe adopted:d j i2:~ N(0, )(2)to represent <strong>the</strong> distortion in <strong>the</strong> data from <strong>the</strong>idealized plane. In o<strong>the</strong>r words, <strong>the</strong> orthogonaldistances are identically and independentlynormally distributed with mean zero and variance 2 . Therefore, <strong>the</strong> likelihood function for <strong>the</strong> set <strong>of</strong>seismic event points P={P j } can be defined as:L2m ( d j:i )m 22( P;F,ej1) 1 2 (3)given a set <strong>of</strong> fractures F={F i } and <strong>the</strong> matchingfunction (.). The product <strong>of</strong> this likelihood withpriors <strong>of</strong> F gives <strong>the</strong> posterior distribution for Fand <strong>the</strong> attention now is to estimate <strong>the</strong> posteriordistributions <strong>of</strong> F and hence <strong>the</strong> parameters <strong>of</strong> <strong>the</strong>fracture set. A Markov chain can be used togenerate samples from <strong>the</strong> posterior distributionwhich is commonly constructed by <strong>the</strong> Metropolis-Hastings algorithm using <strong>the</strong> Monte Carloacceptance/rejection technique imposed by <strong>the</strong>Hastings’ ratio:( t )( t ) ( P)q(F | P) F , P min1,( t )( t) (4) ( F ) q(P | F ) where (.) is <strong>the</strong> posterior (target) distribution andq(.) is a transition kernel which is usually chosenso that it is easy to sample from.A more detailed description <strong>of</strong> this model can befound in Mardia et al (2007) where a similar modelwas developed to generate fracture modelsconditional on intersection points betweenfractures and boreholes drilled on a regular grid.The Habanero Point CloudThe point cloud used in this study is <strong>the</strong> Q-Conprocessed dataset <strong>of</strong> locations <strong>of</strong> seismic eventsrecorded during <strong>the</strong> hydraulic fracture stimulation<strong>of</strong> Habanero 1 between November 6 andDecember 22, 2003 (Weidler, 2005). A total <strong>of</strong>23,232 seismic events are recorded in thisdataset which covers an area roughly <strong>of</strong> 2.5 km 2 .Figure 1 shows <strong>the</strong> absolute hypocentre locations<strong>of</strong> <strong>the</strong>se events.Figure 1 Absolute hypocenter locations<strong>of</strong> <strong>the</strong> seismic eventsClearly an ideal sub-horizontal reservoir has beenformed by <strong>the</strong> stimulation process which is gentlydipping in <strong>the</strong> South-west direction. Earlyanalysis has revealed that <strong>the</strong> major part <strong>of</strong> <strong>the</strong>reservoir is confined within a sub-horizontal layer<strong>of</strong> approximately 30m (Baisch et al. 2006). Figure2 shows ratios <strong>of</strong> increments in <strong>the</strong> volume <strong>of</strong> <strong>the</strong>reservoir, <strong>the</strong> geographical extents in <strong>the</strong>horizontal, East-west and North-south verticalplanes covered by <strong>the</strong> seismic events during <strong>the</strong>stimulation period. Note that <strong>the</strong> increments areplotted on a relative scale where <strong>the</strong> ordinaterepresents <strong>the</strong> ratios against <strong>the</strong> volume orgeographical extents <strong>of</strong> <strong>the</strong> reservoir covered byseismic events on November 6, 2003.250200150100500HorizontalVolumeNSEWDays after Nov. 6 20030 10 20 30 40 50Figure 2 Increments in volume and geographicalextents covered by seismic eventsHabanero Fracture ModelA total <strong>of</strong> 20052 fractures were initially generatedbased on a non-homogeneous point process witha non-parametric density model estimated by <strong>the</strong>point cloud shown in Figure 1. Fracture locations(x i , y i , z i ), i=1,…,20052, are generated. Thefollowing parameters are used for initial fracturegeneration:100


Fracture orientation: Fisher distribution with=1. Orientation parameters ( i , i , i ) are<strong>the</strong>n calculated.Fracture size: lognormal distribution withmean = 80m and variance = 12,000 m 2 .<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong> 100064MCMC method described was <strong>the</strong>n applied toupdate <strong>the</strong> fracture network. The followingtransition kernels are used in <strong>the</strong> MCMC process: Fracture orientation ( i , i , i ): normalproposal with standard deviation <strong>of</strong> 0.1 (inradian). Fracture location (x i , y i , z i ): normal proposalwith standard deviation <strong>of</strong> 1.0.Fracture size is not optimised in <strong>the</strong> current trial.Fractures without any association with any pointafter 100,000 iterations were removed from <strong>the</strong>system. After 2M iterations, <strong>the</strong> fracture modelobtained is shown in Figure 3.20864-5 -3 -1 1 3 5(a) initial model 100020-0.4 -0.24 -0.08 0.08 0.24 0.4(b) optimised modelFigure 4 Histogram <strong>of</strong> dj:i for intial and optimised fracturemodelsFigure 3 Habanero fracture modelafter 2M MCMC stepsThis fracture model includes 10,995 fractures.Figure 4 shows <strong>the</strong> distribution <strong>of</strong> d j:i before andafter <strong>the</strong> application <strong>of</strong> <strong>the</strong> MCMC updatingprocess. Comparison <strong>of</strong> statistics is given inTable 1. Clearly <strong>the</strong> reliability <strong>of</strong> <strong>the</strong> model hasbeen significantly improved.Orientations <strong>of</strong> fractures have also changedsignificantly. There is no clear indication <strong>of</strong>orientation preference in <strong>the</strong> original fracturemodel (see <strong>the</strong> lower hemispherical projections <strong>of</strong>poles <strong>of</strong> fracture planes in Figure 5a). Thefracture pole plot after optimisation (Figure 5b)clearly demonstrates a great proportion <strong>of</strong> subhorizontalfractures. This is encouraging as itagrees well with <strong>the</strong> propagation pattern <strong>of</strong> <strong>the</strong>seismic event point cloud observed duringstimulation (Baisch et al. 2006).Table 1 Comparison <strong>of</strong> statistics <strong>of</strong> dj:ibefore and after MCMC optimisationInitialmodelOptimisedmodelNumber <strong>of</strong> fractures 20052 10995Minimum d j:i -116 -0.35Maximum d j:i 303 0.39Mean value <strong>of</strong> d j:i 0 0Variance <strong>of</strong> d j:i 12.5 0.0028d 2 j:i291437 6699% <strong>of</strong> d j:i within range [-11, 34] [-0.17, 0.17]101


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>signals (Baisch et al. 2009). The hydraulicconductance between wells can <strong>the</strong>n beestimated.(a) initial model(b) optimised modelFigure 5 Hemispherical projections <strong>of</strong> poles <strong>of</strong> fractureplanesConclusionsThis is a preliminary trial to demonstrate <strong>the</strong>application <strong>of</strong> MCMC in fitting a fracture modelusing a point cloud dataset. Clearly <strong>the</strong> method iseffective, however <strong>the</strong>re are still many remainingchallenging issues. Fracture join/split (Mardia etal. 2007) is not yet considered in this work. Theeffect <strong>of</strong> <strong>the</strong> initial point process model has notbeen assessed and this will affect <strong>the</strong> totalnumber <strong>of</strong> fractures retained in <strong>the</strong> final fracturenetwork. The illustrated fracture model is by nomeans <strong>the</strong> ultimate optimal model for <strong>the</strong>Habanero fractured reservoir and fur<strong>the</strong>rinvestigation is needed to achieve such a model.The next stage <strong>of</strong> <strong>the</strong> process is to assess <strong>the</strong>connectivity <strong>of</strong> <strong>the</strong> fracture network between wells(e.g., between Habanero 1 and 3). Hydraulicapertures <strong>of</strong> fractures can be estimated from <strong>the</strong>degree <strong>of</strong> seismicity recorded in <strong>the</strong> seismicReferencesBaisch S., Weidler, R., Vörös R., Wyborn D. Andde Graaf, L. (2006) Induced seismicity during <strong>the</strong>stimulation <strong>of</strong> a geo<strong>the</strong>rmal HFR reservoir in <strong>the</strong>Cooper Basin, Australia, Bulletin <strong>of</strong> <strong>the</strong>Seismological Society <strong>of</strong> America, 96, No. 6,2242–2256.Baisch S., Vörös R., Weidler R. and Wyborn D.(2009) Investigation <strong>of</strong> fault mechanisms duringgeo<strong>the</strong>rmal reservoir stimulation experiments in<strong>the</strong> Cooper Basin, Australia, Bulletin <strong>of</strong> <strong>the</strong>Seismological Society <strong>of</strong> America, 99, No. 1, 148–158.Bercovier, M., Luzon, M., Pavlov, E. (2002)Detecting planar patches in an unorganized set <strong>of</strong>points in space, Advances in ComputationalMa<strong>the</strong>matics, 17, 153 – 166.Dowd, P.A., Martin, J.A., Xu, C., Fowell, R.J. andMardia, K.V. (2009) A three-dimensional data set<strong>of</strong> <strong>the</strong> fracture network <strong>of</strong> a granite. InternationalJournal <strong>of</strong> Rock Mechanics and Mining Sciences,46, 5, pp.811-818.Dowd, P. A., Xu, C., Mardia, K. V. and Fowell, R.J. (2007) A comparison <strong>of</strong> methods for <strong>the</strong>simulation <strong>of</strong> rock fractures, Ma<strong>the</strong>maticalGeology, 39, 697 – 714.Kulatilake, P. H. S. W., Um, J., Wang, M.,Escandon, R. F. and Narvaiz, J. (2003),Stochastic fracture geometry modelling in 3Dincluding validations for part <strong>of</strong> Arrowhead EastTunnel, California, USA, Engineering Geology,70, 131-155.Mardia, K. V., Nyirongo, V. B., Walder, A. N., Xu,C., Dowd, P. A., Fowell, R. J., Kent, J. T. (2007)Markov Chain Monte Carlo implementation <strong>of</strong> rockfracture modelling, Ma<strong>the</strong>matical Geology, 39,355 – 381.Mardia, K. V., Walder, A. N., Xu, C., Dowd, P.A.,Fowell, R. J., Nyirongo, V.B., Kent, J. T. (2007a),A line finding assignment problem and rockfracture modelling. Bayesian Statistics and itsApplications, Eds. Upadhaya, S.K., Singh, U.,Dey, D.K. Anamaya Pubs, New Delhi; ISBN 1081-88342-63-7; ISBN 13 978-81-88342-63-1. 319-330.Moriya, H., Nakazato, K., Niitsuma, H. And Baria,R. (2002) Detailed fracture system <strong>of</strong> <strong>the</strong> Soultzsous-ForêtsHDR field evaluated usingmicroseismic multiplet analysis, Pure and AppliedGeophysics, 159, 17-541.Weidler, R. (2005), The Cooper Basin HFRproject 2003/2004: findings, achievements andimplications, Technical report, Geodynamics Ltd.Xing, H., Zhang, J., Liu, Y. and Mulhaus, H.(University <strong>of</strong> Queensland, 2009) Enhancedgeo<strong>the</strong>rmal reservoir simulation, <strong>Proceedings</strong> <strong>of</strong><strong>the</strong> <strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong> <strong>Conference</strong>2009, Brisbane.102


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Xu, C. and Dowd, P. A. (<strong>2010</strong>), A new computercode for discrete fracture network modelling,Comps & Geosc., 36, 292-301.Zhang, X. Jeffrey, R. and Wu, B. (CSIRO, 2009)Two basic problems for hot dry rock reservoirstimulation and production, <strong>Proceedings</strong> <strong>of</strong> <strong>the</strong><strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong> <strong>Conference</strong> 2009,Brisbane.103


Progress in CO 2 -based EGS<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Aleks D. Atrens 1 *, Hal Gurgenci 1 , Victor Rudolph 11The Queensland Geo<strong>the</strong>rmal <strong>Energy</strong> centre <strong>of</strong> Excellence.Mansergh Shaw Building (#45),The School <strong>of</strong> Mechanical & Mining Engineering, The University <strong>of</strong> Queensland, QLD 4072The concept <strong>of</strong> Engine ering Geo<strong>the</strong>rmal Systems(EGS) usin g CO 2 a s a he at extractio n fluid ha sbeen exp anded sin ce it was first p roposed. Abetter <strong>the</strong> oretical un derstanding is av ailable fo r<strong>the</strong> be haviour in <strong>the</strong> reservoir, process de sign,corrosion & co ndensation i ssues, and ro ckgeochemistry, although knowl edge <strong>of</strong> som e <strong>of</strong><strong>the</strong>se systems i s i ncomplete. S ufficientunderstanding is now available to provide a powerplant design given site and reservoir parameters,and viability ca n be e stimated. A numbe r <strong>of</strong>challenges re main, h owever, a nd th ese mu st b eaddressed for <strong>the</strong> concept to be realisable. Thosechallenges a re contextua lised h ere to provid efocus for <strong>the</strong> most urgent issues to be addressed.Keywords: Carbon dioxide, CO 2 , EGS, enhancedgeo<strong>the</strong>rmal systems, <strong>the</strong>rmosiphon, hot dry rock,hot wet rockIntroductionCO 2 -based EGS have been discussed previously(Brown 2000; Pruess 2 006; Pruess an d Azaroual2006; Gurgenci et al. 2008; Pruess 20 08; Atrenset al. 20 09a; Atren s et al. 2009 b; Atrens et al.<strong>2010</strong>). A full discussio n <strong>of</strong> <strong>the</strong> technical andeconomic issues related to CO 2 -based EGS havebeen reported (Gu rgenci 2009). Many <strong>of</strong> thoseissues a re broadly applicable to all E GS; thosewill not be discussed here. There are a number <strong>of</strong>issues that are unique to CO 2 -based EGS. T hesehave prim arily been la ck <strong>of</strong> unde rstanding <strong>of</strong> <strong>the</strong>process design, perfo rmance in th e reservoi r,CO 2 -H 2 O interactions, CO 2 -H 2 O-rock interactions,<strong>the</strong>rmodynamic performance, etc. Som e <strong>of</strong> <strong>the</strong>seissues have been ad dressed in varyin g levels <strong>of</strong>detail.Many tech nical challe nges for <strong>the</strong> concept toovercome re main. Th ese ca n b e g rouped undertwo bro ad ca tegories: gen eral challe nges, whi chare overarching an d ap ply to any u se <strong>of</strong> CO 2 inEGS, and reservoir challenges, which are specificto <strong>the</strong> reservoir type.General ChallengesThere a re a number <strong>of</strong> challenges tha t must b eaddressed to make CO 2 -based EGS viable. Each<strong>of</strong> <strong>the</strong>se is effectivel y sh ow-stopping if th eassociated issues are unresolvableThe ove rarching challe nges that must b eaddressed are: CO2 Sourcing CO2 turbomachinery Solubility and re activity <strong>of</strong> roc kcompounds and elements in pure or nearpureCO 2Legal/regulatory issues with sub surfaceCO 2 .Reservoir ChallengesBeyond <strong>the</strong> overa rching issue s, <strong>the</strong> re a re anumber <strong>of</strong> issue s that depen d on th e type <strong>of</strong>reservoir b eing exami ned. The individualchallenges f or <strong>the</strong> different re servoir types arediscussed below.Un-dryable ReservoirsThis term is used to group reservoirs that are wellhydraulically connected, a nd initially sa turated oroversaturated with water. This g rouping wouldinclude h ot sedimenta ry a quifer systems (HSA),and EGS project s su ch as in <strong>the</strong> Cooper Ba sinwhere hig h pre ssure implies l ong-distanceconnectivity. These type <strong>of</strong> systems have anassociated challenge <strong>of</strong> extreme di fficulty increating a d ry CO 2 -rich operating zone within <strong>the</strong>reservoir, eit her due to t he large energy inp utnecessary to displa ce wa ter, or <strong>the</strong> difficulty incontaining CO 2 within <strong>the</strong> desired region.Dryable ReservoirsDryable reservoirs signify a re servoir grouping <strong>of</strong>those which are under-saturated with water at <strong>the</strong>outset, or have a limited initial volume <strong>of</strong> waterthat is ea sily displa ceable. Examples <strong>of</strong> thiscategory are <strong>the</strong> Fenton Hill reservoir, which wasacknowledged a s b eing un connected an drelatively lacking in water content, o r <strong>the</strong> Hijorireservoir system, which experie nced signifi cantlosses <strong>of</strong> injected fluid into <strong>the</strong> reservoir formation(implying an ease in displ acing existing reservoirfluids). The challenges associated with systems <strong>of</strong>this type are <strong>the</strong> time period req uired to dry <strong>the</strong>reservoir, an d <strong>the</strong> p r<strong>of</strong>ile over time o f fluid los sinto <strong>the</strong> reservoir formation.Wet ReservoirThis category is used for systems that are have aliquid water pha se coexi sting with CO 2 -rich fluidnear <strong>the</strong> reservoir o perating zo ne. CO 2 -rich fluidmay be prod uced in this ca se, allowing a single -loop, but <strong>the</strong>re are important issues <strong>of</strong> both waterand carbon dioxide being present in <strong>the</strong> reservoir.The challen ges a ssociated with this type <strong>of</strong>104


system are related to <strong>the</strong> water-CO 2 relationships:time re quired until sufficie ntly pure CO 2 can berecovered, CO 2 -H 2 O dyn amics i n <strong>the</strong> reservoi r(horizontally and verti cally), rock-water-CO 2interactions including mi neral t ransformation /dissolution / deposition (permeability change) andgeo-sequestration, and <strong>the</strong> <strong>the</strong>rmodynamic effects<strong>of</strong> high water content in <strong>the</strong> CO 2 -rich phase.CO 2 -Rich ReservoirThere is also <strong>the</strong> po ssibility <strong>of</strong> operatin g a CO 2 -based EGS system i n a reservoir th at is al readyCO 2 -rich. Th is co uld b e a naturally occurringreservoir, or artificial as <strong>the</strong> result <strong>of</strong> a rtificial CO 2injection for rea sons o <strong>the</strong>r than CO 2 -basedgeo<strong>the</strong>rmal power ge neration. The challen geassociated with this re servoir type is id entifying areservoir that contains or may in <strong>the</strong> future containCO 2 , and is also suitable for geo<strong>the</strong>rmal powe rgeneration.DiscussionThere is a continuum between <strong>the</strong> three form erreservoir types, an d so me <strong>of</strong> <strong>the</strong> challengesrelating to CO 2-H 2 O interactio ns overla p.Separating reservoirs into <strong>the</strong> catego riesdiscussed a bove cl arifies <strong>the</strong> range <strong>of</strong> <strong>the</strong>seinteractions that are vital to co nsider for differentsituations. Th e implicatio n <strong>of</strong> this is that <strong>the</strong>re isan opportunity to target th e proposed CO 2 -basedEGS technol ogy towards situation s whe re th echallenges are more readil y overcome. This maybe useful where <strong>the</strong>re are particular issues relatedto certai n systems that may not be feasibl yanswered i n <strong>the</strong> fore seeable future, o r that maybe m ost suitably be resolved by field trials in areservoir <strong>of</strong> a different type.It is recom mended th at cu rrent goals to wardsimplementation <strong>of</strong> a CO 2-based EG S p owersystem fo cus on re servoirs that ca n fe asibly bedried, as th ese have a sm aller nu mber <strong>of</strong>associated challenges. Reservoirs <strong>of</strong> this type arealso le ss li kely to be targeted for use for wate r-based EGS, so <strong>the</strong> re is le ss risk <strong>of</strong> co mpetitivelydisadvantaging one technology over ano<strong>the</strong>r.<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>ReferencesAtrens, A. D. , H. Gurge nci, et al., 2009a., "CO2<strong>the</strong>rmosiphon for competiti ve powe r ge neration."<strong>Energy</strong> & Fuels 23(1): 553-557.Atrens, A. D., H. Gurgenci, et al., 2 009b., Exergyanalysis <strong>of</strong> a CO2 <strong>the</strong> rmosiphon. T hirty-fourthworkshop on geoth ermal re servoir e ngineering.Stanford University, Stanford, California.Atrens, A. D., H. Gurgenci, et a l., <strong>2010</strong>. ,"Electricity g eneration u sing a carbon-dioxide<strong>the</strong>rmosiphon." Geo<strong>the</strong>rmics.Brown, D. W., 2000., A h ot dry rock g eo<strong>the</strong>rmalenergy concept utilizing supercritical CO2 instead<strong>of</strong> water. Twenty-Fifth Wo rkshop on G eo<strong>the</strong>rmalReservoir Enginee ring, Stanford University,Stanford, California.Gurgenci, H., 2009., Electricity generation using asupercritical CO2 geo<strong>the</strong>rmal siphon. Thirty-fourthworkshop on geoth ermal re servoir e ngineering.Stanford University, Stanford, California.Gurgenci, H., V. Rudolph, et al., 2008.,Challenges for ge o<strong>the</strong>rmal en ergy utilisation .Thirty-Third Workshop on Geo<strong>the</strong> rmal Reservoi rEngineering. Stanford Un iversity, Stanford,California.Pruess, K. 2 006. "Enhanced geo<strong>the</strong>rmal systems(EGS) using CO 2 a s working fluid —A nove lapproach for gene rating renewable e nergy withsimultaneous seq uestration <strong>of</strong> ca rbon."Geo<strong>the</strong>rmics 35: 351–367.Pruess, K., 2008., "On production be haviour <strong>of</strong>enhanced g eo<strong>the</strong>rmal systems with CO2 a sworking fluid." Energ y Conversi on andManagement 49: 1446-1454.Pruess, K. and M. A zaroual, 2006., On th efeasibility <strong>of</strong> usi ng supercritical CO2 as heattransmission fluid in an e ngineered ho t dry roc kgeo<strong>the</strong>rmal system. Thi rty-first workshop o ngeo<strong>the</strong>rmal reservoir engine ering. StanfordUniversity, Stanford, California.105


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Exploration and assessment <strong>of</strong> Hot Sedimentary Aquifer (HSA)geo<strong>the</strong>rmal resources in <strong>the</strong> Otway Basin VictoriaPeter Barnett and Tim EvansHot Rock Limited, GPO Box 216, Brisbane QLD 4001peter.barnett@hotrockltd.com and tim.evans@hotrockltd.comThe Otway Basin contains a n umber <strong>of</strong> Ho tSedimentary Aquifer (HSA) geo<strong>the</strong> rmal resourceswith p otential for commercial development. T hemethodology Hot Rock Limited has u sed toassess <strong>the</strong> se resource s i s detailed in t his pa per.The re sulting stored he at estimate s for <strong>the</strong> HSAresources <strong>of</strong> <strong>the</strong> Otway Basin i s larg e, even byworld geo<strong>the</strong>rmal standards. A total <strong>of</strong> 550,000PJ <strong>of</strong> HSA resou rces have been so fa r estimatedand declared by three companies.While <strong>the</strong>re is confid ence in <strong>the</strong> estimation <strong>of</strong> inplaceheat in <strong>the</strong> Otway Basin HSA resources and<strong>the</strong> rate that heat in geo<strong>the</strong>rmal water recoveredto surface can be converted to electricity, <strong>the</strong>re isless ce rtainty as yet on <strong>the</strong> amount <strong>of</strong> heat thatcan b e re covered a nd <strong>the</strong> rate it can berecovered. Both <strong>of</strong> <strong>the</strong>se variables are determinedby permeability in <strong>the</strong> geo<strong>the</strong>rmal reservoir.By comp arison with bot h HSA a nd volcani cgeo<strong>the</strong>rmal systems el sewhere, and a detail edassessment <strong>of</strong> <strong>the</strong> structural geology at <strong>the</strong> OtwayBasin tenements, HRL c onsiders th at <strong>the</strong> HSAresources i n <strong>the</strong> Otway Basin are do minated bysecondary fracture perm eability, with primarypermeability being subordinate. HRL i sproceeding to drill in early 201 0 two pro <strong>of</strong> <strong>of</strong>concept w ells in to its flag ship H SA project a tKoroit. Th ese wells a re specifically targeted onboth primary and secondary permeability, with <strong>the</strong>firm expectat ion that se condary pe rmeability willprove to be dominant and that comm ercial gradetemperatures and well flow rates will be obtained.Keywords:Geo<strong>the</strong>rmal, Otway Basin, Hot S edimentaryAquifer, HSA, resource assessment, Monte Carlo,pro<strong>of</strong> <strong>of</strong> concept, gen eration potential, welltargeting.IntroductionHot Rock Limited (HRL) holds a large geo<strong>the</strong>rmaltenement position in Vi ctoria <strong>of</strong> 2 7,500km 2 in fivepermits. Some 15,000km 2 <strong>of</strong> this holding containsrocks <strong>of</strong> t he Crayfish S ubgroup i n th e on shoreportion <strong>of</strong> <strong>the</strong> Otway Ba sin within Vi ctoria. Theseare predominantly sandstones <strong>of</strong> Creta ceous ageand have known geo<strong>the</strong>rmal potential.They occur in a series <strong>of</strong> individual depositionarycentres (shown coloured in both ligh t and da rkgreen in Fig ure 1 ), dep osited o nto <strong>the</strong> tops o fsubsiding basement fault blocks developed along<strong>the</strong> nor<strong>the</strong> rn margin <strong>of</strong> <strong>the</strong> rift zone whi ch led toAustralia sep arating fro m Antarctica durin g <strong>the</strong>breakup <strong>of</strong> Gondwanaland in late Cretaceoustimes.The crustal t hinning prod uced in thi s extensionaltectonic environment allows for elevated heat flowthrough <strong>the</strong> Palaeo zoic ba sement into th eoverlying sediments over most <strong>of</strong> <strong>the</strong> Otway Basinwhere geo<strong>the</strong>rmal gradients <strong>of</strong> 35 to 45 o C/km aremeasured. This combination <strong>of</strong> re gional sh allowheat and larg e areal exten t, thickness and hencevolume <strong>of</strong> geo<strong>the</strong>rmal re servoir ro ck make s th eOtway Basin a significant terrain for potential HSAgeo<strong>the</strong>rmal develo pment, even by worldstandards.Figure 1: Series <strong>of</strong> fault bound rift basins containing thickaccumulations <strong>of</strong> Crayfish subgroup rocks developed along<strong>the</strong> nor<strong>the</strong>rn margin <strong>of</strong> <strong>the</strong> onshore Otway Basin.Exploration <strong>of</strong> HSA resourcesAlthough <strong>the</strong> HSA geo<strong>the</strong>rmal plays in t he OtwayBasins a re esse ntially blind – i .e. withou tobservable discharge <strong>of</strong> h eat or ma ss at surface,HRL h as be en abl e to define <strong>the</strong> se resource s atdepth from t he exten sive geoscientific data thathave been acquired over <strong>the</strong> past 40 t o 50 yea rsby parti cularly <strong>the</strong> petroleum a nd g roundwaterindustries in Vic toria. Th ese d ata have b eensystematically archived by State an d Fe deralgovernment agencies such as <strong>the</strong> Department <strong>of</strong>Primary Industries and Geosciences Australia andare readily accessibleExisting data includ e g ravity, magnetics an dstratigraphy whi ch are applicable at relativelycoarse scal e to regio nal scale studies. Mo re106


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>detailed data, <strong>of</strong> value for prospect scale studies,include seismic refle ction data, geol ogical log sand co res from existing petrole um a nd groundwater wells, and mea surements <strong>of</strong> temperaturesand o<strong>the</strong>r data in <strong>the</strong>se wells.In additio n t o u se <strong>of</strong> ex isting data, HRL h asapplied to it s HSA expl oration stu dies in <strong>the</strong>Otway Ba sin a n umber <strong>of</strong> exploratio n meth odsthat are rout inely use d in <strong>the</strong> exploration an ddelineation <strong>of</strong> volcanic geo<strong>the</strong>rmal systems. Themost significant <strong>of</strong> th ese ha s been t he u se <strong>of</strong>magneto-telluric (MT) resistivity surveying and <strong>the</strong>application <strong>of</strong> ge o<strong>the</strong>rmal geochemistryinterpretative methods t o grou nd water a ndpetroleum well fluids analyses.Key deliverables from <strong>the</strong> HRL exploration studiesinclude <strong>the</strong> following:Starting Point: An initial review <strong>of</strong> geo<strong>the</strong>rmalgradients a s a tool for prioriti zing areas fordetailed geo<strong>the</strong>rmal assessment.End Point: A rang e <strong>of</strong> 3-D mod els gridded attypically 100 m cente rs ov er ge o<strong>the</strong>rmal resourceareas <strong>of</strong> typically 3 00 to 500 km 2 areal extentwhich include: Stratigraphic model s defining fo rmation top s,bottoms, vert ical (cro ss sections) and hori zontalsections (slices in plan) Structural geological models Thermal m odels showing di stribution o fiso<strong>the</strong>rms in 3-D, i so<strong>the</strong>rmal sectio ns in 2-Dcombined with geology, estimates <strong>of</strong> temperaturein each grid block at any depth Multi discipli ne, integ rated, co nceptual hydrogeological models which form <strong>the</strong> basi s fo rsubsequent resource assessm ent, an dformulation <strong>of</strong> exp loration drilling anddevelopment strategy.Assessment <strong>of</strong> HSA ResourcesThe Otway Basin HSA resources have beenassessed in terms <strong>of</strong> in-place stored heatcontained in <strong>the</strong> Crayfish subgroup reservoirrocks between assigned upper and lower depthlimits. This involves initially considerations <strong>of</strong>resource thickness, lateral extent and hencevolume, followed by considerations <strong>of</strong> porosityand temperature from which heat contained inboth <strong>the</strong> rocks in <strong>the</strong> resource volume and hotwater contained in pores and factures in <strong>the</strong>reservoir rocks can be estimated.The upper depth limit to <strong>the</strong> resource is referred toas <strong>the</strong> resource temperature cut <strong>of</strong>f (orabandonment temperature) and <strong>the</strong> lower depthlimit is an assumed depth limit to whichgeo<strong>the</strong>rmal fluids can be reasonably recoveredfrom <strong>the</strong> resource, and is taken to be a practicaldrilling depth limitation.Estimates <strong>of</strong> temperature values throughout <strong>the</strong>resource volume have been obtained from 3D<strong>the</strong>rmal modelling. Porosity has been assessedconservatively at 10% throughout and althoughthis in important parameter in considering <strong>the</strong>amount and rate at which hot water can berecovered from <strong>the</strong> geo<strong>the</strong>rmal resource, <strong>the</strong>amount <strong>of</strong> heat stored in <strong>the</strong> rock and <strong>the</strong> water isrelatively insensitive to porosity.The values used for <strong>the</strong> above parameters inHRL’s assessment <strong>of</strong> HSA resources are given inTable 1 where <strong>the</strong>y are compared with a range <strong>of</strong>values used by o<strong>the</strong>r developers working in <strong>the</strong>HSA environment. Relative to <strong>the</strong>se o<strong>the</strong>rvalues, those used by HRL are conservative.Table 1: Comparison <strong>of</strong> parameters used by HRL forestimating <strong>the</strong> thickness, volume and in-place heat <strong>of</strong> HSAgeo<strong>the</strong>rmal resources.ParameterMinimum resourcetemperaturePower plant rejectiontemperatureResource base: i.e.practical depth limit forrecovery <strong>of</strong> geo<strong>the</strong>rmalfluidsValues used byHRL130 o C (GEP6 and 23) 125 0 C140 o C (GEP-8)70 o C 70 o C4500mValues used byo<strong>the</strong>rs in OB5000mPorosity 10% 5 % to 15%Minimum reservoir 500mNil to 250 mthicknessThe computation <strong>of</strong> in-place heat has beenundertaken by HRL on a probabilistic basis usinga purpose developed Monte Carlo simulationmodel in which probability distributions are usedto characterise <strong>the</strong> key resource assessmentparameters. The stored heat is summed overindividual resource blocks for which formationtops, top and bottom resource limits and modelledtemperature distribution have been gridded at1000m intervals. The Monte Carlo model is run2,000 times to obtain <strong>the</strong> frequency distributionsand cumulative probability distributions for <strong>the</strong>stored heat contained in <strong>the</strong> geo<strong>the</strong>rmal resourcevolume.The results <strong>of</strong> <strong>the</strong> resource assessments arereported in accordance with <strong>the</strong> AustraliaGeo<strong>the</strong>rmal Reserve Reporting Code (1st edition,2008) in terms <strong>of</strong> in-place stored heat. At thisstage in <strong>the</strong> exploration <strong>of</strong> HRL’s Otway BasinHSA resources, two types <strong>of</strong> geo<strong>the</strong>rmalresources have been determined: “Inferred resource” – where tem peratures a renot directly measured, and107


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong> “Indicated resource” wh ere tempe ratures aremeasured in-situ within <strong>the</strong> geo<strong>the</strong>rmal resource.Typically th e form er is declared wheretemperatures are measured in petroleum and / ordeep ground water wells that have not penetratedas d eep a s <strong>the</strong> geo<strong>the</strong> rmal reservo ir in th eCrayfish Subgroup and <strong>the</strong> latter is where existingwells have been drilled into <strong>the</strong> Crayfish thu sallowing for temperatures to be measured directlywithin <strong>the</strong> geo<strong>the</strong>rmal resource. If a nd when wellsdrilled i nto <strong>the</strong> geot hermal re source a resuccessfully f low t ested <strong>the</strong>n <strong>the</strong> “Inferredresource” estimate can be upgraded to “Measuredresource”.Results <strong>of</strong> Resource AssessmentsHRL has completed r esource assessments at <strong>the</strong>following Crayfish Subgroup depostionary centresin <strong>the</strong> Victorian portion <strong>of</strong> <strong>the</strong> Otway Ba sin. Thesecentres are shown outlined in pink in Figure 1 andinclude (from west to east): GEP-23: Penola Trough GEP-6: Penola Trough GEP-6: Tantanoola Trough GEP-8: Koroit Trough GEP-8:Ross Creek Trough GEP-8/9: Elingamite TroughFrom <strong>the</strong>se assessments a number <strong>of</strong> geo<strong>the</strong>rmalresources have been declared, as summarised inTable 2.Table 2: Results <strong>of</strong> estimations <strong>of</strong> Inferred and IndicatedHSA geo<strong>the</strong>rmal resources identified and declared by HRLwithin GEP-6, GEP-8 and GEP-23 in <strong>the</strong> Otway Basin.Resource Tenement ResourceAreaResourceVolumeIndicated InferredResource ResourceReportDatekm2 km3 PJ PJKoroit GEP‐8 50 47 7,600Koroit GEP‐8 400 340 59,000Koroit GEP‐8 450 387 7,600 59,000 1‐Oct‐09Penola GEP‐23 20 24 5,000Penola GEP‐23 120 150 29,000Penola GEP‐6 8 9 1,700Penola GEP‐6 290 306 55,000Penola GEP23 & 6 440 490 6,700 84,000 27‐Jul‐10Tantanoola GEP‐6 180 130 22,000 27‐Jul‐10Totals 1,070 1,010 14,300 165,000 180,000Power Generation PotentialThe estim ated geo<strong>the</strong> rmal resource s decla redtodate by HRL in <strong>the</strong> Otway Basin total 15,000 PJfor Indi cated re sources and P1 65,000 PJ fo rInferred re sources, at <strong>the</strong> P50 level. Thesefigures re present very la rge sto re <strong>of</strong> geo<strong>the</strong>rmalheat, however, not all <strong>of</strong> this h eat is av ailable forconversion to electricity. Only a small amount <strong>of</strong><strong>the</strong> geo<strong>the</strong>rmal heat will be recoverable from <strong>the</strong>resource an d only a sma ll amount <strong>of</strong> <strong>the</strong> heatrecovered t o surface will be converted t oelectricity in a po wer plant due to t hermal tomechanical energy losses.Figure 2: “Inferred” and “Indicated” geo<strong>the</strong>rmal resourcesdeclared in <strong>the</strong> Koroit area, GEP-8 (Source: HRL, 2009).Representative value s for HSA geoth ermalresource ar e 5 % a nd 12%, r espectively, w hichmeans that o nly about 1% <strong>of</strong> <strong>the</strong> in-pl ace heat in<strong>the</strong> geoth ermal re servoir will be converted t oelectricity. On this ba sis, only som e 1,000 PJ o f<strong>the</strong> total value <strong>of</strong> 180,000 PJ <strong>of</strong> heat contained in<strong>the</strong> Koroit g eo<strong>the</strong>rmal resource, would be able tobe extracte d and co nverted to electri city.None<strong>the</strong>less, 1000 PJ <strong>of</strong> energy in electri calenergy term s is still a la rge value, equivalent toabout 300,000GWh. To achieve generation at thislevel a power plant with a gene ration capacity <strong>of</strong>about 1300MWe would be required to operate ata capacity factor <strong>of</strong> 90% for a period <strong>of</strong> 30 years.Figure 3: “Inferred” and “Indicated” geo<strong>the</strong>rmal resourcesdeclared in <strong>the</strong> Penola and Tantanoola Troughs in GEP-23and GEP-6 (Source: HRL, <strong>2010</strong>)In addition to <strong>the</strong> 1 80,000 P J geo<strong>the</strong> rmalresources estimated by HRL, two o<strong>the</strong>rgeo<strong>the</strong>rmal develop ers have also deline ated,108


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>assessed and de clared HSA geo<strong>the</strong> rmalresources in <strong>the</strong> western and ea stern ends <strong>of</strong> <strong>the</strong>Otway Basin, on ei<strong>the</strong> r side <strong>of</strong> HRL’ s tenements.The total de claration <strong>of</strong> geo<strong>the</strong>rmal resources todate from th e three com panies for th e onshoreOtway Basin in both Vi ctoria and S outh Australiatotals some 550,000 PJ (Table 3 ). On <strong>the</strong> sam ebasis a s <strong>the</strong> cal culations above for Koroit, thi samount <strong>of</strong> t hermal en ergy has th e potential togenerate so me 9 00,000 GWh <strong>of</strong> electricity an dthis wo uld require a po wer plant g eneratingcapacity <strong>of</strong> some 3,500 MWe for 30 years.Table 3: Summary <strong>of</strong> all declared HSA geo<strong>the</strong>rmal resourceassessments over <strong>the</strong> greater Otway Basin4. The pin k line i s a regression fit f or channelsands in <strong>the</strong> Pretty Hill and <strong>the</strong> red li ne is <strong>the</strong>same for bar sand s in <strong>the</strong> Pretty Hi ll. Clea nchannel sands are <strong>the</strong> prime target for geo<strong>the</strong>rmaldevelopment being more coarse grained and withboth highe r poro sity and perme ability at anydepth.As well as variation in pri mary permeability in <strong>the</strong>Otway Ba sin with d epth t here is also significantvariation in t he character and q uality <strong>of</strong> <strong>the</strong> rCrayfish Subgroup reservoir facies, depending onprovenance <strong>of</strong> sou rce m aterial a nd e nvironment<strong>of</strong> deposition.Trough inOtway BasinTenement DeveloperHSAInferredResourcePJHSAIndicatedResourcePJHSAMeasuredResourcePJHSAEstimatedTotalPJTantanoola GEP‐6 HRL 77,000 1,700 78,700Koroit GEP‐8 HRL 59,000 7,600 66,600Penola GEP‐23 HRL 29,000 5,000 34,000Anglesea GEP10 GreenEarth40,000 40,000Tantanoola GEL‐170, Panax171, 172130,000 130,000Rendelsham GEL‐170, Panax184, 21217,000 17,000Rivoli St Clair GEL‐173 Panax 53,000 53,000Penola GEL‐223 Panax 89,000 32,000 11,000 132,000Totals 494,000 46,300 11,000 551,300The in-place heat stored in <strong>the</strong> HSA resources in<strong>the</strong> Otway Basin a nd t he pote ntial gene ratingcapacity <strong>of</strong> <strong>the</strong>se a re larg e, eve n by worldgeo<strong>the</strong>rmal standa rds con sidering that <strong>the</strong>geo<strong>the</strong>rmal industry ha s a glo bal install edcapacity <strong>of</strong> 11,000 MWe.The confidence in <strong>the</strong> e stimation <strong>of</strong> h eat in-placein <strong>the</strong> Otw ay Bas in H SA r esources is r elativelyhigh, as i s <strong>the</strong> rate at which <strong>the</strong> heat ingeo<strong>the</strong>rmal water recove red to surfa ce can b econverted to electricity. Of lesser certai nty is <strong>the</strong>amount <strong>of</strong> h eat that can be re covered from <strong>the</strong>HSA re source and <strong>the</strong> rate at whi ch i t can berecovered - both <strong>of</strong> <strong>the</strong> se are dete rmined bypermeability in <strong>the</strong> geo<strong>the</strong>rmal reservoir.PermeabilityPermeability in Otway Ba sin HSA reservoirs canbe <strong>of</strong> two types (1) primary permeability,associated with natu ral porosity in th e CrayfishSubgroup sa ndstone re servoir ro cks, and/or (2)secondary permeability associated with faults andfractures in <strong>the</strong> reservoir rocks.Primary permeabilityThe petrol eum indu stry has generatedconsiderable data on poro sity and permeabilitythroughout th e Otway Basin from geolo gical an delectrical logging and a nalysis <strong>of</strong> core s andcuttings from petroleum wells. Poro-perm data for<strong>the</strong> Pretty Hil l sandstone from petroleum wells i nboth Victo ria and S outh Au stralia (butpredominantly from <strong>the</strong> latter) are shown in FigureFigure 4: Summary <strong>of</strong> declared geo<strong>the</strong>rmal resourceassessments in <strong>the</strong> greater Otway Basin with HSAgeo<strong>the</strong>rmal development potential Source: 3DGeo (2009)From a d etailed analy sis <strong>of</strong> seismi c data andpetroleum well data, th e Koroit g eo<strong>the</strong>rmalresource is assessed to have pa rticularly go odreservoir facie s cha racteristics hav ing thic kaccumulations <strong>of</strong> cle an coa rse grained san ds,with mini mal lithic m aterial, espe cially in <strong>the</strong>Lower Prett y Hill Form ation (3 DGeo 2009 ).Based on statistical analysis <strong>of</strong> th e poro-permdata in Figure 3, estimate s have be en <strong>of</strong> poro sityand permeability potential with de pth in <strong>the</strong> Koroitgeo<strong>the</strong>rmal resource (3D Geo, 200 9). The seestimates are for bette r t han average poro p ermvalues than occur for <strong>the</strong> Otway Basin.The variation in poro pe rm with de pth in Figure 4is instructive as it confirms: porosity in <strong>the</strong> Pretty Hi ll Formatio n to bereducing with depth, from 20% at 2500 m to 14%at 3500m, and permeability decreasing by two orders <strong>of</strong>magnitude between 2500 and 3500m.In spite <strong>of</strong> t hese re ductions i n po ro-perm withdepth, <strong>the</strong> evidence is that permeability within <strong>the</strong>Pretty Hill at Koroit will still be sufficient to giv ecommercial geo<strong>the</strong>rmal well flows from prima ryreservoir p ermeability alone. Fo r example,assuming, as a conservative case, that <strong>the</strong> lowervalue in <strong>the</strong> range <strong>of</strong> <strong>the</strong> permeabilities predictedat each <strong>the</strong> 3 depth ranges in Figure 4 apply, anda net to gro ss ratio <strong>of</strong> 50%, <strong>the</strong>n a tra nsmissivity109


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong><strong>of</strong> 13 Dm would be expected over <strong>the</strong> depth range<strong>of</strong> 2500 to 3 500m, with an expected temperaturerange <strong>of</strong> 130 to 17 0 o C For t his t ransmissivityvalue, a standard size geo<strong>the</strong>rmal well completion(with a 9-5/8 inch diameter open production hole)can be expected to yield a flow rate <strong>of</strong> 90 kg/sec,and for a large diameter well completion (with 12-1/2 inch di ameter production hole) to yield a flo wrate <strong>of</strong> 160 kg/sec (SKM, 2009).Secondary permeabilityThe importance <strong>of</strong> secondary permeability in HSAgeo<strong>the</strong>rmal system s se ems not to be wellappreciated in <strong>the</strong> Australia n geo<strong>the</strong> rmalcommunity. Few if any geo<strong>the</strong>rmal systems in <strong>the</strong>world, <strong>of</strong> a ny type, prod uce from on ly prima rypermeability. For example, for <strong>the</strong> fol lowing twokey oversea s analo gues for HSA geo<strong>the</strong>rmalresources in Australia: Heber a nd East Me sa fields in S ou<strong>the</strong>rnCalifornia: secondary pe rmeability controls anupflow <strong>of</strong> h ot geo<strong>the</strong> rmal fluids from basementinto overlyin g fluvial sed iments where prima rypermeability i s hi gh. Ge o<strong>the</strong>rmal well s producefrom b oth f ractures around th e u pflow a ndprimary permeability in <strong>the</strong> sediments Sou<strong>the</strong>rn Germany: high flow rates ( up to 140kg/sec) a re o btained from deep inte rsections (atdepths <strong>of</strong> u p to 4500m) <strong>of</strong> well bores withfractures in Malm lime stone with little if anyevidence <strong>of</strong> primary permeabilityIn co nventional vol canic geoth ermal syste msdeveloped in sedimentary reservoir rocks, fracturepermeability is al so t he major control ongeo<strong>the</strong>rmal fl uid hydrol ogy and well p roductivity.For example: The large and very well documented Geysersgeo<strong>the</strong>rmal f ield in California produces steamfrom fra ctured greywa cke baseme nt rocks whichhave low primary porosities and permeabilties. The Oh aaki geo<strong>the</strong> rmal fi eld in Ne w Z ealandhas go od produ ction well flows from fracture dgreywacke b asement rocks which under lie lavasand volcaniclastics.In <strong>the</strong> Otway Basin <strong>the</strong>re are well developed faultsand structures at both large and small scale whichaffect both t he Pala eozoic ba sement rocks a nd<strong>the</strong> overly ing sedim entary su ccessions,particularly <strong>the</strong> Crayfish Su b group. The presentdayst ress re gime i n <strong>the</strong> Otway Ba sin is on <strong>the</strong>boundary between o blique-slip an d reversefaulting. The NW–SE maximum ho rizontal stre ssorientation is cal culated at ~140 d egrees N.Analysis <strong>of</strong> structural ge ologic data has beeninterpreted t o sho w that faults and fractu resorientated approximately WNW-ESE to NE-S Ware consistent with <strong>the</strong> present day stress regimeand structures o n th ese o rientations areconsidered t o be m echanically o pen, with g oodpotential for providing secondary permeabilitychannels for geo<strong>the</strong> rmal fluid flow (3D-G eo,2009). The potential f or second ary fracturepermeability is <strong>the</strong>refore considered to be good in<strong>the</strong> HSA resources <strong>of</strong> <strong>the</strong> Otway Basin.HRL is proceeding in early <strong>2010</strong> to drill two pro<strong>of</strong><strong>of</strong> concept wells at its fla gship Koroit geo<strong>the</strong>rmalproject. These two wells are specifically targetingmajor faults at depth as primary well targets. Asubordinate target is po rosity in <strong>the</strong> upper level sin <strong>the</strong> op en production h ole where p orosity andpermeability prosects are best. Having <strong>the</strong>highest geot hermal gradi ent in <strong>the</strong> Ot way Basin(<strong>of</strong> up to 46o C/km) at <strong>the</strong> Koroit re source, aminimum production temperature <strong>of</strong> 130 o C can betargeted at t he top <strong>of</strong> th e ge o<strong>the</strong>rmal re servoirwithin <strong>the</strong> Crayfish Forma tion at depths <strong>of</strong> only2500m. At this comparatively shallow depth, poropermp rosects are m uch better than at greate rdepth, particularly belo w 3500m as evident fromFigure 4.HRL’s “Pro<strong>of</strong> o f C oncept w ells” ar e th ereforedesigned to intersect an o ptimum combination <strong>of</strong>primary and secondary p ermeability and HRL i soptimistic <strong>of</strong> su ccessful outcomes in term s <strong>of</strong>good pe rmeability and transmi ssivity result s andcommercial grade tempe ratures a nd well flowrates.Figure 5: Geological section, Koroit HSA resource, showingpro<strong>of</strong> <strong>of</strong> concept well targeted on (1) deep intercept withmajor fault target and (2) primary porosity target (upper andlower Pretty Hill Formations from 2500m) Source: 3DGeo(2009)Summary and ConclusionsThe Otway Basin contains a nu mber <strong>of</strong> HSAgeo<strong>the</strong>rmal resources wit h good p otential forcommercial development.These resources exi st as a result <strong>of</strong> th efavourable combination <strong>of</strong>: elevated geo<strong>the</strong>rmal g radients <strong>of</strong> t ypicallyaround 40 o C/km, but as high as 46 o C/km in primeresource areas such as Koroit in GEP-8. Thermal gradients in this range are sufficientto obtain com mercial grade geo<strong>the</strong> rmaltemperatures within practical drilling depths110


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong> The fortuitous occurrence <strong>of</strong> thick stratigraphicsequences <strong>of</strong> quart z ri ch sand stones in <strong>the</strong>Crayfish Subgroup reservoir rock within <strong>the</strong> samedepths that comm ercial temperatures occur an dwithin practical drilling reachThe stored heat contained in <strong>the</strong> HSA resources<strong>of</strong> <strong>the</strong> Otwa y Basin a re larg e, even by wo rldgeo<strong>the</strong>rmal standards. A total <strong>of</strong> 550,000 PJ o fHSA re sources have b een so far estimated a nddeclared by t hree comp anies. Altho ugh currentexpectations are that o nly some 0.5% <strong>of</strong> this inplaceheat can be recovered from <strong>the</strong> geo<strong>the</strong>rmalresources and converte d to ele ctricity, <strong>the</strong>generation p otential on e ven this ba sis i s la rge,requiring some 3,500MWe <strong>of</strong> g eneration capacityfor 30 years.There is confidence in <strong>the</strong> estimation <strong>of</strong> heat inplacein <strong>the</strong> Otway Basin HSA resources and <strong>the</strong>rate that he at in geo<strong>the</strong> rmal wate r re covered tosurface can be converted to electricity. However,<strong>the</strong>re i s less certainty yet on <strong>the</strong> amo unt <strong>of</strong> heatthat can b e recovered fro m <strong>the</strong> HSA resourcesand <strong>the</strong> rate at which this can be recovered - both<strong>of</strong> <strong>the</strong>se variables are determined by permeabilityin <strong>the</strong> geo<strong>the</strong>rmal reservoir.HSA resou rces se em to be viewe d by <strong>the</strong><strong>Australian</strong> g eo<strong>the</strong>rmal co mmunity as having o nlyprimary permeability. B y comparison with bothHSA and volcanic geo<strong>the</strong>rmal systems elsewhere,and a detai led a ssessment <strong>of</strong> <strong>the</strong> structuralgeology <strong>of</strong> its Otway Basin tenements, HRL views<strong>the</strong> Otway Basin resources to be do minated bysecondary fracture perm eability, with primarypermeability being subordinate to this.HRL is proceeding in early <strong>2010</strong> to drill two pro<strong>of</strong><strong>of</strong> con cept wells at <strong>the</strong> Koroit HSA resource ,specifically targeting b oth primary and secondarypermeability with <strong>the</strong> firm expectation thatsecondary permeability will prove to be dominantand that commercial grade temperatures and wellflow rates will be obtained.Statement <strong>of</strong> Competent PersonThe inform ation in this pape r that relates t oExploration Results, Ge o<strong>the</strong>rmal Re sources orGeo<strong>the</strong>rmal Reserves i s based on i nformationcompiled by Peter Barn ett who is a full timeemployee <strong>of</strong> Hot Rock Limited. He has sufficientexperience which is relevant to <strong>the</strong> style and type<strong>of</strong> geo<strong>the</strong>rmal play under consideration and to <strong>the</strong>activity which he is un dertaking to q ualify as aCompetent Person as defined in <strong>the</strong> Code. In thiswork he ha s drawn fre ely from reports o n HSAgeo<strong>the</strong>rmal resources i n <strong>the</strong> Otway Basinprepared u nder his supe rvision, by b oth staff <strong>of</strong>Hot Ro ck Li mited and b y external consultants,notably 3D-Geo <strong>of</strong> Melbourne. The assessment <strong>of</strong>stored heat and levels <strong>of</strong> Indicated an d Inferre dResources and <strong>the</strong> repo rting <strong>of</strong> <strong>the</strong>se have beenundertaken solely by Pete r Barnett. Peter Barnettconsents in writing to <strong>the</strong> inclusion in <strong>the</strong> report <strong>of</strong><strong>the</strong> matters based o n hi s i nformation in <strong>the</strong> fo rmand context in which it appears.AcknowledgmentsThis paper draws freely on graphical materialprepared by 3D Geo <strong>of</strong> Melbourne under contractto HRL, particularly <strong>the</strong> power point presentationfor this paper to be given at <strong>the</strong> conference.References3D Ge o Pty Limited, 200 9, Otway Basin Proj ect.Koroit Area WP2 Re port. Unpu blished re portprepared u nder contract to Hot Rock Limited2009.AGEA and AGEG, 200 8, Australi an Code fo rReporting <strong>of</strong> Exploration Re sults, G eo<strong>the</strong>rmalResource a nd Geoth ermal Re serves, 200 8Edition. Prep ared by <strong>the</strong> Australi an G eo<strong>the</strong>rmalCode Committee, AGEA and AGEG,Hot Ro ck Li mited, 2009, Statement <strong>of</strong> EstimatedGeo<strong>the</strong>rmal Resources for <strong>the</strong> K oroit Geo<strong>the</strong>rmalPower Proje ct, Victoria, Geo<strong>the</strong>rmal ExplorationPermit GEP- 8. Hot Rock Internal report, preparedby Peter Barnett, 30 September, 2009. A full copyis available at:http://www.hotrockltd.com/IRM/Company/ShowPage.aspx?CPID=1224&EID=16267720Hot Ro ck Limited, <strong>2010</strong>, Characte rization andAssessment <strong>of</strong> Geo<strong>the</strong>rmal Resources in GEP-23& GEP-6, Ho t Rock Inte rnal re port, p repared byPeter Barnett, June <strong>2010</strong>. A full copy available at:http://www.hotrockltd.com/IRM/Company/ShowPage.aspx?CPID=1227&EID=77703804Sinclair Knig ht Merz (SKM), 2009, several wellbore flo w mo delling stu dies. Unpubli shed rep ortprepared u nder contract to Hot Rock Limited2009.111


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Validation <strong>of</strong> Geo<strong>the</strong>rmal Exploration Techniques for Analysing HotSedimentary Aquifer and Enhanced Geo<strong>the</strong>rmal Systems.J.E. Davey & J.T. Keetley3D-GEOLevel 5 / 114 Flinders Street, Melbourne, 3000.Validated g eo<strong>the</strong>rmal re source e stimates a rebased o n ge ological mo dels that combine th egeology fro m <strong>the</strong> surface to b asementincorporating prope rties such as lithology,structure, fluids, comp action, po rosity andpermeability with <strong>the</strong>rm al models consisting <strong>of</strong>heat flow, condu ctivity and <strong>the</strong>rm al gradi ents.These models must extend beyond single pointwell an alysis, and provide a bal anced andgeologically rea sonable estimate <strong>of</strong> <strong>the</strong> size,structure, a ccessibility and m aturity <strong>of</strong> asubsurface t hermal system. To achieve ageologically rea sonable model, all availabl egeological and ge ophysical d ata m ust beconsidered. H owever, d ata se ts an dmeasurements mu st be analysed, interp retedand weighted in a manne r that reduces error for<strong>the</strong>rmal models.This pa per focuse s o n building validatedgeo<strong>the</strong>rmal resource evaluations from geologicaland g eophysical i nterpretations f or HotSedimentary Aquifer (HSA) and EnhancedGeo<strong>the</strong>rmal Systems (E GS). Thi s p aper al s<strong>of</strong>ocuses on limitations <strong>of</strong> some d ata sets, andthis can be realized when modeling.Limitations in Thermal ModelingFor a ny given geolo gical data set (field, well,seismic, rem ote sensing, temperature ) virtuallyan infinite numb er <strong>of</strong> 2D an d/or 3 Dinterpretations can be made. However, <strong>the</strong> set <strong>of</strong>physically possible geological interpretations arefar more lim ited. The tests for such physicalplausibility derive from our knowledge <strong>of</strong> <strong>the</strong>processes which co ntrol sedim ent deposition,structural ev olution, and geo<strong>the</strong> rmal system s.Interpretations which can pass <strong>the</strong>s e tes ts maynot be correct, but <strong>the</strong>y are more li kely to be so,and can b e labeled with that highl y soughtappellation: Validated.Limitations occur with <strong>the</strong>rmal modeli ng that arenot as preva lent in o<strong>the</strong>r f orms <strong>of</strong> su bsurfacemodeling. The main limitation i s <strong>the</strong> abundanceand re presentation <strong>of</strong> temperature th roughout<strong>the</strong> system. Tempe rature mea surements a retypically limited to single point measurem entsobtained from wells and bores previously drilled.While heat is <strong>the</strong> basis <strong>of</strong> all g eo<strong>the</strong>rmalsystems, temperature is only ever measuredfrom a singl e point. This provide s <strong>the</strong> verticalcomponent <strong>of</strong> a temperat ure g radient at thatpoint source ma king it a n isotro pic a nalysis <strong>of</strong>temperature. While this is an ideal measurementfor volcanic and plutonic rocks where heatflow isprimarily in <strong>the</strong> vertical domain, it d oes notaccount for <strong>the</strong> a nisotropic ‘radia l’ heatdistribution t hat occu rs in se dimentary an dmetamorphic ro cks (Clau ser & Hu enges 1 995).The tempe rature-depth p r<strong>of</strong>ile from a well can<strong>the</strong>refore be thought <strong>of</strong> a s <strong>the</strong> vertical summing<strong>of</strong> <strong>the</strong> geoth ermal g radients e stablished within<strong>the</strong> individu al layers withi n <strong>the</strong> sedime nt pile atthat location. Such a pr<strong>of</strong>ile is ra rely linear withdepth.However, when extra polating temp erature from<strong>the</strong> well p r<strong>of</strong>iles, <strong>the</strong> ani sotropic component <strong>of</strong>heat distribution within a sedimentary basin mustbe a ccounted for. Be cause <strong>of</strong> thi s, th e <strong>the</strong>rm alcomponent <strong>of</strong> <strong>the</strong> model is highly de pendent onincorporating ot her f actors such a s structure,lithological distrib ution, fluids, porosity andpermeability, hydrocarbo ns and fracturing tocontrol <strong>the</strong> d istribution <strong>of</strong> heat thro ughout <strong>the</strong>model. Because <strong>of</strong> this, a geological model mustbe created first. This will help to generate <strong>the</strong>112


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>properties needed to consider for <strong>the</strong> anisotropicextrapolation <strong>of</strong> tempe rature. The rmal modelingwill be revisited later in this paper.Subsurface Geo<strong>the</strong>rmal ModelingUtilizing all t he availabl e data to construct ageological model will aid in validating ageo<strong>the</strong>rmal resource. In t errains currently beingexplored with Australia, available data includes:wells, 2D-3 D remotely sensed imag ery, 2D-3 Dseismic, potential field dat a sets (namely gravityand m agnetics), petro physical l ogs andoccasionally magnetotelluric data sets.WellsWells provi de geolo gical truthing to anysubsurface model. Ba sic informatio n su ch aslithology, formation de pth, fluid pre sence andtemperature are recorded.Because te mperature is currently o nlymeasurable in situ, wells provide <strong>the</strong> basis <strong>of</strong> <strong>the</strong><strong>the</strong>rmal mo deling. Do wn hole tools deployedduring drilli ng and after drilling a re used torecord temperature at different stag es within <strong>the</strong>well. T his inform ation is co mbined wi<strong>the</strong>stimates or meas urements <strong>of</strong> conduc tivity togenerate information on heatflow. This is in turnused a s <strong>the</strong> ba sis for extra polating atemperature model across <strong>the</strong> area.Wells <strong>of</strong>ten h ave vital information colle cted fromdown hole logging tools employed during drillingor j ust after. These to ols collect info rmation o ntemperature, pressure, flow rate s, densities andeven fra cturing. A seld om use d, bu t highlybeneficial te chnique for E GS an d HSA is do wnhole vertical con ductivity and horizontalresistivity measurements. These techniques aredesigned to i dentify fractu re o rientation as wellas what orientation <strong>of</strong> fracture is open (that is, apotential flui d con duit) in <strong>the</strong> well. Bothmeasurements are o btained whil e drilling.Horizontal resistivity measures <strong>the</strong> resistivity <strong>of</strong> aformation by dispe rsing a cu rrent flowing in ahorizontal plane. Vertical cond uctivity ismeasured in a simil ar m anner, ho wever in th evertical plane. The se mea surements a reobtained by using wireline logging tools such aslaterologs a nd pro pagation logs. T wo surveytypes a re u sed, a s single o rientation pla nesurveys (i.e. vertical or horizontal) cannot takemeasurements in <strong>the</strong> plane parallel to t he planewhere th e e lectromagnetic current is flowing.Vertical cond uctivity is u sed for imagi ng hig hangle f racturing (f ractures with di p 20 -70 o ) an dsub-horizontal fracturi ng (dip 70 o ). Th e su rveys a re analysedand plotted as frequency diagrams indicating <strong>the</strong>primary orientation <strong>of</strong> <strong>the</strong> open fracturing.Information about <strong>the</strong> contemporary stress fieldsin <strong>the</strong> area can be obtai ned f rom well data .Borehole bre akouts reflect a measu rement <strong>of</strong><strong>the</strong> orientation <strong>of</strong> disintegration <strong>of</strong> <strong>the</strong> well duringdrilling as a result <strong>of</strong> com pressive stress failure.The orientation <strong>of</strong> <strong>the</strong> breakout is parallel to <strong>the</strong>orientation o f <strong>the</strong> minimum hori zontal stre ss.This o rientation is p erpendicular to <strong>the</strong>orientation <strong>of</strong> <strong>the</strong> d rilling ind uced tensil efractures, <strong>the</strong> orientation in whi ch <strong>the</strong> t angentialstress is below tensil e ro ck strength. Thisorientation is parallel to th e maximum horizontalstress. Information a bout co ntemporary stresscan assist with drilling and also with determining<strong>the</strong> nature a nd ori entation <strong>of</strong> any stru cture th atmay be active or ‘open’ within <strong>the</strong> system.Surficial G eology and Remotely SensedImageryGeo<strong>the</strong>rmal exploration i s greatly aid ing fromsurficial geology and re motely sen sed image ryas it p rovides approximate groun d truths tostructure an d morphol ogy interpreted in <strong>the</strong>subsurface. Not all subsurface ge ology has asurficial rep resentation, a significant portiondoes. Actual exposure <strong>of</strong> <strong>the</strong>se features helps tounderstand <strong>the</strong> magnitude and style <strong>of</strong> stru ctureand <strong>the</strong> physical properties <strong>of</strong> rocks at depth. Animportant co mponent <strong>of</strong> this is developing a nunderstanding <strong>of</strong> <strong>the</strong> cover rocks and how <strong>the</strong>ymay aid in assisting or impeding <strong>the</strong> success <strong>of</strong><strong>the</strong> geo<strong>the</strong>rmal resource. Regolith mapping andremotely sensed im agery such a s radi ometricsare being u sed to find a reas <strong>of</strong> surface fluid113


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>leakages a nd pote ntial conduit fa ulting in sealanalysis and reservoir integrity studies.Magnetotellurics and Potential Field SurveysMagnetotellurics (MT) and potential field surveyscan be u sed to d efine <strong>the</strong> ba sic li mits <strong>of</strong> areservoir. MT has been an industry standard forover 20 years for defin ing geo<strong>the</strong>rmal reservoi rlimits and boun daries. The ‘fuzzy’ imagingproduced b y MT can pick up resistivityanomalies typically a ssociated with flui d bodies,large scale structures, a nd cap rocks. Thi stechnique h as bee n used within Australia withvarying su ccess, whi ch is <strong>of</strong>ten a produ ct <strong>of</strong>survey design as opposed to <strong>the</strong> reliability <strong>of</strong> <strong>the</strong>technique. M T modeli ng requires trial and e rror<strong>of</strong> forwa rd m odeling (Ara ngo et al. 200 9). Thisprocess generates different models that could fit<strong>the</strong> data, and trie s to a ssign th e m ost li kelymodel. Reliability <strong>of</strong> <strong>the</strong> MT is compromised as aresult <strong>of</strong> this . Ac cessory data r efines this err or;such <strong>the</strong> te chnique is better used in conjunctionwith o<strong>the</strong>r modeling techni ques. The mostimportant result from MT models is <strong>the</strong> ability toidentify <strong>the</strong> p resence <strong>of</strong> geo<strong>the</strong>rmal flu ids. Thi sis particularly useful in <strong>the</strong> identification <strong>of</strong> HSAreservoir systems. However, <strong>the</strong> recognition <strong>of</strong><strong>the</strong> fluid is still limited to <strong>the</strong> erro rs definedabove.MT is comm only being combine d with potentialfield modelin g. Magnetic and gravity survey shave be en used with geo<strong>the</strong>rmal p rojects todefine large scale stru ctures an d al so as <strong>the</strong>basis for d eterministic lithological varianceidentification sub surface. Potential fieldinversions are <strong>of</strong>ten co upled with p etrophysicallogs su ch as sonic and d ensity logs to create‘layer cake’ model s th at accumul ate to <strong>the</strong>potential field signatu res produ ced by <strong>the</strong>surveys. These te chniques provid eapproximately <strong>the</strong> same resolution <strong>of</strong> data as <strong>the</strong>MT tech niques do; h owever ca n be cheaper,and manipulated in different ways to account fordifferent geological scenarios.Seismic InterpretationsSeismic interpretation is not commonly used asa tool for EGS and HSA resou rce mod elevaluation. Seismic is typically used as a tool in<strong>the</strong> petroleum industry to extrapolate li thologicalboundaries across l arge area s with <strong>the</strong>assistance <strong>of</strong> well s. F eatures in cluded o nseismic are: formation and st ratigraphicboundaries, sedimentary features such as onlapand down la p patterns, f acies and sequencestratigraphy, stru cture, an d tectono stratigraphicrelationships. These features are all essential forcreating balanced geological models.A benefit <strong>of</strong> seis mic interpretation is that 2D and3D seismic surveys a re availabl e from mo stbasin and foldbelt terrains in Australia as a result<strong>of</strong> previou s petroleu m or acade mic wo rkconducted.Basic int erpretations can create t he basis <strong>of</strong> ageological m odel, an d can be t ru<strong>the</strong>d to o<strong>the</strong> raspects su ch as wells and pote ntial fieldsurveys.Advanced seismi c interpretation s can beconducted by pro cession <strong>of</strong> <strong>the</strong> seismic d atasuch that th e me chanical sig natures <strong>of</strong> <strong>the</strong>seismic t races a re tran sformed in particularways to hig hlight specific features (Nourollah etal. <strong>2010</strong> ). An example <strong>of</strong> this te chnique that isbeneficial in HSA syste ms is a p rocess calledNeural Network Inversio n Modeling (NNIM ).NNIM attemp ts to builds relation ships betwe endata sets si milar to <strong>the</strong> way <strong>the</strong> hu man b rainperceives an d analy ses d ata. The me chanicalsignature <strong>of</strong> a seismic wa velet is compared to aknown source, such as a well log, and particularfeatures characterized in <strong>the</strong> log are m atched to<strong>the</strong>ir co rresponding sei smic sig nature. Oncerelationships are built b etween well log s an dseismic traces using well defined data sets, thismodel can b e applied to o<strong>the</strong>r sei smic tracesaway from th e known well locations to gene ratetarget log s from sei smic sections. This processcan be used to define sand bodies in a potentialreservoir, fluids such a s gas and water an dassociated m igration pathways, p otential se alsand different lithological patterns that were not114


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>obvious in <strong>the</strong> initial seismic interpretation and tohighlight structures. Oth er fo rms <strong>of</strong> sei smicprocessing can produce similar results.Integration <strong>of</strong> Geological InterpretationsThe integ ration <strong>of</strong> interp retations in geo<strong>the</strong>rmalsystems i s rare. E xploration techni ques are<strong>of</strong>ten con sidered to be unique so urces <strong>of</strong>information, ra<strong>the</strong> r than part <strong>of</strong> a dynamicsystem. However, this is far from <strong>the</strong> truth.The integrating <strong>of</strong> th e full suite <strong>of</strong> available dataconstraints, inclu ding 2 D/3D rem ote sen sing,field, 2D-3D seismic, an d welllogs/picks/production v alidates g eologicalmodels and provides <strong>the</strong> basis for a constrainedHSA and EGS model.Techniques such a s g ravity and magneti cinversion which are co nsidered to be lowresolution interpretations c an have <strong>the</strong>irresolution increased by using petrophysical logs,seismic interpretation s, a nd surface data tobetter constrain <strong>the</strong> layers in <strong>the</strong> model. Seismiccan also beti de to surfa ce feature s, pa rticularlystructure to help defin e attitudes an d confirmstructure. Th e combi nation <strong>of</strong> <strong>the</strong>se te chniquesincreases <strong>the</strong> validation <strong>of</strong> <strong>the</strong> model.Revisiting Temperature modelingThermal ConductivityThermal conductivity <strong>of</strong> a ro ck determines th eefficiency (o r oth erwise) with which heat i spropagated through it. It is controlled by lithologyand state o f <strong>the</strong> ro ck (that is co mpaction,fracturing and meta morphic a ttributes).Accessory factors such as <strong>the</strong> presence <strong>of</strong> fluidssuch as water and gas also play a big role in this(Clauser & Hueng es 1995; Vasseur et al. 1995;Beardsmore 2004).Two primary methods are employed with respectto measuring conductivity: in situ measurementsconducted wi thin <strong>the</strong> sub surface usi ng loggingtools; a nd, la boratory m easurements preformedon small sections <strong>of</strong> rock. In situ measurementsare considered to be <strong>the</strong> best form <strong>of</strong> measuringconductivity as <strong>the</strong>y are done so within <strong>the</strong>actual surroundings that <strong>the</strong> ro ck exist s within.This i ncorporates f actors such as f luids,fracturing, pressure and compaction better thana sa mple done in a l ab. In situ me asurementsalso represent an ave rage over a la rge area o frock (Clauser & Huenges 1995).Lab measured samples have a higher precision,because fa ctors inhibiti ng to <strong>the</strong> in situmeasurements su ch a s e quipment difficultie s,drilling inte rference a nd general control issue sare negated. This ma kes <strong>the</strong> measurementmore precise, however, not more accurate.In places wh ere th ere is no data avail able fo rthis modeli ng, default <strong>the</strong>rmal con ductivities forend-member lithologie s that can bema<strong>the</strong>matically averag ed to reflect li thologicalmixtures as necessary, and so do not rely on <strong>the</strong>laboratory m easurement <strong>of</strong> co nductivities o ndown-hole samples can be used. This has beenrecognized as a useful a nd reasonably accuratetool as it do es not hav e t he large extrapolatio nand e rrors th at are a ssociated with <strong>the</strong> pre ciselaboratory m easurements (Cla user & Huenges1995). Estimating <strong>the</strong> conductivity <strong>of</strong> a rock canoccasionally miss fact ors such as mi norlithological changes, small fractu re zo nes an dpressure ch anges (Va sseur et al. 1995).However th ese tent to have minima l impactwhen avera ged ove r th e syste m, e speciallywhen used within a detailed geological model.Temperature ModelingModeling temperature a cross a large are arequires <strong>the</strong> measured te mperatures t o be fedinto a constructed geological mo del an dpropagated according to <strong>the</strong> physical constraintsinterpreted. Come rcially available s<strong>of</strong>tware ca n<strong>the</strong>n b e u sed to construct a m ore a nisotropic<strong>the</strong>rmal model. Burial hi story modeling s<strong>of</strong>twarethat is routinely used in petroleum exploration for<strong>the</strong> prediction <strong>of</strong> <strong>the</strong> degree and timing <strong>of</strong> sourcerock m aturation, re servoir tempe rature i sfavored a s it can inco rporate <strong>the</strong> physicalproperties o f rocks as well a s structure.Lithostratigraphic data from a well, or fromseismic interpretation, can be input to <strong>the</strong> burialhistorymodeling s<strong>of</strong>tware package and modeled115


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Salamander-1 – a geo<strong>the</strong>rmal well based on petroleum explorationresultsBertus de Graaf*, Ian Reid, Ron Palmer, David Jenson, Kerry ParkerPanax Geo<strong>the</strong>rmal Ltd, PO Box 2142, Milton, Qld 4064, Australia.Corresponding author: bdegraaf@panaxgeo<strong>the</strong>rmal.com.auSalamander-1 and <strong>the</strong> PenolaGeo<strong>the</strong>rmal ProjectSedimentary Aquifer (HSA) system <strong>of</strong> <strong>the</strong>Limestone Coast Geo<strong>the</strong>rmal Project.Panax Geo<strong>the</strong>rmal Ltd (“Panax”) has securedseveral Geo<strong>the</strong>rmal Exploration Licences (GELs),within troughs or grabens in <strong>the</strong> Otway Basin insou<strong>the</strong>ast South Australia (Fig 1). Toge<strong>the</strong>r <strong>the</strong>licences cover an area <strong>of</strong> more than 3,000 km 2 .The initial development <strong>of</strong> <strong>the</strong> Limestone CoastGeo<strong>the</strong>rmal Project is focused on <strong>the</strong> PenolaTrough (GEL 223 and GEL 484; Fig. 2) -promoted by an existing comprehensive database<strong>of</strong> historical informaton from extensive oil and gasexploration and production.The Penola Trough has been subjected tointensive oil and gas exploration, including 27deep petroleum wells with wireline logging andconventional core measurements <strong>of</strong> reservoirporosity and permeability. In addition, 321 km 2 <strong>of</strong>3D seismic and a significant amount <strong>of</strong> 2Dseismic data have been acquired in this area. All<strong>of</strong> this data is available as part <strong>of</strong> a public openfile database.Figure 1. Panax's geo<strong>the</strong>rmal licences in <strong>the</strong> LimestoneCoast Geo<strong>the</strong>rmal Project – demonstrating proximity toinfrastructureGeological settingThe Penola Geo<strong>the</strong>rmal Project lies within <strong>the</strong>Penola Trough, which is a Cretaceous-agedextensional basin formed on top <strong>of</strong> Palaeozoicbasement. It is covered in South Australia by GEL223 and GEL 484. The Penola Trough forms part<strong>of</strong> <strong>the</strong> Otway Basin, a rift basin initiated during <strong>the</strong>Cretaceous, on what is now <strong>the</strong> sou<strong>the</strong>rn margin<strong>of</strong> <strong>the</strong> <strong>Australian</strong> mainland. The trough contains athick accumulation <strong>of</strong> Cretaceous sediments andis bounded to <strong>the</strong> nor<strong>the</strong>ast by <strong>the</strong> PadthawayRidge, and to <strong>the</strong> southwest by <strong>the</strong> KalangadooHigh. Well and seismic data indicate that <strong>the</strong>sediment pile is six kilometres thick or more, in<strong>the</strong> deepest sections <strong>of</strong> <strong>the</strong> trough, including over1,000m thick sections <strong>of</strong> cretaceous Pretty HillFormation (sandstones).The Penola Trough area <strong>of</strong> <strong>the</strong> Limestone CoastProject bears many similarities with <strong>the</strong> ImperialValley area <strong>of</strong> California which includes <strong>the</strong> EastMesa and Heber geo<strong>the</strong>rmal areas (Bergosh etal., 1982). The East Mesa reservoir sandstonesare similar to <strong>the</strong> Pretty Hill Formation sandstone,which is <strong>the</strong> target reservoir <strong>of</strong> <strong>the</strong> propsed HotFigure 2. Panax's geo<strong>the</strong>rmal licences in <strong>the</strong> LimestoneCoast Geo<strong>the</strong>rmal Project – outlining four major troughzones, including <strong>the</strong> Penola Trough and <strong>the</strong> PenolaGeo<strong>the</strong>rmal ProjectThe Pretty Hill Sandstone was deposited by a lowsinuosity, high energy, sand-rich river system(Scholefield et al, 1996). Its good reservoir qualityhas been known from petroleum activities for117


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>some time. Significant permeability is preserved in<strong>the</strong> formation at depths <strong>of</strong> up to 3,500m.3D seismic data has been particularly useful inmapping <strong>the</strong> distribution <strong>of</strong> <strong>the</strong> porous sandstones<strong>of</strong> <strong>the</strong> Pretty Hill Formation. The seismic responseevident on 3D data represents to some extent <strong>the</strong>porosity distribution within <strong>the</strong> Pretty HillFormation (Boult & Donley, 2001). The loweracoustic impedance <strong>of</strong> <strong>the</strong> more poroussandstones can be identified on <strong>the</strong> basis <strong>of</strong> <strong>the</strong>data (with varying degrees <strong>of</strong> success), and hasbeen used to map <strong>the</strong> distribution <strong>of</strong> individualsandstone bodies.TroughLimestone Coast Geo<strong>the</strong>rmal Resources 1.Measured(PJ)Indicated(PJ)Inferred(PJ)Total(PJ)Report Da tePenola 11 ,000 32,000 89,000 132,000 18/02/2009Rivoli & St. Clair 53,000 53,000 28/01/2009Rendelsham 17 ,000 17,000 28/01/2009Tantanoola 130,000 130,000 31/03/2009Total 11,000 32,000 289,000 332,0001.by Dr. Graeme Beardsmore <strong>of</strong> Hot Dry Rocks Pty Ltd, Melbourne, AustraliaTable 1 - Reproduced from <strong>the</strong> 2008 Penola Trough Reportby Dr. Graeme Beardsmore (Hot Dry Rocks Pty Ltd)Temperature data, and rationale forSalamander-1A numerical model was generated for <strong>the</strong> PenolaTrough to compute, in three dimensions, <strong>the</strong>distribution <strong>of</strong> temperature which best matches<strong>the</strong> observed surface heat flow distribution, whilerespecting <strong>the</strong> laws <strong>of</strong> conductive heat transfer,and <strong>the</strong> <strong>the</strong>rmal properties <strong>of</strong> <strong>the</strong> geologicalstrata. The model predicted that <strong>the</strong> temperatureis relatively constant around 160°C at 4,000 mwithin most <strong>of</strong> <strong>the</strong> Penola Trough. Thistemperature modeling and a knowledge <strong>of</strong> <strong>the</strong>reservoir quality provided <strong>the</strong> rationale for <strong>the</strong>drilling <strong>of</strong> <strong>the</strong> first geo<strong>the</strong>rmal well, Salamander-1,in <strong>the</strong> Penola Trough in <strong>the</strong> first quarter <strong>of</strong> <strong>2010</strong>.Additionally, Beardsmore (2009), assessed <strong>the</strong>Limestone Coast Geo<strong>the</strong>rmal Project for itsgeo<strong>the</strong>rmal potential and determined a “MeasuredGeo<strong>the</strong>rmal Resource” <strong>of</strong> 11,000PJcomplemented by an additional 32,000 PJ <strong>of</strong>“Indicated Geo<strong>the</strong>rmal Resource”, see Table 1below. This resource classification was inaccordance with <strong>the</strong> <strong>Australian</strong> Code forReporting <strong>of</strong> Exploration Results, Geo<strong>the</strong>rmalResources and Geo<strong>the</strong>rmal Reserves, 2008edition.This highly encouraging resource classification,<strong>the</strong> third in Australia and second-ever resourceclassification <strong>of</strong> a HSA, confirmed <strong>the</strong> highpotential <strong>of</strong> geo<strong>the</strong>rmal energy development insedimentary basins.The ability to directly assess this significantgeo<strong>the</strong>rmal resource potential is courtesy <strong>of</strong> <strong>the</strong>long history <strong>of</strong> petroleum exploration withnumerous wells and seismic surveys, see figure 3below.Figure 3. GEL 223 – Penola Geo<strong>the</strong>rmal Project showingoutline <strong>of</strong> <strong>the</strong> Measured Geo<strong>the</strong>rmal Resource, andinformation relating to prior petroleum wells drilled in <strong>the</strong>area.Salamander-1 drilling objectivesSalamander-1 is <strong>the</strong> first geo<strong>the</strong>rmal well in <strong>the</strong>project area. It was drilled in Panax’s Geo<strong>the</strong>rmalExploration Licence 223 (GEL223), in <strong>the</strong> firstquarter <strong>of</strong> <strong>2010</strong>.The drilling objective for Salamander 1 was tointersect <strong>the</strong> Pretty Hill Formation (reservoir) at adepth <strong>of</strong> 3,000m and continue to 4,000m tosecure an intersection <strong>of</strong> 1,000m <strong>of</strong> <strong>the</strong> reservoir.To minimise <strong>the</strong> risk <strong>of</strong> intersecting gas, <strong>the</strong> wellwas sited 5km away from <strong>the</strong> closest gasproducing well (now depleted) and at least 500mvertically down dip <strong>of</strong> any gas producing well.Also, a fur<strong>the</strong>r drilling requirement was that nosignificant faults should exist between <strong>the</strong> closestgas producing well, and Salamander 1 - that couldpotentially be a gas seal.To minimise friction losses in a future productionenvironment, <strong>the</strong> casing scheme was designed aswide as possible, although standard casing118


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>dimensions and safety issues took precedence.Figure 4 below presents <strong>the</strong> casing scheme forSalamander 1.DrillingSalamander was drilled with Wea<strong>the</strong>rford’s Rig828 and <strong>the</strong> design and management <strong>of</strong> <strong>the</strong> wellwas contracted to AGR.Penetration (ROP), Panax elected to set 13-3/8”casing at this depth. The 13-3/8” casing was runand cemented at 1764m.The 12 ¼” hole was drilled using Schlumberger’sPower V system, an auto-vertical seekingdirectional drilling tool, to maintain verticality. TheROP in <strong>the</strong> 12-1/4” section was extremely goodand intersected <strong>the</strong> top <strong>of</strong> Pretty Hill Formation at2,900m, some 150m shallower than <strong>the</strong> originalprognosis.Figure 5. Salamander-1 Well Completion SchematicFigure 4. Schematic illustration <strong>of</strong> <strong>the</strong> well design and wellcasing design – Salamander-1WDI Rig 828 was handed over to Panax at <strong>the</strong>rig’s previous engagement at 20:00 on 12December, 2009. The rig move to Salamander 1was disrupted due to poor wea<strong>the</strong>r restrictingtruck access to <strong>the</strong> rig, in particular <strong>the</strong> largertransporters. Salamander-1 was spudded at 23:45on 31 January <strong>2010</strong>.The 24” hole was drilled from <strong>the</strong> base <strong>of</strong> <strong>the</strong> 26”conductor to 503m, and 18-5/8” casing was runand cemented at 499m (Figure 4).The 17-1/2” hole was drilled from <strong>the</strong> 24” casingshoe to 1,766m. Due to lower Rates <strong>of</strong>A cement plug was set from 2,800 – 2,900m tostabilise this zone, and <strong>the</strong> 9 5/8” liner was runand cemented at 2,896m.The 8-1/2” hole section was drilled to 4,025m witha bit change made at 3,670m. An EMS directionalsurvey was recorded at TD and Open Hole logswere run. A 7” perforated liner was run and set tobottom.Following displacement <strong>of</strong> <strong>the</strong> drilling fluid withbrine, and with <strong>the</strong> wellhead and Christmas treeinstalled, <strong>the</strong> rig was released at 1500 hrs 26March, <strong>2010</strong>.The well was drilled to a total depth <strong>of</strong> 4,025metres in 45 days (inclusive <strong>of</strong> 3 rig repair days)119


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>using only 6 drilling bits, setting a new drillingrecord for <strong>the</strong> <strong>Australian</strong> geo<strong>the</strong>rmal sector.Importantly, <strong>the</strong> Salamander-1 drilling programmewas concluded with zero Lost Time IncidentsWireline loggingThe wire-line logging services were provided bySchlumberger, and four trips were planned. Themain objectives <strong>of</strong> <strong>the</strong> wire-line logging were to: i)determine formation acoustic velocities to tie in<strong>the</strong> well with 3D surveys, ii) observe pressureregimes to determine <strong>the</strong> absence <strong>of</strong> anyhydrocarbons, and iii) collect information aboutformation density and porosity. The wire-lineprogramme is presented in Table 2 below.LogXY Cal-GRDLL MSFLLDT CNL-GRHNGSSonicScannerMDT-GRVSI-4Interval2890 – 1750m4021.5 – 2898m3738 – 28984025 – 29892900 – surface. Sonicscanner switch modes toCement Bond Log37 points (could not pass3845m)3810 to 99mTable 2 – Wireline Logs ObtainedSalamander-1 Well ResultsThe recently announced 15.4°C increase in <strong>the</strong>measured bottom hole temperature (“BHT”) <strong>of</strong> <strong>the</strong>Salamander-1 well, from 156°C to 171.4°C, whichis likely to have been caused by breakthroughfrom <strong>the</strong> well bore to <strong>the</strong> reservoir, has confirmedpredictions <strong>of</strong> <strong>the</strong> regional 3D temperaturemodelling by Hot Dry Rocks Pty Ltd (HDR Report,2008). Figure 6 below shows that <strong>the</strong> 3Dmodelled temperature at 4,025m for <strong>the</strong>Salamander-1 well <strong>of</strong> 172°C is very close to <strong>the</strong>recently measured BHT at 4,000m <strong>of</strong> 171.4°C.This figure also shows that projectedtemperatures at 4,000m increase to <strong>the</strong> south andsouth-east into Panax’s GEL484, reaching 180°Cwithin 4km <strong>of</strong> Salamander-1.The new BHT <strong>of</strong> Salamander-1 combined with <strong>the</strong>new 3D temperature modelling is likely toincrease <strong>the</strong> geo<strong>the</strong>rmal resources <strong>of</strong> GEL223.More importantly, it upgrades <strong>the</strong> overall regionalpotential <strong>of</strong> <strong>the</strong> Penola Geo<strong>the</strong>rmal Project, withhigher temperatures allowing <strong>the</strong> proposed poweroutputs to be achieved with lower flow rates.Figure 6 - Penola Trough, 3D conductive heat flow modelling(HDR, 2008) - predicted 172°C @ 4,025m, while <strong>the</strong> actualmeasured temperature at Salamander-1 for this depth was171.4°C – recently measured.A borehole seismic survey (vertical seismic pr<strong>of</strong>ileor VSP) was recorded by Schlumberger in <strong>the</strong>near vertical Salamander-1, on 19 March <strong>2010</strong>.This VSP allowed a good correlation <strong>of</strong> <strong>the</strong>Salamander-1 penetrated geology with <strong>the</strong> 3Dseismic data. Examination <strong>of</strong> <strong>the</strong> seismic datacorrelated to Salamander-1 located towards <strong>the</strong>sou<strong>the</strong>ast <strong>of</strong> <strong>the</strong> GEL, shows an excellentcorrelation, with a more reflective seismicpackage in <strong>the</strong> upper section <strong>of</strong> <strong>the</strong> Pretty HillFormation. Seismic attributes <strong>of</strong> reflectionstrength, and volume attributes <strong>of</strong> RMS reflectionstrength were used to determine <strong>the</strong> arealdistribution <strong>of</strong> <strong>the</strong>se more porous sandstones. Asingle reservoir body is interpreted extending from<strong>the</strong> Ladbroke Grove gasfield area, through <strong>the</strong>Salamander-1 well, and 6.5km to <strong>the</strong> south east -covering an area <strong>of</strong> approximately 22.5km 2 . Thiszone is interpreted as having similar reservoirproperties to those in <strong>the</strong> well.Full analysis <strong>of</strong> <strong>the</strong> petrophysical review arecurrently in progress and will be available at <strong>the</strong>time that <strong>the</strong> paper is presented in November<strong>2010</strong>.A review <strong>of</strong> <strong>the</strong> wireline logging data <strong>of</strong> <strong>the</strong> openhole section <strong>of</strong> <strong>the</strong> Salamander-1 well (from2,900m to 4,025m) for estimating <strong>the</strong> reservoirquality <strong>of</strong> <strong>the</strong> target reservoir rocks (<strong>the</strong> Pretty HillSandstone) has been completed by Down UnderGeosolutions (“DUGEO”) based in Perth. Wehave been advised that <strong>the</strong> combination <strong>of</strong> <strong>the</strong>“Lin-Log and MDT methods” are <strong>the</strong> mostappropriate to estimate <strong>the</strong> “transmissivities” (≈120


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>reservoir quality) <strong>of</strong> <strong>the</strong> intersected targetreservoir rocks.DUGEO has advised that <strong>the</strong> transmissivities inDarcy metres (Dm) <strong>of</strong> <strong>the</strong> Pretty Hill Sandstone in<strong>the</strong> open hole section <strong>of</strong> Salamander-1 well rangefrom 6.7 Dm to 13.5 Dm, as set out in Table 3below:MostLikelyCaseMaximumCaseMethodAverageLin-LogrelationshipOptimisticLin-LogrelationshipTransmissivity(Dm)6.713.5Table 3. Transmissivity RangeA number <strong>of</strong> depleted gas wells withinapproximately a 5km radius <strong>of</strong> Salamander-1were checked for injection potential. It isestimated that 4 <strong>of</strong> <strong>the</strong>se wells could accept morethan 100 l/s in <strong>the</strong>ir current configuration andmore than 200 l/s after workover, with fur<strong>the</strong>rimprovement possible with additional perforation.The costs <strong>of</strong> working over <strong>the</strong>se wells are in <strong>the</strong>range $2-3m each, which is a much moreeconomic proposition than drilling a purpose builtreinjection well.Salamander-1 Reservoir Testing Program –Step 1 :Transmissivity is loosely described as <strong>the</strong>capacity <strong>of</strong> <strong>the</strong> reservoir to flow water. The “MostLikely Case” <strong>of</strong> 6.7 Dm is lower than <strong>the</strong> minimumrequirements <strong>of</strong> 10 Dm for a flow rate <strong>of</strong> 175 l/sec@ 145°C. However, with higher geo<strong>the</strong>rmaltemperatures now apparent (from <strong>the</strong> most BHTmeasurement in Salamander-1, and consistentwith <strong>the</strong> 3D temperature modelling), flow ratescould be reduced as <strong>the</strong>se two inputs areinversely proportional. Also, <strong>the</strong> “Maximum Case”estimate provides <strong>the</strong> upside.Salamander-1 Well TestingSalamander-1 was discharged using air lift to a10,000m 3 capacity HDPE lined pond. Steam wasvented to atmosphere from a flash tank and waterflow was measured using a weir plate.The reservoir fluids collected in <strong>the</strong> pond will beused for <strong>the</strong> injection test which is <strong>the</strong> last test tobe carried out on <strong>the</strong> well.a. Flow well using air lift;b. Measure pressure, temperature and flow(surface), down hole logging tools in <strong>the</strong>target reservoir measure pressure,temperature and flow.Salamander-1 Reservoir Testing Program –Step 2 :Analysis <strong>of</strong> downhole pressure and temperaturedata obtained during short cleanup flows,although indicating higher than expectedtemperatures, up to 171 deg C also indicatedinitial mud damage that arose during drilling.The well was acidized using 15% acetic acid inorder to remove <strong>the</strong> skin damage caused bycalcium carbonate and flowed again usingnitrogen gas lift. Results <strong>of</strong> this operation areawaited.Results <strong>of</strong> production and injection testing arepending. Based on <strong>the</strong> results <strong>of</strong> <strong>the</strong>se tests, <strong>the</strong>feasibility <strong>of</strong> installing a pilot plant will beinvestigated.121


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>c. Re-inject produced geo<strong>the</strong>rmal brineusing filtration unit and high pressurepump;d. Down hole logging tools in <strong>the</strong> targetreservoir measure pressure, temperatureand flow.Sand81-7008, Terra Tec Inc under contract toSandia National Laboratories.Boult, P.J., and Donley, J., 2001, VolumetricCalculations Using 3D Seismic Calibrated AgainstPorosity Logs — Pretty Hill Formation Reservoirs,Onshore Otway Basin. Eastern <strong>Australian</strong> BasinsSymposium, 2001Scholefield, T., North, C.P., and Parvar, H.L.,1996, Reservoir characterisation <strong>of</strong> a lowresistivity gas field – Otway Basin, SouthAustralia, APPEA Journal 1996.Figure 7. Salamander-1 Well clean-up flow test, May <strong>2010</strong>.Salamander-1 – Interpretation AndAnalysis Of Well Testing ResultsAt <strong>the</strong> time <strong>of</strong> writing this Abtract, this work iscurrently being undertaken.This will be available for presentation at <strong>the</strong> timethat <strong>the</strong> paper is presented in November <strong>2010</strong>.ReferencesBeardsmore, G. R., 2008, Limestone CoastProject: Penola Geo<strong>the</strong>rmal Play. Statement <strong>of</strong>Geo<strong>the</strong>rmal Resources. Hot Dry Rocks Pty Ltd,2008.Bergosh et al 1982, Mechanisms <strong>of</strong> FormationDamage in Matrix Permeability Geo<strong>the</strong>rmal Wells,122


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Petrophysical Methods for Characterization <strong>of</strong> Geo<strong>the</strong>rmal ReservoirsBen Clennell 1 , Lionel Esteban* 1 , Ludovic Ricard 1,3 , Mat<strong>the</strong>w Josh 1 , Cameron Huddlestne-Holmes 1 , JieLiu 2 , Klaus Regenauer-Lieb 1,2,31 CSIRO Earth Science & Resources Engineering, ARRC, 26 Dick Perry Avenue, Kensington2 University <strong>of</strong> Western Australia, M004, 35 Stirling Av., 6009 Crawley3 Western <strong>Australian</strong> Geo<strong>the</strong>rmal Centre <strong>of</strong> Excellence, ARRC, 26 Dick Perry Avenue, KensingtonAbstract: Australia has a unique wealth <strong>of</strong> nonvolcanicgeo<strong>the</strong>rmal resources. To tap <strong>the</strong>se forlocal and distributed energy needs, optimaltargeting and development strategies for <strong>the</strong>reservoirs are needed. In <strong>the</strong> case <strong>of</strong> HotSedimentary Aquifers (HSA), many tools forformation evaluation developed in <strong>the</strong> oil and gasindustry for High Pressure/ High Temperatureenvironments could be applied directly; thisapplies both to downhole tools and laboratorycharacterization methods. The standard suite <strong>of</strong>petrophysical methods is adequate fordetermining basic matrix and fluid characteristics,but for full characterization <strong>of</strong> flow andgeomechanical parameters advanced acousticand nuclear magnetic resonance tools could finda place, at least for high value resources. In bothcrystalline rock and HSA plays, image logs are avital tool, not least for enabling improved core-tologworkflows. Understanding <strong>of</strong> <strong>the</strong> <strong>the</strong>rmalproperties <strong>of</strong> rock and how that relates to fieldscale <strong>the</strong>rmal structure is ano<strong>the</strong>r challengeunfamiliar to most petrophysicists. Modelling frompore/grain through to formations scale is vital forassessing both <strong>the</strong>rmal and flow performance.CSIRO and <strong>the</strong> Western <strong>Australian</strong> Geo<strong>the</strong>rmalCentre <strong>of</strong> Excellence have brought toge<strong>the</strong>rexperience and capabilities in rock physical and<strong>the</strong>rmal properties and in this paper review whatpetrophysical tools and methods are available to<strong>the</strong> geo<strong>the</strong>rmal industry and illustrate some <strong>of</strong> <strong>the</strong>research currently underway.Keywords: Petrophysics, Reservoir CharacterizationThermal Conductivity, Heat Capacity,Porosity, Permeability, HP/HT.IntroductionAustralia’s immense geo<strong>the</strong>rmal energy resourceshave <strong>the</strong> potential to contribute significantly to ournation’s demand for affordable and sustainableclean energy. However, for <strong>the</strong> efficientexploitation <strong>of</strong> geo<strong>the</strong>rmal energy a goodcharacterization <strong>of</strong> <strong>the</strong> reservoir is a prerequisite.Petrophysics is <strong>the</strong> systematic investigation <strong>of</strong>rock and fluid physical properties to understand<strong>the</strong> rock type and fluid flow performance <strong>of</strong>underground formations. Petrophysicaltechniques measure <strong>the</strong> physical and chemicalproperties <strong>of</strong> <strong>the</strong> rock ei<strong>the</strong>r in situ (well logging)or in a lab (core and chips). The data generatedfrom <strong>the</strong>se analyses can be used to characterize<strong>the</strong> reservoir rock’s composition, structure,porosity and permeability, temperature, pressureand mechanical properties, leading to a betteroverall understanding <strong>of</strong> <strong>the</strong> resource.Petrophysical methods for <strong>the</strong> characterization <strong>of</strong>geo<strong>the</strong>rmal reservoirs have progressedsignificantly overseas particularly for <strong>the</strong> extremeenvironments such as HR and volcanic sources.In this paper we describe CSIRO’s expertise in<strong>the</strong> Petroleum sector, which is directly applicableto HSA. It is our intention to grow this expertisefur<strong>the</strong>r into <strong>the</strong> HR domain.Our petrophysical characterization <strong>of</strong> geo<strong>the</strong>rmalreservoirs forms part <strong>of</strong> a larger collaborativeinitiative <strong>of</strong> CSIRO and Universities working withindustry and government with <strong>the</strong> aim to reduce<strong>the</strong> risks <strong>of</strong> implementing geo<strong>the</strong>rmal technologythrough computationally assisted guidance <strong>of</strong>drilling programs to target locations and depths.The core <strong>of</strong> <strong>the</strong> required scientific innovation willbe to develop new data assimilation inversiontools, which ensure that all available information,including geologic, geophysical, geomechanics,fluid dynamics, rock physics, geochemistry andeconomic data is integrated into <strong>the</strong> subsurfaceand above-ground geo<strong>the</strong>rmal design. In thiscontribution we focus on <strong>the</strong> petrophysicalmethods for characterization <strong>of</strong> geo<strong>the</strong>rmalreservoirs. These comprise <strong>the</strong> characterization <strong>of</strong>rock mechanical, <strong>the</strong>rmal, geochemical and fluidpermeability properties.Standard petrophysical tools andcharacterization workflowsSince <strong>the</strong> Schlumberger bro<strong>the</strong>rs invented <strong>the</strong> firstdownhole electric log in <strong>the</strong> 1920s, <strong>the</strong> oil and gasindustry has provided <strong>the</strong> platform to develop awide range <strong>of</strong> petrophysical logging tools, (seeEllis and Singer 2007). The range <strong>of</strong> physicalproperties that can be sensed today is impressive(Table 1). While <strong>the</strong> uptake <strong>of</strong> down-holetechnologies in water, mining and environmentalsectors has largely been limited by cost to a basicsuite, certain slim-hole and extreme environmenttools have been developed outside <strong>of</strong> oil and gas,most notably for borehole imaging.Petrophysical characterization serves three mainpurposes, each with its own workflow to: (1)define <strong>the</strong> lithostratigraphy, and <strong>the</strong>refore help ingeological correlation between wells and definition<strong>of</strong> reservoir structure; (2) quantify matrix, fluid and123


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Table 1Type <strong>of</strong> tool Physics employedwhatis measuredResistivitygalvanicResistivityinductionGamma raystandardSpontaneouspotential (SP)Density logPhotoelectriceffectNeutron logSonic LogGamma rayspectralMagneticsusceptibilityGeochemicalLogging ToolElementalCaptureSpectroscopyDielectric logNuclearmagneticresonanceWaveformsonicDirect currentinjected into <strong>the</strong>formation, usuallyfocused electrodearray.Coil magnetic fieldtransmitter inducesground loops information, measuresconductivity <strong>of</strong>formationScintillator detectstotal radioactivity <strong>of</strong>formationElectrochemicallyand electrokineticallyinduced potentialsUses backscatteredgamma rays from aradioactive source,typical 137 Cs.Measured fromrelative energyabsorption from <strong>the</strong>density sourceDetects neutronabsorption fromhydrogen nucleiGeo<strong>the</strong>rmalapplicationRelations betweenporosity, watersaturation and watersalinity.Relations betweenporosity, watersaturation and watersalinity.Shaliness, heatproductionPore water salinity.Indicator <strong>of</strong> clay layersvs sand layers,permeability <strong>of</strong> <strong>the</strong>latter.Sensitive to formationbulk density, based onatomic numbercontrasts.Indicates mineralelectron densitySensitive to watercontent including claybound waterPorosity and strengthCompressional wavevelocity(stiffness) <strong>of</strong> formation<strong>Energy</strong> sensitivity Shaliness, rockdetectors distinguish geochemistry heatU, Th and K productionMeasures magneticpermeability <strong>of</strong> <strong>the</strong>formation byinductive coupling oro<strong>the</strong>r means.Measures spectra <strong>of</strong>gamma absorptionre-emissionMeasures gammaspectra from nucleiactivated by neutroncapturePermittivity fromattenuation andphase <strong>of</strong> propagatingelectromagneticwaveTransverserelaxation time <strong>of</strong>hydrogen nucleiCompressional andshear wavesCan provide goodlithologicaldiscrimination, even <strong>of</strong>very thin layers, and incrystalline rocksIdentifies a wide range<strong>of</strong> specific elements,especially heavy onesIdentifies a narrowrange <strong>of</strong> specificelements, especiallyheavy onesPorosity/saturationindependent <strong>of</strong> salinity.Shale and textureindicatorFluids content, poresize and permeabilityestimateGeomechanicsflow properties <strong>of</strong> <strong>the</strong> reservoir and (3) assessstresses and geomechanical properties in situ.1. For definition <strong>of</strong> lithology and structure one islooking to use tools, such as gamma ray,resistivity and sonic, which show substantialcontrasts between different lithologies. At thisstage, quantitative relationships are less importantthan <strong>the</strong> signatures that mark boundaries betweencorrelated rock units. In crystalline rock situationsmagnetic susceptibility (not generally used in oiland gas exploration) is valuable to identify certaingeological markers. At <strong>the</strong> next level <strong>of</strong> detail werequire identification <strong>of</strong> features such as tiltedbeds, coal seams, igneous dykes, faults andfractures. Dip logs and image logs are most usefulhere. The best type <strong>of</strong> imaging tool for ageo<strong>the</strong>rmal hole (borehole televiewer for air orclean water filled holes, ultrasonic scanning tool)may be different from that used mostly in oil andgas (formation resistivity array imager). Incrystalline rocks, flow properties begin and endwith fractures, so image logs are especially vital.Resistivity images have <strong>the</strong> advantage that openand flowing fractures may have different contrastto closed or non-flowing ones.In <strong>the</strong> laboratory we gain complimentarylithological information from petrographic analysis<strong>of</strong> cores and cuttings samples, usually aided byoptical and electron microscopy. Structurallogging <strong>of</strong> core can define fault and fracture sets,determine relative timing, and differentiate naturalfrom drilling-induced fractures, which is notalways possible from borehole images alone.2. For quantitative formation evaluation for a HSAtarget reservoir, combining <strong>the</strong> basic “oilfield”tools performs a vital function. Density andneutron tools enable porosity to be delineated,along with some understanding <strong>of</strong> matrixmineralogy and especially clay content. Neutronporosityto density porosity ratio can indicatezones not completely saturated with water, andwith gamma ray, indicates clay content. Clayfraction has a first order effect on permeability,even if porosity is constant. Sonic logs canreinforce <strong>the</strong> interpretation <strong>of</strong> porosity, andindicate zones that are more or less fractured.Resistivity and spontaneous potential can beanalysed toge<strong>the</strong>r with an understanding <strong>of</strong> <strong>the</strong>clay content and porosity, to deduce pore watercontent, saturation and salinity. This informationalso helps integrate downhole observations withsurface electromagnetic geophysical surveyssuch as deep resistivity or magnetotellurics (MT).Wireline-conveyed formation testing (e.g. MDT*)is <strong>the</strong> final technology used in a standard “oilfield”petrophysical evaluation. Drawdown and build-uptests define permeability and can also becombined with fluid sampling. Wireline testers<strong>of</strong>fer a much more versatile solution than largerscale packer tests or drill stem tests, though <strong>the</strong>124


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>latter are required in crystralline rocks oro<strong>the</strong>rwise low-matrix-permeability settings.Laboratory measurements on core substantiallyreduce <strong>the</strong> uncertainty in formation evaluation. At<strong>the</strong> CSIRO petrophysics laboratory for example,we routinely measure porosity and permeability <strong>of</strong>core samples under overburden conditions,electrical properties at a wide range <strong>of</strong>frequencies corresponding to different loggingtools, and sonic compressional and shear wavevelocities under conditions <strong>of</strong> (P, T) in situ stress.3. Stresses in <strong>the</strong> Earth are complex, and definingstress conditions in a borehole can be a difficultprocess. Generally it is based on <strong>the</strong> analysis <strong>of</strong>break-out and fracture patterns observed in imagelogs, complimented by formation pressure testsdesigned to open natural fractures and/or inducenew fractures. To interpret <strong>the</strong>se results andmake predictions <strong>of</strong> reservoir performance,“fracture-ability”, well stability in <strong>the</strong> reservoir andoverburden, it is desirable to have core suitablefor geo-mechanical testing. From core testsunconfined compressive stress, cohesive strengthand frictional strength parameters can bedetermined directly and used to construct aMechanical Earth Model. At CSIRO we conductsuch tests routinely, and have recently obtained aHigh Pressure (to 150 MPa confining, >500 MPaaxial) High Temperature (to 200 C) triaxial rig andwith 20 channel acoustic emission to monitor in3D <strong>the</strong> development and coalescence <strong>of</strong>fractures. Sonic logs are used widely forgeomechanical interpretation, and coremeasurement <strong>of</strong> P and S velocities and <strong>the</strong>iranisotropy is very helpful for defining rock physicsand mechanical property models. This also closes<strong>the</strong> loop for seismic-to-log-to-core workflows.Smarter petrophysics: geo<strong>the</strong>rmalapplications <strong>of</strong> non-standard tools.The limited scope <strong>of</strong> standard tools has led tomore exotic physics being applied to formationevaluation in oil and gas. Some special tools haveobvious HSA applications but require cost/benefitto be proven. Extreme condition versions <strong>of</strong> someadvanced oilfield tools do not even exist yet.An obvious “upgrade” is to use a spectral gammaray tool that quantifies <strong>the</strong> U, Th and K content <strong>of</strong><strong>the</strong> formation. This enables quantification <strong>of</strong> in situheat production, and is also useful for rock typing.Natural gamma tools can be cross-calibrated withlaboratory spectral gamma ray detectioninstruments used for recovered cores or chips.Geochemical Logging Tool (GLT* ) and neutronactivation (e.g. ECS* or FLEX*) logs can beemployed to quantify a subset <strong>of</strong> <strong>the</strong> chemicalelements in <strong>the</strong> formation. The GLT has been* MDT, GLT and ECS are marks <strong>of</strong> Schlumberger.FLEX is a mark <strong>of</strong> Baker Hughesused in both sedimentary and crystalline rocks,including hydro<strong>the</strong>rmal zones, in <strong>the</strong> OceanDrilling Program, with excellent results. The GLTis complex, having active neutron and gammasources coupled with filtered detectors and apassive natural gamma ray spectroscopy module.Hot sources raise obvious issues <strong>of</strong> HSEpermitting. The ECS approach can be engineeredto use a non-chemical neutron source called aminitron, essentially a small particle accelerator in<strong>the</strong> tool. However, <strong>the</strong> number <strong>of</strong> elementsdetected by ECS is limited, as is its track recordfor hard rock situations.Ano<strong>the</strong>r oilfield technology <strong>of</strong> potential value inhot sedimentary aquifers is Nuclear MagneticResonance (NMR) spectroscopy. NMR toolsmeasure <strong>the</strong> magnetic spin relaxation <strong>of</strong> hydrogennuclei, and <strong>of</strong>fer <strong>the</strong> only way to determine rockpore size distribution and <strong>the</strong>reby estimateformation permeability in a continuous way. Thisis an excellent way to interpolate pointmeasurements from permeability tests on core,and compare with formation tests from MDT.NMR also provides a salinity-independent totalporosity and an estimate <strong>of</strong> clay content. CSIROis currently comissioning an elevated P/T NMRcore testing capability which will help to assess<strong>the</strong> value proposition <strong>of</strong> NMR petrophysics forHSA geo<strong>the</strong>rmal applications.Temperature limits on measurementsSome technologies such as NMR, which dependson magnets, and some spectroscopic tools withcrystal detectors have inherent temperaturelimitation making <strong>the</strong>ir application to hottergeo<strong>the</strong>rmal settings unlikely. On <strong>the</strong> o<strong>the</strong>r hand,various logging tools have been developedspecifically for geo<strong>the</strong>rmal boreholes: <strong>the</strong> extremeenvironment televiewer for example. Theexploitation <strong>of</strong> ultra-deep (>5000 m) and HighPressure High Temperature (HPHT, or >150 C >70 MPa) oil fields has also driven <strong>the</strong>development <strong>of</strong> sophisticated petrophysical toolsthat can perform in extreme environments,leading to a convergence <strong>of</strong> technology towards<strong>the</strong> needs <strong>of</strong> <strong>the</strong> burgeoning geo<strong>the</strong>rmal market.Major players like Schlumberger, Baker Hughesand Wea<strong>the</strong>rford compete in this market withsmall and specialised tool suppliers, including agrowing number from Australia. Standard toolsare available up to at least 260 C and 200 MPa.We <strong>the</strong>refore see expanding options to deploysuch oilfield tools—or cheaper versions <strong>of</strong> <strong>the</strong>m—into <strong>the</strong> geo<strong>the</strong>rmal marketplace.In <strong>the</strong> laboratory also, standard oilfield analysisequipment for porosity, permeability, resistivityetc. is not designed for <strong>the</strong> extremes <strong>of</strong>geo<strong>the</strong>rmal conditions. A typical operating rangeis 70 MPa and 100C. At least in a researchcontext, systems have been engineered enablingall <strong>of</strong> <strong>the</strong>se parameters to be obtained under in125


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>situ formation conditions and throughoutprolonged experiments (e.g. Milsch et al. 2008).Understanding <strong>the</strong> <strong>the</strong>rmal structureWhe<strong>the</strong>r it is a Hot Sedimentary Aquifer (HSA) orEnhanced Geo<strong>the</strong>rmal System (EGS), appraisaland exploitation <strong>of</strong> a geo<strong>the</strong>rmal reservoirrequires a detailed characterization <strong>of</strong> <strong>the</strong>rmalproperties and heat flows. The temperaturedistribution on <strong>the</strong> underground is driven by <strong>the</strong>surface climate, <strong>the</strong> characteristics <strong>of</strong> <strong>the</strong> rocks toconduct, produce and accumulate <strong>the</strong> heat andalso <strong>the</strong> fluid circulation into <strong>the</strong> rocks and <strong>the</strong>basal (or mantle) heat flow. When estimating <strong>the</strong>temperature at depth, we have to consider <strong>the</strong>main mechanism driving <strong>the</strong> <strong>the</strong>rmal flow andtemperature distribution according to <strong>the</strong>controlling equation.T C V. grad T div .grad T Az0tHere ρ is mass density, C <strong>the</strong> specific heatcapacity, T <strong>the</strong> temperature, V <strong>the</strong> fluid velocityvector, lambda <strong>the</strong> <strong>the</strong>rmal conductivity, and A <strong>the</strong>specific heat production per unit rock volume. In<strong>the</strong> absence <strong>of</strong> fluid flow, rock <strong>the</strong>rmalconductivity estimation is adequate for <strong>the</strong>characterization <strong>of</strong> <strong>the</strong> <strong>the</strong>rmal conduction regime.An estimation <strong>of</strong> <strong>the</strong> specific heat <strong>of</strong> <strong>the</strong> rock willprovide direct insights on <strong>the</strong> stored heat. Thisparameter will also play an important role during<strong>the</strong> production <strong>of</strong> <strong>the</strong> reservoir as <strong>the</strong> rockreleases <strong>the</strong> stored energy to <strong>the</strong> working fluid.The radiogenic heat production rate <strong>of</strong> <strong>the</strong> rocksin combination with stratigraphic information willenable us to estimate <strong>the</strong> local heat flow value. Ifadvection is significant, in <strong>the</strong> system, <strong>the</strong>npermeabilities, porosity and fracturecharacterization are needed to quantify V andthus <strong>the</strong> contribution <strong>of</strong> <strong>the</strong> advective flow to <strong>the</strong>temperature distribution.In terms <strong>of</strong> fluid transport characterization, <strong>the</strong> keyparameters to identify are <strong>the</strong> permeabilities(absolute for water only and relative, when steamand liquid are both present in <strong>the</strong> reservoir),porosity and <strong>the</strong> thickness <strong>of</strong> <strong>the</strong> targetedreservoir. Initial and time lapse values from repeatlogging passes will be <strong>of</strong> interest to design andassess any well stimulation processes and toquantify <strong>the</strong> contribution <strong>of</strong> <strong>the</strong> local hydrogeologyto <strong>the</strong> temperature distribution.Figure 1. Isogeo<strong>the</strong>rms and formation temperature/ depthpr<strong>of</strong>ile in a hypo<strong>the</strong>tical rock sequence (adapted Jorden andCampbell, 1984).These parameter estimations are important at <strong>the</strong>exploration stage to evaluate <strong>the</strong> geo<strong>the</strong>rmalpotential and must be refined at <strong>the</strong> productionstage where <strong>the</strong> underground geo<strong>the</strong>rmal systemwill be significantly affected by <strong>the</strong> production andre-injection <strong>of</strong> a working fluid.Determining <strong>the</strong>rmal propertiesMost <strong>of</strong> <strong>the</strong> research on <strong>the</strong>rmal properties hasfocused on modeling <strong>of</strong> <strong>the</strong> <strong>the</strong>rmal propagation ingeological reservoirs. But <strong>the</strong> needs inpetrophysical data, particularly in geo<strong>the</strong>rmalreservoirs, have never been so important to verifyand validate models. Two main approaches areavailable to provide hard data on <strong>the</strong>rmalstructure and properties downhole logging andlaboratory measurements. Both methods have<strong>the</strong>ir advantages and disadvantages:• Logging data give access to a continuousrecords with depth but with high uncertaintiesbecause <strong>of</strong> some chemico-physical processesthat actively occurs during <strong>the</strong> data recording(heat flow, fluid flow, mudcakes, fracturations...)or simply because <strong>of</strong> <strong>the</strong> limited sensitivity anddepth resolution <strong>of</strong> <strong>the</strong> tools (Beck et al., 1971).Three general logging methods are available: (1)relaxation methods (Wilhelm, 1990), (2) direct<strong>the</strong>rmal measurements downhole with no controlat all on chemico-physical influences and (3) <strong>the</strong>classical correlation methods which combinelogging parameters such as sonic traveltime,hydrogen index, density, porosity, lithology andtemperature (Brigaud et al., 1989; Demongodin etal., 1991; Griffiths et al., 1992). All <strong>of</strong> <strong>the</strong>semethods use empirical models and some form <strong>of</strong>averaging or effective medium <strong>the</strong>ory to predict<strong>the</strong> <strong>the</strong>rmal properties. To calculate <strong>the</strong> <strong>the</strong>rmalconductivity and diffusivity accurately from suchmethods, <strong>the</strong> tools being employed must becapable <strong>of</strong> distinguishing <strong>the</strong> different mineralsand fluids sensitively.126


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>• Lab measurements enable control <strong>of</strong> all <strong>the</strong>parameters (mineralogy, porosity, water content,fractures) but <strong>the</strong> sampling (except for drillcuttings)is never continuous and <strong>the</strong> in-situreservoir conditions are difficult to reproduce in<strong>the</strong> lab. Moreover, lab equipment and protocolsare not infallible. Poor sample quality,representativeness, coupling, effects <strong>of</strong> fracturesetc., limit typical accuracy to around 5% or so. It israre that specific information is ga<strong>the</strong>red onanisotropy: this requires measurement <strong>of</strong> <strong>the</strong>tensor components <strong>of</strong> <strong>the</strong>rmal conductivity anddiffusivity. At <strong>the</strong> highest temperatures, non-linearproperties and especially <strong>the</strong>rmal expansion makegood measurements a challenge.One new technology that can help overcomesome <strong>of</strong> <strong>the</strong>se issues is Optical Thermal Scanning(Fig. 2). OTS is a non-destructive non-contactmeasurement <strong>of</strong> <strong>the</strong> <strong>the</strong>rmal conductivity and<strong>the</strong>rmal diffusivity on rocks and minerals at roomconditions (Popov et al., 1999). OTS is able toscan a sample surface with 3 temperaturesensors in combination with a focused mobile andcontinuously operated constant heat source. Theheat source and sensors move at <strong>the</strong> same speedrelative to <strong>the</strong> sample and are calibrated beforeand after each measurement with rock standards,which leads to high accuracy quoted as 1.5%, asampling size from 1 cm to 70 cm long having anyFig. 2. Optical Thermal Scanner instrument for rock <strong>the</strong>rmalproperty measurements on full cores (modified from Popov etal., <strong>2010</strong>). Optical Head: sensor (1) measure <strong>the</strong> rocktemperature at room condition and sensors (2 and 3)measure <strong>the</strong> rock temperature after heating from <strong>the</strong> heatsource (4).shape, short time measurements (10-30s),contactless tool and without time and cost <strong>of</strong>special sample preparation. Hence <strong>the</strong> OTC <strong>of</strong>fers<strong>the</strong> opportunity to investigate direct <strong>the</strong>rmalconductivity, diffusivity, pore space and geometryon full cores and anisotropic <strong>the</strong>rmal properties <strong>of</strong>samples under various conditions, and with awide range <strong>of</strong> form factor, size, and prevailingconditions (wet/dry, elevated temperature, etc).The combination <strong>of</strong> <strong>the</strong> two petrophysicalapproaches (lab and downhole) can be verypowerful and removes most <strong>of</strong> <strong>the</strong>ir respectivedisadvantages. Lab measurements allowparameter calibrations and better control on <strong>the</strong>logging interpretations. Proper integration <strong>of</strong>petrophysical data from lab and downholesources enables us to test, correct and enhance<strong>the</strong> existing <strong>the</strong>oretical models used to predictsteady state and dynamic <strong>the</strong>rmal behaviour.Petrophysical property modellingThe characterisation <strong>of</strong> geo<strong>the</strong>rmal reservoirs is atypical multi-scale problem. CSIRO andWACOGS have developed a number <strong>of</strong> workflowsto model and upscale rock physical propertiesappropriate for geo<strong>the</strong>rmal problems. An excitingrecent advance with wide uptake in <strong>the</strong> petroleumindustry is <strong>the</strong> incorporation <strong>of</strong> so-called DigitalRock or Digital Core methods whereby highresolution 3D images <strong>of</strong> real rocks form <strong>the</strong> basisfor physical property calculations. In <strong>the</strong> exampleworkflow presented here we analyse small scalerock properties in 3D based on micro-computedtomography (micro-CT), and scale up forhydraulic properties by using percolation <strong>the</strong>ory.Firstly, <strong>the</strong> original images <strong>of</strong> microtomographyare converted to binary images, and 3-D binarymodels are built up from <strong>the</strong> tomography slices.Image processing and segmentation is crucialwhich recognises target phases (pores, differentminerals) according to <strong>the</strong>ir greyscale values in<strong>the</strong> images. Fig. 3 shows <strong>the</strong> pore-structure <strong>of</strong> asyn<strong>the</strong>tic sandstone sample <strong>of</strong> size 1.3*1.3*1.17mm 3 after segmentation in which <strong>the</strong> poreinteriors are “painted” light blue. Micro-scalecharacterisations are analysed based on 3-Dbinary models, including volume fraction (porosityfor pores <strong>of</strong> porous media), percolation (orconnectivity), specific surface area (SSA),tortuosity, and anisotropy.Stochastic analyses <strong>of</strong> all phases are <strong>the</strong> secondstep <strong>of</strong> this multi-scale characterisation. Itconducts scale-dependent probabilities and <strong>the</strong>size <strong>of</strong> representative volume element (RVE). Ourstochastic analysis uses <strong>the</strong> moving windowmethod, in which a cubic sub-volume with variableside-length L moves all over <strong>the</strong> model. In thisway, <strong>the</strong> probabilities <strong>of</strong> volume fraction,percolation and anisotropy <strong>of</strong> different scales areobtained. The size <strong>of</strong> <strong>the</strong> RVE is determined when<strong>the</strong>se probabilities are convergent with <strong>the</strong>increasing sub-volume-size L (Liu et al. 2009).127


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Fig. 3. Pore-structure <strong>of</strong> a syn<strong>the</strong>tic sandstone sample, lightblue denotes inside <strong>of</strong> pores. Model size is 1000*1000*900voxels, resolution <strong>of</strong> voxels is 1.3 μm.Once at <strong>the</strong> RVE size or larger, <strong>the</strong> estimatedproperties are reliable for application to thatparticular rock type. Meanwhile, <strong>the</strong> probabilitydistribution functions can be used to create “digitalrocks” at any size which have certain commoncharacteristics, but vary in <strong>the</strong>ir details. Forexample, one may vary porosity, connectivity, orfracture density and see <strong>the</strong> effects.Physical properties <strong>of</strong> geo<strong>the</strong>rmal reservoirs, inparticular, permeability, elastic parameters, and<strong>the</strong>rmal expansion coefficient are calculated on<strong>the</strong> digital rock elements using numericalsimulations. Permeability can be simulated byusing <strong>the</strong> finite difference Stokes equation solverPermsolver and based on micro-scale porestructures. Fig. 4 is a RVE <strong>of</strong> size 1 mm 3 <strong>of</strong> asyn<strong>the</strong>tic sandstone sample. The simulatedpermeability is 1763 millidarcy. Thermomechanicalproperties are computed by using afinite element method based on <strong>the</strong> mineralproperties and structure. Fig. 5(a) is a RVE <strong>of</strong> adigital rock which includes two weak minerals <strong>of</strong>different shapes. Fig. 5(b) gives <strong>the</strong> relationships<strong>of</strong> stress and strain components <strong>of</strong> <strong>the</strong> RVE andmatrix, respectively. Although matrix and weakinclusive minerals are all isotropic, <strong>the</strong>microstructure makes <strong>the</strong> upscaled properties <strong>of</strong><strong>the</strong> RVE remarkably anisotropic, see Fig.5(b), inwhich red and black lines correspond to x and z-directions, respectively. As stress and strainvalues in Fig. 5(b) are volumetric means onelement sets, <strong>the</strong> relationships for <strong>the</strong> matrix showa slight anisotropy over all elements in <strong>the</strong> RVE(see blue and green lines in Fig.5b), which isreasonable. With <strong>the</strong>se simulated results, <strong>the</strong>rmomechanicalproperties <strong>of</strong> <strong>the</strong> representativevolume element can be computed.To extrapolate properties from microscale tomacroscale it is necessary to combine microscaleproperties with scaling laws. We usepercolation <strong>the</strong>ory to extract <strong>the</strong> main criticalparameters including fractal dimension, criticalFig.4 A RVE <strong>of</strong> a syn<strong>the</strong>tic sandstone sample forpermeability simulation.(a)(b)Fig.5 (a) RVE <strong>of</strong> a digital rock with two weak minerals <strong>of</strong>different shapes, matrix is not shown; (b) relationships <strong>of</strong>stress and strain in x and z-directions for matrix and RVE,respectively. Oriented microstructure makes <strong>the</strong> RVE beremarkably anisotropic, although minerals <strong>of</strong> matrix andinclusions are all isotropic.exponent <strong>of</strong> correlation length, percolationthreshold, and crossover length, for <strong>the</strong> purpose<strong>of</strong> upscaling.For <strong>the</strong> syn<strong>the</strong>tic sandstone sample shown in Fig.4, <strong>the</strong> critical exponent <strong>of</strong> correlation length and<strong>the</strong> fractal dimension extracted from microtomographyare close to <strong>the</strong> <strong>the</strong>oretical values.The percolation threshold <strong>of</strong> this structuredmedium is 3.94%, while <strong>the</strong> sample has a porosity<strong>of</strong> 24.4%, which is far above <strong>the</strong> percolationthreshold. In addition, <strong>the</strong> crossover length <strong>of</strong> <strong>the</strong>critical model is smaller than 50 μm. Based upon<strong>the</strong>se observations, we can directly use <strong>the</strong>transport properties obtained from <strong>the</strong> micro-scaleanalysis for upscale modelling in <strong>the</strong> macro-scale.128


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>The simulated permeability <strong>of</strong> 1763 md in 1 mmscale is close to <strong>the</strong> experimental testpermeability on a plug sample <strong>of</strong> 2567 md.Results show that <strong>the</strong> detection <strong>of</strong> <strong>the</strong> scaledependence <strong>of</strong> permeability is accurate from <strong>the</strong>crossover length <strong>of</strong> 50 micron to <strong>the</strong> cm laboratoryscale (Liu et al. <strong>2010</strong>).These upscaling methods based on statisticalphysics on small rock samples (potentially evencuttings) can be combined with more geologicallyinformed methods <strong>of</strong> geostatistics, based on coreandlog based lith<strong>of</strong>acies or flow units, to populatereservoir models at <strong>the</strong> larger scale.SummaryThe characterization <strong>of</strong> geo<strong>the</strong>rmal reservoirsrequires <strong>the</strong> integration <strong>of</strong> field, laboratory andcomputational petrophysical methods. Theformulation and parameterization <strong>of</strong> rock propertymodels is based on proper combination <strong>of</strong>remotely sensed (e.g. seismic) downhole andcore measurements. These methods combininginterpretation and modelling provide critical inputsto <strong>the</strong> understanding <strong>of</strong> <strong>the</strong> geo<strong>the</strong>rmal reservoir.From early exploration, hard petrophysical dataand good physical understanding will help toconstrain and develop regional and reservoirmodels <strong>of</strong> <strong>the</strong> geo<strong>the</strong>rmal resources not only toevaluate <strong>the</strong> resources but also to plan itsproduction. At <strong>the</strong> development stage, <strong>the</strong>se datacontribute to reduce <strong>the</strong> risk on <strong>the</strong> well design,well stimulation, hydraulic fracturing but also <strong>the</strong>field sustainability during production.CSIRO, with WAGCOE and o<strong>the</strong>r partners aroundAustralia, is investing in applied R&D and criticalinfrastructure to improve <strong>the</strong> application <strong>of</strong>petrophysics to <strong>the</strong> geo<strong>the</strong>rmal energy sector.Demonstration projects now underway in WA willprovide an excellent testbed for several <strong>of</strong> <strong>the</strong>methods described here.ReferencesBaker Hughes <strong>2010</strong>. Logging services web pagehttp://www.bakerhughes.com/products-andservices/drilling-and-evaluation/formationevaluation-/wirelineservices/petrophysics/nautilus-ultra-hphtBeck, A.E., Anglin, F.M. and Sass, J.H., 1971.Analysis <strong>of</strong> heat flow data-in situ <strong>the</strong>rmalconductivity measurments. Canadian J. Earth Sc.,8, 1-19.Brigaud, F., Vasseur, G. and Caillet, G., 1989.Use <strong>of</strong> well log data for predicting detailed in situ<strong>the</strong>rmal conductivity pr<strong>of</strong>iles at well sites andestimation <strong>of</strong> lateral changes in main sedimentaryunits at basin scale. Rock at great depth, Eds.Maury and Fourmaintraux, Rotterdam, A.A.Balkema. ISBN 90 6191 975 4, Vol.1, 403-409.Demongodin, L., Pinoteau, B., Vasseur, G. andGable, R., 1991. Thermal conductivity and welllogs: a case study in <strong>the</strong> Paris basin. Geophys. J.Int., 105, 675-691.Ellis, D.V. & Singer, J.M., 2007. Well Logging forEarth Scientists. Second Edition, Springer, 2007.Griffiths, C.M., Brereton, N.R., Beausillon, R. andCastillo, D., 1992. Thermal conductivity predictionfrom petrophysical data: a case study. GeologicalApplications <strong>of</strong> Wireline Logs II. GeologicalSociety Special Publication, 65, 299-315.Jorden, J.R. and Campbell, F.L., 1984. WellLogging I – Rock Properties, BoreholeEnvironment, Mud and Temeprature logging. SPE<strong>of</strong> AIME, N.Y., Dallas, 131-146.Liu J., Regenauer-Lieb K., Hines C., Liu K.,Gaede O., and Squelch A., 2009. Improvedestimates <strong>of</strong> percolation and anisotropicpermeability from 3-D X-ray microtomographicmodel using stochastic analyses andvisualization. Geochem., Geophys. Geosyst.,10,Q05010, doi: 10.1029/2008GC002358.Liu J. and Regenauer-Lieb K., <strong>2010</strong>. Application<strong>of</strong> percolation <strong>the</strong>ory to microtomography <strong>of</strong>structured media: percolation threshold, criticalexponents and upscaling, submitted to PhysicsReview E.Ocean Drilling Program Downhole Logging Guide.http://www.ldeo.columbia.edu/BRG/ODP/LOGGING/TOOLS/geochem.htmlPopov, Y., Pribnow, D.F.C., Sass, J.H., Williams,C.F. and Burkhardt, H., 1999. Characterization <strong>of</strong>rock <strong>the</strong>rmal conductivity by high-resolutionoptical scanning. Geo<strong>the</strong>rmics, 28, 253-276.Popov, Y., Miklashevskiy, D., Romushkevich, R.,Safonov, S. and Novikov, S., <strong>2010</strong>. Advancedtechnique for reservoir <strong>the</strong>rmal propertiesdetermination and pore space characterization.<strong>Proceedings</strong> World Geo<strong>the</strong>rmal Congress, Bali,Indonesia, 25-29 April <strong>2010</strong>.Schlumberger <strong>2010</strong>. Logging services web pagehttp://www.slb.com/en/services/additional/geo<strong>the</strong>rmal.aspxWilhelm, H., 1990. A new approach to <strong>the</strong>borehole temperature relaxation method,Geophysical Journal International, 103, 469-481.129


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>GEOTHERMAL POWER PLANT COMPETITIVENESS IN INDONESIA:ECONOMIC AND FISCAL POLICY ANALYSISFarizal 1,* and Prashanti Amelia Anisa 21, 2 Department <strong>of</strong> Industrial Engineering. The University <strong>of</strong> Indonesia. Depok, 16424, Indonesia* Corresponding author: farizal@ie.ui.ac.idThis paper assesses ge o<strong>the</strong>rmal p ower pla nt(GPP) co mpetitiveness through eval uating itsproduction costs a nd <strong>the</strong> appli cation <strong>of</strong>government incentive s, i.e. <strong>the</strong> Cle anDevelopment Mecha nism (CDM) and <strong>the</strong>implementation <strong>of</strong> ca rbon tax. Then <strong>the</strong> GPPcompetitiveness is compared to coal power plant.The results show that <strong>the</strong> effect <strong>of</strong> duty free, valueadded tax free (VA T), implem entation o finvestment tax credit, and pre survey governmentincentive ca n de crease <strong>the</strong> ge o<strong>the</strong>rmal sellin gprice by US 0,75 ¢/KWh, 0,91 ¢/KWh, 0,23 ¢/KWhand 0,6 9 ¢/K Wh, respe ctively. Implementation <strong>of</strong>CDM and carbon tax o n coal also improves GPPcompetitiveness. Geo<strong>the</strong> rmal can co mpete wit hcoal in <strong>the</strong> year 4.Keywords: geo<strong>the</strong> rmal electri city price, fiscalpolicy, carbon tax, competitivenessElectricity demand in Indonesia increases with <strong>the</strong>rate 5.9%. T his rate i s bi gger than th e ele ctricitysupply gro wth. This situation turn s o ut to be anelectricity cri sis. Sched uled bla ck out occurs inmany places including at <strong>the</strong> industrial areas.Depending on notorious fossil b ased fuels to fulfilelectric energy is not a sustaina ble policy due to<strong>the</strong> fuels are not re newable, means <strong>the</strong>ir depositis dimini shing by time, a nd <strong>the</strong>y a re also notenvironmentally friendly. The go vernmentproposed National <strong>Energy</strong> Mix 2025 to reduce <strong>the</strong>dependency on fossil fuel s and at <strong>the</strong> same timeto promote t he utilizatio n <strong>of</strong> rene wable energyincluding g eo<strong>the</strong>rmal (Fi gure 2 ). It is projecte dthat geo<strong>the</strong>rmal will contribute 5% to total ene rgysource at <strong>the</strong> time <strong>of</strong> 2025.IntroductionIndonesia i s ran ked th e fourth, after USA,Philippines, and Mexi co, among co untries thatutilizes geo<strong>the</strong>rmal energy to generat e electricityeventhough she has <strong>the</strong> large st p otency in <strong>the</strong>world, i.e. 27.169 MW or approximately 30 to 40%<strong>of</strong> worl d g eo<strong>the</strong>rmal p otency. The potencyspreads along <strong>the</strong> volcani c belt from th e island <strong>of</strong>Sumatra to Timor (Figure 1). Of 27,169 MW, only1052 M W or less than 5 % <strong>of</strong> <strong>the</strong> capacity havebeen u sed. One reaso n why geo<strong>the</strong> rmalutilization has not been used opt imally isIndonesia stil l dep ends heavily on fo ssil b asedfuels a s prim ary ene rgy reso urces for electri citygeneration and <strong>the</strong> competitiveness <strong>of</strong> geo<strong>the</strong>rmalplant.Figure 2. National <strong>Energy</strong> Mix 2025As addition to its sca rcity and environmenta limpact, ano<strong>the</strong>r issue is <strong>the</strong> price <strong>of</strong> fossil fuels isnot sta ble. T he p rice vol atility genera tes d oubtabout l ong term stability <strong>of</strong> <strong>the</strong> energy in <strong>the</strong>future. In contrast, geoth ermal energy is pollutionfree a nd environmental fri endly. Its fu el cost i srelatively stable during <strong>the</strong> whole period <strong>of</strong> a GPP.The i ssue related to its utilization i s explorationand drilling costs whi ch are quite high. Could <strong>the</strong>low and stable pri ce <strong>of</strong> GPP set <strong>of</strong>f its highexploration and dr illing costs? What is <strong>the</strong> impact<strong>of</strong> taxation schem es to GPP com petitiveness?How competitive is <strong>the</strong> GPP compare to coal firedpower plant? Those are some questions that willbe addressed here.Figure 1. Indonesia Geo<strong>the</strong>rmal PotencyResearch MethodologyThis study is based on <strong>the</strong> pr<strong>of</strong>itabilit y indicator<strong>the</strong>ory. Pr<strong>of</strong>itability indicators indicate <strong>the</strong> level <strong>of</strong>taking a n investment de cision fro m <strong>the</strong> investo rstandpoint. Investment de cision is a d ecision t oprocure fixed assets which include resources andfunds at <strong>the</strong> present time to obtain series <strong>of</strong> longtermp r<strong>of</strong>itability in <strong>the</strong> fu ture. Th ree i ndicators,130


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>net pre sent value, intern al rate <strong>of</strong> re turn, an dpayback period are used on this study.Net pre sent value (NPV ) <strong>of</strong> a proje ct is <strong>the</strong> totalcash flo w p er ea ch unit <strong>of</strong> time that has beencharged to <strong>the</strong> pre sent value <strong>of</strong> <strong>the</strong> investmentthat have b een cashed. NPV is calculated byadding up all <strong>the</strong> ca sh flows occur from period <strong>of</strong>zero, so-called as investment, to <strong>the</strong> last period <strong>of</strong><strong>the</strong> project.where:I: investmentr : rate <strong>of</strong> returnAn: cash flow / proceedn: economic value <strong>of</strong> investmentsVn :salvage value <strong>of</strong> i nvestments at t he e nd <strong>of</strong>economic periodIf NPV turns out to be positive, <strong>the</strong>n <strong>the</strong> project isfeasible to run. Po sitive NPV in dicates th einvestment has achieved favourable condition.Internal rate <strong>of</strong> return (IRR) is a percent increasein <strong>the</strong> value <strong>of</strong> money c ontained in <strong>the</strong> cu rrentcash flow. IRR ca n be in terpreted al so as <strong>the</strong>discount ra te that produ ces zero NPV .In gen eral, i nvestment d ecision ba sed on NPVand IRR will give a consistent result which mean ifan inve stment propo sal is considered fea siblebased on <strong>the</strong> NPV, <strong>the</strong> p roposal assessed basedon IRR is also feasible.Payback period (PBP) is <strong>the</strong> time needed to fullyrecover <strong>the</strong> costs and li abilities incurred in aproject.Where:PBP: Payback Period, yearsm: Year <strong>of</strong> <strong>the</strong> CCF negative after a positive CCFm+1: Year <strong>of</strong> <strong>the</strong> CCF p ositive after a neg ativeCCFCCF m : Cumulative Cash Flow in m (0)Although P BP doe s not refle ct pr<strong>of</strong>itabilityindicator <strong>of</strong> an invest ment pro posal and <strong>the</strong>calculation d oes not co nsider time value <strong>of</strong>money, but it is <strong>of</strong>ten used to compl ement <strong>the</strong>feasibility analysis <strong>of</strong> investment proposal s. PBPmay reflect <strong>the</strong> liquidity <strong>of</strong> an investment proposal.Pr<strong>of</strong>itability indicators al so consider investorrequired rate <strong>of</strong> return (RRR). RRR is influen cedby two main factors, ri sk free rate and ris kpremium project with rel ationship as RRR = riskfree rate + ri sk p remium project. RRR is definedby <strong>the</strong> investor. The hig her <strong>the</strong> ri sk <strong>of</strong> a proje ct,<strong>the</strong> higher <strong>the</strong> RRR is. Geo<strong>the</strong>rmal electric pricesare considered fea sible if <strong>the</strong>y can generate anIRR more than RRR . In this study, RRR is set as16%. In Indo nesia, gove rnment regulations li mit<strong>the</strong> sale p rice <strong>of</strong> geot hermal ele ctricity notexceeding US 9.7 ¢/KWh . Geo<strong>the</strong> rmal ele ctricityprice i s con sidered competitive if <strong>the</strong> price do esnot exceed 9.7 ¢/KWh.Input FactorsGovernment poli cy on tax and incentive sinfluence th e competiti veness <strong>of</strong> GPP. InIndonesia, g overnment p olicy on tax inclu desinvestment tax credit, duty-free im port, free valu eadded tax, a nd g overnment initial surv ey. Whileincentives include clean development mechanismand carbon tax.Investment tax creditBusiness tax rate for GPP is 30%. Investment taxcredit is assumed to reduce <strong>the</strong> basic tax rate to acertain extent, up to 5%, over six year period.Duty-Free ImportThrough import duty policy, <strong>the</strong> govern ment frees<strong>the</strong> import d uty that used to be 5 percent to 0percent.Free Value Added Tax (VAT)PMK 24/PMK.011/201 0 policy states thatgeo<strong>the</strong>rmal exploration activities are borne by <strong>the</strong>government. With his p olicy, <strong>the</strong> governm entbears <strong>the</strong> V AT payable on <strong>the</strong> impo rtation <strong>of</strong>goods that are used for geo<strong>the</strong>rmal e xplorationactivities.Government Initial surveyPreliminary survey con ducted by <strong>the</strong> governme ntin <strong>the</strong> ea rly stages <strong>of</strong> G PP develop ment is aneffective way to red uce <strong>the</strong> ri sk <strong>of</strong> d evelopinggeo<strong>the</strong>rmal resource s. The su rvey include ssurface surv eys and drilli ng <strong>of</strong> two test wells. Allsurvey results are t ransferred to privatedevelopers at no cost.Implementation <strong>of</strong> Clean DevelopmentMechanismClean development mechanism (CDM) scheme isa scheme in which developed countries are ableto use <strong>the</strong> amou nt <strong>of</strong> ca rbon di oxide (CO 2 )reduction as a result <strong>of</strong> joint proje ct betwee ndeveloped a nd devel oping count ries. Certifie d131


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Emission Redu ction Credit (CER) is issu eddepending on <strong>the</strong> amo unt <strong>of</strong> green house g asesreduction. CER credit can be traded on marketthus can be used to improve <strong>the</strong> pr<strong>of</strong>itability <strong>of</strong> <strong>the</strong>project. CER value is assumed to be US$ 10 perton CO 2 and <strong>the</strong> emission factor is 0.819 ton CO 2per MWh.Application <strong>of</strong> Carbon TaxCarbon tax a pplied to fossil fuel plants will makesome changes in <strong>the</strong> structure <strong>of</strong> en ergy p ricesthus will ma ke geo<strong>the</strong>rmal more attra ctive (Table1).Assumptions on GPP project used in this study:• Type <strong>of</strong> project: Th e total proje ct (proj ectdownstream + upstream)• Scale <strong>of</strong> project: 110 MW which consisted <strong>of</strong> twounits <strong>of</strong> 55 MW• Period <strong>of</strong> contract: 35 years (5 yea rs for pr eproduction and <strong>the</strong> rest for production)• Capacity Factor: 90%• Success Ratio:• exploration wells: 50%, production wells: 80%• Decline Rate 3% per year• Steam Production• exploration wells: 8 MW, production wells: 12MW• Income Tax Rate: 30%• D epreciation Me thod: Declining Ba lance w ith 8years• Investment Tax Credit 5% per year for 6 Years• Free Value Added Tax: 10%• Duty-Free ImportSummary <strong>of</strong> GPP costs is shown in Figure 3:Figure 3. Geo<strong>the</strong>rmal Power Plant costsThe number <strong>of</strong> wells drilled in <strong>the</strong> pre productio nis 20 wells. Among <strong>the</strong>m nine make up wells for a30-year production periods (year <strong>of</strong> p roduction 2,5, 9.12, 15, 18, 21, 24, 27).Result and DiscussionThe calculation result for 110 MW GPP found thatusing <strong>the</strong> p rice <strong>of</strong> US 9.7 0 ¢/KWh, <strong>the</strong> I RR, NPV,and PBP are 15.16%, US$ 17,570, and 10 years,respectively. The IRR is slightly less thandeveloper’s RRR, which is 16%. Meanwhile, whenusing developer’s RRR <strong>the</strong> electricity price will bea bit highe r than 9.70 ¢/KWh, i.e. 10.0 7 ¢/ KWh.<strong>the</strong> NPV is US$ 30,578 and nine years PBP.A 10% reduction on capacity factor and electricityprice ca uses a decrea se in IRR <strong>of</strong> 1.6 8%, whileon <strong>the</strong> o<strong>the</strong>r side a 10% addition <strong>of</strong> capacity factorand <strong>the</strong> price <strong>of</strong> ele ctricity increa ses 1.22% <strong>of</strong>IRR. Reduction <strong>of</strong> investment costs by 10% leadsto an increase <strong>of</strong> IRR by 1.51%, while <strong>the</strong> additioncost <strong>of</strong> inve stment with <strong>the</strong> same amount causesa decrease in 1.28% IRR (Figure 4)132


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Figure 4. Capacity Factor, Investment Costs and Price <strong>of</strong>Electricity; Sensitivity Analysis on IRRToward <strong>the</strong> NPV, a 1 0% red uction <strong>of</strong> ca pacityfactor and electri city price ca uses <strong>the</strong> NPVdecreases o f $27.83, while <strong>the</strong> 10 % additioncauses a n increase <strong>of</strong> $19.32. Reduction <strong>of</strong>investment costs by 10% lead s to an increa seNPV <strong>of</strong> $ 1 9.63, whil e <strong>the</strong> ad dition decreasesNPV <strong>of</strong> $ 19.59 (Figure 5).Figure 7. IRR Pr<strong>of</strong>ile at Different Capacity FactorAt government electricity price <strong>of</strong> US 9.70 ¢/KWh,<strong>the</strong> IRR may be more than 16% if <strong>the</strong> in vestmentcost ca n be pre ssed n ot less than 1 0%. If <strong>the</strong>investment cost red uces by 10%, <strong>the</strong> IRR wo uldincrease by 1.18%, 1.51 % and 1.76 % on <strong>the</strong>geo<strong>the</strong>rmal electricity prices <strong>of</strong> US 7 ¢/KWh, 9.70¢/KWh and 12 ¢/KWh, resp ectively. On <strong>the</strong>contrary, If t he inve stment co sts in creases by10%, <strong>the</strong> IRR will drop by 1%, 1.28% and 1.51%on <strong>the</strong> geo<strong>the</strong>rmal prices <strong>of</strong> 7 ¢/KWh, 9.70 ¢/KWhand 12 ¢/KWh, re spectively. If <strong>the</strong> investmentcosts d ecreases by 1 0%, <strong>the</strong>n <strong>the</strong> feasi blegeo<strong>the</strong>rmal electricity price at 16% IRR will not beless than $ 9.5 ¢/KWh (Figure 8).Figure 5. Capacity Factor, Investment Cost and Price <strong>of</strong>Electricity; Sensitivity Analysis on NPVFor <strong>the</strong> PBP, a 10% reduc tion in capacity fac torand electricity price causes a sl ower PBP withone yea r, while <strong>the</strong> 10 % addition causes <strong>the</strong>payback pe riod a year earlier. Reduction <strong>of</strong>investment cos ts by 10% c auses PBP a yearearlier, while <strong>the</strong> addition causes a slower PBP byone year (Figure 6).Figure 8. Pr<strong>of</strong>ile <strong>of</strong> IRR at Different Investment CostsThe m ost i nfluential in centive im proving th eproject I RR is <strong>the</strong> 10% VAT-Free incentivefollowed b y import duty-free ince ntive,government prelimi nary survey, and investmenttax credit (Figure 9).Figure 6. Capacity Factor, Investment Cost and Price <strong>of</strong>Electricity; Sensitivity Analysis on PBPWith <strong>the</strong> governments’ geo<strong>the</strong>rmal electricity price<strong>of</strong> US 9.70 ¢ /KWh, with a capacity factor <strong>of</strong> 90%(base case, CF 90%), th e IRR will be less than16%. If <strong>the</strong> capa city factor redu ces to 80%, withgeo<strong>the</strong>rmal electricity prices <strong>of</strong> US 7 ¢/KWh, 9.70¢/KWh and 12 ¢/KWh, <strong>the</strong> IRR will fall by 1.55%,1.87% and 2. 13%, respectively. In <strong>the</strong> base case(CF 90% ) with IRR 16%, geoth ermal electricityprice is fe asible if it is ab ove 10.2 ¢/K Wh (Figure7).Figure 9. Analysis <strong>of</strong> <strong>the</strong> effect <strong>of</strong> Government Incentiveson IRR and Electricity Prices133


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>The effect <strong>of</strong> free d uty, free VAT, <strong>the</strong>implementation <strong>of</strong> invest ment tax credit, and <strong>the</strong>preliminary survey i ncentive re duces th egeo<strong>the</strong>rmal electricity price by $ 0.75 ¢/KWh, 0.91¢/KWh, $ 0 .23 ¢/KWh and $ 0.69 ¢/KWh,respectively (Table 2).In scena rio 1, at <strong>the</strong> el ectricity pri ce <strong>of</strong> 9.7 0¢/KWh, <strong>the</strong> I RR only reaches 14.6 6%. Electricityprices that fe asible at IRR 16% i s 10.5 4 ¢/KWh(Figure 11).Table 2. Effect <strong>of</strong> Government Incentives on Electricity PricesIncentivesElectricity Price At IRR=16%No Incentives 12Investment Tax Credit 11.77Initial Survey by <strong>the</strong> Government 11.25Free Duty 11.31Free VAT 11.09The effect <strong>of</strong> <strong>the</strong> impleme ntation <strong>of</strong> CDM redu ces<strong>the</strong> electricity price by 0.82 ¢/KWh and increases<strong>the</strong> IRR to 16.53% whi ch is a bit above <strong>the</strong>desired RRR (Figure 10).Figure 11. Analysis <strong>of</strong> <strong>the</strong> effect <strong>of</strong> Scenario 1 on IRR andPriceResults <strong>of</strong> scen arios 1 t o 6 are sum marized atTable 4 bellow:Figure 10. Analysis <strong>of</strong> <strong>the</strong> effect <strong>of</strong> CDM on IRR andElectricity PriceTable 3 b elow lists 6 sce narios <strong>of</strong> imp lementingcombination <strong>of</strong> government tax and incentives.Scenario123456Table 3. List <strong>of</strong> ScenariosFiscal PolicyDuty FreeVAT FreeITC 5% for 3 yearsNo Survey IncentivesNo CDM SchemeDuty FreeVAT FreeITC 5% for 8 yearsNo Survey IncentivesNo CDM SchemeDuty FreeVAT FreeITC 5% for 5 yearsSurvey IncentivesNo CDM SchemeDuty FreeVAT FreeITC 5% for 5 yearsNo Survey IncentivesCDM SchemeDuty FreeVAT FreeITC 5% for 5 yearsSurvey IncentivesCDM SchemeDuty 5%VAT 10%No ITC 5% for 5 yearsNo Survey IncentivesNo CDM SchemeTable 4. IRR and Geo<strong>the</strong>rmal Electricity PriceIRR (%)Scenariowhen electricityprice is set as 9.70cents/KWhElectricity Price(cents/KWh)when IRR is set by16%1 14.66 10.542 15.29 10.233 16.02 9.64 16.53 9.265 18.72 8.686 14.53 10.5According to National <strong>Energy</strong> Mix 202 5, coal willstill play as primary energy source, but it role willbe re duced. As su bstitution, geoth ermal willcontribute 5% <strong>of</strong> total energy sou rce (Figure 2). Itis im perative to check GPP competitivenesstoward coal power plantThe a ssumptions used i n cal culating t he cost <strong>of</strong>coal fired power plant are as follow:• Capacity: 300 MW• Capital Cost: US$ 2,500/MW• O & M Cost: US$ 88/KW• Operation time: 7000 hours a year• Carbon Tax: Rp 60/KWh• Fuel Consumption: 0.439 Kg/KWhThe fact that geo<strong>the</strong>rm al fuel cost is quite stabl eduring <strong>the</strong> lif e time <strong>of</strong> GP P, while on t he contrarycoal fuel cost is in creasing by time. Using US $24.76/MWh for geoth ermal energy cost for 3 0years, g eo<strong>the</strong>rmal cost will be less than co al inyear 1 4. At <strong>the</strong> time coal fuel cost i s US$ 2 4.78(Figure 12).134


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>promote GP P. Without i mplementation <strong>of</strong> ca rbontax, <strong>the</strong> cost <strong>of</strong> geo<strong>the</strong>rmal electricity can competewith coal in t he year 14. The impl ementation <strong>of</strong>carbon tax to coal plant improve s <strong>the</strong>competitiveness <strong>of</strong> G PP. Geo<strong>the</strong>rmal cancompete with coal in <strong>the</strong> year 4.Figure 12. Levelized Cost Comparison BetweenGeo<strong>the</strong>rmal and CoalMeanwhile, when applying carbon tax, geo<strong>the</strong>rmalwill outperform even earlier, i.e. in fourth year,where <strong>the</strong> co st <strong>of</strong> coal is $ 24.88. Application <strong>of</strong>carbon tax adds to <strong>the</strong> cost <strong>of</strong> coal Power Plant to$ 1.26/MWh (Figure 13).Figure 13. Levelized Cost Comparison BetweenGeo<strong>the</strong>rmal and Coal with Carbon TaxConclusionThe current policy, refe rs to PM KNo. 21/PMK.011/<strong>2010</strong> with <strong>the</strong> highestgeo<strong>the</strong>rmal price US 9.70 cent/KWh, is not able toprovide <strong>the</strong> investor desired IRR, i.e.16%. To fulfil<strong>the</strong> investo r IRR with <strong>the</strong> government elect ricityprice, <strong>the</strong> investment costs must be reduced to atleast 10% or increase <strong>the</strong> capacity factor by 10%.Free VAT a pparently ha s <strong>the</strong> mo st significantinfluence on <strong>the</strong> I RR and th e g eo<strong>the</strong>rmalelectricity price followed by free import duty, initialsurvey by go vernment in centive, and i nvestmenttax credit. The effect <strong>of</strong> th ose poli cies can lo wer<strong>the</strong> selling price by US 0.91 cent/KWh, 0.75 cent/KWh, 0.69 cent/KWh, and 0.23 cent/KWh,respectively. The effect a nd <strong>the</strong> impl ementation<strong>of</strong> CDM reduces <strong>the</strong> pri ce by US 0.82 cent/KWhand increases <strong>the</strong> IRR to 16.53%.From th e six scena rios studied, o nly scen ario 3(combination <strong>of</strong> Duty-Free, Free <strong>of</strong> VAT, <strong>the</strong> ITCis 5%, a nd government pre su rvey), scena rio 4(Duty-Free, Free <strong>of</strong> VAT, <strong>the</strong> ITC is 5%,application <strong>of</strong> <strong>the</strong> CDM ) a nd scenario 5 that ca nenhance GPP competitivene ss . Amo ng <strong>the</strong>sethree sce narios, scen ario 5 (Duty Fre e, free <strong>of</strong>VAT, ITC i s 5%, gove rnment survey and <strong>the</strong>application <strong>of</strong> <strong>the</strong> CDM) i s <strong>the</strong> be st scenario toReferencesAkmal, F, H. Darn ell, and P. Sugiharto (2000 ).The geo<strong>the</strong> rmal power busi ness in Java Bali:trading m echanism, com petitiveness with fossilfuel and challenges to Its dev elopment.<strong>Proceedings</strong> World Geo<strong>the</strong>rmal Congress pp 777-783. Kyush u-Tohoku, Jap an, May 28 – Jun e 10,2000.Ministry <strong>of</strong> Ener gy and M ineral Resour ces(2006). Blu eprint Natio nal Ener gy P olicy 200 6-2025, Th e Rep ublic <strong>of</strong> I ndonesia. J akarta,IndonesiaCanada, J.R., W.G. Su llivan, and J.A. White(1996). Capital Invest ment Anal ysis fo rEngineering and M anagement, 2 nd ed ., PrenticeHall, Inc. Upper Saddle River.Danar, A.S. (201 0). Geo<strong>the</strong>rmal ele ctricity pri cedetermination based on investme nt deci sion.World Geot hermal Co ngress. Nu sa Dua,Indonesia (in Indonesia language)Dardak, E (20 07). Inco rporating en ergycommodity price vol atility in economi c cost <strong>of</strong>supply analysis for elect ricity expansion plan. The10 th International Confe rence on QIR (Quality inResearch). Jaka rta, Indonesia, 4 – 6 De cember2007.Darnell, H. and A.R.T. Artono (200 1). An analysison <strong>the</strong> g eo<strong>the</strong>rmal electricity competitiveness. <strong>the</strong>Annual S cientific Confe rence <strong>of</strong> In donesianGeo<strong>the</strong>rmal Association. Jogya karta, Indonesia,February 2001.135


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>A METHOD FOR CALIBRATING AUSTRALIAN TEMPERATURE-DEPTHMODELSDesmond Fitzgerald 1* and Raymond Seikel 11 Intrepid Geophysics Unit 2, 1 Male Street, Brighton Victoria, Australia 3186.*Corresponding author: des@intrepid-geophysics.comThe Au stralian ge o<strong>the</strong>rmal indu stry i s movin grapidly, an d i n that pr ocess requi res a lot fromgeophysics t o aid in ch aracterising regio nalprospectivity for exploitable heat resources.Various grou ps are usi ng hybrid me thods toestimate ‘Curie point’ te mperatures at depth, o ralternatively, <strong>the</strong> temperature at 5 kilometresbelow <strong>the</strong> surface. D eep drilling observationsand airborne magnetic compilations are <strong>the</strong> ke ycomponents, toge<strong>the</strong>r with a basem ent geologyinterpretation. Several ge nerations <strong>of</strong> this workare already published with more to come.A method to test <strong>the</strong> se maps an d al so helpcharacterise uncertainty is proposed based upona deep 3D continental model scale, extending to<strong>the</strong> lithosph ere. Variable surfa ce tem peratureand heat flow grids, based upon remote sensingare u sed, to ge<strong>the</strong>r with a simple lith osphereboundary condition. Th e heat diffu sion is th enemployed to test <strong>the</strong> temperature -depth map s.Progress on applying this method to Au stralia isreported.Key words: Sensin g Heat Flow Anoma lies, EMspectrum, Hi gh <strong>Energy</strong> photon s, Co ntinentalscale 3d Geology modelsIntroductionNot enough attention is paid to <strong>the</strong> influ ences <strong>of</strong>heat, both on-going and its history, in <strong>the</strong> field <strong>of</strong>exploration g eoscience. Scant rega rd i s paid toheat alterati on mineral prod ucts, unl ess it isobviously a primary indicator <strong>of</strong> an economicallyviable re source. A more holistic a pproach tocreating 3 D earth m odels that em brace al laspects <strong>of</strong> heat an d its i nfluence on rocks i srequired. Th e ch allenge (Stein) i s th e classicalone <strong>of</strong> usi ng <strong>the</strong> mea sured tem perature a ndtemperature gradient at an obje ct’s su rface toinfer <strong>the</strong> te mperature field at d epth, T(x,t), afunction <strong>of</strong> position x and time t. Near <strong>the</strong> earth’ssurface, th e t emperature g radient is e ssentiallyvertical, so t he out ward heat flow q s is <strong>the</strong>product <strong>of</strong> <strong>the</strong> vertical gradient <strong>of</strong> th etemperature T(z), whi ch is most eve rywherepositive downwards (temperature increases withdepth z), and <strong>the</strong> me asured o r estimate d<strong>the</strong>rmal conductivity <strong>of</strong> <strong>the</strong> material, k.<strong>Australian</strong> developmentsThe syste matic gath ering <strong>of</strong> boreh oleobservations <strong>of</strong> downhol e temperatu res, ro ckheat cond uctivities and tempe rature gradientswith depth below su rface were <strong>the</strong> basis <strong>of</strong>producing th e first g enerations <strong>of</strong> p redictedtemperatures 5km below <strong>the</strong> su rface for <strong>the</strong><strong>Australian</strong> continent (Chopra & Holgate, 2005).,see figure 1.Figure 1: Map <strong>of</strong> estimated crustal temperatures at a depth<strong>of</strong> five kilometres.Maus, 1997 develo ped <strong>the</strong> id ea thatcompilations <strong>of</strong> <strong>the</strong> ma gnetic anomaly mapcould form <strong>the</strong> basis for estimating <strong>the</strong> depth to<strong>the</strong> Curie point. This requires a technique to find<strong>the</strong> bottom s <strong>of</strong> ca usative bodi es. A movingwindow method using a modified Spector-Granttype algorith m was initia lly propo sed for thistask.In re cent ti mes, Geoscience Au stralia ha sproduced <strong>the</strong> 5th gene ration mag netic anomalygrid an d with this edition <strong>the</strong>re i s much greaterconfidence that <strong>the</strong> longe r wavelengthanomalies (g reater than 50 km ) are faithfullyreproduced. Thi s follo ws from <strong>the</strong> AWAGSsurvey, fund ed by <strong>the</strong> "Securi ng Australi a's<strong>Energy</strong>" initiative. Also , more <strong>the</strong>oretical workhas been done on automatic depth to basementtechniques, such that <strong>the</strong> ability to separatetop/bottom and centres <strong>of</strong> causative bodies. (seeStavrev and Reid 2007).Several groups have forme d to ta ckle thi sproblem and <strong>the</strong> recently reported progress from<strong>the</strong> USGS team (Bouli gand et al 2009) isencouraging. In this work, a v ariety <strong>of</strong>approaches were applied to th eCalifornia/Utah/Nevada re gion whe re o ver 25 %<strong>of</strong> all g eo<strong>the</strong>rmal po wer station capacity for <strong>the</strong>136


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>world i s lo cated. The se heat sources a relabelled "conventional" as <strong>the</strong>y follow f rom nearsurface v olcanic sources as sociated with t heRocky Mountains and Yellowstone.In Australia, a signifi cant initiative is beingmounted a round <strong>the</strong> so -called South Australi aHeat Flow anomaly. This was first recognized bySandiford 19 98, as th e burial <strong>of</strong> a basementsequence en riched i n h eat pro ducing e lementsduring <strong>the</strong>rmal subsidence following rif ting. Thismajor rift in <strong>the</strong> Aust ralian continent fromAdelaide north to <strong>the</strong> Coope r Ba sin, has amassive granitic intrusion which is Uranium rich.Naturally o ccurring lo w grade th ermo-nuclearheating <strong>of</strong> th is gra nite pe aks at aro und 4 kmdeep. This type <strong>of</strong> play i s termed an EnhancedGeo<strong>the</strong>rmal System.GeochemistryIt is mai nly t he oil ind ustry that h as come torealise ju st how im portant <strong>the</strong> heat history <strong>of</strong>rocks and sedimenta ry packa ges is, in <strong>the</strong>prospectively <strong>of</strong> basins for oil or gas finds.Observationally, <strong>the</strong> key technique i s defining<strong>the</strong> mine ral alteration produ cts and f romexperiment, just wh at must have bee n <strong>the</strong> heathistory to have left t his l egacy. Diam ondexploration has also traditionally lo oked fo rindicator minerals that im ply <strong>the</strong> ne cessary heathistory.Structural geologyMost stru ctural geology phen omena have anunderlying genesis where he at ha s played amajor role.1. A deep pipe from <strong>the</strong> ma ntle to <strong>the</strong> surfac ecan form as nature “vents" heat in explosiveevents. Kimb erlite pi pes retain a re cord o fheat altered minerals that can b e interpretedfor temperatures during formation.2. Granite intrusions in general.3. All tectonic a nd plate scal e movement s ar ethought to be manifestation s <strong>of</strong> hea tcirculation effects in <strong>the</strong> mantle.4. Volcanic a ctivity is most ly asso ciated wit hcrustal faulti ng, <strong>of</strong>ten on a plate b oundary.Basalt flows and flood pl ains, and sills areremnants <strong>of</strong> this activity.5. Rifting or failed rifts.Observational geophysicsAll <strong>the</strong> m easurable ge ophysical phenomenasuch as gravity, magnetics, deep crustal seismicand radiometrics can i ndirectly be u sed to hel pinterpret stru ctural geology and defi ne heatprovince boundaries.Missing f rom <strong>the</strong>se lowe r cost, bul kobservational methods, is a viable methodologyto ei<strong>the</strong>r dire ctly or i ndirectly obse rve heat ortemperature. Thi s would lead to near surfacetemperature and/or heat flow maps th atsignificantly improve upon Figure 1. So what i s<strong>the</strong> physics and why do we stru ggle with thischallenge?Electro-magnetic spectrumThermal radi ation is emitted by all su bstancesabove a bsolute ze ro and inclu des visible an dinfrared radiation and some ultra-violet radiation.Thermal radi ation o ccurs in soli ds, liqu ids, an dgases, at <strong>the</strong> speed o f light and ha s noattenuation in a va cuum. Thermal radiation canoccur between two bodies with a colder mediumin bet ween. Actually, <strong>the</strong> ele ctromagneticspectrum can be expressed in te rms <strong>of</strong> energy,wavelength, or freq uency. Each way <strong>of</strong> thinki ngabout <strong>the</strong> EM spectrum is related to <strong>the</strong> o<strong>the</strong>rs ina precise ma<strong>the</strong>matical way.Wavelength(m)Frequency(Hz)<strong>Energy</strong> (J)Radio > 1 x 10 -1 < 3 x 10 9 < 2 x 10 -24Microwave 1 x 10 -3 - 1 x 10 -1 3 x 10 9 - 3 x10 11 2 x 10-24 - 2 x 10 -22InfraredOptical7 x 10 -7 - 1 x 10 -3 3 x 1 011 - 4 x 2 x 10 -22 - 3 x 10 -10 14 194 x 10 -7 - 7 x 10 -7 4 x 10 14 - 7. 5 x 3 x 10 -19 - 5 x 10 -10 14 19UV 1 x 10 -8 - 4 x 10 -7 7.5x10 14 -3x10 16 5 x 10 -19 - 2 x 10 -17X-ray1 x 10 -11 - 1 x 10 -83 x 1016 -3 x 2 x 10 -17 - 2 x 10 -10 19 14Gamma-ray < 1 x 10 -11 > 3 x 10 19 > 2 x 10 -14Table 1 : shows <strong>the</strong>se relationships..So why do we have three ways <strong>of</strong> describingthings, each with a diff erent set <strong>of</strong> physi calunits? After a ll, frequency is measured in cyclesper second, wavelength is measured in meters,and energy is measured in electron volts and i sinversely proportional to <strong>the</strong> wavelength.By conventi on, ga mma-rays are reported i nelectron volts, with <strong>the</strong> hig hest en ergy going to<strong>the</strong> right hand side. Figure 2 below has <strong>the</strong> orderreversed, an d sh ows th e EM s pectrumwavelengths increasing t o <strong>the</strong> rig ht, in what i s<strong>the</strong> conve ntional man ner for visible light, heatetc.137


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>This tra ditional view also i s some whatmisleading with <strong>the</strong> lab el "<strong>the</strong>rmal radiation".This type <strong>of</strong> heat i s a rguably <strong>the</strong> l east wellunderstood. While at th e sam e time, mostpeople are very familiar with <strong>the</strong> wea <strong>the</strong>r an dsensing radi ant heat. The body is rece ptive,largely due to <strong>the</strong> i nteraction <strong>of</strong> parts <strong>of</strong> <strong>the</strong> EMspectrum with water and to a lesser extent, o<strong>the</strong>rorganic molecules. With this in mind, it is normalto associate heat with infra-red ba nd, terra-hertzband a nd th e ultra-viol et band s (sun -burn). Wehave evolve d to se nse visible lig ht whichradiates from <strong>the</strong> sun due to <strong>the</strong>rmal black bodyradiation at 5800K. What this is really showing is<strong>the</strong> range <strong>of</strong> Plank's law (see Figure 3) and howparts <strong>of</strong> <strong>the</strong> spe ctrum relate to "blac k body"radiation fro m <strong>the</strong> Eart h. As can be se en,microwaves are not con sidered to be <strong>the</strong>rmalradiation, yet clea rly that have a ve ry effectivecapacity to "heat". At <strong>the</strong> hi gh end <strong>of</strong> <strong>the</strong> energyscale, gamma rays are part <strong>of</strong> <strong>the</strong> mix in nucl earpower plants that, <strong>of</strong> course, gene rate heat priorto conversion to electricity.From a g eophysical poi nt <strong>of</strong> view, any EMemission fro m <strong>the</strong> Ea rth could b e h arnessed t oextract heat. The ch allenge <strong>of</strong> how to do this i slargely an engineering problem.Figure 3 Plank's law and Black Body radiation. At normalsurface temperatures <strong>of</strong> <strong>the</strong> Earth, <strong>the</strong> range <strong>of</strong>wavelengths still emitting radiation is large, while <strong>the</strong>overall energy (<strong>the</strong> area under <strong>the</strong> curve), falls <strong>of</strong>fdramatically.There are two types <strong>of</strong> radiation categories Volumetric p henomenon – ra diation e mittedor a bsorbed throu ghout gases, tran sparentsolids, some fluids Surface ph enomenon – radiatio n t o/fromsolid or liquid surface.Initially, heat is emitted fro m <strong>the</strong> surface <strong>of</strong> th eearth and <strong>the</strong>n it is "attenuated" and absorbed in<strong>the</strong> atmosphere.The ma gnitude <strong>of</strong> <strong>the</strong> radiation va ries withwavelength – it’s spectral. The wavelength <strong>of</strong> <strong>the</strong>radiation is a major factor in what its effects wil lbe. This is illustrated in Figure 4.Figure 2. Radiation Spectrum, showing wavelengths. Note,it is not usual to think <strong>of</strong> <strong>the</strong>rmal radiation extending into <strong>the</strong>higher energy parts <strong>of</strong> <strong>the</strong> spectrum e.g. X Rays.Radiation is made up o f a continuo us, non -uniform distribution <strong>of</strong> m onochromatic (sin glewavelength)components.The m agnitude a nd spectral di stribution (how<strong>the</strong> radiation varies with wavelength) varies withtemperature and type <strong>of</strong> emitting surf ace. Weare inte rested in <strong>the</strong> continental crust an dregional va riations due to <strong>the</strong> a ge an dcomposition <strong>of</strong> <strong>the</strong> rocks.138


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Attenuation <strong>of</strong> signalFigure 4. Shows varying emissivity with wavelengthsRadioactive (crustal) heat productionThe contine ntal crust cont ains a relatively highdensity <strong>of</strong> radioactive isotopes, primarily those <strong>of</strong>uranium, thorium, and potassium.Hence, within a region <strong>the</strong> heat flow depends on(1) radioactivity in <strong>the</strong> crust,(2) tectonic setting, and(3) heat flux from <strong>the</strong> mantle below.For a given area, te rmed a heat -flow province,<strong>the</strong> me asured he at flow " q" varie s li nearly with<strong>the</strong> near surface radioactive heat production.The tech nology to obse rve ra diometricsemissions f rom <strong>the</strong> ea rth o r g amma-rays h astraditionally a lways ig nored <strong>the</strong> "low channels",due to hi gh cou nts a nd diurn al effe cts, <strong>of</strong>tenlabelled "skyshine". Very fe w observations using<strong>the</strong>se instruments have ever been done at night,when <strong>the</strong>se diurnal effect s are mini mised. With<strong>the</strong> ne wer hardware now availa ble and th esensitivities and counting capacities increased, a66 litre system, de signed for 1 024 channelsand/or a Ge Li purpo se b uilt system, would beable to ob serve a con siderable po rtion <strong>of</strong> <strong>the</strong>"<strong>the</strong>rmal radiation" tail. The first channel <strong>of</strong> aradiometrics instrument cove rs mo st <strong>of</strong> th econventional EM sp ectrum, cove ring f rom 0 to12 keV. Figure 5 recasts <strong>the</strong> EM spectra into <strong>the</strong>form favoured for measuring gamma rays.Counts/sec/chan8060402000 1 2<strong>Energy</strong> (MeV)Figure 5 Typical Gamma Ray spectrum view, observedremotely within 100 m. <strong>of</strong> ground.3Radiant ene rgy from <strong>the</strong> earth i s readilyabsorbed a nd attenuat ed in <strong>the</strong> lowe ratmosphere. At lower energies, <strong>the</strong> photoelectriceffect is mo stly responsible for this. Radiometricairborne surveys are conducted at flying heights<strong>of</strong> aroun d 100m, to ensure emissi onscharacteristic <strong>of</strong> particul ar mine rals can beobserved bef ore thi s attenuation sm ooths th echaracteristic spe ctral p eaks. Thi s requiredobservation distan ce reduces as <strong>the</strong> energy <strong>of</strong><strong>the</strong> photons reduces, if in dividual characteristicsare to b e se en. If one re-examines <strong>the</strong>generalized " Black Body" diffuse curve at 3 00degrees Kelv in, it is ve ry smooth an d covers abroad ra nge <strong>of</strong> energie s, with no p ossibility <strong>of</strong>peaks from good emitting minerals.This appears to be an a rea that req uires ei<strong>the</strong>rmore research, or pr actical ob servations indiffering te rrains and na tural lig ht condition s.Towards th e cla ssic heat po rtion <strong>of</strong> <strong>the</strong>spectrum, bo lometers exis t th at h ave b eendeployed at large di stances, to ob serve thatportion <strong>of</strong> th e sp ectrum. (TIMS, ASTER et c.)The rea son <strong>the</strong>se sho w any signal, is tha twavelengths are chosen that minimi zeabsorption with water vapour.Modelling construtsThe o ceanic lithosphere is relatively un iform i ncomposition, and little heat is gene rated within itby radioactivity, oceanic heat flow i s essentiallya si mple functio n <strong>of</strong> age. In contrast, acontinental cru st is hetero geneous incomposition, due to its much lo nger tectoni chistory. M oreover, th e heat flo w dep endscritically on radioa ctive heat prod uction in <strong>the</strong>crust. The two prim ary effects are thus thatcontinental heat flow i s prop ortional to <strong>the</strong>surface crustal radio activity in a given region,and decreases with <strong>the</strong> time since <strong>the</strong> last majortectonic event.A rational way to con struct a 3 D continentalscale earth model that is to serve <strong>the</strong> purpose <strong>of</strong>constraining <strong>the</strong> complexity while still honouring<strong>the</strong> impo rtant facto rs i s to use t he n ewradiometrics map <strong>of</strong> Australia, to d efine tectonicand cratonic provin ces characterised by <strong>the</strong>radiogenic rock content. The big unknown is <strong>the</strong>depth extent <strong>of</strong> each <strong>of</strong> <strong>the</strong>se u nits. It is alsohere th at ge ophysics is n eeded to pla y a part.To date, se e Figure 1, no geological influencesare ta ken int o acco unt when inte rpolating <strong>the</strong>temperatures away from observation points.At <strong>the</strong> same time, great strides are being madeto construct large scale 3D solid geology modelsthat are co nsistent wi th st ructural geol ogyobservations and all <strong>the</strong> geophysical datasets.139


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>In Australia, we have 3 D models for T asmania,most <strong>of</strong> Vict oria, and ab out on e thi rd <strong>of</strong> Sout hAustralia. (Prelimina ry 3D geolo gical models o f<strong>the</strong> Curnamo na b asin a nd Ga wler craton). I naddition, some pu rpose built 3 D he at/geologymodels for <strong>the</strong> Coop er ba sin h ave bee nconstructed with a vie w to ch aracterising <strong>the</strong>heat flow domains and defining uncertainties onthis resource.Numerical/computationalcomplexitiesA current challenge is thus to deal with all <strong>the</strong>secomplexities, deciding on <strong>the</strong> 4 or 5 mostimportant a spects <strong>of</strong> <strong>the</strong> ge oscience, an dconstruct m ore reali stic and <strong>the</strong>ref ore u sefulmodels. It turns out <strong>the</strong>re is a ba rrier with <strong>the</strong>numerical m ethods u sed to solve t he h eatdiffusion equ ation. The m ethods do n ot scalewell. F or s imple s ituations, a ll is w ell, but w hen<strong>the</strong> re quirements <strong>of</strong> 3 D, structu ral geolo gy,material in homogeneity and continent al scal eare stated, n o really viabl e tech niques pre sent<strong>the</strong>mselves. For thi s reason, lea ding ed genumerical methods, u sing F ast Fouri ertransforms etc., are bei ng follo wed up. T wosignificant re cent publi cations point <strong>the</strong> wayhere. Carat ori 200 9, elegantly sho ws ho wgravity and magnetic forward mo delling in 3 Dcan be rapidly achieved using 3D FFT methods.Li, 2007, loo ks at faste r methods for <strong>the</strong> heatdiffusion equation, but ju st <strong>the</strong> h omogenouscase.ConclusionsCraton scale and larger 3D nume rical models,with st ructural geol ogy constraints, p ropertiesand bou ndary condition s <strong>of</strong> measu red surfa ceheat flows, and more fu zzy "Curie Point" depths,can b e integ rated to cre ate heat flow anomalymaps th at wi ll be a vast improvement on <strong>the</strong>existing practise.with a fra ctal model for crustal magnetization, J.OF Geophysical Research, VOL. 114.Caratori T ontini F., Cocch i L., Carmi sciano C.,2009, Rapid 3-D fo rward model <strong>of</strong> potentia lfields with application to <strong>the</strong> Palinu ro Seamountmagnetic an omaly (south ern Tyrrhe nian Sea,Italy) J. OF Geophysical Research, VOL. 114.Chopra, P., and Holgate, F., (200 5) A GISanalysis <strong>of</strong> tempe rature in <strong>the</strong> Austral ian crust,<strong>Proceedings</strong> <strong>of</strong> <strong>the</strong> Worl d Geo<strong>the</strong>rmal Congress2005, Antalya, Turkey, 24-29 April 2005.Li J-R.,Greengard L., 2007, On <strong>the</strong> numericalsolution <strong>of</strong> <strong>the</strong> heat equation I:Fast solvers in f ree spa ce. Journal <strong>of</strong>Computational Physics 226.Maus S., Go rdon D., Fairhead D. 199 7, Curie -temperature depth estimation using a self-similarmagentization mod el, G eophysics J. Int 129,163-168.Sandiford M., Hand M., McLa ren S., 19 98, Highgeo<strong>the</strong>rmal gradie nt metamorphi sm durin g<strong>the</strong>rmal subsidence, Earth and Pl anetaryScience Letters 163, 149–165.Stavrev P., Reid A., 2007, Degrees <strong>of</strong>homogeneity <strong>of</strong> Potential fields and structuralindices <strong>of</strong> Euler deconvolution, Geophysics,Vol.72, NO. 1.Stein, C.A. 1995, Gl obal Earth P hysics AHandbook <strong>of</strong> Physical Con stants AGUReference Shelf 1.The EM s pectra and its measurement continueto provide challen ges a nd insight s in to wholeearth processes. The abil ity to interpre t <strong>the</strong> EMspectra f rom <strong>the</strong> sta ndpoint <strong>of</strong> extractin ginformation a bout cru stal heat de serves mo rethought and development.A better un derstanding <strong>of</strong> how Pla nk's Law and<strong>the</strong> physi cs i mplied by it woul d be im portant i ninterpreting non-solar inf luenced ea rth heatemissions.ReferencesBouligand C., Glen J., Blakely R., 2009,Mapping Curie temperature depth in <strong>the</strong> westernUnited States140


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Evidence <strong>of</strong> impact shock metamorphism in basement granitoids,Cooper Basin, South AustraliaAndrew Y. Glikson 1* and I.Tonguç Uysal 21 <strong>Australian</strong> National University2 Queensland Geo<strong>the</strong>rmal <strong>Energy</strong> Centre <strong>of</strong> Excellence, The University <strong>of</strong> Queensland*Corresponding author: Andrew.Glikson@anu.edu.auThe o riginal observation <strong>of</strong> parallel clo selyspaced (micron s to te ns <strong>of</strong> micro ns) plan arfeatures in quartz g rains from basementgranitoid samples <strong>of</strong> Cooper Basin drill holes byI.T. Uysal, followed by Universa l stage,scanning el ectron mi croscope (SE M) a ndenergy disp ersive spe ctrometry (EDS) tests byA.Y. Glikso n, identify intracrystalli ne plan ardeformation features (P DF) in qu artz whichcorrespond to unique Miller indices diagnostic <strong>of</strong>shock meta morphism. U-Stage mea surements<strong>of</strong> angl es be tween <strong>the</strong> C-optic axis o f qua rtz(C qz ) an d pol es to plana r deformation features(P pdf ) in <strong>the</strong> same qu artz grains (87 p lanar s etsin quartz 54 grains) define intracrystalline planarorientations dominated b y {10 - 13} a nd {10 - 12}Miller indices, correl ated with shock pressuresabove 1 0 G pa and ab ove 20 G pa, respectively(Engelhard a nd St<strong>of</strong>fler, 1968; F rench, 1968;St<strong>of</strong>fler, 197 4; St<strong>of</strong>fler an d Lan genhorst, 1994;Grieve et al., 1996; F rench, 1998). These Millerindices are cha racteristic <strong>of</strong> large impactstructures, i ncluding Chesapeake B ay (D~85km), Woodl eigh (D~1 20 km) and o<strong>the</strong> r impactstructures. S EM/EDS studies <strong>of</strong> core sample sindicate fe atures consistent with sh ockmetamorphism, including recrystallizedpseudotachylite veins an d micro breccia vein sinjected into resorbed quartz g rains. E xtensivealteration <strong>of</strong> feldspar to seri cite and illiterepresent hydro<strong>the</strong>rmal effects. NegativeBouguer anomalies <strong>of</strong> c. -20 µm/s 2 below parts<strong>of</strong> <strong>the</strong> Cooper Basi n reflect lo w den sitybasement sectors (2.64-2.7 6 gr/ cm 3 ) a scompared to adjacent hi gh den sity basem entterrains (2.9-2.99 gr/cm 3 ), consistent with impactfracturing <strong>of</strong> target rocks. L ow magneticanomalies <strong>of</strong> c. -2 00 n T asso ciated with <strong>the</strong>Moomba st ructural dom e and similar structu resto <strong>the</strong> nor<strong>the</strong>a st ma y repre sent resetmagnetisation su ch a s is comm only a ssociatedwith impact structures. An extension <strong>of</strong> <strong>the</strong>Bouguer a nd magneti c a nomalies ov er a >80km-long belt defines <strong>the</strong> minimum extent <strong>of</strong> <strong>the</strong>shock meta morphosed basement, consi stentwith mea sured sho ck p ressures <strong>of</strong> a bove 20GPa. A regional altered zone at <strong>the</strong> top <strong>of</strong> <strong>the</strong>basement ap proximately 10.000 km 2 large an dup to 524 m eters de ep (Boucher, 2001) maycorrespond t o <strong>the</strong> impa ct aureole. Domalseismic stru ctural elem ents a nd overlyingunconformities in ov erlying sedimentarysequence <strong>of</strong> <strong>the</strong> Cooper Basin may be related topost-impact i sostatic uplift <strong>of</strong> impa ct-fracturedlow-density basement sectors. The evidence forimpact bears potential im plications for <strong>the</strong> o rigin<strong>of</strong> K-U-Th e nrichment in t he basement in term s<strong>of</strong> an imp act-triggered hydro<strong>the</strong> rmal cell,mobilization and re concentration <strong>of</strong> radiogenicelements.Fig. 1. Planar deformation features (PDF) in quartzdeflected along a post-impact fracture, McLoed-1 3745 m.141


Identification <strong>of</strong> planar deformationfeatures (PDF)Penetrative intracrystalline plana r d eformationfeatures (P DF) in q uartz po ssess sp ecificcrystallographic Miller indi ces with orientationsdiagnostic <strong>of</strong> shock metamorphism at pressures inexcess <strong>of</strong> levels asso ciated with e ndogenicprocesses such a s s eismic shock, v olcanicexplosions a nd shear pro cesses which p roducemetamorphic deformation lamella (MDL) in quartz(Engelhard and St<strong>of</strong>fler, 1968; Fre nch, 196 8;St<strong>of</strong>fler, 1974; St<strong>of</strong>fler and Lan genhorst, 19 94;Grieve et al. , 1996; Fren ch, 199 8; French andKoeberl, 20 10) (Figs 1 - 5 ). PDFs are (1)restricted to individual grains, i.e. <strong>the</strong>y do notcross grain boundaries; (2) are <strong>of</strong>ten multiple, withN sets per grain; (3) have a strict planar characterthough <strong>the</strong>y can be deflected along shear zo nesand fractu res and in some insta nces fa n out; (4)are typi cally 2-4 mi cron wide; (5) are closelyspaced, typ ically 1 0-20 micron; (6) consist <strong>of</strong>glassy or recrystallized quartz mosaic lamellae, orare m arked by arrays <strong>of</strong> fluid in clusions; (7)possess unique crystallographic orientations.Shock metamorphic features are cla ssified in <strong>the</strong>following terms (French, 1998):1. Mineral fracturing {0001} and {10 - 11} inquartz: 5–7 GPa2. Basal Brazil twins {0001}: 8-10 GPa3. PDF in quartz {10 - 13}: >10 GPa4. Transformation <strong>of</strong> quartz to stishovite: 12-15GPa5. PDF in quartz {10 - 12}: >20 GPa6. Transformation <strong>of</strong> quartz to coesite - >30 GpaThe results <strong>of</strong> universal st age measurements arepresented in Figs 4 and 5. U-stage analysis o fPDF o rientations i s complicated by a n umber <strong>of</strong>factors, ari sing from d ifferential d eformationrelated to <strong>the</strong> attenuation <strong>of</strong> shock <strong>of</strong> quartz grainsby envelopin g hydro us phases, a s well as p ostshockdeformation (Figs 1, 2) and recrystallization<strong>of</strong> quart z gra ins). Thi s in cludes su perposition <strong>of</strong>multiple set s <strong>of</strong> planar feature s, incl uding welldefined pa rallel micro n-scale to tens <strong>of</strong> micron -scale PDF sets (Fig. 3) a nd less well -defined topoorly d efined pa rallel or u ndulating pla narfeatures, in cluding defo rmed P DF and pl anarfeatures (PF ) formed by p re-impact an d/or po stimpactd eformation (Fi gs 1, 2). By contra st toPDFs planar feature s m ay sho w de grees <strong>of</strong>undulation and wavin ess and may beaccompanied by fluid inclu sions an dcryptocrystalline clou ding (Fig. 3). Rarely are<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>PDFs completely expressed and a high proportion<strong>of</strong> grains display only one or two PDFs.Planar features displayed by quart z grains <strong>of</strong> <strong>the</strong>Moomba-1 and McLoed-1 sam ples includegenuine PDFs defined by:1. Penetrative planar parallel sets with spacingson <strong>the</strong> scale <strong>of</strong> few microns to few tens <strong>of</strong>microns (Figs 1 - 3).2. Differential development <strong>of</strong> PDFs betweengrains and within grains.3. Common association <strong>of</strong> PDFs with less-welldefined inclusion-marked somewhat curvedfracture sets (Fig. 3).4. Post-impact deformation indicated by dragfoldfeatures along younger micr<strong>of</strong>ractures(Fig. 1) and wavy deformation <strong>of</strong> PDFs withingrains (Fig. 2).In <strong>the</strong> pre sent study PDFs were me asured onplanar sets displ aying high degree <strong>of</strong> parallelorientation at a few mi crons to few tens <strong>of</strong> micronintervals. PDFs m easured in q uartz grains <strong>of</strong> th eMoomba-1 and McLoed-1 samples are plotted inFigs 4 an d 5 in terms <strong>of</strong> percent fre quency <strong>of</strong>PDFs which co rrespond within me asurementaccuracy <strong>of</strong> ±3 o to specific Miller indices <strong>of</strong> {10 -13}, {10 - 12}, {11 - 22}, {11 - 21}, {10 - 11} and {51 - 61}.The plots demonstrate a prevalence <strong>of</strong> PDFs withMiller indices <strong>of</strong> {10 - 13} and {10 - 12} in Moomba-1core samples and <strong>of</strong> Mille r index <strong>of</strong> {10 - 12} in th eMcLoed-1 co re sa mples (Figs 4, 5), sugge stingshock pre ssures <strong>of</strong> >20 GPa in both cores i naccord with criteria indi cated in studi es <strong>of</strong> sh ockdeformation <strong>of</strong> qua rtz (E ngelhard an d St<strong>of</strong>fler,1968; F rench, 1968; Robertson et al., 1968;St<strong>of</strong>fler, 1974; St<strong>of</strong>fler and Lan genhorst, 19 94;Grieve et al. , 1996; Fren ch, 199 8; French andKoeberl, 201 0). O<strong>the</strong> r m easured Mill er indi cesdiagnostic <strong>of</strong> sho ck m etamorphic ef fects in clude{11 - 21}, {11 - 22}, {10 - 10}, {10 - 11} and {51 - 61}.PDF indices correlated wi th sho ck p ressures <strong>of</strong>>20 GPa are found in la rge to ve ry la rge i mpactstructures, including Yarrabubba impact structure,Western Au stralia (M acdonald et al., 2003 ),Woodleigh i mpact struct ure, Western Au stralia(D=120 km; age ~359 Ma) (Glikson et al., 2005A,B), Chesapeake Bay imp act structure (D=85 km;age ~35 Ma) a nd l arge Ca nadian impa ctstructures (Type D) (French and Koeberl, <strong>2010</strong>).142


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Fig. 2. Three quartz grains bearing planar deformation features (PDF): Note <strong>the</strong> wavy planar structure <strong>of</strong> <strong>the</strong> right-hand grain,representing post-impact plastic deformation <strong>of</strong> <strong>the</strong> quartz grain. Moomba-1 2857.4 m PPL.Fig. 3. Planar deformation features (PDF) (NNW-trending at lower and right-hand part <strong>of</strong> image) and inclusion-dotted planarfractures (at left side <strong>of</strong> image). Moomba-1 2857.4 m, PPL.143


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Fig. 4. Percent frequency distribution <strong>of</strong> <strong>the</strong> Miller-indexed angles between C-optic axis <strong>of</strong> quartz grains (CQzOA) and <strong>the</strong> pole toplanar deformation features (PPDF) in 62 planar sets in 35 quartz grains from Moomba-1 granitoid core samples. Planes areindexed within measurement accuracy <strong>of</strong> ±3% <strong>of</strong> Miller indices.Fig. 5. Percent frequency distribution <strong>of</strong> Miller-indexed angles between C-optic axis <strong>of</strong> quartz grains (CQzOA) and <strong>the</strong> pole toplanar deformation features (PPDF) in 22 planar sets in 19 quartz grains from McLoed-1 granitoid core samples. Planes areindexed within measurement accuracy <strong>of</strong> ±3% <strong>of</strong> Miller indices.144


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Scanning electron microscopyand energy dispersivespectrometryThree sampl es were a nalysed by scan ningelectron mi croscopy (SEM) and <strong>Energy</strong>Dispersive S pectrometry (EDS) o n a Jeol-6400electron microscop e at <strong>the</strong> Research School <strong>of</strong>Biological Studies, <strong>Australian</strong> National University(analyst: A. Glikson; su pervisors: F. Brink, H.Chen). SEM/EDS analytical procedures includedpoint a nalyses <strong>of</strong> elem ent ab undances atdetection levels <strong>of</strong> >2000 ppm. Using a 15 KeVaccelerating voltage, spot analyses were carriedwith a 1 micro n-size be am, with a spe ctrumcollection time <strong>of</strong> 80 se conds (120 seconds realtime) at 8 000 cps. A ccuracy an d p recision arebased on referen ce standards by AstimexScientific Li mited MINM 25-53 (Se rial Numb er95-050) u sing standard olivine, diopside,almandine garnet, albite and barite.Studied samples include:Moomba-1 2857.4 m (Fig. 6): Altered coarsegrainedgranitoid consisting <strong>of</strong> quartz withresorbed grained boundaries injected bymicrobreccia veins which consist <strong>of</strong> micron totens <strong>of</strong> micro-scale quartz, sericite/illite, sulphideand minor magnetite.McLoed-1 3745.9 m: Altered coarse-grainedgranitoid containing K-feldspar, albite andsericite/illite, injected by microbreccia veins.Hydro<strong>the</strong>rmal alteration is manifested by partlycorroded/resorbed quartz grains and magnetitegrains.Big Lake -1 3057m : K-feldspa r-albite-quartzgranitoid consi sting o f reso rbed quart zfragments injected by microbreccia.EDS analyses indicate an abundance <strong>of</strong> sericiteand occa sional pre servation <strong>of</strong> K-feldspa r an dalbite. Ob servations relev ant to <strong>the</strong> search fo rshock metamorphic features include:1. Planar d eformation featu res ide ntified byoptical microscopy do not display on ei<strong>the</strong>relectron ba ckscatter mod e or se condaryelectron (SE1) sca nning mode. T hisindicates PDF lam ina consist <strong>of</strong>cryptocrystalline qua rtz <strong>of</strong> similar ele ctrondensity as <strong>the</strong> host quartz.2. The inje ction <strong>of</strong> microb reccia veins in toquartz grai ns is con sistent with, althoughdoes not prove, shock effects.3. The co rroded boun daries <strong>of</strong> quartz a ndmagnetite g rains (Fi g. 6) an d <strong>the</strong>abundance <strong>of</strong> se ricite and illite a reconsistent wi th hydro<strong>the</strong> rmal alteratio n <strong>of</strong><strong>the</strong> granitoids.The extre me fine g rained texture <strong>of</strong> <strong>the</strong>microbreccia veins su ggests <strong>the</strong>ir possiblederivation by recrystallization <strong>of</strong> pse udotachyliteveins con sisting <strong>of</strong> impact -generatedcomminuted and fluidized materi al simila r toveins found arou nd expo sed impact structu res(Spray, 1995; Spray and T hompson, 199 5;Reimold, 1995, 1998).145


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Fig. 6. Moomba-1 2857.4 m: SEM image <strong>of</strong> hydro<strong>the</strong>rmally altered microbreccia-injected granitoid. (A) backscatter image <strong>of</strong>microbreccia veins injected into quartz grains; (B) SE1 image <strong>of</strong> frame A; (C) secondary magnetite within microbreccia veins; (D)magnified view <strong>of</strong> microbreccia vein consisting <strong>of</strong> quartz, sericite and magnetite.Implications for structure and<strong>the</strong> origin <strong>of</strong> geo<strong>the</strong>rmalanomaliesBoucher (1996, 2001 ), o n <strong>the</strong> ba sis <strong>of</strong> wireli nelog sign atures and d rill core s, rep orted analtered zone up to 524 meters-thick at <strong>the</strong> top <strong>of</strong><strong>the</strong> top <strong>of</strong> e arly to mi d Palaeozoic b asementunderlying th e Coope r B asin. Bo ucher (200 1)considered t he o rigin <strong>of</strong> this zone in terms <strong>of</strong>ei<strong>the</strong>r wea<strong>the</strong>ring o r hyd ro<strong>the</strong>rmal alte ration, o rmerely as a wireline logging anomaly.The prese nce <strong>of</strong> si gnatures <strong>of</strong> sho ckmetamorphism within <strong>the</strong> altered top basementzone may sug gest extensive hyd ro<strong>the</strong>rmalactivity trigge red by a la rge aste roid im pact, a shas been documented in large impact structures(Allen et al., 1982; Naumov, 2002; Pirajno, 2005;Glikson et al., 2005; Fren ch, 1998; Uysal et al.,2001, 2002; French and Koeberl, <strong>2010</strong>). Basedon a ssociation <strong>of</strong> hyd ro<strong>the</strong>rmal alte ration withimpact effects, <strong>the</strong> extent <strong>of</strong> <strong>the</strong> impact aureolemay be outlined by <strong>the</strong> altered zo ne, whichcovers a n a rea large r tha n 10,00 0 km 2 in <strong>the</strong>Cooper Basin (Boucher, 2001; Fig. A8).Shock m etamorphism <strong>of</strong> ba sement sectors isconsistent with ge ophysical an d structuralevidence fo r low de nsity (2.64 –2.76 g/cm 3 )basement sectors underlying <strong>the</strong> Moomba-1 andMcLoed-1 holes, as compared to hig her densitybodies (2.8 – 3.0 g/cm 3 ) in adjacent terrain(Meixner et al., 2000 ). The lo w-densitybasement sectors likel y represents intensehydration and fracturing related to <strong>the</strong> impact, asis <strong>the</strong> ca se with <strong>the</strong> Woodl eigh impact structure(Glikson et al., 2005 a, 2005b ), Gnargooprobable imp act structure (Iasky a nd Glikson,2005) and Mount A shmore proba ble impa ctstructure (G likson et al., <strong>2010</strong>). T he lo wmagnetic an omalies a ssociated with th e gravitylows (Meixne r et al, 2000) are con sistent withdemagnetisation <strong>of</strong> impa cted ba sement zon es,observed in a num ber <strong>of</strong> impa ct structures(Grieve and Pilkington, 1996).The evid ence fo r im pact b ears potentialimplications for <strong>the</strong> origin <strong>of</strong> K-U-Th enrichmentin <strong>the</strong> Coo per Basi n in terms <strong>of</strong> a n impacttriggeredhy dro<strong>the</strong>rmal cell an d a ssociatedmobilization and reco ncentration <strong>of</strong> radiog enicelements. Tempe ratures over 22 5 o C at 5 kmdepth (T 5km ) occur over a n area about 79,000km 2 large under an insulating sedimentary coverabout 3.5 – 4.5 km-thi ck at <strong>the</strong> Na ppamerriTrough between Moomba dome and Innaminckawhere geo<strong>the</strong>rmal gradie nts a s hi gh as 55-60 o C/km are measure d (Middleton, 1979;Wyborn et al., 2004; Rad ke, 2009). Th e highest146


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>temperatures occu r n ear Innamin cka in <strong>the</strong>proximity <strong>of</strong> McLo ed-1, where maximum sho ckpressures <strong>of</strong> > 20 G pa are me asured (Fig. 5) .Extreme total heat flo w <strong>of</strong> 7.5-1 0.3 mWm -3originate from enrichment <strong>of</strong> <strong>the</strong> Big L ake Suitegranites in ra diogenic heat-producing elements,including Uranium (13.7, 16.5 pp m), Thori um(46, 74 p pm) and Potassi um (5.2, 6.0 % K2O)(Middleton, 1979; Sandiford and McLaren, 2002;Chopra, 2003; McLaren and Dunlap, 2006). Thepresence <strong>of</strong> a highly radiogenic basement within3-4 km <strong>of</strong> <strong>the</strong> surface may in part refle ct upwardmigration an d re -concentration <strong>of</strong> la rge ionlithophile el ements a ssociated with a n impactgeneratedhy dro<strong>the</strong>rmal cell, as is <strong>the</strong> case insome imp act structu res, including Woodlei gh(Glikson et al. 20 05), Shoem aker imp actstructure an d Yarrab ubba imp act structure(Pirajno, 2005).ReferencesAllen, C. C., Gooding, J. L., Keil, K. 1982.Journal <strong>of</strong> Geophysical Research 82, 10083 –10101.Boucher, R.K., 1996. MESA Journal, 21, 30-32.Boucher, R.K., 2001. Nature and origin <strong>of</strong> <strong>the</strong>altered zone at <strong>the</strong> base Cooper Basinunconformity, South Australia. South Australia.Department <strong>of</strong> Primary Industries andResources, Report Book 2001/012.Chopra, P., 2003. Preview <strong>Australian</strong> Society <strong>of</strong>Exploration Geophysics, 107, 34-36.Engelhard, W.V., Stöffler, D., 1968. in: ShockMetamorphism <strong>of</strong> Natural Materials. MonoBook Corp, Baltimore, MD, 159–168.French, B.M., 1968. In: Shock Metamorphism <strong>of</strong>Natural Materials. Mono Book Corp, Baltimore,MD, 1–17.French, B.M., 1998. Traces <strong>of</strong> catastrophe: ahandbook <strong>of</strong> shock-metamorphic effects interrestrial meteorite impact craters. Lunar andPlanetary Institute, Houston, TX, ContributionCB-954. 120 pp.French, B.M., Koeberl, C., <strong>2010</strong>. The convincingidentification <strong>of</strong> terrestrial meteorite impactstructures: What works, what doesn't, andwhy. Earth-Science Reviews, 98, 123–170.Glikson, A. Y., Eggins, S., Golding, S., Haines,P. W., Iasky, R. P., Mernagh, T. P., Mory, A.J., Pirajno, F. Uysal, I. T., 2005. <strong>Australian</strong>Journal <strong>of</strong> Earth Sciences, 52, 555-573.Glikson, A. Y., Mory, A. J., Iasky, R. P., Pirajno.F., Golding, S. D., Uysal, I. T. 2005. <strong>Australian</strong>Journal <strong>of</strong> Earth Sciences, 52, 545–553.Glikson, A. Y., Jablonsky, D., Westlake, S.,<strong>2010</strong>. <strong>Australian</strong> Journal <strong>of</strong> Earth Sciences,57, 411–430.Grieve, R.A.F., Pilkington, M., 1996. <strong>Australian</strong>Geological Survey Organisation Journal <strong>of</strong><strong>Australian</strong> Geology and Geophysics, 16, No.4, 399-420.Grieve, R.A.F., Langenhorst, F., Stöffler, D.,1996. Meteoritics and Planetary Science, 31,6–35.Iasky, R. P., Glikson, A. Y. 2005. <strong>Australian</strong>Journal <strong>of</strong> Earth Sciences, 52. 575–586Macdonald, F.A., Bunting, J.A., Cina, S., 2003.Earth and Planetary Science Letters, 213,235-247McLaren, S., Dunlap, W.J., 2006. BasinResearch, 18, 189–203.Meixner, T.J., Gunn, P.J., Boucher, R.K., Yeats,A.N., Murray, L., Yeats, T.N., Richardson,L.M., Freares, R.A., 2000. South AustraliaExploration Geophysics, 31, 024-032Middleton, M.F. (1979) Bulletin <strong>of</strong> <strong>the</strong> <strong>Australian</strong>Society <strong>of</strong> Exploration Geophysics.Naumov, M. V. 2002. In: Impacts in PrecambrianShields, pp. 117 – 173. Springer Verlag,Berlin.Pirajno, F., 2005. <strong>Australian</strong> Journal EarthScience, 52, 4/5, 587-606.Radke, B., 2009. Geoscience Australia Record2009/25.Reimold, W.U., 1995. Earth Science Reviews,39, 247–265.Reimold, W.U., 1998. Earth Science Reviews,43, 45–47.Robertson, P.B., Dence, M.R., Vos, M.A., 1968.Shock Metamorphism <strong>of</strong> Natural Materials.Mono Book Corp, Baltimore, MD, pp. 433–452.Sandiford, M., McLaren, S., 2002. EarthPlanetary Science Letters, 204, 133-150.Spray, J.S., 1995. Geology, 23, 1119–1122.Spray, J.G., Thompson, L.M., 1995. 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<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Geo<strong>the</strong>rmal <strong>Energy</strong> in India: Past, Present and Future PlansHarinarayana, T., National Geophysical Research Institute, Hyderabad (Council <strong>of</strong> scientific andindustrial research)AbstractIt is well known that a mong th e vari ousnew a nd rene wable e nergy sou rces,geo<strong>the</strong>rmal energy is known to be one <strong>of</strong><strong>the</strong> cl ean en ergy without smoke an d a lsowithout e nvironmental ha zards. Altho ughit’s importa nce is realized long b ack ino<strong>the</strong>r countri es, it’s exploi tation is still faraway in Ind ia, mainly due to lack <strong>of</strong>knowledge on <strong>the</strong> de ep sub surfacestructure and lack <strong>of</strong> ded icated p rogramon dee p dril ling in high pre ssure, h ightemperature conditions. Geological Survey<strong>of</strong> India (GS I) and National Geo physicalResearch In stitute (NG RI) have madeconcerted efforts in i dentifying <strong>the</strong> seresources in different parts <strong>of</strong> our countryfor po ssible exploitati on. In thisdirection, different ge o<strong>the</strong>rmal regi onshave bee n investigate d in recent yearsusing dee p electroma gnetic geop hysicaltechnique, n amely <strong>the</strong> Magnetotell urics.The g eo<strong>the</strong>rmal regions inve stigatedinclude Pu ga in higher Himalaya s <strong>of</strong>Jammu and Kashmir, Tattapani <strong>of</strong> Su rgujadistrict in Chattisgarh, Surajkund <strong>of</strong>Jharkhand, Tapovan -Vishnugad, Loh ari-Nag-Pala, Badrin ath re gions <strong>of</strong>Uttarakhand, Kullu-Ma nali regi ons <strong>of</strong>Himachal Prade sh. The se investigati onshave provided <strong>the</strong> quant itative dimensions<strong>of</strong> <strong>the</strong> anom alous su bsurface st ructuresrelated to geo<strong>the</strong>rmal he at source. In t histalk, an ove rview <strong>of</strong> <strong>the</strong> d etails <strong>of</strong> p resentday knowl edge <strong>of</strong> g eo<strong>the</strong>rmal ene rgy atdifferent locations with estimated potentialbased on th e ge ophysical stu dies a ndshallow b oreholes tempe rature log s arediscussed. Con crete pl ans a nd futuredirections are also provided to develop thisuntapped resource.148


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Aquifer heterogeneity – is it properly assessed by wellbore samplesand does it matter for aquifer heat extraction?Peter Leary*, Peter Malin, Eylon Shalev & Stephen OnachaInstitute <strong>of</strong> Earth Sciences and Engineering, University <strong>of</strong> Auckland58 Symonds Street, Auckland 1142, New Zealandp.leary@auckland.ac.nzAbstractOil field reservoir formations are sampled forporosity and permeability on <strong>the</strong> tacit assumptionthat small scale well-log and well-core data arerepresentative <strong>of</strong> <strong>the</strong> formation flow properties atarbitrary distances from <strong>the</strong> wellbore. In formalterms, this statistical assumption is valid only if<strong>the</strong> formation properties are adequatelycharacterised by a mean and standard deviation,or, equivalently, if variations in formationproperties are spatially uncorrelated on all scalelengths. This statistical validity condition is,however, violated by crustal rock; well-log andwell-core data are spatially correlated over a widerange <strong>of</strong> scale lengths. It is, <strong>the</strong>refore, formallywrong to assume that small scale sample meansand standard deviations adequately representlarge-scale variation <strong>of</strong> aquifer reservoir/formationproperties.As a practical matter, <strong>the</strong> formal failure <strong>of</strong> oil fieldwell-log and well-core sampling to adequatelyestimate large-scale formation flow propertyvariation is buffered by (i) <strong>the</strong> high energy density<strong>of</strong> hydrocarbons, (ii) lack <strong>of</strong> need for largedrainage flow rates, (iii) ability to drill infill wells ifde facto well drainage volumes are too small, and(iv) ability <strong>of</strong> time-lapse seismic imaging to detectfluid substitution volumes to determine large-scaleformation flow structures that are not inferred fromsmall-scale formation sampling strategies.As an equally practical matter, however, <strong>the</strong>above caveats do not apply to producing hotaquifer fluids: (i) geo<strong>the</strong>rmal energy density is farsmaller than hydrocarbon energy content; (ii) highflow rates are essential to geo<strong>the</strong>rmal powerproduction; (iii) infill wells are at high risk to notintersect large drainage volumes unless guided byreliable auxiliary information; (iv) time-lapse hotaquifer imaging has no fluid-substitution signal.An alternative strategy to aquifer production wellsitingbased on small-scale wellbore sampling <strong>of</strong><strong>the</strong> aquifer focuses on measuring large-scaleaquifer fracture-structures. Experience withmagnetotelluric (MT) detection <strong>of</strong> in situ fracturevolumes in geo<strong>the</strong>rmal fields suggests that MTsurveys can form <strong>the</strong> basis for physically accuratesampling <strong>of</strong> large-scale aquifer fracture/flowstructure.Keywords: fractures, faults, porosity, permeabilityIntroduction – Treating aquifers as oilfield reservoir formationsThe following statement, made at <strong>the</strong> Bali <strong>2010</strong>World Geo<strong>the</strong>rmal Congress, succinctly describesan approach to hot aquifer energy productionbased on oil/gas reservoir formationcharacterisation using wellbore samples.As part <strong>of</strong> <strong>the</strong> drilling <strong>of</strong> <strong>the</strong> petroleum wells, asignificant amount <strong>of</strong> wireline logging, coresampling and resulting petrophysical evaluationwere undertaken…... The porosity <strong>of</strong> <strong>the</strong> target….section was determined…based on wirelinelogs calibrated to porosity samples fromconventional cores and sidewall cores. The coreporosities were calibrated to measuredpermeabilities using all <strong>the</strong> cores from a largerdatabase…... Several studies…..provide insightsinto <strong>the</strong> petrophysical evaluation….and itscalibration <strong>of</strong> porosity to permeability. Using <strong>the</strong>calibration <strong>of</strong> porosity to permeability, and <strong>the</strong>calibrated porosity derived from wireline loggingand cores, it is thus possible to determine <strong>the</strong>permeability….sandstone section and integratethis across <strong>the</strong> borehole to get <strong>the</strong> transmissivityor permeability metres. (de Graaf et al <strong>2010</strong>).Parallel statements were made at <strong>the</strong> WGC<strong>2010</strong>by Clauser et al (<strong>2010</strong>) and Vogt et al (<strong>2010</strong>).The working assumption is that formation wellboredata recorded by geophysical logging tools and/orrecovered in well core adequately samples <strong>the</strong>formation properties at all relevant scales. Whileindisputably <strong>the</strong> wellbore data sample specificgeological formations, it does not follow that withina geological formation any or all importantgeophysical properties conform to a small-scalesample mean throughout <strong>the</strong> formation, or thatimportant geophysical property variations within<strong>the</strong> formation are confined to <strong>the</strong> formation.Ra<strong>the</strong>r <strong>the</strong> evidence from well-log datasystematics is precisely <strong>the</strong> opposite: variation <strong>of</strong>geophysical properties within a formation can besubstantial and <strong>the</strong>se variations can be connectedto <strong>the</strong> enclosing crustal volumes outside <strong>the</strong>formation. Well-log systematics thus indicate thatnear-wellbore samples do not accurately assess<strong>the</strong> degree <strong>of</strong> large-scale spatial variationexpected for in situ formation properties, and that<strong>the</strong> spatial distributions <strong>of</strong> formation variationscannot be adequately estimated from small-scalesampling.149


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>These general statements are illustrated by welllogand well-core data for Perth Basin formationsencountered by <strong>the</strong> 3km-deep Cockburn1 well.10 10 SONIC EXP: -1.05 -1.34Well-log and well-core sample data forPerth Basin sedimentary formationsPerth Basin formations were drilled, logged andcore-sampled by <strong>the</strong> 3km-deep Cockburn1 oilexploration well on <strong>the</strong> coast 18km southwest <strong>of</strong>Perth (Smith 1967). Well-log data in general, andfor <strong>the</strong> 1200m thick Yarragadee aquifer inparticular, conform to well-log in situ geophysicalproperty variations observed worldwide. Figure 1shows <strong>the</strong> well-log systematics for specific aquiferformations in <strong>the</strong> Cockburn1 well sequence.Well-log power-law scaling systematicsThe Fourier power-spectra <strong>of</strong> in situ spatialvariations <strong>of</strong> rock properties measured by welllogs worldwide closely conform to a specificpower-law scaling form (Leary 2002):S(k) 1/k 1 , (1)where k is spatial frequency and S is <strong>the</strong> well-logfluctuation power at scale length k. Dependingupon <strong>the</strong> well log, <strong>the</strong> spectral scale-length rangek tends to ~3 decades in <strong>the</strong> overall 5-decadescale range ~1cycle/cm to ~1cycle/km. Highspatial frequency data at ~1cycle/cm are recordedby formation microscanner tools measuringelectric resistivity with mm-scale electrodes. Kmlongwell logs <strong>of</strong> gamma activity, acoustic velocity,neutron density, electron density and electricalresistivity logs routinely return low spatialfluctuation power data at ~1cycle/km.Well-log spectral form (1) is important for threereasons: It is power-law over all scale lengthsrelevant to reservoir performance andcrustal deformation processes;The power-law exponent is <strong>the</strong> same foressentially all in situ properties, rocktypes, and geological settings; The non-zero power-law exponentdestroys <strong>the</strong> basis for standard statisticalinferences from standard sampling.Power-law scaling <strong>of</strong> well-log spatial fluctuationsover <strong>the</strong> five-decade cm-km scale range isindisputable evidence that something beyondgeology is at work in <strong>the</strong> brittle crust. A power-lawscaling exponent that is essentially <strong>the</strong> same for arange <strong>of</strong> geologic media and settings is evidencethat power-law scaling derives from fundamentalphysical properties <strong>of</strong> rock with secondary regardto geological details at all scale lengths. Spatiallyfluctuating grain-scale fracture density is a likelycandidate for <strong>the</strong> fundamental parametercontrolling how in situ physical properties <strong>of</strong> rockvary both vertically and horizontally (Leary 2002).10 810 610 0 10 2SPATIAL FREQUENCY (CYCLES/KM)10 11 GAMMA EXP: -1.1 -1.0410 910 710 0 10 2SPATIAL FREQUENCY (CYCLES/KM)10 10 RESISTIVITY EXP: -1.23 -1.2810 810 610 0 10 2SPATIAL FREQUENCY (CYCLES/KM)Figure 1: Well-log fluctuation power-spectra for Cockburn1geological section (blue) and Yarragadee formation (black) fitto power-law trends for sonic velocity, gamma activity andresistivity data. Red line fit to entire section, green line toYarragadee section. Spectral exponent ~1.17 0.13 is nonzero,showing that fluctuations <strong>of</strong> in situ rock physicalproperties <strong>of</strong> <strong>the</strong> Cockburn1 drill site and <strong>the</strong> Yarragadeeaquifer in particular are spatially correlated ra<strong>the</strong>r thanspatially uncorrelated over <strong>the</strong> m-km scale range.The non-zero power-law scaling exponent in (1)means that in situ spatial fluctuations ingeophysical properties are spatially correlated atall scale lengths and hence systematically violate<strong>the</strong> necessary condition <strong>of</strong> <strong>the</strong> central-limit<strong>the</strong>orem upon which standard geostatisticalinferences are commonly based.150


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>The general idea that small-scale sample meansand standard deviations reasonably representlarge-scale property variations within an ensembleis valid only if <strong>the</strong> ensemble property variationsare spatially uncorrelated. Fluctuations are, inturn, uncorrelated only if <strong>the</strong> associatedfluctuation power-law spectrum is ‘white’,S(k) 1/k 0 ~ constant, (2)NORMALISED FLUCTUATIONPOROSITY (blu) -- LOG(PERMEABILITY) (red)2.521.510.50-0.5-1-1.5-20 50 100 150 200SAMPLE NUMBER250at all relevant scale lengths. Figure 1 testsfluctuation power condition (2) for well-logacoustic velocity, gamma activity, and electricalresistivity data over <strong>the</strong> entire Cockburn1 section(blue) and <strong>the</strong> Yarragadee formation (black).Since <strong>the</strong> power-law exponent <strong>of</strong> each spectrumis ~1 instead <strong>of</strong> 0 over <strong>the</strong> 3 decade m-km scalerange, condition (2) for spatially uncorrelatedfluctuations in <strong>the</strong> Cockburn1 well geologicalsection is ma<strong>the</strong>matically untenable. Whateverproperties <strong>of</strong> in situ rock are responsible for <strong>the</strong>variations in well-log readings, it cannot belogically maintained that <strong>the</strong> mean and standarddeviation <strong>of</strong> small-scale sample data accuratelypredicts <strong>the</strong> scale <strong>of</strong> variations in those propertiesat arbitrary distances from <strong>the</strong> wellbore.Well-core poroperm fluctuation systematics –percolation via grain-scale fracturesAn underlying connection between in situfractures and S(k) 1/k power-spectra isplausible since spatial variations in gammaactivity <strong>of</strong> soluble radiogenic minerals, acousticvelocity and electrical resistivity are naturallyrelated to spatial variations in fracture density.That is, crustal volumes with a greater number <strong>of</strong>fractures tend to have greater gamma activity,lower resistivity and lower seismic velocity.However, physically more immediate evidence forspatially variable fracture density is availablethrough <strong>the</strong> systematics <strong>of</strong> well-core porositypermeability(poroperm) spatial fluctuationsmeasured in numerous oil/gas field reservoirformations (Leary & Walter 2008).Figure 2 graphically illustrates <strong>the</strong> systematics <strong>of</strong>poroperm spatial fluctuations for well-core datafrom tight gas reservoir formations in <strong>the</strong> CooperBasin, South Australia. The blue trace tracksvariations in well-core porosity φ and <strong>the</strong> red tracetracks variations in <strong>the</strong> logarithm <strong>of</strong> well-corepermeability as <strong>the</strong> core sequence moves along<strong>the</strong> well. The Figure 2 spatial fluctuation relationbetween porosity φ and logarithm <strong>of</strong> permeability can be written,φ ~ log(), (3)where φ and log() denote respectivelynormalised spatial variations in well-core values <strong>of</strong>porosity and log(permeability) over a well-coresequence.Figure 2: Overlay <strong>of</strong> poroperm fluctuation data for tightsandstone formations in <strong>the</strong> Cooper Basin, South Australia.The blue and red traces denote zero-mean/unit-variancefluctuations in, respectively, well-core porosity and <strong>the</strong>logarithm <strong>of</strong> well-core permeability. Cross-correlation <strong>of</strong> <strong>the</strong>two traces is 85% at zero-lag.High degrees <strong>of</strong> spatial cross-correlation (3) arecommon in <strong>the</strong> abundant well-core poropermsequences acquired for clastic reservoir sections.The cross-correlations have a natural explanationin terms <strong>of</strong> fluid percolation at grain-scalefractures. Consider a core-sized rock volume <strong>of</strong> Ngrain-grain contacts with intact cement bondingand no fluid percolation. Within <strong>the</strong> core,however, a number n


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Thus, if n is <strong>the</strong> number <strong>of</strong> percolating defects in aunit volume <strong>of</strong> rock and n! is proportional to <strong>the</strong>percolation permeability <strong>of</strong> <strong>the</strong> rock sample with npercolation defects, <strong>the</strong>n empirical relation (3) iseffectively a ma<strong>the</strong>matical identity, log(n!) =n(log(n) - 1). The close equivalence <strong>of</strong> (3) and (4)argues that in situ permeability is a percolationprocess in rock volumes whose physicalproperties on all scale lengths are internallydefined by spatially fluctuating populations <strong>of</strong>grain-scale defects consistent with power-lawscaling <strong>of</strong> well-log spectra (1).LOG(PERMEABILITY) (MDARCY)43.532.521.510.500 10 20 30 40POROSITY (%)210-1-20 20 40 60210-1-20 20 40 60 80SAMPLE NUMBER210-1-20 20 40 60210-1-20 5 10SAMPLE NUMBERFigure 3: (Upper) Composite poroperm data as traditionallypresented in oil and gas literature; a sequence <strong>of</strong>poroperm traces are sorted by grain size from coarser onleft to finer on right. (Lower) Same poroperm datarendered in Figure 2 format; spatial fluctuation correlationsbetween porosity and log(permeability) masked in upperdisplay emerge in agreement with spatial fluctuationrelations (3) and (4).It may be useful to useful at this point to contrast<strong>the</strong> multi-scale-length spatially-correlated fracturephenomenology <strong>of</strong> well-log fluctuations (1) andwell-core empirical fluctuations (3) and fracturefluctuationpercolation interpretation (4) with <strong>the</strong>standard treatment <strong>of</strong> poroperm data in <strong>the</strong> oil/gasindustry literature. With reference to empiricalrelation (3), <strong>the</strong> upper plot in Figure 3 showsstandard industry presentation <strong>of</strong> poroperm datafor a sequence <strong>of</strong> size-graded well-core (coarsergrain samples on <strong>the</strong> left grade into finer grainsamples on <strong>the</strong> right). Inherent in this poropermdata presentation is <strong>the</strong> expectation that eachsample is integral into itself, with no reason tosuppose that <strong>the</strong> sample could be systematicallyrelated to neighbouring samples on any particularscale length (except, <strong>of</strong> course, by ‘random’happenstance). The lower subplots <strong>of</strong> Figure 3show, however, that latent in <strong>the</strong> poroperm data is<strong>the</strong> empirical poroperm spatial correlation (3).The subplots render four <strong>of</strong> <strong>the</strong> five upper-plotgrain-size-graded poroperm data trends in <strong>the</strong>zero-mean/unit-variance sequence normalisationformat <strong>of</strong> Figure 2. Spatial correlation (3)between porosity and log(permeability) emergesdirectly from <strong>the</strong> obscurity <strong>of</strong> <strong>the</strong> standardporoperm data presentation.Again in line with <strong>the</strong> industry assumption thatrock samples are only ‘randomly’ related to <strong>the</strong>irneighbours, common oil industry practice uses ageneric permeability dependence on porositysuch as <strong>the</strong> Carman-Kozeny cubic expression(e.g., Dvorkin 2009; Cox et al 2001; Mavko & Nur1997), ~ φ 3 . (5)Poroperm dependency (5) is derived fromestimates <strong>of</strong> tubular flow through clusters <strong>of</strong> porespace without reference to grain-scale fractures orfracture connectivity at any scale. Suchformulations with reference only to <strong>the</strong> smallestscale lengths are consistent with spatiallyuncorrelated rock property heterogeneity (2) but,<strong>of</strong> course, make no contact with <strong>the</strong> essentiallyuniversal well-log observation (1) that in situ rockproperty heterogeneity is spatially correlated overfive decades <strong>of</strong> scale length.Well-log and well-core data thus provide clearlines <strong>of</strong> evidence that1. small-scale (wellbore) sampling <strong>of</strong>permeability does not accurately assesslarge scale in situ permeability variability;2. in situ fractures and fracture-controlledpermeability on all scale lengths are anessential ingredient <strong>of</strong> crustal rockheterogeneity;3. large amplitude in situ permeabilityheterogeneity is expected at large scalelengths.Yarragadee well-core poroperm fluctuationsApplying <strong>the</strong> above argument to <strong>the</strong> Cockburn1well data, Figure 4 shows <strong>the</strong> poroperm spatialfluctuation data for <strong>the</strong> complete Cockburn1 wellcoresuite in <strong>the</strong> Figure 2 format. Dotted datapoints in Figure 4 mark poroperm data for <strong>the</strong>Yarragadee aquifer within <strong>the</strong> Cockburn1 wellsequence. In contrast with typical oil fieldreservoir well-core sample data tightly confined toshort intervals <strong>of</strong> oil-bearing sands, many <strong>of</strong> <strong>the</strong>Cockburn1 well-core samples were taken at 100mto 200m intervals over which formation propertieschange significantly.152


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>COCKBURN1 POROPERM (DOTS=YARRAGADEE)3BLUE = | RED = LOG()210-1-20 5 10 15 20 25 30SAMPLE NOFigure 4: Cockburn1 well-core poroperm data sequencein Figure 2 format (blue = porosity, red = log(permeability)normalised to zero-mean/unit-variance). Compared withstandard oil field reservoir poroperm fluctuations in, say,Figure 2, departures from close spatial correlation aredue to well-core samples being taken at 100m intervals invarying formations.Despite <strong>the</strong> far more variable nature <strong>of</strong> <strong>the</strong>Cockburn1 well rock-type and formation-typeporoperm sampling, Figure 5 shows 60% zero-lagspatial correlation (red trace) between variationsin Cockburn1-well sample porosity and samplelog(permeability). The blue trace indicates <strong>the</strong>typical 20% level <strong>of</strong> cross-correlation excursion <strong>of</strong>spatially-uncorrelated fluctuation sequences withspectral content <strong>of</strong> <strong>the</strong> Cockburn1 poroperm data.The 60% Cockburn1 data cross-correlation peakat zero-lag is statistically significant.XCORR(,LOG()COCKBURN1 WELL POROPERM XCORR0.80.60.40.20-0.2-0.4-150 -100 -50 0 50 100 150LAGFigure 5: (Red) Cross-correlation <strong>of</strong> resampledCockburn1 well-core poroperm data sequences. (Blue)Cross-correlation <strong>of</strong> uncorrelated random sequences withfrequency content <strong>of</strong> well-core poroperm data; 60%correlation between poroperm sequences at a specific lag(here zero) is seen to be statistically significant.Fracture heterogeneity and hot aquiferenergy productionThe foregoing discussion challenges <strong>the</strong> oil/gasindustry reservoir characterisation assumptionthat spatially sparse wellbore samples more orless represent geological formation properties atall larger scale lengths. Plentiful well-log andwell-core data instead point to in situ percolationflow processes controlled by spatially-correlatedrandom fracture networks on all scale lengths.Such random fracture networks are spatiallyerratic and effectively unpredictable from smallscalesparse sampling, leading to a degree <strong>of</strong>ge<strong>of</strong>luid flow spatial heterogeneity consistent with<strong>the</strong> statistics <strong>of</strong> production well drilling success.The following quote assesses <strong>the</strong> success rate <strong>of</strong>drilling geo<strong>the</strong>rmal wells at one half <strong>the</strong> successrate <strong>of</strong> drilling oil/gas wildcat wells:Given <strong>the</strong> extremely high degree <strong>of</strong> uncertaintyinvolved in well siting and design, hydro<strong>the</strong>rmalexploration success rates are around 25%,estimates <strong>the</strong> GEA. That compares with aworldwide oil wildcat success rate <strong>of</strong> 45% in 2003,according to IHS <strong>Energy</strong>, a consultancy.(Petroleum Economist 2009),While a number <strong>of</strong> factors affect both productionwell success/failure rates, two factors stand out: oil and gas are far more energy rich thanhot water; to be pr<strong>of</strong>itable oil and gas do not have tocome <strong>of</strong> out <strong>the</strong> ground at high flow ratesbut hot water does.With <strong>the</strong> chemical energy <strong>of</strong> oil about 50MJ perlitre, and long-term oil field production averagerate ~1 litre per 4 seconds (~15 barrels <strong>of</strong> oil perday for ~5x10 5 US wells for years 1954-2006,www.eia.doe.gov/aer/txt/ptb0502.html), wellheadpower production for a typical oil well is <strong>of</strong> order12MW. In contrast, a geo<strong>the</strong>rmal well dischargingN litres per second <strong>of</strong> water with T o C excesstemperature produces about 4xNxT/1000 MW <strong>of</strong><strong>the</strong>rmal power. For T = 100 o C, it requires N ~25 litre/s to produce 10MW <strong>of</strong> <strong>the</strong>rmal power. Forequal wellhead power production, a geo<strong>the</strong>rmalwell flow rate must thus be <strong>of</strong> order 100 greaterthan an oil well.Translating ge<strong>of</strong>luid flow rate into dollar-rate tocover drilling costs, and taking into account <strong>the</strong>different efficiencies <strong>of</strong> electrical powerproduction, a geo<strong>the</strong>rmal well must flow on order300 times greater rate to produce an incomeequivalent to pure oil recovery. Allowing forproduction <strong>of</strong> water as well as oil, 90% water cutrequires a geo<strong>the</strong>rmal well to flow effectively 30times <strong>the</strong> rate <strong>of</strong> its oil equivalent for comparableincome to cover drilling costs.153


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>These contrasting order-<strong>of</strong>-magnitude well-flowratenumbers for hydrocarbon and geo<strong>the</strong>rmalpower production make it clear that effectivegeo<strong>the</strong>rmal production well siting demandsunderstanding <strong>the</strong> potential for flow heterogeneity<strong>of</strong> <strong>the</strong> target formation. It is not surprising that <strong>the</strong>global success rate for geo<strong>the</strong>rmal production wellsuccess is one half that <strong>of</strong> hydrocarbon wildcatwells. Within a developed hydrocarbon reservoir,<strong>the</strong> rate <strong>of</strong> infill drilling success is probablysubstantially higher than wildcat well success,giving all <strong>the</strong> more reason to be cautious aboutadopting oil field practices regarding aquiferpermeability distributions.To make aquifer energy production commerciallyviable, physical logic and practical experienceindicate that close attention needs to be paid t<strong>of</strong>inding aquifer volumes <strong>of</strong> sufficient size andfracture density that production wells can cover<strong>the</strong>ir cost. To that end, we discuss severalsurveys <strong>of</strong> producing geo<strong>the</strong>rmal fields in which: MT data identified reservoir volumes <strong>of</strong>significant aligned fracture density; production wells drilled in <strong>the</strong> MTidentifiedaligned-fracture reservoirvolumes had flow rates far exceeding<strong>the</strong> field average.An MT approach to sounding for largescaleaquifer fracture structuresMagnetotellurics (MT) is <strong>the</strong> practice <strong>of</strong> measuring<strong>the</strong> natural magnetic field fluctuations <strong>of</strong> <strong>the</strong>earth’s atmosphere as <strong>the</strong>y reach <strong>the</strong> earth’ssurface, and at <strong>the</strong> same time and placemeasuring electric (telluric) currents induced by<strong>the</strong> travelling magnetic fields. By measuring <strong>the</strong>natural magnetic and induced electric fields over awide range <strong>of</strong> temporal frequencies (as high as 1-10kHz to as low as 0.1mHz), <strong>the</strong> electricalconductivity <strong>of</strong> <strong>the</strong> earth at a specific site can beinferred as a function <strong>of</strong> electromagnetic wavedepth penetration.An important aspect <strong>of</strong> MT data is that <strong>the</strong>measurements can register systematic aamplitude differences in electrical currentsrunning along fracture trends versus electricalcurrents running across fracture trends. Sincecurrents move more easily along fracture trends,<strong>the</strong> earth appears more conductive (less resistive)along fracture trends, and less conductive (moreresistive) across fracture trends. MT surveys,thus, are sensitive to a dual phenomenologyclosely relevant to fluids and fractures: over a range <strong>of</strong> (x,y) coordinates asequences <strong>of</strong> MT stations can seek outzones in which electrical currents flowbetter in one direction than <strong>the</strong>y do in <strong>the</strong>orthogonal direction; <strong>the</strong> same MT data can reveal <strong>the</strong>approximate depth to <strong>the</strong> current-flowdirectional anomalies by noting at whichMT field frequencies <strong>the</strong> anomalies firstoccur.Figure 6: Summary <strong>of</strong> 5km MT traverse <strong>of</strong> Krafla, Iceland,geo<strong>the</strong>rmal field. Central figure is deduced resistivitypr<strong>of</strong>ile beneath <strong>the</strong> survey traverse. Peripheral plots areresistivity depth pr<strong>of</strong>ile data in <strong>the</strong> form <strong>of</strong> measured MTfield resistivity versus MT field wavelength. Red curvesdenote data for electric currents along <strong>the</strong> traverse, bluecurves data for electric currents across <strong>the</strong> traverse. Leftends <strong>of</strong> resistivity curves are for shorter wavelengths(shallower depths), right ends for longer wavelengths(deeper depths). Divergence <strong>of</strong> blue/red curvesinterpreted as evidence that current-carrying alignedfractures run in/out <strong>of</strong> <strong>the</strong> section plane, with fracturesconcentrated in <strong>the</strong> volume denoted by <strong>the</strong> red oval at <strong>the</strong>base <strong>of</strong> <strong>the</strong> crustal section.Figures 6-7 illustrate <strong>the</strong> dual phenomenology <strong>of</strong>fracture-related MT surveys over a 5km crustalvolume enclosing <strong>the</strong> Krafla geo<strong>the</strong>rmal field <strong>of</strong>central Iceland (Malin et al 2009; Onacha et al<strong>2010</strong>). The Krafla field sits astride <strong>the</strong> NE-SWtrendingmid-Atlantic rift system as it passesthrough central Iceland. Figures 6-7 show that<strong>the</strong> geo<strong>the</strong>rmal activity along <strong>the</strong> rift system isgreatest where a shallow NW-SE trendingtectonic fault system intersects <strong>the</strong> NE-SW rifttrend.The MT surveyed Krafla crustal volume partitionsinto more resistive rock represented as coldcolours and more conductive rock represented aswarm colours. MT surveys across <strong>the</strong> volumereturn paired sequences <strong>of</strong> resistivity versusdepth pr<strong>of</strong>ile displayed as blue and red curves foreach MT station. The red curve measures <strong>the</strong>resistivity pr<strong>of</strong>ile parallel to <strong>the</strong> MT traverse; <strong>the</strong>blue curve measures resistivity normal to <strong>the</strong>traverse.Figure 6 summarises a rift-parallel SW-NW (leftright)MT traverse <strong>of</strong> <strong>the</strong> Krafla crustal volume.The leftmost survey station resistivity pr<strong>of</strong>ile isshown in <strong>the</strong> lower-left panel. The blue and redMT pr<strong>of</strong>ile curves do not diverge significantly asMT wavelength increases from left to right(shallow data register at left end <strong>of</strong> curve, deepdata register at right end <strong>of</strong> curve). A lack <strong>of</strong>systematic divergence between blue and redresistivity pr<strong>of</strong>ile curves persists over <strong>the</strong> nextthree MT stations moving clockwise from <strong>the</strong>154


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>lower-left panel. When, however, <strong>the</strong> MT surveymoves to <strong>the</strong> vicinity <strong>of</strong> <strong>the</strong> deep conductivityanomaly represented as <strong>the</strong> red oval at depth in<strong>the</strong> crustal section, <strong>the</strong> red and blue resistivitycurves begin to diverge with increasing MT signalwavelength. Relative to <strong>the</strong> electrical currentflowing in <strong>the</strong> plane <strong>of</strong> <strong>the</strong> traverse (red curve),<strong>the</strong> current flow in/out <strong>of</strong> <strong>the</strong> traverse planeincreases, hence <strong>the</strong> effective resistivity drops(blue curve). Except for <strong>the</strong> next station(presumably affected by <strong>the</strong> near-surface lowresistivity red zone), <strong>the</strong> blue-curve-lower-thanred-curveresistivity pr<strong>of</strong>ile relation persiststhrough <strong>the</strong> succeeding four survey stations, thusestablishing <strong>the</strong> existence <strong>of</strong> <strong>the</strong> buried red ovalhigh conductivity structure. This structure, givenby <strong>the</strong> blue resistivity pr<strong>of</strong>iles, defines a NE-SWtrending fracture/fault system intersecting <strong>the</strong> riftorientedNE-SW traverse plane.Figure 7: Map MT station resistivity depth pr<strong>of</strong>iledistribution for <strong>the</strong> Krafla, Iceland, geo<strong>the</strong>rmal field as inFigure 6. The upper-left and right-hand resistivity pr<strong>of</strong>ilesshow that electrical currents travelling NW-SW are strongalong <strong>the</strong> MT station sequence line, while <strong>the</strong> lower-leftresistivity pr<strong>of</strong>ile shows that away from <strong>the</strong> NW-SE line<strong>the</strong> NW-SE electrical currents are reduced. Byinference, <strong>the</strong> 3-station line locates a local fracture/fraulttrend; in <strong>the</strong> Krafla geo<strong>the</strong>rmal field this line collocateswith a known tectonic fracture trend.Figure 7 displays <strong>the</strong> Figure 6 resistivityphenomenology for a map distribution <strong>of</strong> MTstations. The NW-SE trend <strong>of</strong> 3 upper-left + righthandresistivity pr<strong>of</strong>ile panels defines <strong>the</strong> fracturetrend seen as <strong>the</strong> red high-conductivity feature atdepth in Figure 6. For each <strong>of</strong> <strong>the</strong> 3 MT stations,<strong>the</strong> blue resistivity curve diverges strongly from<strong>the</strong> red curve, indicating enhanced ability to carrycurrent along <strong>the</strong> NW-SE trend. In contrast, <strong>the</strong>lower-left MT station sees significantly smallerresistivity pr<strong>of</strong>ile divergence, implying that atdepth at this location <strong>the</strong>re is much reducedfracture alignment to carry electrical currents atdepth. Geologically, <strong>the</strong> 3-station NW-SE MTstation trend in Figure 7 collocates with a knownregional fault system normal to <strong>the</strong> NE-SWtrending rift system.Figure 8: (Upper) Seismicity at <strong>the</strong> Olkaria, Kenya,geo<strong>the</strong>rmal field; <strong>the</strong> NE-SW trends lie along <strong>the</strong> EastAfrica Rift; <strong>the</strong> NW-SE trends lie along a local tectonicfault feature; (centre) MT resistivity distribution summaryin which red/yellow tints denote areas <strong>of</strong> high/lowelectrical conductivity for <strong>the</strong> NW-SE aligned fractures;(lower) production well history along NE-SW rift trend,with lefthand well in yellow tint zone a poor producer andrighthand wells in red tint zone well above averageproducers.The three parts <strong>of</strong> Figure 8 summarise a similarfault-intersection phenomenology observed in <strong>the</strong>Olkaria, Kenya, East Aftrica rift systemgeo<strong>the</strong>rmal field (Simiyu & Malin 2000; Onacha etal 2009). The upper plot <strong>of</strong> Figure 8 seismicallydefines two fault trends, <strong>the</strong> NE-SW trend along<strong>the</strong> rift, and <strong>the</strong> NW-SE trend along a locallydefined tectonic fault. The centre plot is a155


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>composite rendering <strong>of</strong> MT survey data in whichred tints mark MT sites for which NW-SE riftnormalelectrical currents are strong while yellowtints mark MT sites where such electrical currentsare weak. The lower plot summarises <strong>the</strong>production well history: <strong>the</strong> lefthand well drilled in<strong>the</strong> yellow-tinted MT zone is a poor producer,while <strong>the</strong> two righthand wells drilled in <strong>the</strong> redtintedMT zone produce at double to triple <strong>the</strong> fieldaverage production rate.Summary/ConclusionsWe argue:well-log and well-core systematics showthat fracture systems are important,perhaps (probably?) crucial, conduits forge<strong>of</strong>luid flow on all scales in all rock, withparticular reference to aquifer rockcurrently targeted for heat extraction; power-law scaling well-log spectraindicate that small-scale rock samplesfundamentally do not represent <strong>the</strong> range<strong>of</strong> rock property fluctuations likely tooccur at large scale lengths; in absence <strong>of</strong> utility from small-scalesampling <strong>of</strong> rock properties, and in light<strong>of</strong> essentially unlimited fluctuations inrock properties on large scales, it islogical to consider large scale sampling<strong>of</strong> rock formations for information on insitu permeability; large scale measurements <strong>of</strong> fracturedistributions are particularly relevantwhere ge<strong>of</strong>luid flow rates are essential todrill hole success;in geo<strong>the</strong>rmal fields, where fractures arealmost universally acknowledged tocontrol ge<strong>of</strong>luid flow, MT resistivitypr<strong>of</strong>iles indicate that ge<strong>of</strong>luid flow isgreatest where known fracture/faulttrends intersect; enhanced productionwell flow has validated MT data as ageophysical guide to well siting.We conclude from <strong>the</strong>se arguments that MTsurveys <strong>of</strong> potentially exploitable hot aquifers area plausible investment in advance <strong>of</strong> costlydrilling.ReferencesClauser C, Marquart G, Rath V & MeProRiskWorking Group (<strong>2010</strong>) MeProRisk – a Tool Boxfor Evaluating and Reducing Risks inExploration, Development, and Operation <strong>of</strong>Geo<strong>the</strong>rmal Reservoirs, World Geo<strong>the</strong>rmalCongress, Bali April25-30 <strong>2010</strong>.Crude Oil Production and Crude Oil WellProductivity, 1954-2008www.eia.doe.gov/aer/txt/ptb0502.htmlde Graaf L, Palmer R & Reid I (<strong>2010</strong>) TheLimestone Coast Geo<strong>the</strong>rmal Project, SouthAustralia: a Unique Hot Sedimentary AquiferDevelopment, World Geo<strong>the</strong>rmal Congress, BaliApril25-30 <strong>2010</strong>.Dvorkin J (2009) Kozeny-Carman equationrevisited,pangea.stanford.edu/~jack/KC_2009_JD.pdfLeary P (2002) Fractures and physicalheterogeneity in crustal rock, in Heterogeneity<strong>of</strong> <strong>the</strong> Crust and Upper Mantle – Nature, Scalingand Seismic Properties, J. A. G<strong>of</strong>f, & K. Holliger(eds.), Kluwer Academic/Plenum Publishers,New York, 155-186.Leary PC & Walter LA (2008) Crosswell seismicapplications to highly heterogeneous tight-gasreservoirs, Special Topic on Tight Gas, FirstBreak 26, 33-39.Malin P, Leary P, Shalev E & Onacha S (2009)Joint Geophysical Imaging <strong>of</strong> PoropermDistributions in Fractured Reservoirs, GRCTransactions, Vol. 33, 4-7October 2009Mavko, G., and Nur, A., 1997, The effect <strong>of</strong> apercolation threshold in <strong>the</strong> Kozeny-Carmanrelation, Geophysics 62, 1480-1482.Onacha S, Shalev E, Malin P, & Leary P (2009)Joint Geophysical Imaging <strong>of</strong> Fluid-FilledFracture Zones in Geo<strong>the</strong>rmal Fields in <strong>the</strong>Kenya Rift Valley, GRC Transactions Vol. 33, 4-7October 2009Onacha S, Shalev E, Malin P, Leary P &Bookman L (<strong>2010</strong>) Interpreted FractureAnomalies: Joint Imaging <strong>of</strong> GeophysicalSignals from Fluid-Filled Fracture Zones inGeo<strong>the</strong>rmal Fields, <strong>Proceedings</strong> WorldGeo<strong>the</strong>rmal Congress, Bali, Indonesia, 25-29April <strong>2010</strong>Petroleum Economist (2009) Unlocking <strong>the</strong> value<strong>of</strong> <strong>the</strong> world's geo<strong>the</strong>rmal resources,www.petroleum-economist.comSimiyu S & Malin P (2000) A “volcano seismic”approach to geo<strong>the</strong>rmal exploration andreservoir monitoring: Olkaria, Kenya and CasaDiablo, U.S.A. World Geo<strong>the</strong>rmal Congress2000, Kyoto-Tohoku Japan, 1759-1763.Smith DN (1967) Well Completion ReportCockburn No. 1 Well, Western Australia, West<strong>Australian</strong> Petroleum Pty. LtdVogt C, Mottaghy D, Rath V, Wolf A, Pechnig R &Clauser C (<strong>2010</strong>) Quantifying Uncertainty inGeo<strong>the</strong>rmal Reservoir Modeling, WorldGeo<strong>the</strong>rmal Congress, Bali April25-30 <strong>2010</strong>.156


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Automatic Meshing and Construction <strong>of</strong> a 3D Reservoir System: FromVisualization towards SimulationYan Liu 1 , Huilin Xing 1,* , Zhenqun Guan 2 and Hongwu Zhang 21Earth Systems Science Computational Centre (ESSCC), The University <strong>of</strong> Queensland, St. Lucia, QLD4072, Australia;2 Department <strong>of</strong> Engineering Mechanics, State Key Laboratory <strong>of</strong> Structural Analysis <strong>of</strong> IndustrialEquipment, Dalian University <strong>of</strong> Technology, Dalian, China*Corresponding author: xing@esscc.uq.edu.auFinite Eleme nt Method (FEM) Geo computing i sincreasingly important in analysing and evaluatingenhanced g eo<strong>the</strong>rmal rese rvoirs. Due to <strong>the</strong>complexity <strong>of</strong> geologi cal objects, it is difficult tobuild a reasonable m esh fo r F EM. Thedevelopment <strong>of</strong> digital 3 D geolo gical modellingtools and ap plications (such as Ge oModeller andGoCad) makes it possible to establish geometricmodels for 3D geolo gical objects. Our wo rkfocuses on constructing a geoth ermal reservoi rsystem which transforms geometric models usedin 3D geological visualization into FEM models. A3D Geol ogical model for visuali zation i s use d asinput here, a nd <strong>the</strong> tran sformation processes areimplemented fo llowing: ( 1) g enerating atetrahedral mesh by 3D Delaun ay triangul ationmethods; (2) abstra cting boundaries o f differentgeological ob jects; (3) buil ding a well model bytetrahedral mesh refinement, which will be used infuture FEM-based simulations.Keywords: G eoModels; Delaunay Tria ngulation;3D geological modelling; FEM1. IntroductionIn <strong>the</strong> field <strong>of</strong> geoscie nce, modelling <strong>of</strong> geologicalobjects i s <strong>of</strong> great inte rest in visu alization an dsimulation. With <strong>the</strong> development <strong>of</strong> digital 3Dgeological modelling a pplications (su ch asGeoModeller and GoCad), 3D ge ological obje ctsincluding geological units, faults and ore depo sitscan b e ea sily built into GeoMo dels. However<strong>the</strong>se GeoModels a re mainly use d fo rvisualization, and lack topological relations whichare crucial in simulation. Topological query [1-3] isa co mmon i ssue which depends on topologicalrelations bet ween differe nt geologi cal object s.Fur<strong>the</strong>rmore, in <strong>the</strong> field <strong>of</strong> analysing, topolo gicalmodels which are suitable for simulating ar eurgently requ ested. Th e Finite Eleme nt Method(FEM), whi ch is base d on <strong>the</strong> FEM mesh, is a neffective mea ns <strong>of</strong> geo computing. Wh enever 3 Dgeological o bjects a re tra nsformed int o an FEMmesh such as a tetrahedral or hexahe dral grid ,FEM can b e employed to present simulations forfuture analy sing and eva luating. 3D Delaunaytriangulation (DT) [4, 5] is one well studied 3 Dtetrahedral m esh gen eration method, whi ch canbe utilized to transfo rm geometric geologicalmodels into FEM ones. Recently, regarding to DT,scientists [1, 6, 7] have wo rked o n modellin ggeological o bjects innovatively. Ledoux[6] used<strong>the</strong> dual <strong>of</strong> DT name d Voron oi Diag ram (VD) torepresent an d analyze o ceanographic dataset s.Ledoux [7] also compared <strong>the</strong> VT-b ased metho dwith geo graphical info rmation syste ms (GIS) an doutlined shortcomings <strong>of</strong> GIS and merits <strong>of</strong> <strong>the</strong> VDapproach. Pouliot [1] used DT to build t opologicalrelationships between geological objects.Our work focuse s on constructing a g eo<strong>the</strong>rmalreservoir sy stem by transfo rming geomet ricgeological models into a FEM mesh which will beutilized in simulation by FEM. Generally speaking,<strong>the</strong> output <strong>of</strong> geologi cal modelling tools can b eformed into a s et <strong>of</strong> triangles which respect <strong>the</strong>geometric pr<strong>of</strong>iles <strong>of</strong> g eological obje cts. Ta king<strong>the</strong>se tri angular surfaces as i nput, ourtransformation pro cess is outlined a s below: I nsection 2, au tomatic DT mesh g eneration base don 3D ge ological mod elling data, includin gboundary a bstraction o f different geologicalobjects. In section 3, one <strong>of</strong> <strong>the</strong> geological objectsis chosen to illustrate how to build a well modelbased o n te trahedral m esh refinem ent, and aboundary condition will be introduced for FEM i nfuture analy sing. Finally, con clusion a nd fur<strong>the</strong> rwork are discussed in section 4.2. Topological modelling for 3Dgeological objects2.1 3D geological objects data input andrefinementIn this paper, we choose outputs <strong>of</strong> s<strong>of</strong>tware suchas GeoModeller and GoCad as i nput data. It is aset <strong>of</strong> geological obje cts, including two fault sthrough different geolo gical units, as illu strated infigure 1. The model data are in <strong>the</strong> format <strong>of</strong> a set<strong>of</strong> triangula r facets which respe ct bou ndaries <strong>of</strong>different geol ogical obje cts. At <strong>the</strong> beginnin g <strong>of</strong>this file, node coordinate s are provided. And <strong>the</strong>nboundary tria ngular facets are pre sented by <strong>the</strong>indexes <strong>of</strong> nodes.157


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>To demon strate <strong>the</strong> effectivene ss <strong>of</strong> refiningboundaries o f <strong>the</strong> geol ogical m odel, a geologicalunit with larg e area but small thickn ess from ourgeological model is chosen to present ourapproach, a s illustrated in figure 3 (a). Afterperforming boundary re finement on it, largetriangular facets are b roken into smal l piece s;meanwhile, nodes o n its boun daries are denseenough to re present its g eometric feat ure in 3 Dgeological space, as shown in figure 3 (b).(a)Figure 1: Geological model from Geomodeller: (a)<strong>the</strong> whole model; (b) two faults in geological spaceAs our a pproach to extracting b oundariesbetween diffe rent g eological obje cts i s based o ndensity <strong>of</strong> bounda ry nodes, <strong>the</strong> geolo gical modelshould have a set <strong>of</strong> reasonable discretized nodeson its bo undaries. In o<strong>the</strong> r words, nodes used torepresent b oundaries <strong>of</strong><strong>the</strong> geol ogical mod elshould have a specified distance between eacho<strong>the</strong>r. This distance is defined as <strong>the</strong> p recision<strong>of</strong> our transforming process.The Edg e-splitting meth od, whi ch breaks atriangular e dge into two subo rdinate ones, isemployed to refine <strong>the</strong> i nitial geologi cal mod elboundaries. It is simple but effective, as illustratedin figure 2. The middl e point P <strong>of</strong> Edge AB isintroduced to split AB into two edges AP and PB.And <strong>the</strong>n tria ngles linke d with AB are sep aratedinto two triangles respectively.Figure 3: Refinement <strong>of</strong> geological objectboundaries: (a) before refining; (b) after refining.2.2 3D Delaunay triangulationAfter refining <strong>the</strong> bound aries <strong>of</strong> <strong>the</strong> geologicalmodel, nod es on bo undaries app ear with areasonable density due to a spe cified . In orderto distingui sh different parts <strong>of</strong> <strong>the</strong> geolo gicalmodel and construct a topological model for FEM,a tetrahed ral generatio n method should bepresented on <strong>the</strong> cu rrent boun dary n odes <strong>of</strong> <strong>the</strong>geological m odel. Beca use node s that are clo seto each o<strong>the</strong> r (whi ch re spect model bo undaries)are exp ected to con struct tetrahe drons, <strong>the</strong>n <strong>the</strong>Delaunay triangul ation method is adopte d togenerate <strong>the</strong> tetrahe dral mesh for <strong>the</strong> geolo gicalmodel.First <strong>of</strong> all, th e definition <strong>of</strong> Delaun ay triangulationis introduced below:Figure 2: Edge-splitting method: (a) beforesplitting; (b) after splitting158


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>{ PLet k}dbe a set <strong>of</strong> points in R . The Voronoi cellP<strong>of</strong>kVis kdefined byVk { p : p Pk p Pj, j k}{ V. k}forms<strong>the</strong> well-known Voronoi Tessellation <strong>of</strong> <strong>the</strong> entire{ Pdomain co ncerning k}. The Del aunay{ Ptriangulation <strong>of</strong> k}is defined as <strong>the</strong> du al <strong>of</strong> <strong>the</strong>Voronoi Tessellation; it wa s presented in 1930 byDelaunay, who found th e pro perty <strong>of</strong> emptycircumsphere crite rion. In <strong>the</strong> 3D d omain, <strong>the</strong>empty circumsphere criterion can be presented asbelow: for every tetrahedron <strong>the</strong>re are no verticesin its circum sphere except for <strong>the</strong> four vertices <strong>of</strong>its own. Then in 1981, Bo wyer[4] and Watson [5]proposed a method <strong>of</strong> this alg orithm, which i ssimple and efficient. The kernel <strong>of</strong> thi s method i sinserting points step by step. In order to k eep <strong>the</strong>empty circumsphere criterion, correct <strong>the</strong> topology<strong>of</strong> <strong>the</strong> mesh after inserti ng a point. Algorithm 1shows <strong>the</strong> ba sic procedures <strong>of</strong> this method usedin this paper.Algorithm 1: Classical 3D Delaunay triangulationStep 1: Construct a super tetrahedron, whichcontains all points prepared to beinserted. This super tetrahedron boundsa convex domain.Step 2: Insert a point into this convex domain, andextract all <strong>the</strong> tetrahedrons violating <strong>the</strong>empty circumsphere criterion.Step 3: Delete tetrahedrons extracted in Step 2,which leads to construction <strong>of</strong> a convexcavity. Use <strong>the</strong> inserted point to generatetetrahedrons with <strong>the</strong> surface <strong>of</strong> thiscavity.Step 4:Repeat Steps 2-3 until all <strong>the</strong> points areinserted.Step 2: Allocate each geological object auniversal ‘colour’, and calculate its volumeby its components (tetrahedral elements).Step 3: Sort geological objects by <strong>the</strong>ir volumes inan increasing order.Step 4: Extend geological objects to <strong>the</strong>irneighbours one by one, merging <strong>the</strong> gapgenerated by boundary facets.Step 5: Abstract facets shared by tetrahedronswith different colours.In our geolo gical sample, due to two faults, afterabstraction <strong>the</strong> wh ole m odel (a s illu strated i nfigure 4 (a)) is se parated into 25 com ponents (infigure 4 (b)), and colours <strong>of</strong> geological objects areupdated, so <strong>the</strong>y appea r with colou rs differe ntfrom o riginal ones. Boun daries b etween differe ntcomponents have a bstracted i n th e form <strong>of</strong>triangular f acets which co ntain topologi calrelationship informatio n. Becau se th e numbe r <strong>of</strong>boundary tri angular el ements i s to o huge tovisualize cle arly, only one <strong>of</strong> <strong>the</strong> 25 compone ntswhich is a corne r <strong>of</strong> <strong>the</strong> geologi cal model i sillustrated in <strong>the</strong> format <strong>of</strong> triang ular boundary, asshown in figure 4 (c). Fur<strong>the</strong> rmore, two faultsbreak <strong>the</strong> g eological mo del into three blocks, asshown in figure 4 (d) (e) and (f), which is useful forfur<strong>the</strong>r simulation and a nalysing. With <strong>the</strong> help <strong>of</strong><strong>the</strong> topologi cal model gen erated a bove, differentgeological objects can be easily identified and <strong>the</strong>generated tetrahedral mesh is an ideal model forFEM-based simulation.2.3 Abstra ction bou ndaries from differentgeological objectsAs 3 D DT tend s to ge nerate tetrahe drons bynodes close to each o<strong>the</strong>r, most <strong>of</strong> <strong>the</strong> triangulargeological surfaces will construct naturally during<strong>the</strong> process <strong>of</strong> DT. Mark facets which do not haveany edg es l onger tha n (which i s specified insection 2.1) boundaries. And <strong>the</strong>n use Algorithm 2to abstract boun daries <strong>of</strong> different geolo gicalobjects.Algorithm 2: Abstraction <strong>of</strong> geological objectboundariesStep 1: Roughly abstract geological objects in <strong>the</strong>form <strong>of</strong> tetrahedrons by facets which aremarked as boundaries.159


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Figure 4: Topological geological model afterabstraction based on DT: (a) <strong>the</strong> whole model; (b)components <strong>of</strong> geological model; (c) a componentvisualized in <strong>the</strong> form <strong>of</strong> grid; (d) left block <strong>of</strong>geological model; (e) middle block <strong>of</strong> geologicalmodel; (f) right block <strong>of</strong> geological model.3. Refining geological object andbuilding well modelIn <strong>the</strong> field <strong>of</strong> geo<strong>the</strong>rmal exploration, wells areessential facilities. Simulation based on FEMmethods re quests elem ents with small sizearound wells, which can enhance <strong>the</strong> accuracy <strong>of</strong>analysing. To meet this need, first <strong>of</strong> all, acomponent which i s suitable for drilling is chosenby experie nced en gineers (ta ke a componentwhich is far from faults for example, as i llustratedin figure 5 (a)), and <strong>the</strong>n <strong>the</strong> 3D geological modelis refined in <strong>the</strong> following steps: (1 ) choo se aparticular position which is prepared to create <strong>the</strong>well model, as shown in figure 5 (b); (2) refine <strong>the</strong>geological object no rmally, as sho wn in figure 5(c); (3) ac cording to a spe cified precision, restrict<strong>the</strong> element size aro und <strong>the</strong> well; (4 ) refine <strong>the</strong>well in th e g eological m odel ba sed o n eleme ntsize restriction, as shown in figure 5 (d). Finally, adesired tetra hedral mesh whi ch is u sed in futureFEM simul ation an d an alysing i s obta ined, an d<strong>the</strong> local tetrahedral mesh is illustrated in figure 5(e)(a)160


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>4. Conclusion and future workIn this paper, automatic meshing and construction<strong>of</strong> a ge o<strong>the</strong>rmal re servoir system is proposed,which focuses on tran sforming geometric modelsinto an FEM mesh. In order to make a genera linterface bet ween geolo gical s<strong>of</strong>twares (su ch a sGeomodeller and GoCa d) and <strong>the</strong> geo<strong>the</strong> rmalreservoir syst em, <strong>the</strong> input data are de signed in<strong>the</strong> form <strong>of</strong> a set <strong>of</strong> triangl es which pre sents <strong>the</strong>geometric features <strong>of</strong> <strong>the</strong> geological model. Thenin <strong>the</strong> process <strong>of</strong> tr ansforming, in put dat arefinement, tetrahedral mesh gen eration andgeological objects bou ndaries a bstraction a reperformed step by ste p, which focu ses o ngenerating a rea sonable FEM mesh. Finally, <strong>the</strong>well model use d in geo<strong>the</strong>rmal expl oration i sintroduced; automatic me sh gen eration for it isdemonstrated in detail. Our app roach presents away <strong>of</strong> using geological data for visualization toconstruct an F EM me sh for ge o<strong>the</strong>rmalsimulation.Fur<strong>the</strong>r works shoul d be done to enhance th eapproach proposed in this paper: in <strong>the</strong> first place,instead <strong>of</strong> a spe cified precision , bo undaryabstraction sho uld be i mproved to adaptivelydetect small features on geological models; in <strong>the</strong>second pla ce, as geol ogical mod els have bee ndivided into several pa rts, both parallel meshgeneration and FEM analysis should beconsidered.Figure 5: Building well model on particular geologicalobject for FEM analysing: (a) choosing geological object;(b) well location; (c) refining geological object; (d) buildingwell model; (e) local tetrahedral elements for well.AcknowledgementsSupport is g ratefully ac knowledged by <strong>Australian</strong>Research Council through ARC Discovery projectDP0666203, ARC Linkage Internatio nalLX0989423 and ARC Link age project LP0560932with colla boration <strong>of</strong> G eodynamics Li mited. Theauthors are grateful to Helen Gibson <strong>of</strong> IntrepidGeoscience for creatin g <strong>the</strong> 3D ge ological modelwith Geomodeller which used as <strong>the</strong> input data inthis paper.ReferencesPouliot, J., et al., Reasoning ab out geologi calspace: Coupling 3 D G eoModels a nd topologicalqueries a s an aid to spatial data selectio n.Computers & Geoscien ces, 2008. 34(5): p. 529-541.Apel, M., From 3d geomodelling systems towards3d geo science informatio n system s: Da ta model,query fu nctionality, and data ma nagement.Computers & Geoscien ces, 2006. 32(2): p. 222-229.James, W., et al., ADVISER: Immersive ScientificVisualization Applied to Mars Research a ndExploration. Photogra mmetric En gineering &Remote Sensing, 2005. 71(10): p. 1219-1225.161


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Bowyer, A., Computing Dirichlet tessellations. TheComputer Journal, 1981. 24(2): p. 162-166.Watson, D. F., Computi ng <strong>the</strong> n-d imensionalDelaunay tessellatio n with application to Vorono ipolytopes. The Computer Journal, 1981. 24(2): p.167-172.Ledoux, H. and C.M. Gold . A Voronoi-based mapalgebra. in Spatial Data Ha ndling—12thInternational Symposiu m on Spatial DataHandling. 2006: Springer.Ledoux, H. and C.M. Gold, Modellin g threedimensionalgeo scientific fields with <strong>the</strong> Voronoidiagram an d its dual. Internation al Journ al <strong>of</strong>Geographical Information Science, 2008. 22(4-5):p. 547-574.162


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Targeting Faults for Geo<strong>the</strong>rmal Fluid Production: Exploring for Zones<strong>of</strong> Enhanced PermeabilityLuke Mortimer 1,2 , Adnan Aydin 3 and Craig T. Simmons 21 Hot Dry Rocks Pty Ltd, PO Box 251, South Yarra, Victoria 31412 National Centre for Groundwater Research and Training, Flinders University, GPO Box 251, Adelaide, SouthAustralia 51003 Department <strong>of</strong> Geology and Geological Engineering, University <strong>of</strong> Mississippi, PO Box 1848, MS 38677, USAluke.mortimer@hotdryrocks.comFault structures can potentially deliver increasedgeo<strong>the</strong>rmal fluid production by boosting <strong>the</strong> bulkpermeability and fluid storage <strong>of</strong> a productionzone. However, <strong>the</strong> hydromechanical properties<strong>of</strong> faults are inherently heterogeneous andanisotropic, <strong>the</strong>reby, making it challenging todistinguish between permeable and impermeablefaults. This discussion paper outlines <strong>the</strong> keyfeatures that determine fault permeability and how<strong>the</strong> probability <strong>of</strong> locating zones <strong>of</strong> enhanced faultpermeability can be derived from preliminary faultstress state modelling. It is proposed thatpreliminary fault stress state modelling for earlystage exploration projects or in areas <strong>of</strong> unknownor complex geology can reduce <strong>the</strong> uncertaintyand risk <strong>of</strong> exploring for fault-related geo<strong>the</strong>rmaltargets.Keywords: geo<strong>the</strong>rmal, exploration, fault,permeability, in situ stress, hydromechanicalmodelling.IntroductionPermeable fault structures present an attractivegeo<strong>the</strong>rmal exploration target as faults have beenproven to boost substantially reservoirpermeability and fluid production at some existinggeo<strong>the</strong>rmal energy operations (e.g. Dixie Valley,USA; Landau, Germany). However, not all faultsare permeable. Their hydraulic properties areinherently heterogeneous and difficult tocharacterize, making it challenging to distinguishbetween faults acting as fluid conduits and fluidbarriers. This challenge is compounded when afault has no surface expression because toachieve sufficiently high production fluidtemperatures a fault typically must be intersectedat some depth where <strong>the</strong> exact hydrauliccharacter <strong>of</strong> <strong>the</strong> fault is unknown prior to drilling.Therefore, if exploring for permeable faultstructures <strong>the</strong> key questions are: (1) which fault orfault segment has <strong>the</strong> highest probability <strong>of</strong> beingpermeable?; and (2) what information is requiredto reduce <strong>the</strong> uncertainty and exploration risk priorto drill testing? To help answer <strong>the</strong>se questions<strong>the</strong> main objectives <strong>of</strong> this discussion paper are todescribe <strong>the</strong> key features that determine faultpermeability and how <strong>the</strong> probability <strong>of</strong> locatingzones <strong>of</strong> enhanced fault permeability may bederived from preliminary fault stress statemodelling. For illustrative purposes, hypo<strong>the</strong>ticalexamples <strong>of</strong> preliminary fault stress state modelsare provided.Targeting fault structures involves exploring atdepth for zones <strong>of</strong> enhanced natural in situfracture porosity and permeability to maximisegeo<strong>the</strong>rmal fluid production from a prospectivearea. A permeable fault target can be viewed asei<strong>the</strong>r: (1) having sufficient natural in situ porosityand permeability with natural fluid rechargeoccurring at <strong>the</strong> optimal fluid temperature (e.g.Dixie Valley, USA); or (2) as a zone <strong>of</strong> enhancedporosity and permeability that may still requiresome degree <strong>of</strong> reservoir stimulation (e.g.Landau, Germany).Two critical elements considered positive for faultpermeability targets are:(1) Favourable fault orientation with respect to <strong>the</strong>in situ stress field (i.e. ‘critically stressed’); and(2) Hydraulic contact with a significant volume <strong>of</strong>porous/fractured and permeable reservoir (i.e.fluid mass storage).For <strong>the</strong> latter, <strong>the</strong> fluid mass storage may beprovided by <strong>the</strong> fault structure itself or anadjoining and hydraulically connected rock unitsuch as thick, porous sandstone. Fluidoverpressures associated with <strong>the</strong> fault may alsobe beneficial for fluid advection along <strong>the</strong>structure from a connected, deeper andpotentially hotter reservoir and for lowering <strong>the</strong>effective stress state <strong>of</strong> <strong>the</strong> fault.Fault Architecture and HydrogeologyThe architecture <strong>of</strong> a fault structure can varygreatly in form from simple faults where strain isaccommodated along a narrow plane to morecomplex structures where strain is distributed overa composite zone that may include numerousfaults, small fractures, veins, breccias andcataclastic gouge. Generally, fault structures aresubdivided into two simple components being <strong>the</strong>fault core and <strong>the</strong> fault damage zone both <strong>of</strong>which may vary over widths ranging fromcentimetres to hundreds <strong>of</strong> metres (Figure 1;Caine and Forster, 1999; Gudmundsson et al.,2009). These two components are distinguishableby <strong>the</strong>ir distinct mechanical and hydrogeologicalproperties although <strong>the</strong>se are inherentlyheterogeneous and can vary significantly along afault. The fault core refers to <strong>the</strong> main fault planethat takes up most <strong>of</strong> <strong>the</strong> displacement and where163


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong><strong>the</strong> original lithology has been altered throughfault-related processes such as grain sizereduction, hydro<strong>the</strong>rmal alteration and mineralprecipitation in response to mechanical and fluidflow processes (Caine and Forster, 1999). Thecharacter <strong>of</strong> <strong>the</strong> fault core zone is stronglydependent on its protolithology (Caine andForster, 1999). Fault damage zones are definedas <strong>the</strong> adjacent network <strong>of</strong> subsidiary structuresincluding small faults, fractures, veins, cleavage,pressure solution seams and folds that laterallydecrease in density away from <strong>the</strong> fault core zone(Figure 1; Caine and Forster, 1999;Gudmundsson et al., 2009)Figure 1. Illustrative schematic diagram <strong>of</strong> a fault including itsfault core and damage zone. From Gudmundsson et al.(2009).The permeability <strong>of</strong> faults can vary considerablyranging from impermeable flow barriers tosignificant flow conduits with a high degree <strong>of</strong>spatial heterogeneity and anisotropy. Generally,faulting in low porosity, competent rock isexpected to result in an increase in fault zonepermeability whilst faulting in high porositysedimentary rocks may lead to a generaldecrease in fault zone permeability throughcommunition and porosity reduction processessuch grain-size reduction and <strong>the</strong> formation <strong>of</strong>clay-rich fault gouge and deformation bands(Zoback, 2007; Wong and Zhu, 1999). Commonly,fault cores are <strong>of</strong> a relatively lower permeabilitythan <strong>the</strong>ir associated damage zones, which isattributed to porosity reducing processesoccurring within <strong>the</strong> cores (Caine et al., <strong>2010</strong>). Forexample, at <strong>the</strong> Mirrors site, Dixie Valleygeo<strong>the</strong>rmal field, measured core plugpermeabilities ranged from 10 -8 m 2 (10 7 mD) infault damage zones to 10 -20 m 2 (10 -8 mD) in faultcores, however, <strong>the</strong> bulk permeability <strong>of</strong> <strong>the</strong> faultzone is on <strong>the</strong> order <strong>of</strong> 10 -12 m 2 (1000 mD) (Caineand Forster, 1997; Seront et al., 1998). In terms <strong>of</strong>anisotropy, <strong>the</strong> permeability tensor is expected tobe at a maximum parallel to <strong>the</strong> fault, intermediatedown dip <strong>of</strong> <strong>the</strong> fault plane and at a minimumperpendicular to <strong>the</strong> fault, which allows for bothvertical and lateral flow but may limit cross-faultflow (Ferrill et al., 2004). Faults <strong>of</strong> sufficiently highpermeability can also contribute significantly toboth local and regional scale coupledgroundwater flow and heat transport viaadvection/convection processes (e.g. Bachler etal., 2003).Stress-Dependent Fault PermeabilityStress acting on a fault plane can be resolved intonormal and shear stresses, which are <strong>the</strong>components <strong>of</strong> stress that act normal and parallelto a plane, respectively. In nature, <strong>the</strong>se stressesare highly coupled and can cause faults toundergo reactivation and deform. The linkbetween stress, fracture deformation andpermeability is such that as fracture voidgeometries and <strong>the</strong> connectivity <strong>of</strong> a flow networkchange in response to changing in situ stress, <strong>the</strong>storage, permeability and flow pattern is alsoexpected to change in magnitude, heterogeneityand/or anisotropy. Fracture deformation can resultin significant changes in permeability and storagebecause <strong>the</strong> ability <strong>of</strong> a fracture to transmit a fluidis extremely sensitive to its aperture. Forexample, <strong>the</strong> transmissivity <strong>of</strong> an individualfracture (T f ) idealised as an equivalent parallelplate opening can be expressed as:3(2b) gT f =(1)12Where 2b is <strong>the</strong> fracture aperture width (m), is<strong>the</strong> fluid density (kg.m -3 ), g is gravitationalacceleration (m.s -2 ) and μ is <strong>the</strong> dynamic viscosity<strong>of</strong> <strong>the</strong> fluid (kg.m -2 .s).One key aspect <strong>of</strong> exploring for permeable faultsis <strong>the</strong> <strong>the</strong>ory <strong>of</strong> stress-dependant fracturepermeability in deep-seated, fractured rocks. This<strong>the</strong>ory is supported by studies relating tohydrocarbon and geo<strong>the</strong>rmal reservoirs andstudies <strong>of</strong> potential nuclear waste repository sites(e.g. Finkbeiner et al., 1997; Gentier et al., 2000;Hudson et al., 2005). The <strong>the</strong>ory is that in situstress fields exert a significant control on fluid flowpatterns in fractured rocks, particularly, for rocks<strong>of</strong> low matrix permeability. For example, in a keystudy <strong>of</strong> deep (>1.7 km) boreholes, Barton et al.(1995) found that permeability manifests itself asfluid flow focused along fractures favourablyaligned within <strong>the</strong> in situ stress field, and that iffractures are critically stressed this can impart asignificant anisotropy to <strong>the</strong> permeability <strong>of</strong> afractured rock mass. Critically stressed fracturesare defined as fractures that are close to frictionalfailure within <strong>the</strong> in situ stress field (Barton et al.,1995). Specifically, <strong>the</strong> <strong>the</strong>ory <strong>of</strong> stress-dependentfracture permeability predicts preferential flowoccurring along fractures that are orientedorthogonal to <strong>the</strong> minimum principal stress (σ 3 )direction (due to low normal stress), or inclined164


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>~30° to <strong>the</strong> maximum principal stress (σ 1 )direction (due to shear dilation).Frictional sliding along a plane <strong>of</strong> weakness suchas a fault occurs when <strong>the</strong> ratio <strong>of</strong> shear (τ) to <strong>the</strong>effective normal stress (σ’ n ) equals or exceeds <strong>the</strong>frictional sliding resistance. It is based uponAmonton’s Law, which governs fault reactivation:τ = μ.σ’ n (2)Where μ is <strong>the</strong> coefficient <strong>of</strong> friction (a rockmaterial property) and σ’ n is equal to <strong>the</strong> totalapplied normal stress resolved onto <strong>the</strong> planeminus <strong>the</strong> pore fluid pressure (i.e. σ n – P P ). Thevalue <strong>of</strong> μ has been found to typically rangebetween 0.6 and 1.0 (Byerlee, 1978; Zoback,2007). This relationship also shows that pore fluidpressure can have a significant impact as itdetermines <strong>the</strong> effective stress acting on a planeand that increasing pore pressures can destabilisea fault surface by increasing <strong>the</strong> ratio <strong>of</strong>shear to normal stress. The coupling <strong>of</strong> <strong>the</strong>sehydromechanical (HM) processes means that fluidpressure and flow within faults is linked to tectonicstress and deformation through changes inpermeability and storage whilst tectonic stressand deformation is linked to fluid flow throughchanges in fluid pressure and effective stress(NRC, 1996).How exactly a fault will behave under an appliedstress regime depends upon many factors,however, investigating stress-dependent faultpermeability based solely on fault alignment withrespect to <strong>the</strong> in situ stress field is anoversimplification. Just as important are <strong>the</strong>geomechanical properties <strong>of</strong> <strong>the</strong> host rock and itscontained faults. Important intact rock materialproperties include parameters such as density,bulk moduli, uniaxial compressive strength, tensilestrength, cohesion and friction angle that aretypically estimated from laboratory tests. Fracturestiffness is a function <strong>of</strong> both fracture wall surfacecontact (i.e. fracture roughness pr<strong>of</strong>ile) and <strong>the</strong>elastic properties <strong>of</strong> <strong>the</strong> intact rock material (i.e.bulk rock moduli) where for <strong>the</strong> same givenalignment within an in situ stress field relativelystiff fractures deform less than weaker fractures.Fracture normal and shear stiffness are measures<strong>of</strong> resistance to deformation perpendicular andparallel to fracture walls, respectively, and bothincrease with increasing effective normal stress.In general, faults tend to exhibit high stiffness ifformed within hard, competent rocks or if <strong>the</strong>ybecome locked open by earlier deformationepisodes (e.g. shear dislocation) or mineral infilland cementation, and may even become stressinsensitive even if subjected to high effectivenormal stresses (Hillis, 1998; Laubach et al.,2004). In contrast, low stiffness faults can exhibita wide range <strong>of</strong> shear and closure behaviour as<strong>the</strong>ir alignment with respect to σ 1 changes (Hillis,1998). Ultimately, estimates <strong>of</strong> fracture stiffnessattempt to account for more realistic fractureheterogeneity, asperity contact, deformation andtortuous fluid flow. Equations 3 & 4 belowdescribe <strong>the</strong> simplified relationship betweenfracture stiffness and fracture deformation(Rutqvist and Stephannson, 2002):Δμ n = jk n Δσ’ n (3)Δμ s = jk s Δσ s (4)Which states (a) that fracture normal deformation(Δμ n ) occurs in response to changes in effectivenormal stress (Δσ’ n ) with <strong>the</strong> magnitude <strong>of</strong>opening or closure dependent upon fracturenormal stiffness (jk n ); and (b) that <strong>the</strong> magnitude<strong>of</strong> shear mode displacement (Δμ s ) depends upon<strong>the</strong> shear stiffness (jk s ) and changes in shearstress (Δσ s ).Structural permeability within faults is likely to bea transient effect as faults <strong>of</strong>ten become modifiedby porosity reducing processes such ashydro<strong>the</strong>rmal mineralisation, hence, faultdeformation processes compete with permeabilityreduction caused by fluid flow (Sibson, 1996;Zoback, 2007). Active fault slip is typicallyepisodic and can temporarily increase <strong>the</strong>permeability <strong>of</strong> a fault zone by as much as manyorders <strong>of</strong> magnitude (Gudmundsson, 2000).Therefore, for faults to remain effective permeablestructural conduits fault deformation processesmust be at least intermittent to continual. Forexample, in <strong>the</strong> Dixie Valley geo<strong>the</strong>rmal field fluidproduction is sourced from high permeabilityfaults and fractures that are favourably alignedand critically stressed whilst it is inferred that <strong>the</strong>formation <strong>of</strong> fault permeability associated withactive deformation out competes permeabilitydestroying hydro<strong>the</strong>rmal quartz precipitationprocesses (Zoback, 2007).Preliminary Modelling <strong>of</strong> Fault StressStatesThe numerical modelling <strong>of</strong> fault stress states haspreviously been employed by several researchersto identify zones <strong>of</strong> potential fault enhancedpermeability and fluid flux (e.g. Ferrill et al., 2004;Gudmundsson, 2000; Moeck et al., 2009; Zhangand Sanderson, 1996). In a similar methodology,this study uses <strong>the</strong> Universal Distinct ElementCode (UDEC) to simulate <strong>the</strong> coupled HMresponse <strong>of</strong> deformable faulted rock massesunder an applied in situ stress field to derivepreliminary indications <strong>of</strong> fault stress states and,by corollary, <strong>the</strong>ir potential permeability. UDECrepresents a rock mass as an assembly <strong>of</strong>discrete rigid or deformable, impermeable blocksseparated by discontinuities (faults, joints etc) andcan reproduce fully coupled HM behaviour(Itasca, 2004). Fluid pressure and fractureconductivity is dependent upon mechanicaldeformation whilst simultaneously fluid pressures165


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>modify <strong>the</strong> mechanical behaviour <strong>of</strong> <strong>the</strong> fractures(for a comprehensive review <strong>of</strong> <strong>the</strong> UDECgoverning equations see Itasca, 2004). The 2.5DUDEC models describe a geometricalreconstruction that consist <strong>of</strong> 2D horizontal planaror vertical slices <strong>of</strong> <strong>the</strong> conceptual faulted rockmass model and incorporates <strong>the</strong> effects <strong>of</strong> <strong>the</strong>3D stress field (i.e. V , H , and h ). That is, <strong>the</strong>models perform plane strain analyses, whichassumes that <strong>the</strong> model continues indefinitely(and uniformly) out <strong>of</strong> <strong>the</strong> plane <strong>of</strong> analysis withcomputations performed for a slice that is one unitthick (Itasca, 2004). The ultimate aim <strong>of</strong> this type<strong>of</strong> modelling is to distinguish which fault or faultsegments in a specified area are criticallystressed and, <strong>the</strong>refore, a potential explorationdrill target. These models are designed to assistexplorers in areas <strong>of</strong> unknown or complexgeology prior to drilling, however, large modelparameter uncertainties means that <strong>the</strong> resultsare preliminary indications only i.e. a ‘probabilistic’representation <strong>of</strong> potential fault stress states.To illustrate this methodology, three hypo<strong>the</strong>ticalgeological models are presented based upon <strong>the</strong>nor<strong>the</strong>rn Perth Basin as an example setting. Thisinvolves a strike-slip faulting stress regime, stresstensor H > V > h equivalent to 1.25 : 1.0 : 0.75and an east-west principle horizontal stress ( H )orientation (King et al., 2008; van Ruth, 2006). For<strong>the</strong> purposes <strong>of</strong> this illustrative exercise, rockmass parameters (e.g. density, bulk modulus etc)were sourced from <strong>the</strong> UDEC rock propertydatabase although, where possible, <strong>the</strong>se shouldbe based upon measured representative fieldsamples or at <strong>the</strong> very least global averagevalues. The most difficult part <strong>of</strong> this process isassigning fault stiffness values, particularly, as<strong>the</strong>y are expected to vary with host lithology. Asfracture stiffness is a function <strong>of</strong> wall contact area,<strong>the</strong> jk n for smooth planar surfaces canapproximate <strong>the</strong> value <strong>of</strong> <strong>the</strong> Young’s Modulus (E)whereas <strong>the</strong> jk s , for perfectly matching roughsurfaces, can approximate <strong>the</strong> value <strong>of</strong> <strong>the</strong> ShearModulus (G). At shallow depths, estimates can bederived based upon jk n ranging from 1/2 (smooth)to 1/10 (rough) <strong>the</strong> value <strong>of</strong> E and jk s ranging from1/2 (rough) to 1/10 (smooth) <strong>the</strong> value <strong>of</strong> G, whichare compatible with published data and thosederived from empirical relationships (Kulhawy,1978; Norlund et al., 1995). However, prior to drilltesting <strong>the</strong> true nature <strong>of</strong> <strong>the</strong> fault at depth isunknown. As <strong>the</strong> aim is to attempt to evaluaterelative fault stress states, possibly acrossmultiple faults and lithologies, a ‘smooth’ faultstiffness for each respective lithology was chosenalong with zero tensile strength, cohesion anddilation angle values. In <strong>the</strong>ory, <strong>the</strong>segeomechanical properties replicate <strong>the</strong> behaviour<strong>of</strong> a ‘weak’ fault plane, which allows each faultsegment to potentially deform. This is areasonable approach as most active fault zonesare inferred to be weak (Gudmundsson et al.2001; Gudmundsson et al. 2009).The three hypo<strong>the</strong>tical geological model examplesare:Model 1: 4km x 4km horizontal planar model setat -3.5 km depth below <strong>the</strong> surface comprising <strong>of</strong>a single fault with jog hosted within sandstone(Figure 2).Model 2: 5km x 5km cross-section <strong>of</strong> a listric faulthosted with a sedimentary sequence comprising<strong>of</strong> limestone (surface-1km depth), siltstone (1km-2.5km depth), shale (2.5km-3.5km depth),sandstone (3.5km-4km depth) and granite (4km–5km depth) (Figure 3).Model 3: 4km x 4km horizontal planar model setat -3.5 km depth below <strong>the</strong> surface comprising <strong>of</strong>a central, circular, granite batholith <strong>of</strong> 1km radiushosted within a weak shale unit plus three crosscuttingfaults <strong>of</strong> differing orientation (Figure 4).In <strong>the</strong>se models, rock mass deformation wasdefined by <strong>the</strong> Mohr-Coulomb model, which is <strong>the</strong>conventional model used to represent shearfailure in rocks and soils whilst fracture behaviourwas defined by <strong>the</strong> Coulomb-Slip criterion, whichassigns elastic stiffness, tensile strength,frictional, cohesive and dilational characteristics toa fracture (Itasca, 2004). Mechanical boundarieswere defined as fixed velocity (displacement)boundaries and initial in situ and boundary fluidpore pressures are assumed hydrostatic.SandstoneFigure 2. Model 1: 4km x 4km horizontal planar contour map<strong>of</strong> x-direction stress magnitudes highlighting <strong>the</strong>concentration <strong>of</strong> high and low stress zones into quadrantsalong <strong>the</strong> fault jog. This highlights that although faultalignment maybe favourable stress-dependent faultpermeability can be segmented and localised. Note that <strong>the</strong>principle stress (σH) direction is east-west (right-left).Legend: purple, red, brown, green and yellow coloursrepresent a decreasing range <strong>of</strong> high to low stressmagnitudes, respectively.166


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>SandstoneGraniteLimestoneSiltstoneShaleFigure 3. Model 2: 5km x 5km vertical cross-section pr<strong>of</strong>ile <strong>of</strong>contoured y-direction stress magnitudes highlighting alocalised low stress field perturbation closely associated with<strong>the</strong> trace <strong>of</strong> <strong>the</strong> listric fault. This indicates low fault planestress and potentially enhanced fault permeability. Note that<strong>the</strong> principle stress (σH) direction is east-west (right-left).Legend: purple, red, brown, green and yellow coloursrepresent a decreasing range <strong>of</strong> high to low stressmagnitudes, respectively.Granite(circle)ShaleFigure 4. Model 3: 4km x 4km horizontal planar contour map<strong>of</strong> x,y-direction stress magnitudes highlighting a criticallystressed fault intersection (red) which potentially represents<strong>the</strong> location <strong>of</strong> enhanced fault permeability. This intersectionis also coincident with a low stress anomaly in <strong>the</strong> x- and y-direction. Note that <strong>the</strong> principle stress (σH) direction is eastwest(right-left). Legend: purple, red, brown, green andyellow colours represent a decreasing range <strong>of</strong> high to lowstress magnitudes, respectively.ConclusionThe risks <strong>of</strong> targeting permeable faults asgeo<strong>the</strong>rmal reservoirs include: (1) a relatively highpermeability structure may result in fluid pathwayshort-circuiting and accelerated rates <strong>of</strong> reservoir<strong>the</strong>rmal drawdown; (2) multiple fault structureswith varying amounts <strong>of</strong> displacement maytruncate and compartmentalise a reservoir<strong>the</strong>reby reducing accessible reservoir volume;and (3) <strong>the</strong> targeted fault structure may still behydraulically sealed and/or stress insensitive as aresult <strong>of</strong> o<strong>the</strong>r competing natural processes.These risks can be partially mitigated throughinterpretation <strong>of</strong> good quality seismic reflectiondata and with direct drill testing. The fault stressstate models shown in this discussion paper aredeliberately simplistic but specifically designed todemonstrate how this method can be used toidentify zones <strong>of</strong> potentially enhanced faultpermeability prior to any drill testing in areas <strong>of</strong>unknown or complex geology. This method maybe <strong>of</strong> benefit to <strong>the</strong> <strong>Australian</strong> geo<strong>the</strong>rmalexploration sector as target depths are typically inexcess <strong>of</strong> 3 km depth below <strong>the</strong> surface wherenatural in situ porosity and permeability aretypically low and <strong>the</strong>re is a general paucity <strong>of</strong>data.Never<strong>the</strong>less, it is important to note that <strong>the</strong>results <strong>of</strong> such preliminary models can onlyindicate <strong>the</strong> probability <strong>of</strong> encountering enhancedfault permeability and that <strong>the</strong>se 2D modelssimplify <strong>the</strong> 3D reality. It could be argued thatsimply evaluating targets on structural alignmentrelationships within <strong>the</strong> in situ stress field alonemight be sufficient, however, in complex areasthis would neglect <strong>the</strong> influence <strong>of</strong> features suchas multiple rock competency and fault stiffnesscontrasts and fault intersections on perturbing <strong>the</strong>local stress field. The results <strong>of</strong> <strong>the</strong>se numericalmodels are only as accurate as <strong>the</strong> quality <strong>of</strong> <strong>the</strong>input data and this particular methodology caninclude a significant amount <strong>of</strong> model parameteruncertainty (e.g. fault stiffness, estimated orinferred stress field etc). Therefore, thismethodology should be viewed as just one toolthat can form part <strong>of</strong> a broader exploration riskmanagement strategy.ReferencesBachler, D., Kohl, T., and Rybach, L., 2003,Impact <strong>of</strong> graben-parallel faults on hydro<strong>the</strong>rmalconvection-Rhine Graben case study: Physicsand Chemistry <strong>of</strong> <strong>the</strong> Earth, 28, 431-441.Barton, C.A., Zoback, M.D. and Moos, D., 1995,Fluid flow along potentially active faults incrystalline rock: Geology, 23, 683-683.Byerlee, J.D., 1978, Friction <strong>of</strong> rocks: Pure andApplied Geophysics, 116, 615-626.167


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Caine, J.S. and Forster, C.B., 1997, Fault zonearchitecture and fluid flow. An example from DixieValley, Nevada: <strong>Proceedings</strong> 22 nd Workshop onGeo<strong>the</strong>rmal Reservoir Engineering, StanfordUniversity, Stanford, California.Caine, J.S. and Forster, C.B., 1999, Fault zonearchitecture and fluid flow: insights from field dataand numerical modelling, Faults and SubsurfaceFluid Flow in <strong>the</strong> Shallow Crust: AmericanGeophysical Union, Geophysical Monograph 113,101-127.Caine, J.S., Bruhn, R.L. and Forster, C.B., <strong>2010</strong>,Internal structure, fault rocks and inferencesregarding deformation, fluid flow, andmineralisation in <strong>the</strong> seismogenic Stillwaternormal fault, Dixie Valley, Nevada: Journal <strong>of</strong>Structural Geology. In Press.Ferrill, D.A., Sims, D.W., Waiting, J.W. 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<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>An EGS/HSA concept for SingaporeGrahame J.H. OliverDepartment <strong>of</strong> Civil Engineering, National University <strong>of</strong> Singapore.cvegjho@nus.edu.sgAbstractHot springs are a good indicator for geo<strong>the</strong>rmalresources i n Singap ore. An Enginee redGeo<strong>the</strong>rmal System (EG S) for com mercialpower gene ration would requi re 3 km deepdirectional wells in h ot sedimenta ry a quifers(HSA) or in hot, wet, fract ured granite and <strong>the</strong>generation o f electricity from +1 50 o C hotwater through binary c ycle turbines with <strong>the</strong>‘waste’ wate r being recy cled do wn i njectionwells. Pro<strong>of</strong> <strong>of</strong> concept for a 50 MW powe rstation might cost US$ 19 million. Developmentcosts (US$ 200 million) could be written <strong>of</strong>f in6.4 years after produ ction sta rted. Largecorporations and <strong>the</strong> military could benefit fromautonomous geo<strong>the</strong> rmal power sou rces (e.g.electricity, h eat proces sing, dist rict cooling).Several n eighbourhood 5 0 MW geo<strong>the</strong>rmalpower statio ns could provide p art <strong>of</strong> <strong>the</strong>national b ase load with ‘rene wable’, clean,green po wer g eneration <strong>of</strong> st rategicimportance for a country that is vie wed ashaving no natural resources.Keywords: Concept, EGS, Singapore.IntroductionSixty million peopl e living on plate boundariesaround <strong>the</strong> world already obtain <strong>the</strong>ir electricityfrom hydro<strong>the</strong>rmal sources in young m agmaticrocks. Many commentators see <strong>the</strong> return <strong>of</strong><strong>the</strong> US$100-plus barrel <strong>of</strong> crude oil with futuregas prices tracking that rise. Eighty perc ent <strong>of</strong>Singapore’s electri city is gene rated fromimported nat ural ga s. Ge o<strong>the</strong>rmal exp loration<strong>of</strong> bu ried ho t gra nite te rrains i n continentalinteriors is now attrac tive: in Aust ralia andAlaska, EGS exploration has now passed into<strong>the</strong> develo pment pha se. Australia n StateGovernments have commi tted US$ 90 millionfor re search and demo nstration a nd ano<strong>the</strong>rUS$ 7 50 mill ion h as been allo cated to wo rksprograms for <strong>the</strong> perio d 2002 a nd 20 13 (1) . InMay 2009, t he US G overnment anno unced aUS$ 350 million stim ulus boost for USgeo<strong>the</strong>rmal energy (2) .The main heat releasing isotopes in rocks are235 U, 238 U, 232 Th and 40 K. Granites usuallyhave more <strong>of</strong> <strong>the</strong>se el ements than m ost o<strong>the</strong>rrocks. Granites with more than 1 0 ppm U canbe classified as “h ot” and provided <strong>the</strong> granitehas b een allowed to hea t itself up under a<strong>the</strong>rmal blanket <strong>of</strong> overlying rocks, signi ficantlyhigh temperatures can build up over millions <strong>of</strong>years. New tech nology mean s th at boilinggeo<strong>the</strong>rmal water or steam is not required. Thecommercial binary cycle Chena Power Stationin Alaska bo ils R-134a refrige rant with 74 o Cgeo<strong>the</strong>rmal water extracted from Me sozoic hotgranite, and pro duces 2 -300 kWh at US 5cents/kWh (3) . This is i n contrast to th e US 30cents/kWh cost <strong>of</strong> diesel generators previouslyused at Ch ena (3) . The Geysers re gion inCalifornia gene rates electri city at 5cents/kWh (4) . US 5 cents/kWh i s competitiveagainst all forms <strong>of</strong> po wer gene ration exceptfor coal.Geology and hot springs <strong>of</strong>SingaporeSingapore l ies in side <strong>the</strong> stable Asia ncontinental plate called Sundaland. The islandis co mposed mainly <strong>of</strong> Middle Tri assic I-Typegranite an d minor ga bbro, intrude d int o a kmthick bla nket <strong>of</strong> contem porary a cid v olcanicsand p artly covered by Upp er T riassic andLower Jurassic se diments (Fig. 1). Th ere a rethree confirmed hot sprin gs situated at or ne ar<strong>the</strong> coasts (although <strong>the</strong> precise locality <strong>of</strong> <strong>the</strong>one on <strong>the</strong> SW side <strong>of</strong> Pulau Te kong isuncertain b ecause <strong>of</strong> land reclamation).Seeping “steam” (sic) has been reported to mebut not conf irmed from ano<strong>the</strong>r loca tion onSembawang Singapore Air Force base (Fig. 1).The best known hot spring at Sembawang hasbeen d rilled down to 100 m into a 50 m widefault zone in granite: temperatures <strong>of</strong> 7 0.2 o Cwere m easured (Zha o et al. 2002 ). Chemicalanalyses cl assify it a s a p otable neutralchloride spring with total dissolved solids (TDS)measured at 914 mg/l and a Cl content <strong>of</strong> 43 1mg/l (Zhao et al. 2002). I have applied variousgeochemical <strong>the</strong>rmom eters (li sted in Bowen1986) using Si, Na, K, Ca concentrations listed169


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Geology <strong>of</strong> Singapore with hot and cold springsSingaporeterritory10 kmBukit Temahalt 164 mSteamseep?CC ColdSprings24-26 o CKR+UWC+ MFSI+TanjongLokosSembawang70 o CBoreholeSpringsHotColdP. Tekong,~70 o C?Alt 47 mLineamenttrend = 35 o EGeologyGraniteGabbroVolcs &sedsJurongFmOldAlluviumYoungAlluviumLineament trend (35 o E) drawn from geology maps andsatellite images. SI = Sentosa Island. UWC = United WorldCollege. CC = Central Catchment. MF = Mt Faber. KR =Kent RidgeN = 93Figure. 1: Geology map <strong>of</strong> Singapore (after Lee and Zhou 2009)in Zhao et al. (200 2) which i ndicateunderground rese rvoir te mperatures between122 a nd 209 o C: Na/K <strong>the</strong>rmometers givetemperatures <strong>of</strong> ~160 o C.Granite be drock is not n ormally con sidered tobe permeable unless it is well fractured, jointedand faulted. I have investigate d <strong>the</strong> granitequarries a round Bu kit Te mah an d Pul au Ubinand close spaced joi nting is common. Coldsprings occur around Bukit Tema, United WorldCollege and Sentosa Island (Fig. 2).DairyFarmLittleGuilinRose diagrams <strong>of</strong> vertical joint andlineament orientationsN N12 o E35 N25 o Eo EDairyFarmLoc A,n = 41Loc An = 27LittleGuilinLocLoc B,n = 43Loc Bn = 70Figure 2: Structural data from quarriesDairy FarmSingaporelineamentmap N = 93105 o EStrongly jointed graniteThe average maximum horizontal stress (sigma1) in ~100 m boreholes in central Singaporehas a 1 3 o E orie ntation (Zh ou 2001). Myanalysis <strong>of</strong> t he stress ve ctors in <strong>the</strong> Sumatrasection <strong>of</strong> th e Aust ralian Plate colli sion in th eSumatra-Java tren ch and sub duction zone to<strong>the</strong> SW <strong>of</strong> Singapore, sugge sts t hat <strong>the</strong>maximum hor izontal stress in <strong>the</strong> ha ngingwall<strong>of</strong> <strong>the</strong> su bduction zone is oriente d 40 o E. Thepresent day stress map <strong>of</strong> SE Asia (5) , based onearthquake fault sol utions a nd boreholebreakouts and fra ctures, sho ws th at <strong>the</strong>maximum horizontal stress is orientated 40 o E inneighbouring Sumatra. Fur<strong>the</strong> rmore, mylineament map <strong>of</strong> Si ngapore, based ontopography, geolo gical m ap and satell ite datashows a very strong NE/ SW trend (3 5 o E, seeFigs. 1 and 2).The important implication is thatany joints (<strong>of</strong> whatever age) that are orientatedNE/SW could be open in this stress regime andwould b e <strong>the</strong> first to op en at de pth d uring anHF-acid fracture stimulation.I have m easured joints and fault o rientations invarious Sin gaporian granite an d gabb roquarries and <strong>the</strong>re is a NE/SW correlation with<strong>the</strong> lineament map (see Fig. 2). Th e predictionis that g ranite with a strong NE/SW orientation<strong>of</strong> ope n join t sets will preferentially channelground water in a NE/SW dire ction away from<strong>the</strong> wate rsheds. Fig ure 1 sho ws that <strong>the</strong>confirmed hot springs in Singapore are indeed170


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>NE <strong>of</strong> <strong>the</strong>ir associated watershed maxima.Heat flow and geo<strong>the</strong>rmal gradientThere are no direct measurements <strong>of</strong> heat flow,<strong>the</strong>rmal conductivity <strong>of</strong> rocks o r g eo<strong>the</strong>rmalgradient from Singapore territory. Hall & Morely(2003) estimate that base d on an extra polation<strong>of</strong> oil and ga s well data from central S umatra,<strong>the</strong> Malaysian Peninsular and <strong>the</strong> Mala y Basin,<strong>the</strong> heat flow values for Singapore are between110 mW/m 2 in <strong>the</strong> east an d 130 mW/m 2 in <strong>the</strong>west <strong>of</strong> <strong>the</strong> island (Fig. 3).SumatraMalayBasinSingaporeFigure 3: Contoured heat flow map <strong>of</strong> part <strong>of</strong> SE Asia.After Hall and Morley (2003).Applying <strong>the</strong> Fourier Law <strong>of</strong> <strong>the</strong>rmal conductionand a ssuming an ave rage heat flo w value <strong>of</strong>120 m W/m 2 and a n avera ge <strong>the</strong>rm alconductivity for g ranite <strong>of</strong> 3.48 W/mK gives ageo<strong>the</strong>rmal gradi ent <strong>of</strong> 34.5o C/ km. Thisassumes that <strong>the</strong> earth’s crust below Singaporeis made from granite.There is a permanent spring at an alti tude <strong>of</strong>120 m at Jungle Fall s on <strong>the</strong> N si de BukitTemah, <strong>the</strong> highest hill in Singapore (164m) in<strong>the</strong> Central Catchment A rea, indi cating a highwater ta ble (Fig. 1). The temperature <strong>of</strong> thisspring i s 24.0 o C (D. Higgitt pers . comm.). At60 m a sl o n <strong>the</strong> NE si de <strong>of</strong> Bukit Temah,ano<strong>the</strong>r sp ring issue s out <strong>of</strong> <strong>the</strong> granit e along<strong>the</strong> Wallace Trail. The te mperature is 26.0 o C,an in crease <strong>of</strong> 2.0 o C o ver a 60 m drop inaltitude from Jun gle F alls, whi ch co uld beinterpreted a s bei ng cau sed by a ge o<strong>the</strong>rmalgradient <strong>of</strong> 3.3 o C per 100 m (or 33 o C / km).Ground water model for SingaporeThe USGS grou ndwater model (6) for islandswith an un confined a quifer surrounded byseawater can be applie d to Singapo re (Barlow2005). Assu ming seawater h as a de nsity ( Ps)<strong>of</strong> 1.025 g/cc compared with fresh water (Pf) <strong>of</strong>1.0 g/cc, <strong>the</strong>n according to <strong>the</strong> Gyben-Herzbergrelation:z = P f . hP s - P fa head (h) <strong>of</strong> 120m ab ove sea lev el in <strong>the</strong>centre <strong>of</strong> <strong>the</strong> island will d rive cold fre sh wate rdown 4.8 km b elow sea l evel ( z). T hepermanent (24 o C) spring at an altitude <strong>of</strong> 120m on Bukit Temah, (164m), indicates that sucha high water table is present. Assuming that <strong>the</strong>average geo<strong>the</strong>rmal gradient for <strong>the</strong> Si ngaporeregion is 35 o C/km (Mazlan et al. 19 99, andsee discussion above), ground water at 4.8 kmdepth will rea ch 168 + 24 = 192 o C. Beca use<strong>of</strong> <strong>the</strong> high rainfall (2.4 m /year) and <strong>the</strong> 120 mhead, <strong>the</strong> hot ground water will be driven along<strong>the</strong> fre sh wa ter/seawater transition a nd up to<strong>the</strong> su rface at th e coast (F ig. 4 ). As describedbefore, this hot water is li kely to bepreferentially chann eled along NE/SWorientated joints and fractures.slCold sea waterGround water model for SingaporeWater tableRainfall = 2.4 m / yrSembawanghot spring 70 o CslCold fresh waterCold sea waterWarm waterHot waterTemperature at 4 .8 km depth = 192 o CInterfaceFigure 4: Ground water model predicts 192 o C water at4.8 km depth.The Sembawang hot spring is 3.7 m above sealevel whi ch was at sea l evel du ring t he warminterglacial periods at ~80 ka and ~125 ka(Kopp 2009). The Pulau Tekong hot spring is at0.5 m above sea level, and from photographs, itlooks to be i n <strong>the</strong> man grove tran sition, whi chexplains <strong>the</strong> high Cl a nd Mg contents (Lee andZhou 2009).171


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Exploration <strong>of</strong> geo<strong>the</strong>rmal prospectsFigure 5 illustrates <strong>the</strong> th ree prospects in <strong>the</strong>Singapore geo<strong>the</strong>rmal pl ay: Pump te sting <strong>of</strong>100 m deep wells into a fault zone i n <strong>the</strong> BukitTemah granit e at <strong>the</strong> Se mbawang ho t sp ringprospect produced up to 400 l/min at a constant70 o C for many days (Zhao et al. 2002 ).However, thi s rate i s n ot high eno ugh tosupport a commercial p ower plant. Deeperproduction wells are required to intercept hotterwater a nd <strong>the</strong>se nee d to be co upled withinjection wells to supplement <strong>the</strong> artesian flow.Cross Section Across <strong>the</strong> Singapore Geo<strong>the</strong>rmal PlayThree geo<strong>the</strong>rmal prospects (1) Sembawang Hot Spring (HGR), (2) P. TekongHot Springs (HGR, HVR), (3) Jurong (HSA, HGR)Jurong Formation(seds)WSWHGRYoungAlluviumOldAlluviumBasement granite heats up undercarapace <strong>of</strong> volcanics and sedimentsPulau TekongvolcanicsSembawang(3) ? T MF CC (1) 70 o C (2) 70 o C?HSAHGR +150 o C?v v v v v vVv v v v HVRvHGR 100 o C?Figure 5: Geo<strong>the</strong>rmal prospects in Singapore. Arrowsindicate a model for groundwater flow. CC = CentralCatchment Area, MF = Mount Faber recharge area, HGR= hot granite rock, HVR = hot volcanic rock, HAS =hotsedimentary aquifer.The Pulau Teko ng pro spect ha s two hotsprings, one <strong>of</strong> which is estimated to be 70 o C,<strong>the</strong> o<strong>the</strong>r which has be en lo st due to landreclamation. The heat source is unlikely to be in<strong>the</strong> Triassic volcanic/sedimentary carapace butra<strong>the</strong>r in <strong>the</strong> fractured granite underneath. TheJurong Fo rmation p rospect is composed <strong>of</strong>conglomerates, s andstones, mu dstones,limestones and min or co al measures,unconformable lying o r thrust on to p <strong>of</strong> <strong>the</strong>granite ba sement (Lee and Zh ou 2009). If <strong>the</strong>Jurong is thick enough (3 – 4 km?) <strong>the</strong>n it couldhave acte d a s a <strong>the</strong> rmal i nsulator to t he ‘hot’granite ba sement. If <strong>the</strong> Jurong i s p ermeableenough, <strong>the</strong>n any aquifers in conta ct with <strong>the</strong>‘hot’ granite basement could have been heatedto form a hot sedimentary aquifer. Cold springson Santosa Island and fro m near United WorldCollege mi ght be recharged from <strong>the</strong> hi ghvENEground <strong>of</strong> M t Faber an d Kent Ridge. Strongjointing in open folded conglomerates atTanjong L okos (Fig. 1) i ndicates goodpermeability.Geophysical survey s: e. g. gravity, MT, TEM,3D seismics, and heat flow su rveys (i.e. a grid<strong>of</strong> 10 km sp aced 300 m deep bo re h oles) arerequired to locate 2 - 3 km de ep ex plorationwells that will test for high heat flow,geo<strong>the</strong>rmal gradients an d st ress ori entation.These dee p well s might intercept sig nificantlyhot artesi an water (HS A) or hot dry ro cksuitable for EGS. Age d ating <strong>of</strong> spring waterswould be u seful to model artesi an flo w rate s:i.e. 3 H/ 3 He, SF 6 and CFC’s.Pro<strong>of</strong> <strong>of</strong> ConceptFor <strong>the</strong> purpose <strong>of</strong> this study, it is assumed thato150 C geo<strong>the</strong>rmal water will be used in abinary generation system . Obviously, viabilitywill be increased with a hotter source but thatwould requi re drilli ng deeper, m ore ex pensivewells.Pro<strong>of</strong> <strong>of</strong> con cept for an EGS 50 MW powerstation, providing po wer for 50,00 0 ho mes bytapping +150 o C water at 2 km depth might costUS$ 19 milli on: i.e. two 3 km long L-shapedwells at US$ 3 million/km, plus US$ 1 million fora 1 km HF acid-fracture job. The horizontal part<strong>of</strong> <strong>the</strong> wells should be 1 km long and orientatedNW/SE s o as to maximiz e intersec tions <strong>of</strong>NE/SW trending vertical joint and fracture sets(Fig.6).Head= 120mArtesian waterat 190 o CPro<strong>of</strong> <strong>of</strong> concept = USD 19mWater table 24 o Cat surfaceProduction<strong>of</strong> hot waterGeo<strong>the</strong>rmal waterat 150 0 CInjection <strong>of</strong>cold waterHot springat 70 o C2 km500 mFigure 6: Pro<strong>of</strong> <strong>of</strong> concept requires sufficient connectivit ybetween injector and production wells.If this was p roved to be succe ssful, <strong>the</strong>n o<strong>the</strong>rpairs <strong>of</strong> L-sh aped wells could be d rilled from172


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong><strong>the</strong> same dri lling p ad until <strong>the</strong> requisite flowrates were acquired.Development CostsDevelopment cost s for a 1 MW dem onstrationpower station can be estimated by comparisonwith <strong>the</strong> 40 0 kW bina ry gene ration systemconstructed at Chena, Alaska. This uses 74 o Chot sp ring water from shallow wells (~20 0 mdeep) in granite and generates electricity usingmassed p roduced ref rigeration components.Development cost s we re US$130 0/kW (3) , i.e.US$ 1.3 million/MW. Production costs at 5 UScents/kWh and selling at a domestic rate <strong>of</strong> 12US cents/ kWh wo uld g enerate a p r<strong>of</strong>it <strong>of</strong> 7cents/kWh, i.e. US$70/ MWh. Base d on <strong>the</strong>se2007 figu res, and ad ding a notional US$ 1million for deeper drilling than Alas ka, in oneyear a pro<strong>of</strong> <strong>of</strong> concept 1 MW power station (for1000 homes) might make 70 x 1 x 365 x 24 =US$ 0.613 million “pr<strong>of</strong>it” before tax. Thedevelopment costs could b e written <strong>of</strong>f in 2.3 /0.613 = 3.75 years a nd save <strong>the</strong> e quivalent <strong>of</strong>10,000 barrels <strong>of</strong> oil/yea r (with crude oil atUS$100 oil/b arrel thi s i s a saving <strong>of</strong> US$ 1million/year in carbon credits).The cost <strong>of</strong> actually drilling 3 km deepdirectional wells in grani te in Singa pore i sunknown th erefore it i s difficult to e stimatecosts and times to break even for a commercialEGS 50 MW power station. Acco rding to <strong>the</strong>U.S. DoE (2 006) <strong>the</strong> initi al co st for l arger fieldand po wer pl ants was aro und US $ 2.5 millionper installed MW in <strong>the</strong> U.S. At 5% infla tion peryear, this is US$ 3.0 milli on per M W at <strong>2010</strong>prices. Sany o et al. (2007) estimate that EGSwould be US$ 4.0 milli on per M W at 2007prices, i.e. US$ 4.6 million at 2 010 pri ces.Estimates fo r Australi a are equivale nt to US$4.2 per M W at <strong>2010</strong> p rices (see App endix 1 inCooper et a l. <strong>2010</strong> ). An avera ge <strong>of</strong> <strong>the</strong>seestimates is US$ 3.93 million per MW.A 50 MW EG S geo<strong>the</strong>rmal power station might<strong>the</strong>refore cost 50 x 3. 93 = US$ 197 million.Assuming production costs at 5 cent s/kWh andselling at a domestic rate <strong>of</strong> 12 cents/kWhgenerates a pr<strong>of</strong>it <strong>of</strong> 7 cents/kWh, i.e.US$70/MWh. In one yea r a 50 M W powe rstation might make 70 x 50 x 36 5 x 2 4 = US$30.6m “pr<strong>of</strong>it” ex cluding taxes a nd i nterestpayments. Write <strong>of</strong>f would take 197/30.6 = 6.4years: an EGS is assumed to last 30 ye ars. 50MW saves <strong>the</strong> equivalent <strong>of</strong> 0.25 million barrels<strong>of</strong> oil/year which at US$100/ bbl = US$ 25million/year worth <strong>of</strong> carbon credits.MarketsThere is a domestic market <strong>of</strong> 5 million peopleand a so phisticated infra structure <strong>of</strong> transport(electric Mass Rapi d Tran sport system,airports), ind ustrial (coal and bioma ss firedpower stations, oil refine ries, ship and oil rigconstruction), and military installations. Each <strong>of</strong><strong>the</strong>se could benefit from an autonomous supply<strong>of</strong> electri city. Alternatively, hot wate r could b eused directly in proces s industries or to powerdistrict cooling projects using absorption chillertechnology. Neighbourhood 50 MW g eo<strong>the</strong>rmalpower statio ns (co sting US$ 200 millio n each)could b e di stributed a round Sin gapore o nreclaimed or Government land or concentratedon Pulau Tekong, to provide b ase lo adelectricity. Th e gene rating co sts would remai nstatic whilst <strong>the</strong> co st <strong>of</strong> i mported nat ural g asvaries.Environmental ImpactAn environm ental impa ct and ri sk a ssessmentwould be a h igh priority. Geo<strong>the</strong>rmal energy isviewed as re newable, clean a nd g reen with asmall carbon footprint du ring <strong>the</strong> con structionphase. No doubt, a rig capable <strong>of</strong> drilli ng 3 kmlong directional wells would b e di sruptive inSingapore’s mainly urb an environm ent. All th edrilling for a power station could be conductedfrom one noise-pro<strong>of</strong>ed drilling pad.The surface geolo gy in dicates that <strong>the</strong>re i sample pe rmeability in <strong>the</strong> strongly jointedgranite an d Jurong F ormation and it m ight bethat perme ability stimulation at depth is notrequired. Ho wever, any HF a cid-fracture j obwould create micro -seismicity. Sin gaporeexperiences micro-sei smicity fro m <strong>the</strong>Java/Sumatra su bduction zo ne and <strong>the</strong>population is seismically aware. Consequently,any fra c-job would require mo nitoring with aseismic array.The inf ra-structure fo r a 1 M W ‘ pro<strong>of</strong> <strong>of</strong>concept’ po wer station would fit into 2 or 3tennis court s. A 50 MW co mmercial po werstation could perh aps be located und ergroundon an area <strong>the</strong> si ze <strong>of</strong> three or fo ur footballfields. Pipe work a nd high tension transmissionlines would also be placed underground.Water su pply in Singap ore i s an i ssue a nd<strong>the</strong>re would be an ini tial requi rement toaugment <strong>the</strong> workin g hydro<strong>the</strong> rmal f racturesystem with f resh or sto rm water, but not sea173


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>water which coul d cause scalin g. O nce th esystem was pre ssured up a nd if <strong>the</strong>injector/production well conn ections we reefficient, <strong>the</strong> requi rement for augm ented waterwould drop. Air ra<strong>the</strong>r tha n water cooli ng mightbe install ed in tower bl ocks o n top <strong>of</strong> <strong>the</strong>underground gene rating halls to conde nseturbine vapo ur for re cycling. Semba wang h otspring has virtually no sm ell but Pulau Tekonghot spring is reported to b e H 2 S-rich (Lee andZhou 2009); however, bina ry ge neratingsystems d o not rel ease fl uids or ga ses to th eatmosphere.SummaryHot springs i n Singa pore are go od i ndicatorsfor a g eo<strong>the</strong>rmal p ower resource. A 1 M Wdemonstration ge o<strong>the</strong>rmal po wer station in ahot spri ng area <strong>of</strong> Singapore could becommissioned for US$ 2.3 million. Construction<strong>of</strong> a comm ercial ge o<strong>the</strong>rmal po wer g enerationwould involv e <strong>the</strong> drilli ng <strong>of</strong> 3 km deepdirectional b oreholes an d <strong>the</strong> gene ration <strong>of</strong>electricity fro m +150 o C hot water t hroughbinary cycle turbine s with <strong>the</strong> coole d ‘wa ste’water being recycl ed down injection wells.Pro<strong>of</strong> <strong>of</strong> con cept for an EGS 50 MW powerstation might cost US$ 19 million. Developmentcosts (US$ 200 million) could be written <strong>of</strong>f in6.4 yea rs a fter produ ction started. Severalneighbourhood EGS 50 MW geoth ermal powerstations could supply base load electricity to <strong>the</strong>national g rid. This is ‘ renewable’, clea n, greenpower generation <strong>of</strong> strategic im portance for acountry that is viewed as h aving n o natu ralresources.AcknowledgementsThis research wa s fu nded by an internal NUSgrant to P r<strong>of</strong>essor A. Palmer, Depa rtment <strong>of</strong>Civil Engin eering, Nati onal University <strong>of</strong>Singapore, who is than ked for many insig htfuldiscussions.ReferencesBarlow P.M., 2005, Ground water in fresh water- salt water environments <strong>of</strong> <strong>the</strong> Atlanticcoast, United States Geological SurveyCircular, 1262, 26 pp.Bowen, R., 1986, Groun dwater, 2 nd edition,Elsevier, 427 pp.Cooper, G.T ., Beard smore, G. R., Waini ng,B.S., Pollington, N. and Driscoll, J.P., <strong>2010</strong>,The Relative Co sts <strong>of</strong> Engi neeredGeo<strong>the</strong>rmal Sys tem Exploration andDevelopment in Australia. Proce edings <strong>of</strong><strong>the</strong> World Geo<strong>the</strong>rmal Congress <strong>2010</strong>, BaliIndonesia, 25-29 April <strong>2010</strong>.Hall, R. and Morley C.K., 2003. Sundala ndbasins. In: Clift, P. D., Wang, P., Kuhnt, W.,Hall, R. an d Tad a R. (eds.) Continent-Ocean Inte raction within East A sianMarginal Se as. Ge ophysical Mo nographSeries 1949, 55 – 85.Kopp, R.E., Simons, F .J., Mitrovica, J.X.,Malo<strong>of</strong>, A.C. and Op penheimer, M., 2009,Probabalistic asse ssment <strong>of</strong> sea l evelduring <strong>the</strong> la st intergl acial stag e. Natu re,462, 863-867.Lee, K.W. a nd Zh ou, Y., 2009, G eology <strong>of</strong>Singapore, 2 nd Edition, Defence Scie nceand Technology Agency, Singapore, 90pp.Mazlan, M., Abolin s, P., Mohamm ad Jamaaland Mansar, A.,1999, In : PETRONAS. ThePetroleum Geology an d Resource s <strong>of</strong>Malaysia. Kuala Lumpar 171-217.Sanyal, S.K ., Morrow, J .W., Butler, S.J .,Robertson-Tait, A., 2007, Co st <strong>of</strong> electricityfrom e nhanced ge o<strong>the</strong>rmal systems.<strong>Proceedings</strong> Thirty-Seco nd Wo rkshop onGeo<strong>the</strong>rmal Re servoir Engi neering,Stanford.U.S. Depa rtment <strong>of</strong> <strong>Energy</strong>. (200 6).http://www1.eere.energy.gov/geo<strong>the</strong>rmal/m/faqs.htmlZhao, J., Ch en, C.N. and Cai, J.G., 2002, Ahydrological study <strong>of</strong> <strong>the</strong> Semba wang hotspring. Bull etin Engin eering G eologyEnvironment, 61, 59-71.Zhou, Y., 2001, Engineering Geology and RockMass P roperties <strong>of</strong> th e Bu kit Ti mahGranite. Underground S ingapore, 29 -30<strong>Proceedings</strong>, 308-314.Web sources were accessed in May, <strong>2010</strong>.(1)http://www.searchanddiscovery.com/documents/2008/08181goldstein/index.html.(2)http://useconomy.about.com/od/candidatesand<strong>the</strong>economy/a/Obama_(3)http://www.chenahotsprings.com/geo<strong>the</strong>rmal-power/.(4)www.geyser.com.(5)h ttp://wwwwsm.physik.unikarlsruhe.de/pub/stress_data_frame.html(6)http://pubs.usgs.gov/circ/2003/circ1262/#heading156057192.174


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Monitoring EGS Reservoirs Using MagnetotelluricsJared Peacock 1 *, Stephan Thiel 1 , Graham Heinson 1 , Louise McAllister 21 TRaX, School <strong>of</strong> Earth and Environmental Sciences, University <strong>of</strong> Adelaide, SA 5005, Australia2 Petra<strong>the</strong>rm Ltd, Adelaide, Unley, SA 5061, Australia*Corresponding author: jared.peacock@adelaide.edu.auA novel time-lapse mag netotellurics (MT) methodis proposed to monitor and estimate a real extent<strong>of</strong> enha nced geo<strong>the</strong> rmal systems (E GS). Beingdirectly se nsitive to sub surface ele ctricalconductivity, MT has t he capability t o measurefluids at de pth which a re both <strong>the</strong>rmally andelectrically conductive. MT measurements before,during a nd after fluid inj ection are co mpared toestimate <strong>the</strong> lateral extent <strong>of</strong> <strong>the</strong> induced reservoirat Paral ana, South A ustralia. 3 D forwardmodelling shows <strong>the</strong> resi dual MT responsebetween a system with and without con ductivefluids to be small, <strong>of</strong> <strong>the</strong> o rder <strong>of</strong> a few degree s inMT ph ase. It is crucial to obtain a ccurate andprecise MT resp onses through out <strong>the</strong> survey s inorder to produce a reliable model <strong>of</strong> <strong>the</strong> changingsubsurface. Presented a re MT re sponses befo refluid inje ction and afte r <strong>the</strong> first fluid injectio n.Fur<strong>the</strong>rmore, time series mea surement <strong>of</strong> <strong>the</strong>electric an d magneti c fields du ring th e fractu ringprocess may allo w studies <strong>of</strong> EM di sturbancesgenerated by <strong>the</strong> seismi c waves, also known as<strong>the</strong> sei smoelectric effect , which ca n provideinformation about pore fluid inclusion.Keywords: Magnetotelluric, EGS, MonitoringIntroductionEGS has th e potential to sup plement energyproduction a s <strong>the</strong> world slo wly and re sistantlyshifts to wards rene wable energy. On e importa ntconstraint <strong>of</strong> EGS is moni toring where <strong>the</strong> fluidsgo once injecte d into <strong>the</strong> hot lithology.Traditionally, reservoirs a re mo nitored with mi croseismometer a rrays, which me asure se ismicevents generated by frac tures (P hillips et al.,2002). To mography can be a pplied t o e stimatelocation <strong>of</strong> th e fracture (House, 1987), and shearwavesplitting ca n be u sed to e stimate si ze andorientation <strong>of</strong> <strong>the</strong> fracture (Elkibbi and Rial, 2005).Unfortunately, <strong>the</strong>se measurements do n otprovide information about fluid inclusion.Magnetotellurics (MT)MT is a pa ssive volum etric mea surement thatexploits F araday’s la w <strong>of</strong> magn etic i nduction bymeasuring orthogon al co mponents <strong>of</strong> <strong>the</strong> Earth’ snatural m agnetic field and its sub sequentelectrical re sponse. M T is a diffusiv e metho d,which means source energy spreads as a function<strong>of</strong> time and resolution i s prop ortional to sou rceperiod, as defined by <strong>the</strong> skin depth equation. It issensitive to variation s in e lectrical cond uctivity <strong>of</strong><strong>the</strong> subsurface, which makes it a prime techniqueto monitor changes a s elect rically con ductivefluids are introduced. The fluids a re assumed tobe co nductive due to <strong>the</strong>rmal an d dissolved io nenhancement and will provide a larg e contrastwith resistive ho st r ocks (Spichak and Man zella,2009).Test site: Paralana, South AustraliaThe te st site is in <strong>the</strong> nor<strong>the</strong>rn pa rt <strong>of</strong> SouthAustralia, ab out 60 0km due north <strong>of</strong> Adelaid e,near <strong>the</strong> edge <strong>of</strong> <strong>the</strong> Flinders Range s an dParalana hot springs. Here, <strong>the</strong> <strong>the</strong>rmal activity isgenerated by an innat ely large density <strong>of</strong>radiogenic elements, where residual heat is a byproduct<strong>of</strong> millions year s <strong>of</strong> decay (Brugger,2005). The 1590M a crystalline litholo gy <strong>of</strong> <strong>the</strong>uplifted Flinder Ran ges has an estim ated heatflow on <strong>the</strong> orde r <strong>of</strong> 60mW/m2 in (Neumann,2000), compared to a typical basement rock heatflow <strong>of</strong> abou t 10mW/m2. To <strong>the</strong> East <strong>of</strong> <strong>the</strong>Flinders Ranges, <strong>the</strong> hot crystalline rocks areunconformably overlaid by about 4 500m <strong>of</strong>Adelaidian sediment s, wh ich a cts a s a lithologi cblanket keeping heat from escaping. As a result<strong>the</strong> he at flo w i s estimated to be 1 12mW/m2,making <strong>the</strong> area a prime location for EGS.Figure 1: Survey design centred on Paralana 2 drill hole,overlying elevation (m). Two orthogonal lines parallel toassumed principle stress directions provide dense 2Destimation with 22 stations per line. Spacing varies from200m near <strong>the</strong> centre to 1.5km near <strong>the</strong> extremities. Two <strong>of</strong>fdiagonal lines with variable spacing <strong>of</strong> 250m, 500m, 1kmprovide dimensionality constraints with 6 stations each. Onesurvey encompasses a total <strong>of</strong> 58 stations, 56 plus tworemote reference stations.175


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Petra<strong>the</strong>rm and joint venture p artners Be ach<strong>Energy</strong> Ltd and Tru energy Geo<strong>the</strong>rmal Pty Ltdlease a 500km2 tenement where Paralana 2 hasbeen drilled to a de pth o f 4012m and ca sed to3725m. The bottom hole temperatu re has bee nestimated at 190 C and fl uids were en counteredat a depth <strong>of</strong> 3860m. Note <strong>the</strong> proposed EGS willnot be l ocated in <strong>the</strong> ba sement rock, but in <strong>the</strong>sediment p ackage directl y above, which has adominant horizontal stress field. It is proposed thatinducing permeability and po rosity in thissediment pa ckage via m echanical fra cturing willbe a chieved more e asily than i n <strong>the</strong> cry stallinebasement without losi ng much in re servoirtemperature. The propose d reservoir si ze will beabout 1 km i n <strong>the</strong> ea st-west directio n and a bout2km in th e north-south direction and about 400mthick at aro und 36 00m d epth. Perforat ion <strong>of</strong> <strong>the</strong>well casing is pr oposed to co mmence in Aug ust,<strong>2010</strong>, followed by two separate fracturing periodsoccurring in September, <strong>2010</strong> and January, 2011.ProcedureA preli minary su rvey was coll ected to co mpareany changes in o<strong>the</strong>r surveys collected during andafter <strong>the</strong> two fracturi ng pe riods. For al l surveys,<strong>the</strong> basic layout, centred on Paralana 2, containsan ortho gonal pair <strong>of</strong> NNE-SSW and WNW-ESElines employing 22 statio ns e ach, Figure 1. T helines h ave variabl e sp acing <strong>of</strong> ~20 0m near <strong>the</strong>centre increasing to 1.5km near <strong>the</strong> extremities toget maximal coverage at depths <strong>of</strong> inv estigation.Two <strong>of</strong>f diagonal lines containing 6 stations each,again centre d on Paral ana 2, with variablespacing <strong>of</strong> 250m, 500m, 1 km, aid in est imating 3-dimensionality. Each survey will employ 56stations in to tal plus 2 remote refe rence statio ns60km and 80 km so uth <strong>of</strong> Parala na. T he su rveydesign i s based o n fo rward mod elling a ndlogistics. T he goal i s to estimate reservoir extentas a function <strong>of</strong> time by measuring changes in <strong>the</strong>MT responses.Survey 1: Base surveyA base survey was collected in Ma rch, <strong>2010</strong> withAuScope instrument s run by <strong>the</strong> University <strong>of</strong>Adelaide. The sampling rate was 500Hz, with 50mdipole len gths, m easuring h orizontal magn eticfields Bx a nd By, along with horizontal ele ctricfields Ex and Ey, where <strong>the</strong> x comp onentmeasuring <strong>the</strong> field relative to magneti c north andy measurin g <strong>the</strong> field relative to mag netic east.The ve rtical magn etic co mponent Bz wasmeasured for 6 station s. Stainless st eel sta keswere used as dipoles for 51 sites, <strong>the</strong> o<strong>the</strong>r 5 sitesemployed Cu-CuSO4 pot s. Induction coil s wereused as m agnetometers. The average d atacollection time was 22 hours. MT responses werecalculated using BIRRP (Chave, 2004) and an inhouse interfa ce written in Python. It was foundthat 30 sites were not pre cise enou gh due to anunknown source <strong>of</strong> n oise resembling a n onperiodiccharge-recharge pattern in th e ele ctricchannels, Figure 2. The n oise does not appear tocorrelate between stations and does not appear tohave any lo cation objectivity. Different filteringtechniques were employ ed with little effect ontransfer fu nction a ccuracy. The refore, those 30sites have bee n redone using Cu -CuSO4electrodes, which seem to prod uce mo re sta bleand relia ble electri c field measurement s. Mostdata h ave lo w coherency and larger error barsaround 1-10 se conds, Fi gure 5 which is a wellknown d ead band. Also, <strong>the</strong> appa rent resi stivityand pha se p olarizations sugge st a do minant 1Dgeoelectric structure to a period <strong>of</strong> a few seconds,<strong>the</strong>n a multidimensional structure after periods <strong>of</strong>a few se conds. The site i s near a larg e workinguranium mine, Beverly in Fi gure 1, whichproduces 50Hz (and harmonics) EM signal. Thissignal is observed i n <strong>the</strong> time-freque ncyspectrogram, and i n estimate d appa rentresistivities and ph ases below p eriods <strong>of</strong> .1seconds, where <strong>the</strong> estimations are less smooth.Figure 2: Plots <strong>of</strong> time series data for two stations plotting,Bx (counts), By (counts), Ex (mV/m), and Ey (mV/m).Bottom axis is time in hours. Top: station pb44, 5km west <strong>of</strong>Paralana 2, showing a sporadic charge-recharge pattern in<strong>the</strong> electric channels giving irregular estimates <strong>of</strong> <strong>the</strong> MTresponse. Bottom: station pb 24, 500m east <strong>of</strong> Paralana 2,showing smooth response in electric channels giving smoo<strong>the</strong>stimates <strong>of</strong> <strong>the</strong> MT response.176


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>A second base survey was collected in May, <strong>2010</strong>to redo <strong>the</strong> stations from <strong>the</strong> first survey that werenot pre cise e nough. The same parameters andlocations were u sed, but Cu-CuSO 4 electrodeswere used for all station s and no B z signals wererecorded d ue to i nstrument constraints.Unfortunately, at <strong>the</strong> same time thi s survey wasbeing collected <strong>the</strong> Epi c Pipleline, which runsparallel to th e NNE-SSW line ab out 2 km we st <strong>of</strong>Paralana 2, was being tested for corrosion. To dothis an electric 3 second squ are wave is sentdown <strong>the</strong> pi peline every 12 second s, Figure 3.Figure3: Left: time series <strong>of</strong> Bx (counts), By (counts), Ex(mV/m), Ey(mV/m) for station pb37 from second survey,200m near <strong>the</strong> pipeline. Notice <strong>the</strong> dominating 3 secondsquare wave in <strong>the</strong> electric channels and <strong>the</strong> correspondingmagnetic response.Figure 4: Plot demonstrating a method to remove periodicnoise by subtracting <strong>the</strong> average wave form for a 12 secondwindow from <strong>the</strong> data for pb42 Ex channel. Top: Ex (mV/m)with periodic noise removed plotted against time (s). Middle:filter in red compared to <strong>the</strong> raw data plotted against time(s).Bottom: Plot <strong>of</strong> <strong>the</strong> power spectrum <strong>of</strong> <strong>the</strong> raw data in blackand <strong>the</strong> filtered data in red. Notice <strong>the</strong> large notches at 12seconds and its harmonics are removed.Figure 5: MT responses <strong>of</strong> two orthogonal modes Ex/By andEy/Bx. Top are log-log plots <strong>of</strong> apparent resistivity versusperiod. Bottom plots are phase in degrees versus log period.Top: pb24 from first base survey displaying a relative smoothMT response with minimal error bars. Bottom: pb42 fromsecond survey with periodic noise removed. Again notice <strong>the</strong>plots display relative smooth MT responses with minimalerror bars, but still have a coherent biased in periods <strong>of</strong> 1-10sec. Notice in all plots <strong>the</strong> error bars are larger around 10seconds which is where a change in <strong>the</strong> MT response isexpected to occur when fluids are injected. This is also <strong>the</strong>known dead band where <strong>the</strong>re is naturally low signal power.177Because thi s si gnal i s distinctly periodic andregular, si mple time se ries analy sis can rem ovethis from <strong>the</strong> data. By taki ng an average <strong>of</strong> a 1 2second win dow <strong>the</strong> average wave fo rm can b e


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>calculated. That wave fo rm is convolved with aseries <strong>of</strong> del ta function s every 12 seconds. Alinear trend calculated fro m <strong>the</strong> data is add ed to<strong>the</strong> filter time series to fit <strong>the</strong> data better. The filteris <strong>the</strong>n subtracted from <strong>the</strong> ra w data, Figure 4.This method works fine for station s at least 1 kmaway fro m <strong>the</strong> Epic Pi peline, but b reaks d owncloser due to <strong>the</strong> larg e amplitudes <strong>of</strong> th e periodicsignal. Along with t his meth od, remotereferencing i s u sed to constrain th e tran sferfunctions, Fi gure 5. Unfortunately, with <strong>the</strong>periodic noise remove some <strong>of</strong> <strong>the</strong> signal is al soremoved which ads to larger erro r bars around 3-12 se conds. It was deci ded to redo <strong>the</strong> inner 30stations to get <strong>the</strong> best estimate <strong>of</strong> <strong>the</strong> MTresponse as possible and reduce error bars. Thissurvey will be collected at <strong>the</strong> end <strong>of</strong> August, <strong>2010</strong>in conjunction with <strong>the</strong> perforation test.AnalysisThe MT re sponses com monly suffer from nearsurfacegalv anic hete rogeneities that disto rt <strong>the</strong>calculated i mpedance tensor Z. Given <strong>the</strong>existence <strong>of</strong> a sub set with 1D characteristics i n<strong>the</strong> data it is po ssible to fully calculate <strong>the</strong>distortion-free region al im pedance ten sor (Bibbyet al., 2005). In <strong>the</strong> curren t case, <strong>the</strong> p resence <strong>of</strong><strong>the</strong> 1D re sistivity distri bution <strong>of</strong> <strong>the</strong> sedi mentstrata all ows a relia ble e stimate <strong>of</strong> th e regi onalimpedance t ensor. Kn owledge <strong>of</strong> <strong>the</strong> distortionfreeregi onal impedance tenso r ensures a moreaccurate e stimation <strong>of</strong> th e sub surface re sistivity.The regional impedance tensor is inverted in a 2Dsense to obtain <strong>the</strong> re sistivity distri butionunderneath <strong>the</strong> pr<strong>of</strong>iles (Rodi and Mackie, 2001).This has been applied toConclusionsA novel method <strong>of</strong> monitori ng enha ncedgeo<strong>the</strong>rmal system s usi ng <strong>the</strong> magnetotelluricmethod has bee n p roposed be cause M T i ssensitive to t he bul k el ectrical condu ctivity <strong>of</strong> <strong>the</strong>subsurface and <strong>the</strong>refore directly to <strong>the</strong> highconductivity <strong>of</strong> <strong>the</strong> i njected fluid s. The EGSsystem at Paralana wil l be indu ced in <strong>the</strong>sediment package above <strong>the</strong> hot basement rocks.The relatively high conductivity <strong>of</strong> <strong>the</strong> sedimentarybasin nea r <strong>the</strong> su rface requires hi gh quality MTresponses to ensure detection <strong>of</strong> small changes in<strong>the</strong> MT responses before and after <strong>the</strong> injection <strong>of</strong>fluids. Keep in mind <strong>the</strong> base survey to which allchanges are going to be compared to needs to beprecise and accurate. Therefore it is important tocollect <strong>the</strong> b est data p ossible eve n if it mean srepeating su rveys. Learning i s abo ut ma kingmistakes, <strong>the</strong>refore <strong>the</strong> m ore you ma ke <strong>the</strong> moreyou learn.AcknowledgmentsThe autho rs would like to thank Petrat herm an djoint venture partne rs B each Petrol eum andTru<strong>Energy</strong> f or support o f this proje ct. GorenBoren, Jonat hon Ross, Hami sh Ada m, Trista nWurst, and Kiat Low for field work assista nce.IMER and PirSa for financial support.ReferencesBibby, H.M., Caldwell, T.G. and Brown, C.,Determinable and no n-determinable parameters<strong>of</strong> galvani c disto rtion in mag netotellurics,Geophysical Journal International, 1 63, pp 91 5-930.Brugger, J.; Long, N.; McPha il, D. C. & Plimer, I.,An active amagmati c hydro<strong>the</strong> rmal system: <strong>the</strong>Paralana hot spri ngs, No r<strong>the</strong>rn Flin ders Range s,South Austra lia, Chemical Geology, 2005, 222,35-64Chave, A. D. & Th omson, D. J., Bound edinfluence magnetotelluric respon se fun ctionestimation, Geophysical Journal International,2004, 157, 988-1006Elkibbi, M. & Rial, J. A., The G eysers geo<strong>the</strong>rmalfield: results from shea r-wave splitting analysis ina fra ctured re servoir, Geophysical JournalInternational, 2005, 162, 1024-1035House, L. S., Locating mi croearthquakes inducedby hydrauli c fra cturing in crystal line ro ckGeophysical Research Letters, 1987, 14, 919-92Neumann, N.; Sandiford, M. & Foden, J.Regional geochemistry and continental heat flow:implications for <strong>the</strong> origin <strong>of</strong> <strong>the</strong> South <strong>Australian</strong>heat flow anomaly, Earth and Planetary ScienceLetters, 2000, 183, 107-120Phillips, W. S.; Rutledge, J. T.; Hou se, L. S. &Fehler, M. C., Induced mi croearthquake pattern sin hydro carbon an d geot hermal re servoirs: sixcase st udies, Pure and Applied Geophysics,Seismic Research Center, Los Alamos NationalLaboratory, 2002, 159, 345-369Rodi, W. a nd Mackie, R. L. Nonlin ear conjugategradients algorithm fo r 2-D mag netotelluricinversion, Geophysics, 66, pp 174-187.Spichak, V .V., and Manzella, A, 2009,Electromagnetic Soundings <strong>of</strong> Geo<strong>the</strong>rmal Zones,Journal <strong>of</strong> Applied Geophysics, 68, pp459-478178


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Reservoir characterisation and numerical modelling to reduceproject risk and maximise <strong>the</strong> chance <strong>of</strong> success. An example <strong>of</strong>how to design a stimulation program and assess fluid productionfrom <strong>the</strong> Soultz geo<strong>the</strong>rmal field, FranceJoshua Koh 1 , Nima Gholizadeh-Doonechaly 1 , Abdul Ravo<strong>of</strong> 1 and Sheik S Rahman* 1 , Luke Mortimer 21 School <strong>of</strong> Petroleum Engineering, University <strong>of</strong> New South Wales, Sydney2 Hot Dry Rocks Pty Ltd, 1A Yarra Street, South Yarra, VictoriaThis paper describes a predictive, fully coupled poro-<strong>the</strong>rmo-elastic numerical model that isspecifically developed to evaluate and optimise geo<strong>the</strong>rmal reservoir development strategies. Thispaper illustrates this via an investigation into <strong>the</strong> role <strong>of</strong> stimulation to enhance <strong>the</strong> permeability foreconomic hot water production from <strong>the</strong> deep geo<strong>the</strong>rmal site at Soultz-sous-Foréts (France). Thisstudy integrates four key elements: a natural fracture characterization model, a fluid flow simulationmodel, a heat transfer model and a stimulation model. Fluid flow is simulated using a finite elementbased model wherein stresses and temperature are fully coupled to <strong>the</strong> fluid flow equations. The heattransfer model is based on conductive heat transfer within <strong>the</strong> reservoir rock, convective (includingconduction) heat transfer through <strong>the</strong> reservoir fluid and time dependent <strong>the</strong>rmal equilibrium between<strong>the</strong> rock and fluid. The stimulation model integrates shear dilation mechanisms and stress dependentpermeabilities. Effective permeability tensors (based on discrete fracture network) are estimateddynamically and are iteratively used to determine <strong>the</strong> pore pressure, stress and <strong>the</strong>rmal state within<strong>the</strong> reservoir.A numerical reservoir model <strong>of</strong> <strong>the</strong> Soultz-sous-Foréts field was constructed based on <strong>the</strong> dataavailable in <strong>the</strong> open literature. The reservoir was subjected to different pressure cycles to determine<strong>the</strong> degree <strong>of</strong> permeability enhancement that could be achieved. Flow rate and correspondingpressure losses between injector and producers as well as heat recovery <strong>of</strong> <strong>the</strong> produced water werecalculated to assess <strong>the</strong> geo<strong>the</strong>rmal potential <strong>of</strong> <strong>the</strong> reservoir. Results <strong>of</strong> this study show that effectivetensile normal stresses from <strong>the</strong> injected cold fluid tend to increase fracture apertures, and hence,increase fracture permeability within <strong>the</strong> zone <strong>of</strong> cooling. It was also shown that for a nominalstimulation bottomhole pressure <strong>of</strong> 10,000 psi, a maximum number <strong>of</strong> shear dilation events isobserved after a stimulation period <strong>of</strong> 42 weeks for <strong>the</strong> generated Soultz fracture system and thislevel <strong>of</strong> stimulation was sufficient to obtain an economic flow rate <strong>of</strong> 100 L/s (at an acceptablepressure loss <strong>of</strong> 2000psi). Our experience also shows that prior to stimulation, flow rates at anacceptable pressure loss between <strong>the</strong> injector and producers are not sufficient for economic heatextraction. Hence <strong>the</strong>se reservoirs require ei<strong>the</strong>r stimulation to enhance reservoir permeability orinstallation <strong>of</strong> down-hole pumps to lift hot water.In addition, it has been observed that a major factor responsible for heat recovery as well as <strong>the</strong>rmaldrawdown is <strong>the</strong> degree <strong>of</strong> interconnection <strong>of</strong> <strong>the</strong> fractured reservoir. The produced fluid temperaturefor <strong>the</strong> more weakly connected well GPK4 remains very high (~195 0 C) after a production period <strong>of</strong> 14years. During <strong>the</strong> same period <strong>the</strong> average matrix temperature drawdown is in <strong>the</strong> order <strong>of</strong> 20 0 C foran initial reservoir temperature <strong>of</strong> 200 0 C. For <strong>the</strong> case <strong>of</strong> a highly interconnected GPK2 well, <strong>the</strong>179


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>temperature <strong>of</strong> <strong>the</strong> produced fluid falls from an initial temperature <strong>of</strong> 200 0 C to about 130 0 C after 14years <strong>of</strong> production.IntroductionUnderstanding <strong>of</strong> <strong>the</strong> hydraulic flow and heat transfer within crystalline rocks is <strong>of</strong> significantimportance in <strong>the</strong> utilization <strong>of</strong> deep earth (at least 4 km) hot rock (HR) for geo<strong>the</strong>rmal reservoirsystems (Baria et al. 1999; O'Sullivan et al. 2001). The characteristics <strong>of</strong> fluid flow and heat transfer incrystalline rocks are dominated by <strong>the</strong> fracture systems found within <strong>the</strong>m and in-situ stress whichaffect <strong>the</strong> properties <strong>of</strong> <strong>the</strong> fracture system significantly. Modelling <strong>of</strong> coupled hydraulic, <strong>the</strong>rmal andmechanical processes can help in <strong>the</strong> understanding <strong>of</strong> <strong>the</strong> effects <strong>of</strong> in-situ stresses, induced fluidpressure and heat transfer on fluid flow and <strong>the</strong>rmal drawdown <strong>of</strong> naturally fractured geo<strong>the</strong>rmalsystems. The long-term response <strong>of</strong> fracture systems to changes in effective stresses has beeninvestigated by several authors (McDermott and Kolditz, 2006). The change in effective stresses canbe induced by hydraulic and <strong>the</strong>rmo-elastic stress alterations resulting from heat extraction from <strong>the</strong>fractured geo<strong>the</strong>rmal systems (rocks). Circulation <strong>of</strong> cold fluid induces temperature differences within<strong>the</strong> rock matrix due to heat transfer which leads to large amounts <strong>of</strong> stress energy release. In anexperimental study, O'Sullivan et al (2001) observed some degree <strong>of</strong> geo-mechanical effects <strong>of</strong><strong>the</strong>rmal stresses on geo<strong>the</strong>rmal reservoir characteristics (fracture apertures and fracture permeability)and suggested a need for a long term investigation <strong>of</strong> <strong>the</strong> <strong>the</strong>rmal stress effect. In particular, <strong>the</strong>mechanisms that cause phenomena, such as variation <strong>of</strong> injectivity/productivity with <strong>the</strong>rmaldrawdown and occurrence <strong>of</strong> seismicity need to be understood.The response <strong>of</strong> a fracture network to stimulation by injection <strong>of</strong> cool fluid is time dependent and is afunction <strong>of</strong> discrete fracture behaviour (McDermott et al. 2006; Beeler and Hickman 2003). Theindividual response <strong>of</strong> <strong>the</strong> discrete fractures within <strong>the</strong> fracture system are determined by interaction<strong>of</strong> <strong>the</strong> injected fluid and its physical characteristics such as viscosity, heat capacity and temperature.O<strong>the</strong>r factors, such as <strong>the</strong> elastic response <strong>of</strong> <strong>the</strong> rock matrix and pervasive in-situ conditions,including pore pressure and rock temperature have a significant bearing on <strong>the</strong> closure and shearstate <strong>of</strong> a fracture. The effective stress pr<strong>of</strong>iles along fracture surfaces are functions <strong>of</strong> <strong>the</strong> far fieldtectonic stresses, induced hydraulic stresses and <strong>the</strong>rmal stress release (McDermott et al. 2006)during heat extraction. Induced tensile stresses normal to <strong>the</strong> fracture surfaces from cold waterinjection can increase fracture aperture and induce new fractures (Zhou et al., 2009). Therefore,alterations <strong>of</strong> fracture system parameters, such as effective permeability need to be coupled tochanges in <strong>the</strong> pervasive conditions.Recently, Rutqvist and Stephanson (2003) provided a generic overview <strong>of</strong> models used forhydromechanical coupling at an aquifer depth and a number <strong>of</strong> well-known empirical approaches tochanges in <strong>the</strong> normal stress across fractured medium. Most notable, is <strong>the</strong> study by Beeler et al(2000) who applied elastic solutions for elliptical cracks to define <strong>the</strong> deformation responses <strong>of</strong>elliptical fractures under tectonic loading. The effect on <strong>the</strong> surrounding rock mass however, was notincluded.180


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Few authors have investigated <strong>the</strong> effects <strong>of</strong> induced fluid pressure on naturally fractured rock on areservoir scale. Rahman et al. (2002) developed a steady state fluid flow model to study <strong>the</strong> sheardilation effect due to fluid pressure on permeability enhancement. Shaik et al. (2009) consideredporoelastic stresses in <strong>the</strong> stimulation <strong>of</strong> a discrete fracture network by induced fluid pressure. In <strong>the</strong>aforementioned studies, however, <strong>the</strong>rmal stresses were not considered.Kumar and Ghassemi (2005) developed a numerical model to study fluid pressure and permeabilitychanges in a rock mass by taking into account <strong>the</strong> effects <strong>of</strong> <strong>the</strong>rmal stresses and silicaprecipitation/dissolution. The numerical model incorporated a single planar fracture connecting aninjection well and a production well as an idealized reservoir-matrix system. The temporal variation <strong>of</strong>fracture aperture in response to <strong>the</strong> individual and combined effects <strong>of</strong> <strong>the</strong>rmo-elastic stress and silicadissolution/precipitation were examined, however, changes in fracture aperture and pressure inresponse to non-uniform cooling were not addressed.Poroelastic and <strong>the</strong>rmoelastic effects <strong>of</strong> cold-water injection into a single pre-existing fracture in a hotrock matrix was investigated by Ghassemi et al. (2007). Assumptions <strong>of</strong> plane fracture geometry wereused to derive expressions for changes in fracture aperture caused by cooling and fluid leak-<strong>of</strong>f into<strong>the</strong> matrix. The variations in aperture and pressure occurring under non-iso<strong>the</strong>rmal flow conditionswhen <strong>the</strong> fracture is subject to injection and heat extraction were examined. The problem wasanalytically solved for <strong>the</strong> cases pertaining to a constant fluid injection rate with a constant leak-<strong>of</strong>frate using a partially coupled formulation.As part <strong>of</strong> this study, four computationally efficient models are presented in an effort to evaluate andoptimise reservoir development strategies: a natural fracture characterization model, a fluid flowsimulation model, a heat transfer model and a stimulation model. The fully coupled <strong>the</strong>rmo-poroelasticnumerical model is applied to <strong>the</strong> Soultz geo<strong>the</strong>rmal reservoir, France, where several deep wells havebeen drilled and stimulated in <strong>the</strong> Rhine graben (Soultz, France) to evaluate <strong>the</strong> geo<strong>the</strong>rmal Hot DryRock potential <strong>of</strong> <strong>the</strong> deep fractured granite reservoir. Three main boreholes, GPK2, GPK3 and GPK4which reach 5080, 5100 and 5270m depth respectively, intersect a crystalline basement overlain by1400m <strong>of</strong> Cenozoic and Mesozoic sediments. The layout <strong>of</strong> <strong>the</strong> Soultz-sous-Forets EGS site and <strong>the</strong>well traces and locations are presented in Fig. 1 . The novelty <strong>of</strong> this approach lies in its dynamictreatment <strong>of</strong> <strong>the</strong> characteristic properties <strong>of</strong> individual fractures in simulating fluid flow and <strong>the</strong>pervasive response <strong>of</strong> <strong>the</strong> natural fracture system to cold fluid injection. The coupled numericalalgorithm is presented in Fig. 2.Modelling <strong>of</strong> <strong>the</strong> Soultz fracture networkVariably oriented and intersected fractures with different sizes and irregular patterns (i.e. all fracturecomplexities) are characterized with <strong>the</strong> use <strong>of</strong> two integrated methodologies (Tran, Chen et al. 2007).In <strong>the</strong> hybrid neuro stochastic methodology, fracture properties are generated based on <strong>the</strong>ircharacterized statistical distributions. A selective random sampling scheme is used for this purpose.Continuum maps <strong>of</strong> fracture density and multifractal dimensions are integrated in <strong>the</strong> discrete model.Hierarchical simulation technique is used to deal with different degrees <strong>of</strong> heterogeneity in <strong>the</strong>181


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>reservoir. In <strong>the</strong> second methodology, hybrid neuro stochastic methodology is upgraded to handlemore complex measurements. In this methodology, an object based conditional global optimizationconcept is applied. It combines continuum distributions with statistical distributions and correlations <strong>of</strong>discrete fracture properties, thus representing a great improvement over o<strong>the</strong>r object based stochasticsimulation as well as grid based fracture models.Based on <strong>the</strong> observed data recorded, a specified number (say 1000 fractures) <strong>of</strong> unbiased dataspecimens are generated by re-sampling <strong>the</strong> weighting field using a normalized probability method fordifferent fracture classes. Once at least 1000 fractures are created, <strong>the</strong>n <strong>the</strong> fractures are sorted withrespect to <strong>the</strong>ir radii. The sorting is performed based on <strong>the</strong> input value for <strong>the</strong> smallest and <strong>the</strong>largest fractures to be modeled. Once <strong>the</strong> fracture network with specific characteristics is generated,<strong>the</strong> next step is to define <strong>the</strong> fracture density in a square volume <strong>of</strong> rock <strong>of</strong> interest. The fracturedensity is <strong>the</strong> representation <strong>of</strong> <strong>the</strong> fracture area per unit volume <strong>of</strong> rock mass observed in <strong>the</strong> field.The fracture network is stochastically realized within this volume using a pseudo-random numbergenerator. This is accomplished by repeated re-sampling <strong>of</strong> earlier fracture records and placing <strong>the</strong>fractures randomly in <strong>the</strong> volume <strong>of</strong> interest until <strong>the</strong> required fracture density is reached.In this study, <strong>the</strong> statistical analysis <strong>of</strong> <strong>the</strong> fracture networks in <strong>the</strong> Soultz geo<strong>the</strong>rmal reservoir asperformed by Gentier et al. (<strong>2010</strong>) was used. Table 1 presents <strong>the</strong> four main fracture sets F1, F2, F3and F4, with a fifth set F5 defined for fractures not falling within <strong>the</strong> initial four main sets as“background noise” (Gentier et al., <strong>2010</strong>). Two ~N-S striking sets are distinctly recognised,respectively W-dipping (F1) and ENE-dipping (F2). In addition, two NE-SW and NW-SE striking setsare also observed, respectively NW-dipping (F3) and SW-dipping (F4).The fracture data was used to stochastically resample <strong>the</strong> fracture network around <strong>the</strong> wells GPK2,GPK3 and GPK4 in <strong>the</strong> abovementioned manner. The generated fracture network is presented in Fig.3 for a parallelepiped volume <strong>of</strong> 2.5 km (east west) by 3.0 km (north south) by 3.5 km (vertical, 2500m– 6000m).Numerical flow simulationA finite element based poro-<strong>the</strong>rmo-elastic reservoir model is developed for evaluating hot waterproduction. This model fully couples fluid flow, temperature and geomechanics. The governingequations <strong>of</strong> non-iso<strong>the</strong>rmal <strong>the</strong>rmo-poroelasticity is expressed as follows (Kurashige, 1989;Ghassemi et al., 2002): G K ( u) G 3 2k tu p T 0(0.1)21Rp(0.2) ii Q' p T2(1.3)Tf2T (J T ) c T 0(1.4)ffff182


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>T R cTR2TR 0(1.5)where, K is <strong>the</strong> bulk modulus (MPa), G is <strong>the</strong> shear modulus (MPa), u is <strong>the</strong> displacement vector, (ux,uy) (m), α is Biot's coefficient, γ 1 is <strong>the</strong> <strong>the</strong>rmal expansion coefficient <strong>of</strong> solid (K -1 ), γ 2 is <strong>the</strong> <strong>the</strong>rmalexpansion coefficient <strong>of</strong> fluid (K -1 ), T R and T f are <strong>the</strong> rock and fluid temperatures respectively (K), p is<strong>the</strong> pore pressure (Pa). Superconvergent patch recovery (Zienkiewicz et al. 1992) is used to evaluatenodal stress tensors from <strong>the</strong> numerical results <strong>of</strong> nodal displacement, u.Fracture response to stimulationThe naturally fractured medium is pressurised by injecting fluid with a view to stimulate <strong>the</strong> reservoir.In practice, <strong>the</strong> fluid pressure develops gradually and some <strong>of</strong> <strong>the</strong> fractures may start propagatingbefore <strong>the</strong> fluid pressure reaches a threshold level at which shear slippage may takes place for alarge number <strong>of</strong> fractures.The shear slippage criterion similar to Rahman et.al (2000) is applied to identify fractures that arefavorable for shear slippage and dilation. When <strong>the</strong> fracture pressure becomes higher than <strong>the</strong> givenin-situ stress effective normal stress becomes negative and fractures open and surfaces no longerremain in contact. The shear displacement, U s in such condition can be expressed as:U s (1.6)nK swhere K s is <strong>the</strong> fracture shear stiffness and nis <strong>the</strong> access shear stress.The increase in fracture aperture due to shear dilation, a s can be expressed as (Willis-Richards,Watanabe et al. 1996):aseff U s tan( dil )(1.7)The total stimulated aperture can be expressed as (Muskat 1937):aa 19eff0nref as ares(1.8)where a res is <strong>the</strong> residual aperture that usually exists at high effective stress and is considered to bezero in this study. The normal effective stress, σ eff , is <strong>the</strong> resultant normal stress arising from <strong>the</strong>effects <strong>of</strong> induced pressure and <strong>the</strong>rmal contraction at <strong>the</strong> fracture surface. The total stimulatedaperture, a can finally be expressed by ma<strong>the</strong>matical manipulation as:aa0Us tan( dil) (1.9)19eff nrefThe above equation is used in <strong>the</strong> evaluation <strong>of</strong> permeability enhancement by numerical simulation <strong>of</strong>fluid flow within <strong>the</strong> stimulated fractured network.183


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Numerical algorithmThe algorithm <strong>of</strong> <strong>the</strong> design methodology is shown in Fig. 2. Initially, real field data, such as <strong>the</strong>fracture orientation, size and o<strong>the</strong>r fracture parameters that influence reservoir performance areacquired from <strong>the</strong> open literature.An analysis <strong>of</strong> hot water productivity in terms <strong>of</strong> well placement is performed for three wellconfigurations. Well location and distance between wells are chosen based on <strong>the</strong> Soultz EGSsystem and used to investigate common problems associated with development <strong>of</strong> EGS, such asshort circuiting and high pressure loss between injector and producer wells, and at <strong>the</strong> same time aperform a hydraulic stimulation program to provide sufficient permeability enhancement.For <strong>the</strong> configuration, <strong>the</strong> reservoir permeability is calculated based on <strong>the</strong> discrete fracture networkdata and fluid flow simulation. Then <strong>the</strong> injector is pressurised and <strong>the</strong> pore pressure, temperatureand stress tensor across <strong>the</strong> reservoir at each time step are evaluated. Shear slippage and dilationthat may occur as a result <strong>of</strong> change in local stress and pore pressure are determined and evaluated.Numerical results <strong>of</strong> stress and pore pressure are used to calculate current total aperture (accountingfor <strong>the</strong> contributions <strong>of</strong> fracture opening (mode I), shear dilation (mode II)) for every individual naturalfracture and update <strong>the</strong> permeability <strong>of</strong> <strong>the</strong> reservoir.Using <strong>the</strong>se results, reservoir simulation is carried out to calculate flow rates at <strong>the</strong> producers fordiscrete values <strong>of</strong> injector-producer pressure drops as well as temperature pr<strong>of</strong>iles <strong>of</strong> both <strong>the</strong> rockand fluid within <strong>the</strong> reservoir.Results and DiscussionIn <strong>the</strong> current <strong>the</strong>rmo-poroelastic numerical model, flow between <strong>the</strong> injection well and productionwells are assumed to be planar and is approximated through <strong>the</strong> open hole interval (3500m to 5100m)through a statistically representative trace. This is achieved by alteration <strong>of</strong> <strong>the</strong> fractal dimension,which is used to spatially distribute <strong>the</strong> fractures within a defined volume. A statisticallyrepresentative trace <strong>of</strong> <strong>the</strong> Soultz fracture network between a depth <strong>of</strong> 2500 m and 6000 m ispresented in Fig. 4 . The well placements on <strong>the</strong> plane are taken as <strong>the</strong>ir separation at a depth <strong>of</strong>4430m, which is midway through <strong>the</strong>ir depth-averaged open hole sections. The reservoir ispressurized by injecting fluid through <strong>the</strong> injection well (GPK2). To increase <strong>the</strong> injectivity, a pair <strong>of</strong> coplanarfractures <strong>of</strong> half length <strong>of</strong> 30m, is placed at <strong>the</strong> injection well. The pressurization was carriedout over a period <strong>of</strong> one year and <strong>the</strong> results recorded at different stages (8 weeks, 24 weeks, 40weeks and 52 weeks). During <strong>the</strong> pressurization, <strong>the</strong> change in fracture width for each individualnatural fracture and <strong>the</strong> resulting permeability tensor were calculated. Following stimulation <strong>of</strong> <strong>the</strong>reservoir, a flow test was carried out over a period <strong>of</strong> 14 years. During <strong>the</strong> flow test, changes infracture apertures due to <strong>the</strong>rmo-poro-elastic stresses and <strong>the</strong> consequent changes in permeabilitieswere determined. Also estimated was <strong>the</strong> <strong>the</strong>rmal drawdown <strong>of</strong> <strong>the</strong> Soultz EGS.184


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Effect <strong>of</strong> stimulation time on shear dilationResults <strong>of</strong> shear dilation are presented as average percentage increase in fracture aperture anddilation events with time (see Figs. 5 and 6a-6d). From Fig. 5, it can be seen that <strong>the</strong>re exists threedistinct aperture histories: 0-28 weeks, 28-42 weeks and greater than 42 weeks. Until about 28weeks, <strong>the</strong> rate <strong>of</strong> occurrence <strong>of</strong> dilation events due to induced fluid pressure <strong>of</strong> 10,000 psi(bottomhole) remains fairly constant. Following this time, <strong>the</strong> rate <strong>of</strong> occurrence increases sharplyuntil about 42 weeks, after which, no significant dilation events can be observed (a plateau <strong>of</strong> eventsis reached). This infers that for every set <strong>of</strong> reservoir and stress parameters as well as injectionschedule, a maximum level <strong>of</strong> shear dilation can be achieved.In Figs. 6a, 6b, 6c and 6d, <strong>the</strong> events <strong>of</strong> shear dilation at different stimulation times are presented.From <strong>the</strong>se figures, it can be seen that by 8 weeks, distribution <strong>of</strong> shear dilation events is relativelynon-uniform. This can be attributed to rapid propagation <strong>of</strong> pressure through well interconnectedfractures.As pressure continues to build up, more fractures are dilated in <strong>the</strong> vicinity <strong>of</strong> <strong>the</strong> active shear dilationfront (see Figs. 6c and 6d). In Fig. 7, permeability enhancement in <strong>the</strong> form <strong>of</strong> <strong>the</strong> root mean square(RMS) permeability tensor, at <strong>the</strong> end <strong>of</strong> 16 weeks and 42 weeks <strong>of</strong> stimulation, respectively, arepresented. The low initial permeabilities can be attributed to high in situ closure stresses in <strong>the</strong>reservoir. After 42 weeks <strong>of</strong> stimulation, reservoir permeability has been significantly increased, bothdue to pressure induced inflation (temporary) and shear dilation (retainable) <strong>of</strong> <strong>the</strong> fracture network.The RMS permeabilities local to <strong>the</strong> major fractures are roughly an order <strong>of</strong> magnitude greater after42 weeks <strong>of</strong> stimulation than after 16 weeks.Effect <strong>of</strong> well placement on reservoir stimulation and hot water productionAs shown in Fig. 4, <strong>the</strong> two production wells, GPK2 and GPK4 are separated from <strong>the</strong> injection well,GPK3, by roughly 480m and 440m respectively. During stimulation, <strong>the</strong> production wells are keptclosed. Once a desired stimulation is achieved at <strong>the</strong> end <strong>of</strong> <strong>the</strong> stimulation period (42 weeks) <strong>the</strong>fluid was circulated over a period <strong>of</strong> 14 years. During this circulation period, production rates fromeach well, fluid velocities throughout <strong>the</strong> reservoir produced fluid temperatures and average matrixtemperature drawdown were estimated. The production parameters are listed in Table 2. Results <strong>of</strong>hot water production over <strong>the</strong> 14 year circulation period after an initial 42 weeks <strong>of</strong> stimulation arepresented in Figs. 8 through 13.In Fig. 8, <strong>the</strong> RMS fluid velocities after 10 years <strong>of</strong> production are presented. It can be observed fromthis figure that <strong>the</strong>re exists distinct fluid flow paths connecting <strong>the</strong> injector and <strong>the</strong> producers. The flowpaths connecting <strong>the</strong> injector and GPK4 however, are not as prominent (not well connected) as that <strong>of</strong>GPK2. In addition, it can be observed that <strong>the</strong> fluid velocities are much greater for <strong>the</strong> 42 weekstimulation case than <strong>the</strong> 16 week stimulation case. Fluid velocities up to 1 x 10 -3 m/s through <strong>the</strong>major connected pathways is reached after 42 weeks which is three times higher than that after 16weeks <strong>of</strong> stimulation. In Fig. 9 , <strong>the</strong> reservoir temperature pr<strong>of</strong>ile after 10 years <strong>of</strong> production ispresented. It is apparent from <strong>the</strong> figure that <strong>the</strong> high flow rates experienced between <strong>the</strong> injector and185


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>producers (see Fig. 8) resulted in significant cooling <strong>of</strong> <strong>the</strong> reservoir rock along <strong>the</strong>se flow paths.Once <strong>the</strong>rmal breakthrough has taken place through to GPK2, <strong>the</strong> temperature <strong>of</strong> <strong>the</strong> produced fluidbegins to decline steadily. This <strong>the</strong>rmal breakthrough takes place at about 8 years <strong>of</strong> production (seeFig. 10 ). From Fig. 10, it can also be observed that <strong>the</strong> produced fluid temperature drops to about140 o C in well GPK2, while in well GPK4, <strong>the</strong> produced fluid temperature remains high after <strong>the</strong> sameperiod. The variation <strong>of</strong> produced fluid temperature from different wells is caused by several factors,namely, <strong>the</strong> number <strong>of</strong> hydraulically active flow paths between <strong>the</strong> injector and producer, <strong>the</strong> hydrauliclength <strong>of</strong> <strong>the</strong>se flow paths and <strong>the</strong> temperature difference between invading fluid and rock matrixalong <strong>the</strong>se flow paths. In general, a high number <strong>of</strong> flow paths originating from <strong>the</strong> injector, whichspan considerable distances before intersecting <strong>the</strong> producers, tends to delay <strong>the</strong> onset <strong>of</strong> <strong>the</strong>rmalbreakthrough (due a high heat-sweep efficiency). It may be noted from Fig. 10 that <strong>the</strong>rmalbreakthrough begins to occur at GPK4 at around 11 years.Effect <strong>of</strong> <strong>the</strong>rmally induced stresses on hot water productionIn Figs. 11a and 11b, <strong>the</strong> estimated reservoir impedances for two different degrees <strong>of</strong> stimulation arepresented. Stage I stimulation (Fig. 11a) is over 26 weeks and stage II stimulation (Fig. 11b) over 42weeks. As shown in Fig. 11b, <strong>the</strong> production rates at GPK2 increase rapidly for roughly one year andcontinue to increase but at a slower rate until about 8 years. Following this, a quasi steady stateproduction with fluctuations is reached. The initial production period <strong>of</strong> one year is characterized by asteep increase in production rate as pressure builds up through <strong>the</strong> well connected network <strong>of</strong>stimulated fractures. The steady increase in production after one year can be attributed to <strong>the</strong> cooling<strong>of</strong> <strong>the</strong> rock matrix which induces <strong>the</strong>rmal stresses (see Figs. 12a and 12b). These <strong>the</strong>rmal stressesconsequently increase permeability <strong>of</strong> <strong>the</strong> fractured network, leading to changes in <strong>the</strong> pressuredistribution and hence, <strong>the</strong> flow rates.The effective stresses in <strong>the</strong> reservoir rock at early production time (3 years) and late production time(10 years) are presented in Figs. 12a (x direction) and 12b (y direction). It should be noted again thata geomechanics sign convention is adopted for stresses (positive for compression). From both plots,it is apparent that <strong>the</strong> effective stresses in reservoir at late time (10 years) are significantly lesscompressive than those at early time. The decreases in effective stresses causes fracture dilation and<strong>the</strong>refore permeability enhancement. The continuous decrease in matrix temperature at an increasingrate can be observed in Fig. 13.Effect <strong>of</strong> level <strong>of</strong> stimulation on reservoir impedanceThe production flow rates at GPK2 were recorded for injector-producer pressure drops <strong>of</strong> 2000 psiand 1500 psi, for both stage I and II <strong>of</strong> stimulation. In Fig. 11a for <strong>the</strong> case <strong>of</strong> stage I stimulation, <strong>the</strong>production rates rise with time, until roughly 1.5 years, when a quasi-steady state pressure pr<strong>of</strong>ile isattained. At this point, a 2000 psi pressure drop results in a production rate <strong>of</strong> roughly 30L/s while a1500 psi pressure drop, roughly 16 L/s. Following this, <strong>the</strong> production rates continue to rise but at amuch slower rate which was explained in <strong>the</strong> previous section. Peak production <strong>of</strong> 43 L/s is observedwith a pressure drop <strong>of</strong> 2000 psi and 23 L/s with a pressure drop <strong>of</strong> 1500 psi.186


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>In Fig. 11b, <strong>the</strong> production rate as a function <strong>of</strong> time after 42 weeks <strong>of</strong> stimulation is presented. It canbe seen that <strong>the</strong> production rates with injector-producer pressure drops <strong>of</strong> 2000 psi and 1500 psi beara similar trend to <strong>the</strong> case <strong>of</strong> stage I stimulation. The production rates begin to reach quasi-steadystate (as observed in Fig. 11b) at around 1 year production time. Similarly, <strong>the</strong>rmally induced stressesincrease <strong>the</strong> production rates after this period for both cases <strong>of</strong> pressure drop. The production ratewith a pressure drop <strong>of</strong> 2000 psi peaks around 100 L/s and around 63 L/s with a pressure drop <strong>of</strong>1500 psi. The increased production rates were achieved by increasing <strong>the</strong> stimulation time from 26weeks to 42 weeks.ConclusionsIn this paper, a poro-<strong>the</strong>rmo-elastic reservoir model is developed and used to study <strong>the</strong> effects <strong>of</strong>induced fluid pressure and <strong>the</strong>rmal stresses (cooling effect) on reservoir permeability and consequentincrease in hot water production. The model is applied to <strong>the</strong> Soultz geo<strong>the</strong>rmal reservoir, France.The paper also investigates <strong>the</strong> effect <strong>of</strong> well placement on hot water production and <strong>the</strong>rmaldrawdown. From <strong>the</strong> results <strong>of</strong> this study, <strong>the</strong> following conclusions can be drawn.It has been shown that for every geo<strong>the</strong>rmal system <strong>the</strong>re exists an optimum injection schedule(injection pressure and duration). Fur<strong>the</strong>r increases in stimulation effort, i.e. stimulation time for agiven stimulation pressure, does not enhance any fur<strong>the</strong>r reservoir permeability. In this study, for abottomhole stimulation pressure <strong>of</strong> 10,000 psi, a stimulation time <strong>of</strong> 42 weeks has been foundoptimum.Fracture connectivity has a significant bearing on <strong>the</strong>rmal breakthrough, produced hot watertemperature, temperature drawdown and <strong>the</strong> hot water production rate. Also demonstrated, was <strong>the</strong>non-uniform spatial distribution <strong>of</strong> shear event occurrences with time.Thermal stresses induced during <strong>the</strong> circulation <strong>of</strong> cold water have a significant effect on <strong>the</strong> longterm production rate. As <strong>the</strong>rmal drawdown <strong>of</strong> <strong>the</strong> rock matrix takes place, tensile <strong>the</strong>rmal stressesare induced which allow residing fractures to dilate and enhance permeability. This graduallyincreases <strong>the</strong> fluid velocities between <strong>the</strong> injector and producer, yielding increasing production rateswith time.ReferencesBaria, R., Baumg¨artner, J., G´erard, A., Jung, R., Garnish, J., 1999. European HDR researchprogramme at Soultz-sous-Forˆets (France) 1987–1996. Geo<strong>the</strong>rmics 28, 655–669.Beeler, N. M., Wong, T. F. & Hickman, S. H., 2003. On <strong>the</strong> expected relationships among apparentstress, static stress drop, effective shear fracture energy, and efficiency. Bull. Seismol. Soc.Am. 93, 1381-1389.Beeler, N.M., Simpson, R.W., Hickman, S.H. and Lockner, D.A., 2000. Pore fluid pressure, apparentfriction, and Coulomb failure, J. Geophys. Res. 105, 25533– 25542.Gentier, S., Rachez, X., Ngoc, T. D. T., Peter-Borie, M. and Souque, C. (<strong>2010</strong>). "3D Flow Modelling <strong>of</strong><strong>the</strong> Medium-Term Circulation Test Performed in <strong>the</strong> Deep Geo<strong>the</strong>rmal Site <strong>of</strong> Soultz-Sousforets(France). <strong>Proceedings</strong> Worlf Geo<strong>the</strong>rmal Congress <strong>2010</strong> - Bali, Indonesia, 25-29 April<strong>2010</strong>.187


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Ghassemi, A. and G. Suresh Kumar (2007). "Changes in fracture aperture and fluid pressure due to<strong>the</strong>rmal stress and silica dissolution/precipitation induced by heat extraction from subsurfacerocks." Geo<strong>the</strong>rmics 36(2): 115-140.Ghassemi, A., Nygren, A., Cheng, A., 2008. Effects <strong>of</strong> heat extraction on fracture aperture:A poro–<strong>the</strong>rmoelastic analysis. Geo<strong>the</strong>rmics 37, 525–539.Jing, Z., J. Willis-Richards, et al. (2000). "A three-dimensional stochastic rock mechanics model <strong>of</strong>engineered geo<strong>the</strong>rmal systems in fractured crystalline rock." J. Geophys. Res. 105.Kumar, G.S. and Ghassemi, A., 2005. Numerical modeling <strong>of</strong> non-iso<strong>the</strong>rmal quartzdissolution/precipitation in a coupled fracture–matrix system. Geo<strong>the</strong>rmics 34 (2005) 411–439.McDermott, C.I. and Kolditz, O., 2006. Geomechanical model for fracture deformation underhydraulic, mechanical and <strong>the</strong>rmal loads. Hydrogeol. J. 14, 487–498.Muskat, M. (1937). The Flow <strong>of</strong> Homogeneous Fluids Through Porous Media, Edwards Publisher.Narayan, S. P., Z. Yang, et al. (1998). HDR reservoir development by fluid induced shear dilation: Anumerical study <strong>of</strong> <strong>the</strong> Soultz and <strong>the</strong> Cooper Basin granite rock. International Hot Dry Rock -Forum, Strasbourg, France.O’Sullivan, M.J., Pruess, K., Lippmann, M.J., 2001. Geo<strong>the</strong>rmal reservoir simulation. The state <strong>of</strong>practice and emerging trends. Geo<strong>the</strong>rmics 30 (4), 395–429.Rahman, M. K., M. M. Hossain, et al. (2000). "An analytical method for mixed-mode propagation <strong>of</strong>pressurized fractures in remotely compressed rocks." International Journal <strong>of</strong> Fracture 103(3):243-258.Rahman, M. K., M. M. Hossain, et al. (2002). "A Shear-Dilation-Based Model for Evaluation <strong>of</strong>Hydraulically Stimulated Naturally Fractured Reservoirs." Int. J. for Numerical and AnalyticalMethods in Geomech. 26(5).Sanyal, S. K., E. E. Granados, et al. (2005). An Alternative and Modular Approach to EnhancedGeo<strong>the</strong>rmal Systems. World Geo<strong>the</strong>rmal Congress 2005, Antalya, Turkey.Sausse, J., Desayes, C. and Genter, A. (2007). "From geological interpretation and 3D modelling to<strong>the</strong> characterization <strong>of</strong> <strong>the</strong> deep seated EGS reservoir <strong>of</strong> Soultz (France)." <strong>Proceedings</strong>European Geo<strong>the</strong>rmal Congress 2007, Unterhaching, Germany, May 30-June 1, 2007.Shaik, A. R., M. A. Aghighi, et al. (2008). "An Innovative reservoir simulator can Help Evaluate HotWater Production for Economic Development <strong>of</strong> <strong>Australian</strong> Geo<strong>the</strong>rmal reservoirs." GRCTransactions 32: 97-102.Shaik, A.R., Koh, J., Rahman, S. S., Aghighi, M. A. and Tran, N. H., 2009. Design and evaluation <strong>of</strong>well placement and hydraulic stimulation for economical heat recovery from enhancedgeo<strong>the</strong>rmal systems. GRC Annual Meeting October 4–7, 2009, conference proceedings.Tran, N., Z. Chen, et al. (2007). "Characterizing and modelling <strong>of</strong> fractured reservoirs with objectorientedglobal optimization." Journal <strong>of</strong> Canadian Petroleum Technology 46(3): 39-45.Willis-Richards, J., K. Watanabe, et al. (1996). "Progress toward a stochastic rock mechanics model<strong>of</strong> engineered geo<strong>the</strong>rmal systems." J. Geophys. Res. 101.Zhou, X. X., Ghassemi, A. and Cheng, A. H.-D., 2009. A three-dimensional integral equationmodel for calculating poro- and <strong>the</strong>rmoelastic stresses induced by cold water injection intoa geo<strong>the</strong>rmal reservoir. Int. J. Numer. Anal. Meth. Geomech. 2009; 33,1613–1640188


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Figures and TablesFig. 1. Schematic geological map <strong>of</strong> <strong>the</strong> Rhine Graben and location <strong>of</strong> <strong>the</strong> Soultz-sous-Forets EGS site (a and b). Locationand traces <strong>of</strong> <strong>the</strong> Soultz deep geo<strong>the</strong>rmal wells; solid lines correspond to well traces (b and c). (Sausse et al., 2006)189


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Fig 2. Flow chart describing <strong>the</strong> numerical procedure and integration between <strong>the</strong> various models.Fig. 3. Generated fracture network <strong>of</strong> <strong>the</strong> deep geo<strong>the</strong>rmal Soultz reservoir based on statistical data from Gentier et al.(<strong>2010</strong>).190


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Fig. 4. A Soultz natural fracture network trace wells GPK2, GPK3 and GPK4 open holes at 4430 m. Trace plotted forfractures with radius greater than 60 m.191


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Fig. 5. Increase in average fracture aperture (retainable) with stimulation time. Injection pressure is 10,000 psi.Fig. 6a. Cumulative shear dilation events in <strong>the</strong> fracture network after 8 weeks <strong>of</strong> stimulation (10,000 psi injection pressure)in a strike-slip stress regime. Marker sizes are proportional to <strong>the</strong> log <strong>of</strong> <strong>the</strong> event magnitudes.192


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Fig. 6b. Cumulative shear dilation events in <strong>the</strong> fracture network after 24 weeks <strong>of</strong> stimulation (10,000 psi injection BHFP) ina strike-slip stress regime. Marker sizes are proportional to <strong>the</strong> log <strong>of</strong> <strong>the</strong> event magnitudes.Fig. 6c. Cumulative shear dilation events in <strong>the</strong> fracture network after 40 weeks <strong>of</strong> stimulation (10,000 psi injection BHFP) ina strike-slip stress regime. Marker sizes are proportional to <strong>the</strong> log <strong>of</strong> <strong>the</strong> event magnitudes.193


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Fig. 6d. Cumulative shear dilation events in <strong>the</strong> fracture network after 52 weeks <strong>of</strong> stimulation (10,000 psi injection BHFP) ina strike-slip stress regime. Marker sizes are proportional to <strong>the</strong> log <strong>of</strong> <strong>the</strong> event magnitudes.194


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Fig. 7. Log10 RMS effective permeability pr<strong>of</strong>ile (magnitudes <strong>of</strong> diagonal terms) after 16 weeks (left) and 42 weeks (right) <strong>of</strong>stimulation with 10,000 psi injection pressure, pre-production phase.195


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Fig. 8. Log10 fluid RMS velocity pr<strong>of</strong>iles (magnitudes) after 10 years production for injector-producer pressure drops <strong>of</strong> 2000psi, stimulation time prior to running <strong>the</strong> production case was 16 weeks (left) and 42 weeks (right).196


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Fig. 9. Rock temperature pr<strong>of</strong>ile after 10 years production for a injector-producer pressure drops <strong>of</strong> 2000 psi. Blue indicatesrock at 80 o C and red indicates rock at 200 o C, stimulation time prior to running <strong>the</strong> production case was 16 weeks (left) and42 weeks (right).197


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Fig. 10. Produced fluid temperatures vs. production time for GPK2 and GPK4. Stimulation time prior to running <strong>the</strong>production case was 42 weeks.Fig. 11a. GPK2 production rates for injector-producer pressure drops <strong>of</strong> 2000 psi and 1500 psi over 15 years, with areservoir stimulation time <strong>of</strong> 26 weeks.198


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Fig. 11b. GPK2 production rates for injector-producer pressure drops <strong>of</strong> 2000 psi and 1500 psi over 15 years, with areservoir stimulation time <strong>of</strong> 42 weeks.Fig. 12a. Effective stresses in <strong>the</strong> x direction at 3 years (left) and 10 years (right) injection time. Stimulation time prior torunning <strong>the</strong> production case was 42 weeks.199


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Fig. 12b. Effective stresses in <strong>the</strong> y direction at 3 years (left) and 10 years (right) injection time. Stimulation time prior torunning <strong>the</strong> production case was 42 weeks.200


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Fig. 13. Average matrix temperature vs. production time for 1.2 km (North-South) by 1.0 km (East-West) block enclosingwells GPK2, GPK3 and GPK4. Stimulation time prior to running <strong>the</strong> production case was 42 weeks.Table 1. Characteristics <strong>of</strong> statistical fracture sets obtained from Gentier et al. (<strong>2010</strong>). Plane direction is measured positiveclockwise from North and dip positive downward from horizontal.201


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Rock PropertiesYoung’s modulus (GPa) 40Poisson’s ratio 0.25Density (kg/m 3 ) 2700Fracture basic friction angle (deg) 40Shear dilation angle (deg) 2.890% closure stress (MPa) 20In situ mean permeability (m 2 ) 9.0 x 10 ‐17Fracture propertiesFractal Dimension, D 1.2Fracture density (m 2 /m 3 ) 0.12Smallest fracture radius (m) 15Largest fracture radius (m) 250Stress dataMaximum horizontal stress (MPa) 53.3Minimum horizontal stress (MPa) 78.9Fluid propertiesDensity (kg/m 3 ) 1000Viscosity (Pa s) 3 x 10 ‐4Hydrostatic fluid pressure (MPa) 34.5Injector pressure, stimulation (MPa) 68.9Injector pressure, production (MPa) 44.8Producer pressure, stimulation N/AProducer pressure, production 31.0O<strong>the</strong>r reservoir dataWell radius (m) 0.1Number <strong>of</strong> injection wells 1Number <strong>of</strong> production wells 2Reservoir depth (m) 4430Table 2. Stress and reservoir data for strike-slip stress regime.202


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Status <strong>of</strong> <strong>the</strong> Paralana 2 Hydraulic Stimulation ProgramP. W. Reid *, L. McAllister * and M. Messeiller **Petra<strong>the</strong>rm Limited, 129 Greenhill Rd, Unley 5061, South AustraliaThe Paral ana Enginee red Geo<strong>the</strong> rmal Project i slocated 600 km north <strong>of</strong> t he city <strong>of</strong> Adelaid e inSouth Aust ralia (Fig ure 1). The p roject is te stingfor viable geo<strong>the</strong> rmal resou rces, within asedimentary basi n that lies immediatel y east <strong>of</strong>known high heat p roducing Me soproterozoicbasement rocks <strong>of</strong> <strong>the</strong> Mt Painter Regi on. In thisarea, 2D reflection sei smic su rvey data andpotential field geo physical (aeromagnetic,magneto-telluric and grav ity) data delineate amajor half graben info rmally termed <strong>the</strong> Poontan abasin. Based on <strong>the</strong> interpreted geophysical data,Petra<strong>the</strong>rm postulates t hat <strong>the</strong> hi gh he atproducing basement rocks o bserved i n out crop,continue under <strong>the</strong> in sulating cover material, with<strong>the</strong> maximum thickness <strong>of</strong> <strong>the</strong> sedim entary coverin section s <strong>of</strong> <strong>the</strong> Poo ntana Sub -basin beingmodeled at greater th an five kilom etres. Thi sfavourable arrangement <strong>of</strong> thick sedi mentsoverlying anomalously ra diogenic ba sementsuggests th at <strong>the</strong> Parala na a rea is an id eallocation to test <strong>the</strong> development <strong>of</strong> an EngineeredGeo<strong>the</strong>rmal System.Paralana 2 was de signed as an injector with <strong>the</strong>advantage <strong>of</strong> sim plifying <strong>the</strong> well d esign an dallowing learning from this well to be incorporatedinto <strong>the</strong> well design and planning <strong>of</strong> <strong>the</strong> productionwell (Pa ralana 3) to maximize <strong>the</strong> ch ances <strong>of</strong>achieving a commercial flow rate.During drilling <strong>of</strong> <strong>the</strong> l ower 8 ½” section severalfractures we re e ncountered b elow 34 00 m. H ightorques, drilling breaks, an increase in well-bor edeviation followe d by inflow <strong>of</strong> geoth ermal ove rpressurized brine s p rovide stro ng indi cations fo r<strong>the</strong> presence <strong>of</strong> a natu ral and permeable fracturesystem between d epths <strong>of</strong> about 3 690 m a nd3864 m. Increa sed rates <strong>of</strong> penetrati on duri ngdrilling through <strong>the</strong> fract ured zones indicate achange in ro ck strength p ossibly relate d to openfractures. Shut in pre ssures indi cated a noverpressure <strong>of</strong> app roximately 3,300 p si an d th emud system required weighting up to 1 3.2 ppg tostop <strong>the</strong> inflow, and allo w drilling to continu esafely.Petra<strong>the</strong>rm Limited in joint venture with a major oiland ga s (B each <strong>Energy</strong>) and po wer indu stryenergy utilities (T RUenergy) are initiall y see kingto build a 7.5 M We com mercial po werdevelopment to sup ply a local min e. In <strong>the</strong>second half <strong>of</strong> 2009 a deep geoth ermal wel l(Paralana 2) was drilled to 4012m. The well wa sdesigned as an inje ctor, <strong>the</strong> first <strong>of</strong> an initial twowell program to p rove circulation b etween wells.An innovative strategy for d evelopment <strong>of</strong> th eEGS re servoir i s pl anned, involving massiv ehydraulic stimulation <strong>of</strong> multiple ta rget zone swithin <strong>the</strong> sedimentary overburden. Multiple zonestimulation in creases th e cha nce <strong>of</strong> achieving acommercial flow rate which is <strong>the</strong> key commercialbarrier for EGS developments around <strong>the</strong> world.Keywords: EGS, Drilling, Fracture StimulationParalana 2 Well CompletionThe planned multizon e stimulation <strong>of</strong> Paralana 2involved <strong>the</strong> well being fully cased a nd cementedto allow better control on what intervals in <strong>the</strong> wellwould be stimulated in a cost effective manner. In<strong>the</strong> past, open hole hydraulic stimulations resultedin <strong>the</strong> main frac d eveloping at <strong>the</strong> zon e <strong>of</strong> leastresistance w hich is u sually at <strong>the</strong> base <strong>of</strong> th ecasing shoe (lowest pressure point) or a locationswhere large natural fractures already occur. Thisin effect leaves much <strong>of</strong> <strong>the</strong> open hole unaffectedby <strong>the</strong> stimulation pro gram. Being <strong>the</strong> first well,Figure 1: Regional Locality Map and extent <strong>of</strong> SAHFA(SAHFA modified from Neumann et. al . 2000)Due to wellbore stability problems <strong>the</strong>characterization <strong>of</strong> this zon e wa s limited tologging while drilling measurements down to 3740m depth. Th e final 7” casing stri ng was run to adepth <strong>of</strong> 3725 m as below this depth <strong>the</strong> well wastoo unstable to be abl e to set casing and cementin place (Figure 2).203


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Paralana 2 GeologyThe litho- stratigraphic and structural environment<strong>of</strong> <strong>the</strong> Paral ana Proj ect area i s co mplex andweakly con strained. T he interp retation <strong>of</strong> <strong>the</strong>stratigraphic succe ssion and litholo gy <strong>of</strong> <strong>the</strong>overlying Phanerozoic seq uences and <strong>the</strong>ircontact with <strong>the</strong> un derlying Adelai dean strata atParalana-2 i s based on <strong>the</strong> result s <strong>of</strong> drillingParalana-1B, drilled 1.5 km to west <strong>of</strong> P aralana-2.The Cambrian-Adelaidean un conformity isinterpreted at 1115m and <strong>the</strong> sequ ence b eginswith <strong>the</strong> A mberoona F m. The T apley HillFormation was e ntered a t 1612m in Paralana2and its co ntact with <strong>the</strong> unde rlying SturtianGlacials has been interpreted at about 1803m. At2855m, a 500mete rs thick haematicmetaquartzose with silice ous ce ment underlies<strong>the</strong> tillite and grades to a litharenite with depth. Itsage is am biguous, but <strong>the</strong> metase diment is stillconsidered as Ad elaidean, within t he Sturtia nTillite or <strong>the</strong> Callanna Beds.At 3397m, a major ch ange <strong>of</strong> lithology wa sobserved during <strong>the</strong> drilling, associated with a keyunconformity. It is related to a s trong reflec torobserved on <strong>the</strong> sei smic. Below th e co ntact, <strong>the</strong>lithologies a re mai nly compo sed <strong>of</strong> dolomiti csiltstones and sand stones, inte rbedded withnumerous intervals <strong>of</strong> felsic tuffs. Several dole ritehorizons a re intercalated i n <strong>the</strong> pa ckage, from adepth <strong>of</strong> 3450m to <strong>the</strong> bottom <strong>of</strong> <strong>the</strong> hole. Zirconsextracted from <strong>the</strong> volc anic tuff returned a207 Pb/ 208 Pb age <strong>of</strong> 1585±11Ma using a LA-ICPMStechnique at <strong>the</strong> University <strong>of</strong> Adelaide. At 3910m,Paralana 2 e ntered a felsi c intru sive, confirmin ghigh h eat p roduction rate <strong>of</strong> <strong>the</strong> basement <strong>of</strong>approximately 10 to 12µWm-3 , and showi ng asimilar Mesoproterozoic age <strong>of</strong> 1580±10Ma.Numerous intervals <strong>of</strong> fractures were encounteredin <strong>the</strong> lower zone <strong>of</strong> <strong>the</strong> well based oninterpretation <strong>of</strong> <strong>the</strong> logs and expe rienced during<strong>the</strong> drilling operation. A more complex tectoni chistory an d <strong>the</strong> pre sence <strong>of</strong> dole rite in <strong>the</strong>sequence are indi cated by a chaoti c seismi csignature bel ow 3400m. The thi ck h omogenousquartzite ove rlying <strong>the</strong> ba sal sequ ence is highlycompetent with rock stre ngths rangi ng betwee n16,000 (110MPa) an d 2 9,000 p si (2 00MPa) ascalculated fro m <strong>the</strong> sonic l ogs. T his u nit may beconsidered to act a s a to p seal to <strong>the</strong> fractured,overpressured unit below.MEQ arrayThe Paralana Micro-seismic monitoring array hasbeen op erational sin ce A pril 200 8, recordin g <strong>the</strong>background seismi city at <strong>the</strong> Paralan aGeo<strong>the</strong>rmal Project site. The array ha s re centlybe up-graded to a real-time monitoring network toenable Petra<strong>the</strong>rm and <strong>the</strong> joint ventu re partnersto actively re cord, analyse a nd lo catemicroseismic events duri ng <strong>the</strong> stimulation <strong>of</strong> <strong>the</strong>geo<strong>the</strong>rmal reservoir. Th e gro wth <strong>of</strong> <strong>the</strong> fractu renetwork during fr acture stimul ation will bemonitored by sei smologists from <strong>the</strong> I nstitute <strong>of</strong>Earth S cience an d En gineering, Au ckland, NewZealand. The array combines sensitive downholesondes with surface seismometers to enable th einterpretation <strong>of</strong> a wide spe ctrum <strong>of</strong> seismi cevents. All events will be analyse d, with autopickings<strong>of</strong>tware, MIMO, develope d by <strong>the</strong>Norwegian S eismic Array (NORSA R), providi ngdata on <strong>the</strong> event location and magnitude.Figure 2: Paralana Well Completion and Geological log.Stimulation ProgramThe initial stimulation program is to be undertakenin two stages. The Stage 1 Injectivity test involvesperforation <strong>of</strong> <strong>the</strong> steel casing near <strong>the</strong> bottom <strong>of</strong><strong>the</strong> Paral ana 2 well and injectio n <strong>of</strong> a sm allvolume <strong>of</strong> water to co nfirm fractu re ini tiation andpropagation. The test aim s to de rive informatio n<strong>of</strong> <strong>the</strong> insitu stre ss regime, re servoir prop ertiesand determine if <strong>the</strong> well i s already connected t<strong>of</strong>ractures <strong>of</strong> <strong>the</strong> n atural overp ressured zoneencountered during drilling.The Stage 2 fracture stimulation involves injection<strong>of</strong> large r vol ume <strong>of</strong> wate r at highe r rates. Th estimulation aims to create a fracture network andconnect to and e nhance <strong>the</strong> existi ng natu ralfracture network intersected lower in <strong>the</strong> well. Thestimulation also aims to generate significant microseismic events, mea sured by <strong>the</strong> MEQ array,greater th an 500 m etres f rom th e well bore. Thevolume and rate <strong>of</strong> <strong>the</strong> stimulation will bedependent o n <strong>the</strong> micro-sei smic response an dadjusted to meet <strong>the</strong> o bjectives. A se ries <strong>of</strong>stepped inje ction rate te sts are pla nned du ring204


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong><strong>the</strong> stimulation to observe <strong>the</strong> development <strong>of</strong> <strong>the</strong>fracture network. Post <strong>the</strong> main water stimulation,tests will be performed to determine <strong>the</strong> injectivityflow rates. T his will be f ollowed by productiontesting if th e well allo ws, to un derstand lo ngerterm reservoir performance. Acidizing and u se <strong>of</strong>proppant wit h gel in <strong>the</strong> fracture sti mulation iscontingent o n data obtai ned from th e injectivitytest. A se cond inte rval may be stimulateddependent on <strong>the</strong> results <strong>of</strong> <strong>the</strong> initial stimulation.ReferencesNeumann, N. , Sandiford, M., & Fode n, J. (2000)Regional geochemistry and continental heat flow:implications for <strong>the</strong> o rigin <strong>of</strong> <strong>the</strong> South Australi anHeat Flow anomaly. Earth and Planetary ScienceLetters, 183, 107-120.205


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Three Dimensional Reservoir Simulations <strong>of</strong> Supercritical CO 2 EGSAlvin I. Remoroza 1 *, Behdad Moghtaderi 1 , Elham Doroodchi 11 Priority Research Centre for <strong>Energy</strong>, School <strong>of</strong> Engineering (Chemical Eng.), Faculty <strong>of</strong> Engineering & BuiltEnvironment, University <strong>of</strong> NewcastleUniversity Drive, Callaghan, NSW 2308, Australia*Corresponding author: remorozaair@yahoo.comFollowing <strong>the</strong> work <strong>of</strong> Pruess (2008) on <strong>the</strong>production behaviour <strong>of</strong> CO 2 as a working fluid inEGS, a three dimensional (3D) reservoirsensitivity analysis <strong>of</strong> CO 2 mass flow and heatextraction rates on injection temperature, rockpermeability, rock porosity and reservoirtemperature were performed. The 3D reservoirsimulations were performed using <strong>the</strong> TOUGH2modelling code with <strong>the</strong> modified ECO2N module.Keywords: CO 2 -EGS, reservoir simulation,TOUGH2, ECO2NBackground <strong>of</strong> <strong>the</strong> studyThe literature on <strong>the</strong> application <strong>of</strong> supercriticalCO 2 for Engineered Geo<strong>the</strong>rmal System (EGS) isrelatively scarece. Most <strong>of</strong> <strong>the</strong> available literatureare 1D and 2D simulations <strong>of</strong> <strong>the</strong> <strong>the</strong>rmodynamicand transport properties as well as exergyanalysis (Atrens et al, 2008; Atrens et al, 2009;Atrens et al, 2009; Brown et al, 2000; Pruess etal, 2006; Reichman et al, 2008; Remoroza et al,2009).Pruess (2008) performed 2D and 3D reservoirsimulations <strong>of</strong> injection/production behaviour <strong>of</strong> anEGS operated with CO 2 as working fluid usingTOUGH2 with fluid property module “EOSM”which is not commercially available. Hissimulations examine production behaviour in 2Dareal model at different reservoir pressures and<strong>the</strong>n assessed 3D flow effects on energyrecovery. Table 1 lists <strong>the</strong> reservoir and CO 2injection parameters used by Pruess (2008) andin this study.The equivalent permeabilities calculated from <strong>the</strong>Soultz granite inferred from geophysical and flowlog analysis range from 5.2 x10 -17 m 2 to 9.6x10 -16m 2 (Sausse et al, 2006) while intact granite has1.6 to 3.8x10 -19 m 2 permeabilities (Selvadurai,2005). Soultz EGS average equivalentpermeability is 5x10 -16 m 2 .Porosities <strong>of</strong> granite range from 0.2 to 4%(http://www.granite-sandstone.com/granitephysical-properties.html).This study will expand <strong>the</strong> previous 3D reservoirsimulations <strong>of</strong> Pruess (2008) by determining <strong>the</strong>impact <strong>of</strong> injection and reservoir parameters suchas permeability, porosity, reservoir temperatureand CO 2 injection temperature on <strong>the</strong> CO 2 massflow and heat extraction rates. Also, <strong>the</strong>applicability <strong>of</strong> <strong>the</strong> modified fluid property moduleECO2N for EGS will be examined.Table 1. Reservoir and CO2 injection/production parameters.Pruess (2008) This studyFormationThickness, m 305 (5 layers) 305 (5 layers)Fracture spacing, m 50 50Permeable volume fraction 2% 2%Permeability in fracture 50 0.5, 5 and 50domain, x10x10 -15 m 2Nos. <strong>of</strong> MINC 5 5Porosity in fracture domain 50% 50%Permeability in rock 50 0.5, 5 and 50matrix, x10x10 -15 m 2Porosity in rock matrix 0.2%, 2%Rock grain density, kg/m 3 2650 2650Rock specific heat, kJ/kg 1000 1000Rock <strong>the</strong>rmal conductivity, 2.1 2.1W/m- o CInitial conditionsReservoir fluid CO2, H2O CO2, H2OTemperature, o C 200 200, 225Pressure, bar 200 200Production/InjectionProduction area, km 2 1 1Fraction <strong>of</strong> <strong>the</strong> area 1/8 1/4modelledSpatial resolution, m 32.14 and 70.1 20.83, 45.45Injection Temperature, o C 20 20, 35Injection pressure, bar 210 gravityequilibratedfrom top layer210 gravityequilibratedfrom top layerProduction pressure, barMethodology190 gravityequilibratedfrom top layer190 gravityequilibratedfrom top layerBecause <strong>the</strong> fluid property module used in <strong>the</strong>only published 3D reservoir modelling <strong>of</strong> CO 2flows in EGS is not publicly available; a modifiedECO2N fluid property module is used in <strong>the</strong>present study. ECO2N is a fluid property modulefor <strong>the</strong> TOUGH2 simulator (Version 2.0) that wasdesigned for applications to geologicsequestration <strong>of</strong> CO 2 in saline aquifers (Pruess,2005). The temperature limitation <strong>of</strong> this module is10 o C≤ T ≤ 100 o C. In <strong>the</strong> modified version <strong>of</strong>ECO2N <strong>the</strong> restriction on <strong>the</strong> upper temperatureis removed with <strong>the</strong> provision that only pure206


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>phases like CO 2 or H 2 O are present (i.e. nomixture).The 3D simulations in this study were conductedusing TOUGH2 in conjunction with <strong>the</strong> pre andpost-processing graphical interface PetraSim.Because <strong>of</strong> symmetry, only ¼ <strong>of</strong> <strong>the</strong> calculationdomain (1 km 2 five-spot well configuration) wassimulated in this study (Figure 1). Also, a modifiedCO2TAB file was used so that wider ranges <strong>of</strong>pressure and temperature, which are moreappropriate for EGS application, can be studied.CO2TAB lists <strong>the</strong>rmodynamic properties <strong>of</strong> CO 2 atdifferent temperature-pressure conditions whichare <strong>the</strong>n used by TOUGH2.to all layers (Figure 4) and open only to topmost50 m layer (Figure 5).Figure 2: The CO2 mass and heat extraction rates from thisstudy match <strong>the</strong> previous study for a CO2 production wellopen in all six layers using <strong>the</strong> ¼ symmetric model having12x12 areal grids and rock matrix permeability <strong>of</strong> 1.9x10 -14m 2 and porosity <strong>of</strong> 0.2%.Figure 1: The 1/4 section <strong>of</strong> <strong>the</strong> five-spot well configurationshowing an injection-production segment.To validate <strong>the</strong> use <strong>of</strong> <strong>the</strong> modified ECO2N, <strong>the</strong>result <strong>of</strong> <strong>the</strong> previous 3D reservoir simulationswere duplicated by finding <strong>the</strong> appropriate gridsize equivalent to <strong>the</strong> previous model used byPruess (2008). The previous study did not definerock wall specifications in <strong>the</strong> definition <strong>of</strong> fracturedomain, i.e. permeability and porosity <strong>of</strong> <strong>the</strong> rockmatrix. In <strong>the</strong> first attempt, different permeabilitieswere used for fracture domain and rock matrix(wall rock). A match was found for configurationwhere all layers <strong>of</strong> <strong>the</strong> production wells are openusing a 12x12 areal grid (41.67 m side length)and rock matrix permeability <strong>of</strong> 1.9x10 -14 m 2 andporosity <strong>of</strong> 0.2% (Figure 2). However, forconfiguration where only <strong>the</strong> top 50 m <strong>of</strong> <strong>the</strong>production well is open, <strong>the</strong> 12x12 areal grids <strong>of</strong><strong>the</strong> ¼ symmetric model gives higher mass andheat extraction rates (Figure 3).Doubling <strong>the</strong> areal grid size to 24x24 (20.83 sidelength) and defining rock matrix permeabilityequal to fracture domain permeability (5x10 -14 m 2 )and rock matrix porosity to 0.2% gave an almostperfect match both for CO 2 production well openFigure 3: The CO2 mass and heat extraction rates from thisstudy are higher than <strong>the</strong> previous study for a CO2production well open only in topmost 50 m layer using a ¼symmetric model having 12x12 areal grids and rock matrixpermeability <strong>of</strong> 1.9x10 -14 m 2 and porosity <strong>of</strong> 0.2%.The reservoir simulation results from <strong>the</strong> ¼symmetric model with 24x24 areal grid size was<strong>the</strong>n used as <strong>the</strong> reference for sensitivity analysis.The result from this section <strong>of</strong> <strong>the</strong> study alsoproved <strong>the</strong> applicability <strong>of</strong> modified ECO2N forreservoir simulation <strong>of</strong> pure phase CO 2 reservoirflows.Figure 4: CO2 mass and heat extraction rates from a ¼symmetric model having 24x24 areal grids and rock matrix207


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>permeability <strong>of</strong> 5x10 -14 m 2 and porosity <strong>of</strong> 0.2% match <strong>the</strong>previous study from a CO2 production well open in all sixlayers.The 35 o C injection temperature is more or less<strong>the</strong> appropriate value for regions with arid climatelike Australia’s EGS locations.Figure 5: CO2 mass and heat extraction rates using a ¼symmetric model having 24x24 areal grids and rock matrixpermeability <strong>of</strong> 5x10-14 m2 and porosity <strong>of</strong> 0.2% match <strong>the</strong>previous study from a CO2 production well open only intopmost 50 m layer.Results and DiscussionThe high CO 2 mass circulation at a reservoirtemperature <strong>of</strong> 200 o C for a production well opento all layers initially resulted in very high heatextraction rates and rapid decline <strong>of</strong> <strong>the</strong> reservoir<strong>the</strong>rmal content (144 MW to 47 MW) due to<strong>the</strong>rmal depletion <strong>of</strong> <strong>the</strong> reservoir. In contrast,H 2 O mass circulation was found to be low with arelatively slow decline rates and consequentlyslow decline in heat extraction rates (24 MW to 16MW, Figure 6). However, as <strong>the</strong> previous studyrecommended, for <strong>the</strong> case <strong>of</strong> CO 2 EGS whenonly <strong>the</strong> topmost 50 m layer configuration (Figure5) was used in <strong>the</strong> analysis stable massproduction and heat extraction rate <strong>of</strong> 64 MWafter 2 years were resulted.Figure 7: Effect <strong>of</strong> injection temperature on CO2 mass andheat extraction rates in a 200 o C EGS reservoir.Rock matrix permeability has dramatic effect onCO 2 mass production. In our studies <strong>the</strong> massproduction rates dropped from ~400 to 185 and29 kg/s when one and two orders <strong>of</strong> magnitudedecrease in permeability was implemented,respectively. Heat extraction rate, on <strong>the</strong> o<strong>the</strong>rhand, declined to 67 and 11 MW, respectively(Figure 8).Figure 8: Effect <strong>of</strong> rock matrix permeabilities on CO2 massproduction and heat extraction rates.Rock matrix porosity has no significant effect on<strong>the</strong> CO 2 mass production and heat extractionrates (Figure 9).Figure 6: CO2 and H2O pure phase mass and heat extractionrates at 200 o C reservoir.The effect <strong>of</strong> injection temperature on CO 2 massand heat extraction rates is shown in Figure 7.Increase in injection temperature above <strong>the</strong>critical temperature (31.4 o C) resulted in highermass production but lower heat extraction rates.208


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Figure 9: Effect <strong>of</strong> rock matrix porosity on CO2 massproduction and heat extraction rates.The average CO 2 mass flow rates did not varygreatly with reservoir temperature (411 kg/s at200 o C, 398 kg/s at 225 o C, and 395 kg/s at175 o C). Average heat extraction rates for <strong>the</strong> 200and 225 o C reservoir temperatures were found tobe similar at 117 and 113 MW, respectively.However, at low reservoir temperature, <strong>the</strong>average heat extraction rate decreased to about90 MW (Figure 10).Figure 10: Effect <strong>of</strong> reservoir temperature on CO2 massproduction and heat extraction rates.ReferencesSomerville, M., Wyborn, D., Chopra, P., Rahman,S., Estrella, D. and Van der Meulen, T., 1994, HotDry Rocks Feasibility Study, <strong>Energy</strong> Researchand Development Corporation, Report 243,133pp.Atrens, Al.D., Gurgenci, H., and Rudolph, V.,2008, Carbon Dioxide ThermosiphonOptimisation, Paper presented at <strong>the</strong> <strong>Proceedings</strong><strong>of</strong> <strong>the</strong> Sir Mark Oliphant International Frontiers <strong>of</strong>Science and Technology <strong>Australian</strong> Geo<strong>the</strong>rmal<strong>Energy</strong> <strong>Conference</strong>, Rydges Hotel, Melbourne.Atrens, Al.D., Gurgenci, H., and Rudolph, V.,2009a, CO 2 Thermosiphon for CompetitiveGeo<strong>the</strong>rmal Power Generation. <strong>Energy</strong> & Fuels,23(1), 553-557.Atrens, Al.D., Gurgenci, H., and Rudolph, V.,2009b, Exergy Analysis Of A Co 2 Thermosiphon,Paper presented at <strong>the</strong> PROCEEDINGS, Thirty-Fourth Workshop on Geo<strong>the</strong>rmal ReservoirEngineering, Stanford University, Stanford,California.Brown, D.W, 2000, A Hot Dry Rock Geo<strong>the</strong>rmal<strong>Energy</strong> Concept Utilizing Supercritical CO 2Instead Of Water, Paper presented at <strong>the</strong>PROCEEDINGS, Twenty-Fifth Workshop onGeo<strong>the</strong>rmal Reservoir Engineering, StanfordUniversity, Stanford, California.Pruess, K., 2008, On production behavior <strong>of</strong>enhanced geo<strong>the</strong>rmal systems with CO 2 asworking fluid, <strong>Energy</strong> Conversion & Management,49(6), 1446-1454.Pruess, K., and Azaroual, M., 2006, On TheFeasibility Of Using Supercritical CO 2 As HeatTransmission Fluid In An Engineered Hot DryRock Geo<strong>the</strong>rmal System, Paper presented at <strong>the</strong>PROCEEDINGS, Thirty-First Workshop onGeo<strong>the</strong>rmal Reservoir Engineering, StanfordUniversity, Stanford, California.Pruess, K., 2005. ECO2N: A TOUGH2 FluidProperty Module for Mixtures <strong>of</strong> Water, NaCl, andCO 2 . Report LBNL-57952. Earth SciencesDivision, Lawrence Berkeley National Laboratory:Berkeley, University <strong>of</strong> California.Reichman, J., Bresnehan, R., Evans, G., andSelin, C., 2008, Electricity Generation usingEnhanced Geo<strong>the</strong>rmal Systems with CO2 as HeatTransmission Fluid . 189. Paper presented at <strong>the</strong>Proceeding <strong>of</strong> <strong>the</strong> Sir Mark Oliphant InternationalFrontiers <strong>of</strong> Science and Technology <strong>Australian</strong>Geo<strong>the</strong>rmal <strong>Energy</strong> <strong>Conference</strong>, Rydges Hotel,Melbourne.Remoroza, A.I., Moghtaderi, B., and Doroodchi,E., 2009, Power Generation Potential <strong>of</strong> SC-CO 2Thermosiphon for Engineered Geo<strong>the</strong>rmalSystems, Paper presented at <strong>the</strong> <strong>Australian</strong>Geo<strong>the</strong>rmal <strong>Energy</strong> <strong>Conference</strong> 2009, HiltonHotel Brisbane.Sausse, J., Fourar, M., and Genter, A. 2006Permeability and alteration within <strong>the</strong> Soultzgranite inferred from geophysical and flow loganalysis. Geo<strong>the</strong>rmics, 35(5-6), 544-560.Selvadurai, A. P. S., Boulon, M. J., and Nguyen,T. S., 2005, The Permeability <strong>of</strong> an Intact Granite.Pure and Applied Geophysics, 162(2), 373-407.209


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Measuring <strong>the</strong> Success <strong>of</strong> EGS Projects: An Historical toPresent Day PerspectiveCa<strong>the</strong>rine E. Stafford*Granite Power Ltd, Level 6, 9 Barrack Street, Sydney, NSW 2000.*Corresponding author: cstafford@granitepwr.comWorld wide, Enhanced Geo<strong>the</strong>rmal System (EGS)projects have been a round for over 35 years,commencing w ith <strong>the</strong> Fenton H ill research anddevelopment project in New Mexico back in 1972.Many years <strong>of</strong> knowledge have been accumulatedthrough various research a nd commercialprojects.As to be expected with an evolving industry, somesignificant development issues are still to be fullyor properly overcome, such as a ppropriate downwelltechnolo gies a nd ma nagement <strong>of</strong> induce dseismicity. H owever, sev eral f actors i ndicate t hatthis ‘ne w’ typ e <strong>of</strong> ge o<strong>the</strong>rmal technol ogy and it sassociated industry has moved beyond being justa re search and d evelopment concept. Su chfactors incl ude: <strong>the</strong> gro wth in <strong>the</strong> numbe r <strong>of</strong>commercial p rojects, with some <strong>of</strong> <strong>the</strong>se now i nproduction; ceme nting o f <strong>the</strong> indu stry throug hassociations and governm ent incen tives; <strong>the</strong>development <strong>of</strong> geoth ermal re porting cod es forcommercial credibility (i.e. <strong>Australian</strong> andCanadian); and con siderable progre ss in <strong>the</strong>resolution <strong>of</strong> ongoing development issues.This paper provides a perspective on <strong>the</strong> success<strong>of</strong> EGS projects to date. Th is is very much a firstpassassessment as <strong>the</strong> te chnical an dcommercial data publicly available is currently toosparse an d project spe cific to ena ble a rigo rousquantitative study at thi s stage. However, it i sintended to <strong>of</strong>fer a snapshot take on <strong>the</strong> successand evolution to d ate <strong>of</strong> <strong>the</strong> EGS se ctor <strong>of</strong> <strong>the</strong>geo<strong>the</strong>rmal industry. It reveals that m any projectshave be en successful at what th ey set out t oachieve. It is also apparent that EGS developmentin Au stralia is like ly to b e mo re ‘su ccessful’ thanelsewhere because <strong>the</strong> continent’s stress regimeallows fav ourable sub-horizontal fractu redevelopment.Keywords: Enhan ced geo <strong>the</strong>rmal system, EGS,hot dry rock, HDR, success, industry, Hot RockDefinition <strong>of</strong> EGSGeo<strong>the</strong>rmal power ha s been g enerated fromhydro<strong>the</strong>rmal geo<strong>the</strong> rmal resou rces for man ydecades. However, such resources are limited toareas where accessible hydro<strong>the</strong>rmal systems arefound, such as <strong>the</strong> world’s volca nic regions e.g.<strong>the</strong> Pacific Rim countries.Geo<strong>the</strong>rmal exploration in all area s requires abalance <strong>of</strong> a ccessible te mperature, water supplyand an a dequate flow rate in ord er to produ ceelectricity economi cally. Wate r may have to b eintroduced to <strong>the</strong> system or may be p resent. Ingeo<strong>the</strong>rmal plays away from conventionalgeo<strong>the</strong>rmal t erranes, re quired te mperatures willlikely b e f ound at g reater d epth whe repermeability is <strong>of</strong>ten decr eased (tight rocks), soreservoir enh ancement by physical or chemi calmeans is required to obt ain flow rate s that areconsidered economic.Over <strong>the</strong> years <strong>the</strong> concept <strong>of</strong> enha ncedgeo<strong>the</strong>rmal reservoirs h as be en d escribed withseveral acronyms e.g. Hot Dry Rocks (HDR), HotWet Rocks (H WR), Hot Fractured Roc ks (H FR)and HR (Hot Rocks). Such p rojects havecomprised <strong>the</strong> artificial creation <strong>of</strong> an undergroundheat exch anger by <strong>the</strong> drilli ng <strong>of</strong> a we ll into e.g.granite, th e stimulation o f that well to create areservoir (usually by hy draulic stimul ation a nd/orchemical sti mulation), and <strong>the</strong> drilling <strong>of</strong> aproducer well into <strong>the</strong> margi n <strong>of</strong> <strong>the</strong> create dreservoir.In <strong>the</strong> last few years EGS has be come <strong>the</strong> mostaccepted de scriptor in th e north ern hemisphere.Recent definitions include:- “EGS are a new type <strong>of</strong> geo<strong>the</strong>rmal powertechnologies that do not require naturalconvective hydro<strong>the</strong>rmalresources.”(en.wikipedia.org/wiki/Enhanced_Geo<strong>the</strong>rmal_Systems)“EGS are engineered reservoirs created toproduce energy from geo<strong>the</strong>rmal resourcesthat are o<strong>the</strong>rwise not economical due to lack<strong>of</strong> water and/or permeability.” Department Of<strong>Energy</strong>, USA:http://www1.eere.energy.gov/geo<strong>the</strong>rmal/enhanced_geo<strong>the</strong>rmal_systems.html)“An Enhanced Geo<strong>the</strong>rmal System is anunderground reservoir that has been createdor improved artificially.” TP GEOELEC: <strong>the</strong>newly formed GEOELEC-Platform, waslaunched on 2nd <strong>of</strong> December 2009, andcomprises more than 130 geo<strong>the</strong>rmal expertsfrom <strong>the</strong> industry and <strong>the</strong> research sector whovoted on <strong>the</strong> definition <strong>of</strong> EGS in March <strong>2010</strong>.The secretariat <strong>of</strong> <strong>the</strong> panel is managed by <strong>the</strong>European Geo<strong>the</strong>rmal <strong>Energy</strong> Council.(http://www.egec.org/ETP%20Geoelec/Conclusion%20EGS%20definition.pdf)This late st definition, would i nclude allconventional geoth ermal well s th at have b eenstimulated to improve reservoir performance.210


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>During <strong>the</strong> developm ent <strong>of</strong> <strong>the</strong> Geo<strong>the</strong> rmalIndustry Technology Roadmap (DRET, 2008) <strong>the</strong><strong>Australian</strong> community recognised that t erms suchas HFR, HDR and HWR were ra<strong>the</strong>r specific, andthat EGS coul d be a pplied to g eo<strong>the</strong>rmalresources with significant existing permeability.Therefore th e term Hot Rock was a dopted toencompass that end <strong>of</strong> <strong>the</strong> spectrum <strong>of</strong>geo<strong>the</strong>rmal resources th at requi red signifi cantpermeability enhan cement. The term HotSedimentary Aquifers is applied to that end <strong>of</strong> <strong>the</strong>spectrum where si gnificant permeability existsnaturally.Here we co nsider <strong>the</strong> success <strong>of</strong> enhancedgeo<strong>the</strong>rmal system s, with focus o n th eunconventional (non-volcanic related) systems.The Rapid Growth <strong>of</strong> <strong>the</strong> EGS SectorThis preliminary (and non-exhaustive) review hasfound that to date <strong>the</strong>re a re in exist ence, or no wterminated, some fo rty-seven EGS projects (tomid Ju ne 2 010). Th ese proje cts a re listed inTable 1.The data presented i n this com pilation issomewhat incomplete, has been variably sourcedand as a result accuracy cannot be guaranteed. In<strong>the</strong> time-frame available for this preliminary study,project data was <strong>of</strong>ten dif ficult to acqui re o r wa snot acquired. It is re cognised that such omissionsimpact on <strong>the</strong> resul ts and he nce, an yinterpretation <strong>of</strong> those results. For example, it maybe more li kely that <strong>the</strong> re is non -publicity forunsuccessful proje cts or unsucce ssful part s <strong>of</strong>projects. A more rigo rous study is certainlyneeded but at thi s stage <strong>of</strong> <strong>the</strong> indu stry’sdevelopment may not b e po ssible due to <strong>the</strong>limited and site specific nature <strong>of</strong> <strong>the</strong> data.The data sh ow that over <strong>the</strong> last four deca des,over 50% (27) <strong>of</strong> <strong>the</strong> EGS projects commenced in<strong>the</strong> last 5 years (Figure 1 and Table 1 ). Over <strong>the</strong>whole <strong>of</strong> <strong>the</strong> last decade 78% (37) o f <strong>the</strong> tota lprojects were comm enced (Figu re 1 ) with overhalf <strong>of</strong> <strong>the</strong>se proj ects bei ng comme rcially funde das op posed to demon stration or R& D proj ects(Table 1).Conversely, durin g <strong>the</strong> 1 970’s, 80’ s and 90’sprojects were predomi nantly re search-driven(Table 1).The huge growth in <strong>the</strong> n umber <strong>of</strong> pro jects seenover <strong>the</strong> la st five years indicates that confidencein th is se ctor ha s g rown r apidly. T his can beattributed to <strong>the</strong> kno wledge a nd acquired skill sgained from <strong>the</strong> early proje cts, t echnologydevelopment e.g. drilling deeper being moreFigure 1: Bar chart showing <strong>the</strong> number <strong>of</strong> EGS projectscommenced from 1970 to <strong>2010</strong>.easily attain ed and with less ri sk, governm entpolicy an d to <strong>the</strong> perceive d su ccess <strong>of</strong> previou sprojects.Indicators <strong>of</strong> SuccessIn a mature EGS industry, success would likely bemeasured by <strong>the</strong> amount <strong>of</strong> powe r pro duced i.e.in megawatts. However, relatively little d ata is yetavailable wit h only a modest num ber <strong>of</strong> project swell develop ed. Thus, measuri ng succe ss isdifficult at this stage. However, it is suggested thateven a p reliminary evalu ation is u seful as a to olfor all concerned.A broa d-brush a ssessment is presented he relooking at tech nical su ccess a nd commercia lsuccess <strong>of</strong> proje cts, with <strong>the</strong>se bei ng definedbelow.In terms <strong>of</strong> th e development <strong>of</strong> <strong>the</strong> ind ustry, <strong>the</strong>reare many oth er fa ctors, which a re not discussedhere, that ca n be indi cative <strong>of</strong> <strong>the</strong> growth <strong>of</strong> <strong>the</strong>geo<strong>the</strong>rmal industry as a whole, as well as for <strong>the</strong>EGS se ctor. The se incl ude: a cceptance <strong>of</strong> ri skand risk ma nagement; wide ap plication <strong>of</strong> th etechnology; governm ent suppo rt via grants;geo<strong>the</strong>rmal studies; legislation; se rvice indu strysupport via dedi cated group s and re search anddevelopment; numbe r <strong>of</strong> R&D/de monstrationprojects; number <strong>of</strong> commercial projects.211


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Start Where Region Project WhoTable 1: EGS Projects Identified, as <strong>of</strong> Mid-June <strong>2010</strong>SuccessPurposeStatusTechnicalCommercialReservoir rockDepthTemperatureProductiontemperaturePoweroutputMain source Commentkmo Co C MW1 1972 USA NM Fenton Hill R TE Y Y Granite 3.5 195 158 3 1, 7 Producing power for >20 years. Ended 19962 1976 Germany Bavaria Falkenberg R TE Y N Granite 0.3 85 1, 10 Successful fraccing, & short circ tests. Project finished 19853 1976 UK Cornwall Rosemanowes Camborne School <strong>of</strong> Mines R TE Y N Granite 2.7 79 1 Successful drill, frac & circulation for four yrs. Ended 19914 1977 France Le Mayet de Montagne R TE Y N Granite 0.8 33 1, 10 Granite from surface. Successful frac & circ tests.Project ended 19945 1982 Japan Ogachi Y N 1.3 240 1 Volcanic. Poor connectivity (~90% water loss)6 1983 Japan Higashi‐Hachimantai R TE Y N Granite 0.4 60 107 1985 Sweden Fjallbacka R TE Y N Granite 0.5 15 1 Successful 40 day circulation test. Ended 19898 1985 France Soultz‐en‐Foret ENGINE R OP Y Y Granite 4.2 200 155 1.5 1, 7, 8, 9 Prod. power for >15 years.9 1988 Japan Hijiori TE Y N Granodiorite 2.7 270 163 1, 4 A lot <strong>of</strong> short tests, with varied results; & water loss ~50%10 1999 Australia NSW Hunter Valley Pacific Power D TE Granite 1 Elcom. Discontinued due to funding issue. Site later acquire by Geodynamics11 2001 Australia NSW Jerry's Plain Geodynamics C Granite Inferred resource12 2001 Switzerland Basel D TE Y Granite 5 200 2 Fraccing caused 3.4R earthquake). Proj suspended.13 2002 Germany Bad Urach Y Mica‐syenite 3.3 170 2 Series <strong>of</strong> successful short frac & circ tests14 2002 Australia SA Cooper Basin Geodynamics C DR Y Y Granite 4.3 250 200 1, website Pro<strong>of</strong> <strong>of</strong> concept achieved 2009 (flow btw 2 wells)15 2002 USA Coso R y 1 Stimulated same fracture via 2 wells. Second stimulation caused swarm <strong>of</strong> EQs16 2002 USA NV Desert Peak Ormat C 1 Adjacent to conventional geo<strong>the</strong>rmal area.17 2003 El Salvador Berlin C OP Y Y 2 Stimulation <strong>of</strong> tight injection well for existing geo<strong>the</strong>rmal field18 2003 Germany Hanover Horstberg (GeneSys) GEOZENTRUM R TE Y N Sandstone 3.8 2 Single well. Frac & circ was achieved, and inadequate circulation was proved.19 2004 Australia SA Paralana Petra<strong>the</strong>rm C DR Metasediments 4.1 1 Have drilled injector well Paralana‐220 2005 Australia TAS Charlton‐Lemont KUTh C FU Granite website Inferred resource21 2006 Australia SA Olympic Dam Green Rock <strong>Energy</strong> Ltd C FU Granite website Inferred resource22 2006 Australia SA Parachilna Torrens <strong>Energy</strong> C FU Cryst Base/Sandst.155 website Power plant planned operational 201135 2009 Australia SA Roxby Sou<strong>the</strong>rn Gold C FU Granite website Inferred resource36 2009 Australia WA Jurien‐Woodada New World <strong>Energy</strong> C FU website Inferred resource37 2009 Germany Unterhaching C OP Y Y 3.4 122 3.4 2, 5 Commercial. Operating. Commissioned 200938 2009 Switzerland St Gallen Geowatt C 4.1 150 (3‐5) 839 2009 UK Cornwall Eden Project EGS <strong>Energy</strong> C FU Granite 4 (3) website40 2009 UK Cornwall United Downs Geo<strong>the</strong>rmal Engineering Ltd C FU Granite 4.5 (10) website41 2009 USA AK Naknek Geo Project Naknek electric D 4.2 342 2009 USA NV New York Canyon TGP Development D 343 2009 USA OR Newberry Volcanic Bend Altarock/Davenport D PE Volcanics (15) 344 2009 Germany Hannover (Genesys) GEOZENTRUM R DR Sandstone 3.945 <strong>2010</strong> Latvia Riga EGS (3‐4) 846 <strong>2010</strong> Norway Oslo EGS 847 <strong>2010</strong> Germany Rulzheim HotRock Verwaltungs C 3 websiteKEY:‐Purpose Status Technical success Commercial success References (see main text for full references)C Commercial DR Drilling Y indicates project was successful Y Indicates project achieved flow rates 1 MIT Report 2006D Demonstration OP Operational in stimulation and flow testing and temperatures sufficient to enable 2 M Back (re current Germany, pers con, 27/4/09) or M Haring (re Basel, pers con, June 09)R Research and development TE Terminated (if undertaken) a project to be commercially developed 3 Jennejohn <strong>2010</strong>PE Permitting 4 Tezuka 2007FU Fundraising 5 Reif 2009DE Development 6 Baumgartner et al 2007Note: 7 Brown 2009Blank cells indicate data not yet collected or available 8 Holm et al <strong>2010</strong>Paren<strong>the</strong>ses indicate expected power output 9 Cornet 2009Projects in blue indicate assessment for technical success 10 Evans and Valley 2005212


Technical SuccessAt this stage <strong>of</strong> <strong>the</strong> industry’s development, and interms <strong>of</strong> ‘technical su ccess’, a p roject could bedeemed succe ssful if circulation, o r ano<strong>the</strong> rspecific technical goal was achieved e.g. creatinga re servoir. This i s particularly impo rtant whe nconsidering <strong>the</strong> ea rly R&D projects. For example<strong>the</strong> Rosema nowes proje ct, which di d not set outto commercially produce power but to prove rockmechanics concepts behind EGS an d achiev ecirculation. In that conte xt, <strong>the</strong> proje ct wa s asuccess, and as such has been valuable in driving<strong>the</strong> industry forward.There are several environmental factors that canbe said to affect <strong>the</strong> techni cal success <strong>of</strong> aproject. Of th ese arguably <strong>the</strong> m ost important arewater losses and indu ced seismicity. These risk shave impacted on <strong>the</strong> identified projects to varyingdegrees, ra nging fro m little to no imp act to <strong>the</strong>suspension/cancellation <strong>of</strong> <strong>the</strong> project e.g. Basel.These co nstitute risks to <strong>the</strong> proj ect which ne edcareful ma nagement and mitigati on. Suchmanagement and mitig ation strategies have beendeveloped ov er <strong>the</strong> la st fe w years (e.g. Majer etal. 2008, M orelli a nd Malavazos 2008) an dcontinue to develop, wit h this havin g a hug eimpact on th e pu blic perception <strong>of</strong> <strong>the</strong> indu stry.However, fo r <strong>the</strong> pu rposes <strong>of</strong> thi s a ssessment<strong>the</strong>y will not be considered to affect <strong>the</strong> techni calsuccess <strong>of</strong> a project.Commercial SuccessThe ‘comme rcial success’ <strong>of</strong> a proj ect ca n b emeasured wi th rega rd to <strong>the</strong> eco nomics <strong>of</strong> thatproject at th at parti cular site. It is dependent o ndrilling costs, temperatures, location relative topower infrast ructure, ma rkets, and fee d-in tariff sas well as o<strong>the</strong>r fact ors. Seve ral <strong>of</strong> <strong>the</strong>se‘modifying’ fa ctors can change with ti me, as aresult <strong>of</strong> a chan ging or un certain regulato ryenvironment e.g. emission trading schemes a ndpower prices. This means that <strong>the</strong> economics <strong>of</strong> aproject ca n cha nge with time, all o<strong>the</strong>r facto rsbeing constant.Several <strong>of</strong> <strong>the</strong> EGS projects to date did not set outto commercially produce power, but to explore <strong>the</strong>development <strong>of</strong> EGS. Hence, <strong>the</strong>se proje ctscannot be assessed in term s <strong>of</strong> being acommercial success.As a first-p ass and b road-brush ap proach t oassess commercial success, it is defined he re asei<strong>the</strong>r production <strong>of</strong> p ower, or <strong>the</strong> project b eingadvanced e nough to h ave proven it s p otential toproduce power via long-term circulation tests.Environmental factors such as induced seismicityor unsustainable flo w rates can b e d eemed toaffect <strong>the</strong> co mmercial su ccess <strong>of</strong> a proje ct, as<strong>the</strong>y can lead to <strong>the</strong> closure <strong>of</strong> <strong>the</strong> project. Hence,<strong>the</strong>y are considered here.<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Preliminary Assessment <strong>of</strong> <strong>the</strong>Success <strong>of</strong> EGS ProjectsTwenty p rojects all owed a first-p ass assessment<strong>of</strong> technical success, as defined above. Of <strong>the</strong>seprojects o ne wa s deem ed not succe ssful due todrilling difficulties (serpentinite) leadi ng to asuspension <strong>of</strong> <strong>the</strong> proj ect (G eysers). Thi srepresents a 95% techni cal success rate for EGSprojects.Stimulations were noted to be successful within arange <strong>of</strong> lithologies (Table 1).With regard t o <strong>the</strong> c ommercial success <strong>of</strong> <strong>the</strong> seprojects: many <strong>of</strong> <strong>the</strong> earlier (1970-2000) projectsdid no t se t ou t to b e comme rcial, and o f th esenine projects (see Table 1, Rows 1 - 9) only twocan be considered as co mmercially succe ssfuland produced/is producing power (Fenton Hill andSoultz, Table 1, Rows 1 and 8).However, t he seven technically successfulprojects commenced in this last decade, for whichcommercial success could be a ssessed (Coo perBasin, Be rlin, Land au, Bruchsal, Gro ssSchonebeck, Insheim and Unterh aching), all areproducing power or have been proven capable <strong>of</strong>producing power an d a re planni ng developmentfor power production.Reservoir de velopment in Australia h as bee nshown (e.g. Geodynamics, Coo per Ba sin) to b eaided by <strong>the</strong> prevailing continental co mpressivestress regim e (Hillis an d Reynol ds 2000), Under<strong>the</strong>se con ditions, hydraulic re servoir stimulationslikely result i n sub-horizontal fracturing leading toenhanced well connectivity. Hence, in Australia, agreater level <strong>of</strong> success may be anticipated.ConclusionsIt is approp riate to be cau tious about <strong>the</strong> co ncept<strong>of</strong> success here, which has necessarily been keptrelatively s imple. In <strong>the</strong> f uture, <strong>the</strong> geo<strong>the</strong>rmalindustry coul d argu ably better define succe ss a sachieving a t ypical cost o f produ ction for po werdelivered into <strong>the</strong> retail market that is less than orequal to coal (on a pre-carbon tax basis) and <strong>the</strong>nprioritise it s R&D objectives acco rding to <strong>the</strong>prospective contri butions <strong>of</strong> various potentialtechnical a dvances to a chieving that benchma rk<strong>of</strong> success.At this moment in time, <strong>the</strong> early indicato rsgenerated from this industry worldwide show:-An expone ntial gro wth in <strong>the</strong> numb er <strong>of</strong>EGS projects over <strong>the</strong> last 5 yearsA comme rcially dominat ed indu stry in<strong>2010</strong> a s o pposed to R&D d ominatedactivity 10 years ago.Early indications that technical success isconsistently being achie ved with t his213


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>translating into commerc ial success(where this is an aim)The next decade will l ikely be a period <strong>of</strong>consolidation and furth er growth for th is pa rt <strong>of</strong><strong>the</strong> geo<strong>the</strong>rmal sector, with several more projectslikely to b e producing power at <strong>the</strong> e nd <strong>of</strong> thi speriod. As part <strong>of</strong> that evolution, projects are likelyto increase in size.Regulatory frameworks a nd gove rnment polici esare needed which encourage this momentum andhelp consolidate <strong>the</strong> industry over this period withgovernment supp ort continuin g to be mad eavailable at approp riate l evels to fu r<strong>the</strong>r growthand encourage investor interest.ReferencesBaumgärtner, J., Menzel, H., and Hauffe, P.,2007,“The Ge ox GmbH Proj ect in L andau - T he firstgeo<strong>the</strong>rmal p ower project in Pal atinate / UpperRhine Valley ”, in <strong>Proceedings</strong> First EuropeanGeo<strong>the</strong>rmal Review, Geo<strong>the</strong>rmal <strong>Energy</strong> forElectric Power Production, p. 33, Mainz,Rhineland Palatinate, Germany.Brown, D.W. , 2009, Hot dry rock g eo<strong>the</strong>rmalenergy: Important lessons from Fenton Hill. Proc.Thirty-Fourth Workshop on Geo<strong>the</strong>rmal ReservoirEngineeringStanford University, Stanford, California, February9–11.Cornet, F.H. , 2009, Fro m hot dry ro ck toenhanced g eo<strong>the</strong>rmal systems: <strong>the</strong> S oultz-sous-Forets project, AAPG Eur opean Region Annual<strong>Conference</strong>, Paris-Mal maison, Fra nce, 23 -24November 2009DRET (Department o f Re sources, En ergy andTourism) 2008, Canberra, 64pp.Evans, K.F. and Valley, B., 2005, An overview <strong>of</strong>enhanced geo <strong>the</strong>rmal systems,www.geo<strong>the</strong>rmal.ethz.ch/.../Geo<strong>the</strong>rmal%20publications/EvansEtAl_2005_EGS-Overview.pdfHillis, R. R. and Reyn olds, S.D., 2000. Th e<strong>Australian</strong> St ress M ap. Journal <strong>of</strong> <strong>the</strong> GeologicalSociety, London, 157, 915-921.Holm, A., Blodgett, L., Jennejohn, D. A nd Gawall,K., <strong>2010</strong>, Geo<strong>the</strong> rmal <strong>Energy</strong>: Internatio nalMarket Upda te, Geo<strong>the</strong>rm al <strong>Energy</strong> Associ ationReport, May <strong>2010</strong>.Jennejohn, D., 201 0, US G eo<strong>the</strong>rmal Po werProduction and Development Update, Geo<strong>the</strong>rmal<strong>Energy</strong> Association Report, April <strong>2010</strong>Majer, E., Baria, R. and Stark, M., 2008 , Protocolfor Induced Seismicity Associated with EnhancedGeo<strong>the</strong>rmal Systems. Report produced in Task DAnnex I (9 April 2008), Internation al Ene rgyAgency-Geo<strong>the</strong>rmal Imp lementing Agreement(incorporating comm ents by: C. Bromley, W.Cumming, A. Jelacic and L. Rybach).Morelli, C., and Malava zos, M. (2 008), Analysi sand Man agement <strong>of</strong> Seismic Risks Asso ciatedWith Engin eered G eo<strong>the</strong>rmal System Operation sin South Au stralia, in Gurgenci, H. a nd Budd, A.R. (editors), <strong>Proceedings</strong> <strong>of</strong> <strong>the</strong> Sir Ma rk OliphantInternational Frontiers <strong>of</strong> Science and Technology<strong>Australian</strong> Geo<strong>the</strong> rmal <strong>Energy</strong> Confe rence,Geoscience Australia, RecordReif, T., 2009, Economi c aspe cts <strong>of</strong> geo<strong>the</strong> rmaldistrict he ating and powe r gene ration,Presentation, Tallinn Uni <strong>of</strong> Technol ogy, 17 April2009/GeotlS, Geo<strong>the</strong>rmische VereinigungTezuka, K., 2007, Japanese EGS Experience andmodelling efforts - a Review <strong>of</strong> <strong>the</strong> Hijiori HDRproject. ENG INE Worksho p 2, Volte rra, 1-4 Ap ril2007.214


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Estimates <strong>of</strong> sustainable pumping in Hot Sedimentary Aquifers:Theoretical considerations, numerical simulations and <strong>the</strong>irapplication to resource mappingJ. F. Wellmann*, F. G. Horowitz, L. P. Ricard, K. Regenauer-LiebWestern <strong>Australian</strong> Geo<strong>the</strong>rmal Centre <strong>of</strong> Excellence, The University <strong>of</strong> Western Australia, 35Stirling Hwy, WA-6009 Crawley, Australia*Corresponding author: wellmann@cyllene.uwa.edu.auA method for a spatial analy sis <strong>of</strong> potentia lsustainability for <strong>the</strong> e arly stage <strong>of</strong> exploration inHot Sedime ntary Aquifers (HSA) is presentedhere. Our analyses are based on well establishedestimations f or <strong>the</strong> <strong>the</strong> rmal bre akthrough in adoublet well setting. We consider two significantlydifferent sce narios: <strong>the</strong> placement o f a welldoublet in a n aquife r wit hout si gnificant naturalflow, and <strong>the</strong> case whe re a natural ground waterflow exists.We integrate <strong>the</strong>se two analytical estimations intoone workflow with ge ological mo delling a ndgeo<strong>the</strong>rmal simulation. A s a result, we obtainspatial an alyses <strong>of</strong> <strong>the</strong>oretical sustainablepumping rate s for a whole resource area. The semaps are sp ecifically suitable for <strong>the</strong> early sta ge<strong>of</strong> exploration where a potential target area has tobe determined based on limited information.We p resent <strong>the</strong> appli cation <strong>of</strong> our m ethod to ageo<strong>the</strong>rmal reso urce are a in <strong>the</strong> North PerthBasin, from geological modelling, to <strong>the</strong> simulation<strong>of</strong> fluid and heat flow, and finally to map <strong>the</strong>analysis <strong>of</strong> sustainable pumping rates fo r on eaquifer. Th e results con tain a high degree <strong>of</strong>uncertainty, but indi cate t he di stribution <strong>of</strong> futureprospective areas. These maps can be combinedwith o<strong>the</strong>r spatial datase ts, e.g. infrastru cture.Also, as <strong>the</strong>y are integrated into one workflow, anupdate <strong>of</strong> th e analyses i s dire ctly possible whennew data become available.Keywords: Hot Sedim entary Aquife r (HSA);Resource Analysis; Sustai nable Pumpi ng Rate s;Geo<strong>the</strong>rmal Simulation; Geological ModellingIntroductionThis paper presents a novel exploration method toidentify geot hermal p rospects ba sed on <strong>the</strong> rmaland hyd raulic p roperties <strong>of</strong> <strong>the</strong> su bsurface. Wecombine esti mates <strong>of</strong> su stainable pumping rate swith simulations <strong>of</strong> fluid a nd heat flow, and derivemaps <strong>of</strong> e stimations for sustai nable pumpin grates.Our work regards estimates <strong>of</strong> sustai nability forwell do ublet systems. After a certain time t B , <strong>the</strong>reinjected cold water f ront m ay reach th eextraction well and cool down th e extractedtemperature (Fig. 1, red curve). This will affect <strong>the</strong>geo<strong>the</strong>rmal a pplication an d, at some stage, rul eout furth er effective u sage <strong>of</strong> <strong>the</strong> site. Anestimation <strong>of</strong> this breakthrough time t B is re quiredto evaluate <strong>the</strong> sustainability <strong>of</strong> a project.temperature [C]1009590Temperature development at production wellflow parallelno flowflow perpendicular0 10000 20000 30000 40000 50000production time [days]Figure 1: Comparison <strong>of</strong> temperature development at <strong>the</strong>extraction well for three different scenarios: i) If no advectiveflow is present, <strong>the</strong> cold reinjected water may reach <strong>the</strong>production/ extraction well (red curve) and <strong>the</strong> temperature <strong>of</strong><strong>the</strong> pumped water will decrease; ii) For advectivegroundwater flow perpendicular to <strong>the</strong> wells, <strong>the</strong> temperaturedecrease is significantly slower (green curve); and iii) For <strong>the</strong>case that <strong>the</strong> reinjection well is directly downstream <strong>of</strong> <strong>the</strong>production well, no <strong>the</strong>rmal breakthrough occurs (bluecurve).Analytical e stimates <strong>of</strong> a su stainable long -termuse for ge o<strong>the</strong>rmal in stallations ha ve bee napplied for many years (e.g. Gri ngarten, 1978,Lippmann a nd Tsang, 1980). Mo st <strong>of</strong> <strong>the</strong>approaches are ba sed o n many sim plificationsand assu mptions. They n one<strong>the</strong>less d eliver animportant insight into th e distribution <strong>of</strong> promisingareas for sustainable flow in <strong>the</strong> sub surface,especially in <strong>the</strong> ea rly exp loration ph ase, as notonly available temperature and heat in pla ce areconsidered, but also hy draulic parameters likepermeability and porosity.Ano<strong>the</strong>r standard tool in geo<strong>the</strong>rmal exploration isnumerical simulation <strong>of</strong> subsurfa ce fluid and h eatflow. (Se e e.g. O’Sullivan et. al. 2 001 fo r adetailed revision <strong>of</strong> appli cations.) A t horoughlyperformed study ca n deli ver detaile d i nsight int<strong>of</strong>luid and heat movement in <strong>the</strong> subsurface, within<strong>the</strong> usual limitations <strong>of</strong> data availability and modelaccuracy.One problem with both estimations, analytical andnumerical, is that <strong>the</strong>y are usu ally only performedat one lo cation, i.e. at a previo usly identified215


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>target, to evaluate its lo ng term b ehaviour. Wepropose here that it is use ful to perform a ra steranalysis <strong>of</strong> sustainable pumping rate s. This canbe applied from <strong>the</strong> very first stages <strong>of</strong> geo<strong>the</strong>rmalexploration and sub sequently refined duringongoing exploration, wh en mo re data be comeavailable.We p resent here a m ethod to perf orm <strong>the</strong> sespatial analyses. Our approach is implemented ina com plete framework coveri ng geologicalmodelling and fluid and heat flow simulations. Theresults we obtain have to be analysed critically as<strong>the</strong> many a ssumptions th at go into th e analysi sprohibit an a bsolute inte rpretation <strong>of</strong> t he results.For example, an estimated average pumping rate<strong>of</strong> 80 m 3 /s for a lifetime <strong>of</strong> 30 years may contain ahigh d egree <strong>of</strong> uncertaint y. But even if <strong>the</strong> totalvalues might vary, we con sider t he ge neraldistribution <strong>of</strong> <strong>the</strong> anal ysis to be a valuablerepresentation <strong>of</strong> p otential targ et a reas in aresource area.Theoretical considerations andsimulated examplesHere, we b riefly review some <strong>of</strong> <strong>the</strong> commonlyapplied <strong>the</strong>oretical estim ations <strong>of</strong> sustainabilitystudies. All <strong>the</strong> presented estimation s below aresuitable fo r appli cation in Hot S edimentaryAquifer/ po rous m edia sy stems. The situation i smuch m ore c omplex in f ractured sy stems (E GS)and special considerations are ne cessary. Fo rmore detail ed information , see <strong>the</strong> recent revie w<strong>of</strong> Banks (2009).Analytical estimationsThe longevity <strong>of</strong> a do ublet well can be defined as<strong>the</strong> time it ta kes for <strong>the</strong> reinjec ted c ool water toreach <strong>the</strong> extraction well indicated at <strong>the</strong> poin twhen <strong>the</strong> extracted te mperature starts todecrease (e. g. Fig. 1). We are applying thi sdefinition he re, but it should be noted that thistime defines <strong>the</strong> lower en d <strong>of</strong> <strong>the</strong> usability. After<strong>the</strong> <strong>the</strong>rma l bre akthrough, <strong>the</strong> extracte dtemperature will decrease but possi bly <strong>the</strong>application will still be usable (e.g. Lipp mann andTsang, 1980, Banks, 2009).In this paper, we cons ider t wo cases f or t heestimation <strong>of</strong> a sustainable pumping rate, with andwithout advective background flow.Well doublet without advective background flowWe firstly con sider th e ca se <strong>of</strong> hydrauli cbreakthrough. This i s th e time t hyd <strong>the</strong> reinjectedwater tak es to reac h t he extrac tion well. Forsimple cases (flow al ong <strong>the</strong> sho rtest path,homogeneous aq uifer, no di spersion) th ehydraulic breakthrough ti me (e.g. Ho opes a ndHarleman, 1967) can be evaluated for a pumpingrate Q, an aquifer with poros ity , a thic kness hand a spa cing D bet ween extra ction an dreinjection wells as:2Dt hyd h3QThe hydraulic br eakthrough (i.e. th e time when<strong>the</strong> reinjected water reaches <strong>the</strong> extraction well) isnot eq ual to <strong>the</strong> <strong>the</strong>rmal breakthrough (<strong>the</strong> tim ewhen <strong>the</strong> cold tempe rature fro nt re aches <strong>the</strong>extraction well). The temp erature front is delaye dby a retardation factor R th (Bodvarsson, 1972) thatdepends on <strong>the</strong> <strong>the</strong>rmal properties (specific heat cand de nsity ) <strong>of</strong> <strong>the</strong> a quifer rock (a ) and th ewater (w):Rth1 ac cwawTherefore, th e time for <strong>the</strong> arrival <strong>of</strong> <strong>the</strong> <strong>the</strong>rm alfront at <strong>the</strong> extraction well can be calculated as:t<strong>the</strong>2 D h aca3 Q cwwInterestingly, <strong>the</strong> <strong>the</strong>rmal breakthrough time in thiscase do es not depe nd on <strong>the</strong> hydrauli cconductivity / perme ability <strong>of</strong> <strong>the</strong> aquifer, but onlyon geometric and <strong>the</strong>rmal properties.This estimation i s ba sed on ma ny a ssumptions;<strong>the</strong> most important are:1) Fluid prope rties are co nstant and do n otdepend on temperature.2) The flow itself is stea dy-state, inje ctionrate an d te mperature are co nstant and<strong>the</strong>re is n o mixing betwee n <strong>the</strong> reinje ctedfluid and <strong>the</strong> native water.3) The ge ometry <strong>of</strong> <strong>the</strong> aquifer i s verysimple: constant t hickness, co nstantporosity an d it is assumed to behorizontal.4) Cap rock an d bed rock <strong>of</strong> <strong>the</strong> aq uifer areimpermeable.(For a fur<strong>the</strong>r detailed discu ssion see e.g.,Gringarten and Sauty, 1975.)Apart from t hese conditions, ano<strong>the</strong>r co mmonassumption is that <strong>the</strong>re i s no heat transport from<strong>the</strong> aq uifer into <strong>the</strong> surrounding ro cks byconduction. This assu mption is rea sonable inmany cases (see Gringarten and Sauty, 1975, foraccurate criteria) and we will adopt it here as well.Well doublet with advective background flowIf a native h ydraulic gra dient is pre sent in <strong>the</strong>aquifer, th e situation i s more co mplex. It is no wimportant to con sider th e well pl acement withrespect to <strong>the</strong> natural adv ective groundwater flow216


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>v 0 (Fig. 2). An analytical estimation for <strong>the</strong> <strong>the</strong>rmalbreakthrough can be derived for <strong>the</strong> case that <strong>the</strong>reinjection we ll is p laced d ownstream o f <strong>the</strong>extraction well (Lippmann and Tsang, 1980):t<strong>the</strong>whereA 1 acD / v ) c(0Q2hDv 0waw14Aarctan14A4A A1 4 This equation does not have a real solution when<strong>the</strong> natural groundwater velocity is above a criticalvaluev02QhDIn this case, no <strong>the</strong>rmal breakthrough will occurand <strong>the</strong> sy stem i s, in prin ciple, compl etelysustainable and can be operate d without timelimitations.Validity <strong>of</strong> <strong>the</strong> analytical solutionThe a nalytical estim ations <strong>of</strong> hydraulic and<strong>the</strong>rmal b reakthrough depen d on man yassumptions (se e ab ove). In a realist ic setting,some effects might reduce <strong>the</strong> b reakthrough time(hydraulic dispersion, heat conduction in <strong>the</strong> flui dphase) whil e o<strong>the</strong> rs might lea d to long erbreakthrough times (heat re supply fromsurrounding beds, stratification). A carefulexamination <strong>of</strong> <strong>the</strong>se effects i s p ossible withnumerical simulations <strong>of</strong> pumping and reinjection.drawdown i n <strong>the</strong> reservoir. Concerning <strong>the</strong>temperature breakthrough time, we want to havea large well spa cing D, but if we consider th epressure d rawdown, a smaller spa cing i s m orebeneficial. T he optim al value <strong>of</strong> D can not bedetermined analytically, but nume rical solution scan be applied (e.g. Kohl et al., 2003, Wellman net al., 2009).Numerical simulationsThe <strong>the</strong>o retical e stimations d escribed abovedeliver a ve ry useful e stimation ab out potentialgeo<strong>the</strong>rmal t argets. We t herefore consider <strong>the</strong>mas ide al for <strong>the</strong> early ex ploration sta ge. But as<strong>the</strong>y depen d on ma ny assumpti ons andsimplifications, num erical simulations <strong>of</strong>subsurface fluid and heat flow have to be appliedto de rive a more realistic i nsight into th esustainability <strong>of</strong> <strong>the</strong> system.Consideration <strong>of</strong> pressure drawdownIn both case s presented above, with a nd withoutnatural grou ndwater flo w, we can consider amaximum pre ssure dr awdown s at th e extractionwell as ano<strong>the</strong>r criterion for <strong>the</strong> determination <strong>of</strong> asustainable pumping rate. Grin garten (1 978)presented a relationship obtained fro m potentia l<strong>the</strong>ory:s Q2TlnDr wWe can see from this eq uation that <strong>the</strong> pressu redrawdown s depends on pumping rate Q, aquifertransmissivity T and well diameter r w , as can beexpected, but also o n <strong>the</strong> well spacing D, as <strong>the</strong>two wells int eract and a smaller spacing leads toless drawdown.Combined analysisFor a complete sustainability analysis fo r <strong>the</strong> welldoublet, we might co nsider <strong>the</strong> <strong>the</strong>rmalbreakthrough time and a maximum pre ssureFigure 2: Fluid and heat flow representations for <strong>the</strong> threeexample scenarios described below, and presented in Fig.1.In <strong>the</strong> first example, without advective flow, we can see that<strong>the</strong> reinjected cold water (reinjection well: blue triangle)reaches <strong>the</strong> extraction well (red triangle) after a certain time,and <strong>the</strong> produced temperature decreases. Example 2: fornatural advective flow in <strong>the</strong> direction <strong>of</strong> <strong>the</strong> injection well, <strong>the</strong>cold temperature fan does not reach <strong>the</strong> extraction well, and<strong>the</strong> system is completely sustainable. Example 3: for flow217


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>perpendicular to <strong>the</strong> wells, less cold water reaches <strong>the</strong>extraction well, and <strong>the</strong> temperature decrease is reduced.A variety <strong>of</strong> s<strong>of</strong>tware codes exist s t o pe rform<strong>the</strong>se simulations (se e O ’Sullivan et al., 2001).We used SHEMAT (Simulator <strong>of</strong> HEat and MAssTransfer, Cl auser and Bartels, 2003) fo r th eresource scale simulations presented in this paper(e.g. Fig. 3). To test <strong>the</strong> validity <strong>of</strong> <strong>the</strong> analyticalestimation <strong>of</strong> breakthrough times, we si mulated awell d oublet (extra ction a nd reinje ction well) wit hSHEMAT an d, addition ally, with <strong>the</strong> petrole umreservoir engineering so ftware Tem pest/Morefrom Roxar.The plot s i n Fig. 2 show th e te mperaturedistribution (colo ur ma p) and fluid flow vecto rs(grey arrows) in <strong>the</strong> subsurface. The thre eexamples given relate to temperature decrease at<strong>the</strong> extraction well for three different scenarios, asgiven in Fig. 1.In summary:1) Well d oublet in an a quifer withoutgroundwater flow, after <strong>the</strong>rmalbreakthrough occurred. We can see that<strong>the</strong> flow field affect s a wide areaperpendicular to <strong>the</strong> direct con nectionbetween <strong>the</strong> wells.2) Natural g roundwater flo w, <strong>the</strong> reinjectionwell is in <strong>the</strong> downstream direction <strong>of</strong> <strong>the</strong>extraction well. The tem perature field isnow disturbed by <strong>the</strong> natural groundwaterflow. For <strong>the</strong> same pumping rate, wellspacing, and simulatio n time, <strong>the</strong> col dtemperature field does not reach <strong>the</strong>extraction well. No <strong>the</strong>rma l brea kthroughoccurs.3) Natural groundwater flow perpendicular to<strong>the</strong> con nection line <strong>of</strong> <strong>the</strong> well dou blet.The tempe rature field is again cle arlyaffected by <strong>the</strong> groundwater flow field and<strong>the</strong> temperature de crease at <strong>the</strong>extraction well is slowed down.Example: North Perth BasinGeological modelWe a pplied <strong>the</strong> an alytical estimation s presentedabove to exploration-scale simulations <strong>of</strong> fluid andheat flo w. F or <strong>the</strong> first stage <strong>of</strong> exploration, weconsider th ese a nalytical a ssumptions as avaluable i ndication <strong>of</strong> pot ential ge o<strong>the</strong>rmal ta rgetareas.Figure 3: 3-D Geological model for a part <strong>of</strong> <strong>the</strong> North PerthBasin (In inset picture: model location=red square; blackcircle=Perth). Sedimentary formations are overlyingbasement which is <strong>of</strong>fset by normal faults.As a n exam ple he re, we show <strong>the</strong> application <strong>of</strong><strong>the</strong> method t o an area in <strong>the</strong> No rth Perth Basin.The geology is characterised by thick sedimentaryformations cut by normal faults in a graben setting(Fig. 3). The geological model wa s created withan impli cit p otential-field approach (Lajaunie, et.al. 1997 ), impleme nted in <strong>the</strong> G eoModellers<strong>of</strong>tware (Calcagno et al., 2008 ). The model is asimplified ve rsion <strong>of</strong> a more compl ex re gionalmodel.Geo<strong>the</strong>rmal simulationThe geological model is directly processed to aninput file for fluid and h eat flow simulation withSHEMAT (s ee C lauser and Bartel s, 20 03). Rockproperties (permeabilit y, porosity, <strong>the</strong>rmalconductivity and h eat ca pacity) were assign edaccording to sample s i n this re gion wh ereavailable. A strong anisotropy (horizontal / vertical= 10) was applied to all perm eability values toachieve a more realistic model.Figure 4 is a rep resentation <strong>of</strong> <strong>the</strong> simu lated fluidand h eat flo w field fo r t he North P erth Basi nmodel. The effect <strong>of</strong> fluid flow o n <strong>the</strong> temperaturedistribution i s clearly visible. T he re sultingtemperature gradient s appear reasonable andqualitatively in accordan ce with measured value sin <strong>the</strong> area.For a q uantitative analysis <strong>of</strong> <strong>the</strong> re sults, <strong>the</strong>model ha s t o be refin ed and adju sted fur<strong>the</strong>r,especially at <strong>the</strong> b orders (bo undary conditions,see discussion). Resp ecting th ese cu rrentlimitations to model verification, we next apply ourresource an alysis m ethods to thi s mo del. As allsteps are integrated into one workflow, it is easilypossible to update <strong>the</strong> model an d a ll analyse slater, when more data become available.218


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Figure 4: Visualisation <strong>of</strong> <strong>the</strong> temperature and fluid flow fieldsimulated for <strong>the</strong> 3-D geological model <strong>of</strong> <strong>the</strong> North PerthBasin. The orange isosurface shows <strong>the</strong> depth to 120 o C. Theblack lines indicate fluid flow pathways. General flowdirection is N-S.Novel resource analysis methodsNext we use <strong>the</strong> simulated fluid and heat flow fieldto estimate different a spects <strong>of</strong> geo<strong>the</strong> rmalresource sustainability. All <strong>the</strong> examples here areperformed fo r <strong>the</strong> old est sedimentary formatio n(see Fig. 3, light green unit). The minimum lifetimeto co nsider a geo<strong>the</strong>rmal p roject site a s“sustainable” is a ssumed to be 30 ye ars for t hefollowing analyses.Key novel aspects <strong>of</strong> all our analyses are:1) We p erform t he an alyses directly on th ebasis <strong>of</strong> <strong>the</strong> simulated fluid and heat flowfield for <strong>the</strong> resource area, linked to <strong>the</strong> 3-D geological model.2) All asp ects (maxim um su stainablepumping rate, heat i n place, pressuredrawdown) a re evalu ated on a spatialbasis, i.e. we derive 2 -D maps <strong>of</strong> <strong>the</strong>seproperties showing <strong>the</strong>ir distribution.3) All relevant steps a re integrated into oneworkflow, it is <strong>the</strong>refore readily possible toupdate <strong>the</strong> geological m odel and th egeo<strong>the</strong>rmal simulation wh en more databecome available.Maximum sustainable pumping rate, withoutconsideration <strong>of</strong> advective flowFollowing t he definitio n <strong>of</strong> <strong>the</strong> <strong>the</strong>oreti calbreakthrough time for <strong>the</strong> <strong>the</strong>rmal front givenabove, we estimate a maximum pumping rate thatcould be exp ected for a d oublet system. Spatialanalysis is performed step-by-step at every pointin space (Fig. 5).Figure 5: Maximum pumping rates for a doublet system with800 m spacing and a lifetime <strong>of</strong> 30 years. All o<strong>the</strong>r propertiesrequired for <strong>the</strong> estimation <strong>of</strong> <strong>the</strong> pumping rate (seeequations above) are directly taken from <strong>the</strong> simulation (e.g.density) and <strong>the</strong> model (e.g. formation thickness).Consideration <strong>of</strong> natural groundwater flowIn Fig. 4 we can see from <strong>the</strong> di stribution <strong>of</strong> th estreamlines t hat gro undwater flow i s present at<strong>the</strong> regional scale for this specific model. So, if wehypo<strong>the</strong>tically intelligibly place a well doubl et inone <strong>of</strong> <strong>the</strong> flow areas, it is possible to determine apumping rate whe re a <strong>the</strong> rmal b reakthrough will,<strong>the</strong>oretically, never occur (see Exam ple 2 in Fig.2). If we <strong>the</strong>n apply this analysi s agai n at everypoint in our model, we ca n de rive a spatialanalysis <strong>of</strong> t hese pum ping value s (Fi g. 6) fo rwhich <strong>the</strong>rmal breakthrough will never occur.Figure 6: Estimation <strong>of</strong> a maximal pumping rate for <strong>the</strong><strong>the</strong>oretical case <strong>of</strong> no <strong>the</strong>rmal breakthrough (Example 2 inFig. 2), in <strong>the</strong> presence <strong>of</strong> advection. This is <strong>of</strong> practicalsignificance as areas with a high value can also be expectedto allow a higher sustainable pumping rate (for a projectdurance less than infinity).Combination with o<strong>the</strong>r important factorsThese spati al analyses can n ow be u sed i ncombination with o<strong>the</strong>r relevant factors fo rgeo<strong>the</strong>rmal exploration, e.g. mean temperature atdepth for a target formation, or maps <strong>of</strong> local heatin place (Wellmann et al., 2009). Heat in pla ce isreferred to as one absolute number characterising219


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong><strong>the</strong> geo<strong>the</strong>rmal potential <strong>of</strong> a geo<strong>the</strong>rmal reservoirvolume. We define <strong>the</strong> lo cal heat in pl ace as <strong>the</strong>heat in place <strong>of</strong> a tiny subdivision <strong>of</strong> <strong>the</strong> reservoir.A local heat in place map gives crucial informationon <strong>the</strong> conn ectivity <strong>of</strong> <strong>the</strong> ge o<strong>the</strong>rmal re servoirand <strong>the</strong>refore is <strong>of</strong> high interests fo r re servoirengineering studies. As all results a re in mapview, <strong>the</strong>y can ea sily be inclu ded in aGeoInformationSystem (GIS) and combined with,for example, infrastructure considerations.DiscussionWe h ave sh own that it i s po ssible to combi neanalytical co nsiderations <strong>of</strong> re sourcesustainability, with geoth ermal fluid and heat flowsimulations. Our approach enables a direct spatialanalysis <strong>of</strong> relevant factors fo r geo<strong>the</strong> rmalexploration i n Hot Sedi mentary Aq uifers. T hemajor advantage is that geo<strong>the</strong>rmal prospects canbe identified based on ph ysical reasoning (in <strong>the</strong>context <strong>of</strong> geolo gical modelling), geo<strong>the</strong>rmalsimulation, a nd id eally, a ll availabl e data. Wepropose that this method is a step forward for <strong>the</strong>identification <strong>of</strong> geo<strong>the</strong> rmal target a reas from aregional analysis.The example presented above for <strong>the</strong> North PerthBasin is pe rformed for a reso urce-scale model,representative for an earl y stage <strong>of</strong> geo<strong>the</strong>rmalexploration. It contain s a hi gh deg ree <strong>of</strong>uncertainty and <strong>the</strong> de termined nu mbers fo rsustainable pumping rat e are p robably notquantitatively correct. But as <strong>the</strong>y are b ased on afull 3-D inte gration with geol ogical knowledge,physical simulation and all available data, we caninterpret <strong>the</strong> results spatially, i.e. identify areaswhich should be analysed more careful ly. This isa majo r a dvantage to stand ard re sourceestimation methods, e.g. heat in place, where onlyone val ue for <strong>the</strong> wh ole resource area i sdetermined.In a re alistic proj ect scenario, th e n ext stepswould be to refine <strong>the</strong> model and adjust boundaryconditions carefully to <strong>the</strong> loc al setting. But as wehave integrated all rel evant modelling, simulationand resource analysis steps into one workflow, anupdate at every stage is easily possible.We recognise that <strong>the</strong> results a re subject to alarge degree <strong>of</strong> uncertain ty. Two way s we wil laddress this in future work, will be to combine thisworkflow with an u ncertainty si mulation <strong>of</strong>geological modelling (Wellmann et al., <strong>2010</strong>), andwith se nsitivity studies <strong>of</strong> <strong>the</strong> geo<strong>the</strong>rmalsimulation to derive a qu antitative evaluation o f<strong>the</strong> sustainability map quality.AcknowledgementsThis work was en abled by an <strong>Australian</strong>International Postgraduate Re search S cholarship(IPRS) a nd a Top -up S cholarship f rom GreenRock Ene rgy Ltd. The We stern <strong>Australian</strong>Geo<strong>the</strong>rmal Centre <strong>of</strong> Ex cellence (WAGCoE) is ajoint centre <strong>of</strong> Curtin University, The University <strong>of</strong>Western Australia and <strong>the</strong> CSIRO and funded by<strong>the</strong> State Go vernment <strong>of</strong> Western Au stralia. Weare ve ry thankful fo r t he comme nts <strong>of</strong> a nanonymous reviewer. We than k Roxar an dIntrepid Ge ophysics for providing acad emiclicenses <strong>of</strong>, res pectively, Tempes t/More andGeomodeller s<strong>of</strong>tware.ReferencesBanks, David, 2009, Thermogeologicalassessment <strong>of</strong> open-loop well-doublet schemes: areview and syn<strong>the</strong>sis <strong>of</strong> analytical approaches:Hydrogeology Journal, v. 17, no. 5, p. 1149–1155.Bodvarsson, G.,1972, Thermal problems in <strong>the</strong>siting <strong>of</strong> reinjection wells: Geo<strong>the</strong>rmics, v. 1, no. 2,p. 63–66.Calcagno, Philippe; Chilès, Jean-Paul; Courrioux,Gabriel; Guillen, Antonio, 2008, Geologicalmodelling from field data and geologicalknowledge: Part I. 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<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>temperature changes: Ground Water, v. 18, no. 5,p. 452–458.O'Sullivan, M. J.; Pruess, K.; Lippmann, M. J.,2001, State <strong>of</strong> <strong>the</strong> art <strong>of</strong> geo<strong>the</strong>rmal reservoirsimulation: Geo<strong>the</strong>rmics, v. 30, no. 4, p. 395–429.Wellmann, J. F., Horowitz, F. G., Regenauer-Lieb,K., 2009, Co ncept <strong>of</strong> an i ntegrated workflow fo rgeo<strong>the</strong>rmal exploratio n in Hot SedimentaryAquifers; <strong>Australian</strong> Geoth ermal Ene rgy<strong>Conference</strong> (AGEC), Brisbane, Abstracts.Wellmann, J. F.; Horowitz, F. G.; Schill, E.;Regenauer-Lieb, K., <strong>2010</strong>, Towards incorporatinguncertainty <strong>of</strong> structural data in 3D geologicalinversion: Tectonophysics, v. 490, no. 3-4, p.141–151.221


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Hydro<strong>the</strong>rmal Spallation for <strong>the</strong> Treatment <strong>of</strong> Hydro<strong>the</strong>rmal and EGSWells: A Cost-Effective Method for Substantially IncreasingReservoir Production Flow RatesThomas W. Wideman 1, Jared M. Potter 1* , Brett O’Leary 2 , Adrian Williams 2 ,1 Potter Drilling, Inc. 599 Seaport Blvd., Redwood City, CA 940632 Geodynamics Limited, Suite 1A Level 5 South Shore Centre, 85 The Esplanade SOUTH PERTH WA 6151*Corresponding author: jared@potterdrilling.comThere is a n eed in many geo<strong>the</strong>rm al proje cts togreatly in crease th e p roductivity and/o r inje ctivity<strong>of</strong> wells, with a direct impact on proje cteconomics. Flow testing in wells and associatedmodelling <strong>of</strong> EGS reservoi rs has suggested thatlow p roductivity from EGS reservoi rs can resultfrom ne ar-wellbore imp edance, a restriction <strong>of</strong>fluid flow wi thin <strong>the</strong> im mediate vici nity <strong>of</strong> <strong>the</strong>borehole walls. F ur<strong>the</strong>r modelling suggested thataltering <strong>the</strong> geometry <strong>of</strong> an existing wellbore bylongitudinally slotting <strong>the</strong> bore hole wall coul dsignificantly decrease ne ar-wellbore i mpedance.Hydro<strong>the</strong>rmal spallation is an id eal technology tocreate sl ots in <strong>the</strong> hard ro ck fou nd in <strong>the</strong>sereservoirs. This pap er d escribes <strong>the</strong> results <strong>of</strong>tests <strong>of</strong> hydro<strong>the</strong>rmal spallation well enhancementtechnology in <strong>the</strong> laborato ry and initial field trialsas well as its a pplication to incre ase productionfrom geo<strong>the</strong>rmal wells.Keywords: <strong>the</strong>rmal sp allation, hydro<strong>the</strong>rmalspallation, well e nhancement, Engine eredGeo<strong>the</strong>rmal Systems, EGSBackgroundEnhanced Geo<strong>the</strong>rmal Sy stems (E GS) have th epotential to generate cle an, renewable, base loadelectricity using h eated fluid prod uced fro mengineered rese rvoirs. These re servoirs a recreated by enha ncing n atural fractures in hotbasement rock usi ng hydrauli c fracturi ngtechnology. Once <strong>the</strong> stimulation proce ss iscompleted, i njection wells d eliver flui d from <strong>the</strong>surface into <strong>the</strong> reserv oir where t he fluid i sheated, a nd prod uction well s drill ed into <strong>the</strong>fractured rock extract th e heated fluid to drive asurface-based power plant.This EGS te chnology is on <strong>the</strong> verge <strong>of</strong> reachingits tremend ous potential. Projects a round <strong>the</strong>world a re a chieving <strong>the</strong>i r temperature objectives,but face <strong>the</strong> challenge <strong>of</strong> low circulation rates after<strong>the</strong> hydrauli c stimulatio n. Most model s sug gestthat EGS wells must pro duce 80-100 kg/se c <strong>of</strong>fluid at 200 °C per well to be economically viable.However, such rate s ha ve proven difficult toachieve in EGS projects to date. T he potential tocreate additional fracture zones within a reservoirexists, but adds considerable cost an d ri sk to aproject a nd has not been a ccomplished at thi spoint. Meeting <strong>the</strong> prod uctivity targets in EGSwells is critical to realizing <strong>the</strong> full potential <strong>of</strong> thispromising renewable energy technology.Geodynamics Limited ("Geodynamics”), a leadingAustralia-based devel oper <strong>of</strong> EGS proje ctsworldwide, in colla boration with A ustralia’sCommonwealth Scientific and ResearchOrganisation (CSIRO), h as conducted extensivefield testing and a ssociated modelli ng <strong>of</strong> EGSreservoirs. These studi es sugge st that lowproductivity from some E GS reservoi rs prim arilyresults fro m near-wellb ore imp edance, <strong>the</strong>restriction <strong>of</strong> fluid flow within <strong>the</strong> immediat evicinity (sev eral in ches or a few fe et) <strong>of</strong> <strong>the</strong>borehole walls. This could be due to reduction infracture permeability from drilling muds or o<strong>the</strong>rparticulates, but <strong>the</strong> most influential fact or is likelyfluid turbule nce due to rapidly increa sing fluidvelocities n ear <strong>the</strong> well bore. To enter t heproduction well, fluids mu st pass thro ugh po resand fra ctures in <strong>the</strong> walls <strong>of</strong> <strong>the</strong> bore hole. Fluidvelocities in t he vicinity <strong>of</strong> <strong>the</strong> bo rehole are muchhigher than in <strong>the</strong> rest <strong>of</strong> <strong>the</strong> reservoir because <strong>of</strong><strong>the</strong> limited surface area <strong>of</strong> <strong>the</strong> borehole walls andare estimated to excee d 55 km per hour near <strong>the</strong>entry into <strong>the</strong> wellbore in some cases. This nearwellboreimp edance can l imit both <strong>the</strong> output <strong>of</strong>production wells an d, to a lesser extent , <strong>the</strong> inputcapacity <strong>of</strong> injection wells.A simplerepresentation <strong>of</strong> this n ear wellbore effect i sshown in Figure 1.By altering t he g eometry <strong>of</strong> an existin g wellbo rethrough increasi ng <strong>the</strong> effective dia meter, it ispossible to redu ce <strong>the</strong> ne ar well bore effect. Thiscan be a ccomplished by slotting <strong>the</strong> boreh olewall, as illustrated in Figure 2.Spallation h as b een proposed a s a n effectiv emeans <strong>of</strong> expanding <strong>the</strong> diameter <strong>of</strong> a wellb ore ora way to create un derground cave rns. Fo rexample, in Pedernal, Ne w Mexico, Bob Potterand Ed Will iams, from Los Alamo s Nation alLaboratory, demonstrated <strong>the</strong> ability to create 60-cm diam eter holes in hard rock u sing o nly a 10-cm diam eter axially-orie nted flame jet. Anillustration <strong>of</strong> this process is shown in Figure 3.222


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Figure 3: Flame spallation cavity makerFigure 1: Illustration <strong>of</strong> near wellbore impedanceFigure 2: Borehole geometry for reduced wellboreimpedanceFlame jet spallation p rocesses continue to b eused comme rcially. Fo r example, in Can ada,<strong>the</strong>rmal fragmentation mining employs a variatio n<strong>of</strong> this ex cavation techniq ue to extra ct pre ciousmetals in thin, near surface ore depos its. In atypical operation, a small pilot hole is drilled int o<strong>the</strong> ore zone and an 8cm diameter flame jet drill isused to cut large r caverns up to about one m eterin diam eter. The spalls are <strong>the</strong> n p rocessed for<strong>the</strong>ir precious metals.However, this air-ba sed tech nology ca n only beused near <strong>the</strong> surfa ce and to moderat e depths i nregions where air drilling is feasibl e. At <strong>the</strong>depths req uired for EGS, <strong>the</strong> wellbo re will verylikely need to be filled with fluid to preventexcessive water o r ga s flows and maintaincirculation and hol e st ability. For flame jetspallation, a fluid-filled wellbore poses seriouschallenges f or b oth <strong>the</strong> transport <strong>of</strong> chemicalsfrom <strong>the</strong> surface and for down-hole combustion.As a re sult, hydro<strong>the</strong> rmal spall ation has b eeninvestigated as a vi able me ans for <strong>the</strong>enhancement <strong>of</strong> deep, water filled EGS wellbores.Experimental ApplicationA hydro<strong>the</strong> rmal spallatio n test a pparatus wa sused for pro <strong>of</strong>-<strong>of</strong>-concept tests on <strong>the</strong> laborato ryscale. T he t est system shown in Figure 4 iscapable <strong>of</strong> indep endently applying controlle dhydrostatic, confining, a nd axial loa ds on 10 cmrock cores to simulate varying wellbore conditionsto 2400 m.223


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Figure 4: Hydro<strong>the</strong>rmal spallation deep well test rigThis system whi ch u ses su perheated stea m tospall <strong>the</strong> rock was used to create single axial slots<strong>of</strong> <strong>the</strong> desired depth in holes and investigate <strong>the</strong>irinteractions with induced fractures.The process wa s <strong>the</strong>n fu r<strong>the</strong>r scal ed to cut <strong>the</strong>axial slots 10 cm wide and more than 25 cm deepin open-hole sections <strong>of</strong> granite blo cks, as shownin Figure 5, usin g a full-scale well enh ancementtest rig.Figure 5: Axial slots cut into 10 cm open hole section <strong>of</strong>Sierra White Granite using a full scale toolFigure 6: Full scale well enhancement test rig224


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>A 8.8 cm ite ration <strong>of</strong> <strong>the</strong> slotting d rill hea d wasdesigned an d fabri cated f or field trial s. The drillhead interfaces with a dynamic seal to isolate <strong>the</strong>working fluid from <strong>the</strong> cooling water, fol lowed byinstrumentation and controls, tension release, andconnector subassemblies, as shown in Figure 7.Geo<strong>the</strong>rmal <strong>Energy</strong> <strong>Conference</strong>, November 16-19in Adelaide.ReferencesCalaman, J. and Rolseth, H.C., 1961, TechnicalAdvances Expand Use <strong>of</strong> Jet-Piercing Process inTaconite Industry: International Symposium onMining Resources, University <strong>of</strong> Missouri.Dreesen, D. and Betz, R., Coiled-TubingDeployed Thermal Spallation Hard Rock CavityMaker, FWP-02FE15.O’Leary, B., <strong>2010</strong>, Longitudinal Slotting forWellbore Enhancement Purposes: QuantifiedCost Benefit: Geodynamics Report.Potter, R. M., Potter, J. M., and Wideman, T.W.,<strong>2010</strong>, Laboratory Study and Field Demonstration<strong>of</strong> Hydro<strong>the</strong>rmal Spallation Drilling: GRC Meeting,Sacramento, California.Figure 7: Cutaway rendering <strong>of</strong> field prototype bottom holeassemblyA coiled tubing string was assembled for purposeby nesting a 9.5 mm OD stainless steel capillaryand 7-conductor wireline cable inside <strong>of</strong> a 50 m mOD, 3.4 0 wa ll, HS-90 ste el coiled tu bing string.The strin g wa s mounte d on a tracked coile dtubing u nit, shown in Fi gure 8. Rotating swivel sand slip rings ad ded to <strong>the</strong> reel al lowed fortransmission <strong>of</strong> <strong>the</strong> co oling wate r, ele ctrical, an dreactants through <strong>the</strong> hub.Williams, E., 1986, Thermal Spallation Excavation<strong>of</strong> Rock: U.S. Symposium on Rock Mechanics(USRMS), 27th annual meeting.An Evaluation <strong>of</strong> Enhanced Geo<strong>the</strong>rmal SystemsTechnology: Geo<strong>the</strong>rmal Technologies Program,U.S. Department <strong>of</strong> <strong>Energy</strong>, <strong>Energy</strong> Efficiency andRenewable <strong>Energy</strong>; IPGT Workshop, August 27-28, <strong>2010</strong>. Reykjavik, Iceland.Flow Test Update: Geodynamics ASXAnnouncement, released April 22, 2008.The Future <strong>of</strong> Geo<strong>the</strong>rmal <strong>Energy</strong>: Impact <strong>of</strong>enhanced geo<strong>the</strong>rmal systems (EGS) on <strong>the</strong>United States in <strong>the</strong> 21st century, MassachusettsInstitute <strong>of</strong> Technology and Department <strong>of</strong> <strong>Energy</strong>Report, 2006: Idaho National Laboratory INL/EXT-06-11746.Figure 8: Coiled tubing unit for field testing <strong>of</strong> hydro<strong>the</strong>rmalspallation well enhancement.A field locati on was chosen in <strong>the</strong> foot hills <strong>of</strong> <strong>the</strong>Sierra Mountains i n no r<strong>the</strong>rn California, whe recompetent granite co uld be found close to <strong>the</strong>surface.At <strong>the</strong> time <strong>of</strong> publication, <strong>the</strong> results from <strong>the</strong> fielddrilling tests were not yet available. T he result swill be presented orally at <strong>the</strong> <strong>2010</strong> <strong>Australian</strong>225


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Thermal effects on <strong>the</strong> wellbore stabilityBisheng Wu, Bailin Wu, Xi Zhang and Rob Jeffrey*CSIRO Earth Science and Resource Engineering, Clayton, VIC 3168, Australia*Tel: 03-95458354, E-mail: rob.jeffrey@csiro.auAbstractThermal-mechanical behaviour plays an importantrole in wellbore stability <strong>of</strong> enhanced geo<strong>the</strong>rmalsystems (EGS). Based on <strong>the</strong> <strong>the</strong>rmo-poro-elasticmodel proposed by Coussy (1989) and by usingLaplace transformation methods, analyticalsolutions for <strong>the</strong> temperature, pore pressure andstresses around a vertical well are obtained in <strong>the</strong>Laplace space. Then <strong>the</strong> solutions in <strong>the</strong> timedomain are obtained via numerical Laplaceinverse transformation. The results show that <strong>the</strong>cooling <strong>of</strong> <strong>the</strong> wellbore has a considerable effectnot only on <strong>the</strong> pressure, in-plane radial and hoopstresses, but also on <strong>the</strong> vertical stress. It reduces<strong>the</strong> compressive radial and hoop stresses along<strong>the</strong> maximum horizontal stress direction. When<strong>the</strong> wellbore temperature is low enough, <strong>the</strong> hoopstress has a tendency to become tensile leadingto <strong>the</strong> wellbore breakdown and <strong>the</strong> lower verticalstress implies <strong>the</strong> generation <strong>of</strong> an in-planefracture. The possibility <strong>of</strong> wellbore shear failure isfound to exist at places with higher compressivehoop stress.Keywords: <strong>the</strong>rmal effects, wellbore stability,Laplace transformation, numerical simulationIntroductionThe mechanical behaviour <strong>of</strong> a wellbore in a fluidsaturatedporous medium has attracted a greatdeal <strong>of</strong> attention during <strong>the</strong> past several decades(Rice and Cleary 1976; Detournay and Cheng1988; Rajapakse 1993; Ekbote et al. 2004). Most<strong>of</strong> <strong>the</strong>se studies focus on <strong>the</strong> pore pressure andstress distribution around <strong>the</strong> wellbore based onBiot’s formulation <strong>of</strong> linear poroelasticity (Biot1941). It is worthwhile to mention that Detournayand Cheng (1988) first provided <strong>the</strong> poroelastictransient and plane-strain analytical solutionsunder a non-hydrostatic stress field.Thermal effects should be considered ingeo<strong>the</strong>rmal reservoir stimulation and production.Cold fluid is generally injected into <strong>the</strong> wellboreand <strong>the</strong> surrounding rock is at a highertemperature. Due to different <strong>the</strong>rmal coefficientsfor fluid and rock matrix, <strong>the</strong> pore space in <strong>the</strong>rock will deform much less than <strong>the</strong> fluid in <strong>the</strong>pore when subject to a temperature variation.Obviously, this will lead to a higher (or lower) porepressure that affects fluid diffusion. On <strong>the</strong> o<strong>the</strong>rhand, pervasive flow can carry low-temperaturewater into a pore and thus <strong>the</strong> local temperatureequilibrium is broken. To account for <strong>the</strong> <strong>the</strong>rmaleffects, many <strong>the</strong>ories have been developed(McTigue 1986; Kurashige 1989). However, ageneral <strong>the</strong>rmo-poro-elastic <strong>the</strong>ory proposed byCoussy (1989) appears more suitable for <strong>the</strong> loss<strong>of</strong> local temperature equilibrium, which may beimportant to consider for a geo<strong>the</strong>rmal system. Inthis <strong>the</strong>ory, a latent heat associated with <strong>the</strong>increase <strong>of</strong> fluid mass content is introduced with adifferent meaning from <strong>the</strong> conventionalterminology.For <strong>the</strong>rmo-poro-elastic solids, Wang et al. (1994)and Li et al. (1998) obtained analytical solutionsfor stress distributions around a borehole. In <strong>the</strong>irmodels, <strong>the</strong> temperature is decoupled from porepressure. In this paper, <strong>the</strong> fully-coupled solutionsare obtained based on <strong>the</strong> linear <strong>the</strong>rmo-poroelasticmodel proposed by Coussy (1989). As <strong>the</strong>borehole is much longer compared to its diameter,we consider <strong>the</strong> problem by assuming plane strainconditions for cross sections orthogonal to <strong>the</strong>borehole axis.Problem FormulationFigure 1 shows a vertical wellbore subjected to avertical tectonic stress σ v , a maximum and aminimum horizontal stresses, σ max and σ min . Theinitial pore pressure and temperature are P * R andT * R , respectively. When time t>0, <strong>the</strong> wellboretemperature and pressure are kept constants, i.e.maintained at T * w and P * W .Figure 1: Problem geometryGoverning equationsThe equations to be solved and initial andboundary conditions for this problem are listed asfollows:1. Linear <strong>the</strong>rmo-poro-elastic constitutive law:226


K 2 G/3 2GBP3 K Tr B v r i B B K 2 G/3 2GBP3K T 2GrB v i Br K 2 G/3 BP3 K T .z B v i B B2. Compatibility equationsur ur 1 u11uruu r , , r= .r r r 2 r rr3. Equilibrium equations: r1r r r1 r 0, 2 0.r r r r r r4. Governing equations for pore pressure andtemperaturek 2 1 P L Tvw P Bi ,* M tt MTRt2 22 wLP* v wLTAT 3 BKBT R( C v ) ,*M t t MTRtwhere ijare effective stresses, latent heat forfluids is defined as L=T * (3α K -3α K )/ρ /B ,* R u u B B w iP=P * -P R and T=T * -T * R , λ A = λ w +(1-Φ) λ r and C v = Φρ w c w +(1-Φ) ρ r c r . We use <strong>the</strong> sign convention thatstresses are positive if in tension.The initial and boundary conditions for <strong>the</strong>problem are given asPr ( ,0) 0, Tr ( ,0) 0,*rPw at r= rw,r R0 S0cos2 when r , R0 S0cos2 when r ,rS0sin 2 when r ,* *P P P at r= r , P 0 when r ,w R w*w RwT T T * at r= r , T 0 when r .Method for solutionIn order to make <strong>the</strong> problem tractable, <strong>the</strong> in-expressed in terms <strong>of</strong>plane principal stresses areequivalent isotropic (or mean) and deviatoricstresses defined as followsR ( )/2, S ( )/2.0 max min 0 max minThe problem can <strong>the</strong>n be decomposed into twomodes: axi-symmetric (mode I) and deviatoricloading (mode II) (Detournay and Cheng 1988).For <strong>the</strong> first mode, <strong>the</strong> well is subjected to anisotropic far-field mean stress R 0 , boreholepressure P * w and temperature T * w at <strong>the</strong> wellborewall. The second mode is associated with aborehole subject to a remote far-field pure shearstress. Moreover, <strong>the</strong> borehole boundaryconditions are all included in <strong>the</strong> first mode, sothat <strong>the</strong> boundary conditions for <strong>the</strong> second modeare homogeneous. Taking <strong>the</strong> stresses inducedby mode I as σ 1 , σ 1 , σ 1 , and <strong>the</strong> stress inducedr θ rθB<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>by mode II as σ r 2 , σ θ 2 , σ rθ 2 , <strong>the</strong> final stresses for<strong>the</strong> complete <strong>the</strong>rmo-poro-elastic problem arefound by superposition <strong>of</strong> <strong>the</strong> above solutions inLaplace space (Wu et al., 2009).Numerical resultsBy using <strong>the</strong> numerical Stehfest method(Detournay and Cheng 1988), <strong>the</strong> solution in <strong>the</strong>time domain is obtained. The parameters used for<strong>the</strong> example calculations are listed in Table 1, andare for <strong>the</strong> particular case <strong>of</strong> a granite-watersystem. In <strong>the</strong> following figures, <strong>the</strong> black, red andblue curves are for <strong>the</strong> pure elastic, poro-elastic(Detournay and Cheng 1988) and <strong>the</strong>rmo-poroelasticsolutions (<strong>the</strong> present solution),respectively. And, <strong>the</strong>ir difference in time isdiscerned by line types, solid curves for t=0.9 s,medium dashed curves for t =1.5 mins, shortdashed curves for t=2.5 hrs, dotted curves fort=10.4 days, dash-dotted curves for t=2.85 years.Table 1 Parameters for calculationParameterValuesFluid, rock mass density ρw, ρr (Kg/m 3 ) 1000, 2700Fluid, rock specific heat cw, cr (J/Kg/K) 4200, 1000Fluid, rock <strong>the</strong>rmal conductivit y λw, λr (W/m/K) 0.6, 2.4Rock permeability k (mD) 4.0×10 -5Fluid viscosity μ (Pa·s) 0.0004Drained <strong>the</strong>rmal expansion coeff. αB (1/K) 5.0×10 -6Undrained <strong>the</strong>rmal expansion coeff. αu (1/K) 1.0×10 -5Biot coefficient B i 0.47Max principal stress σ max (Pa)-1.7×10 8Min principal stress σmin (Pa) -1.3×10 8Vertical principal stress σ v (Pa)-1.1×108Initial pore pressure PR * (Pa) 7.0×10 7Wellbore pressure P w * (Pa)7.8×10 7Wellbore temperature T w * (K)323, 423Initial temperature T R * (K)523Shear modulus G (Pa) 1.5×10 10Drained and undrained poisson ratio v, vu 0.25, 0.34Porosity Φ 0.09Thermal effects on pore press ureFrom Figure 2(a) it is clear that <strong>the</strong> pore pressureobtained from <strong>the</strong> poro-elastic model for mode lIloading decreases monotonically with radialdistance and time to <strong>the</strong> reservoir pressure.However, for <strong>the</strong> <strong>the</strong>rmo-poro-elastic solutions,<strong>the</strong> pore pressure in <strong>the</strong> region near <strong>the</strong> wellborecan decrease to below <strong>the</strong> reservoir pressure atsmall times if <strong>the</strong> far-field stresses are isotropic.When <strong>the</strong> cold fluid is injected into <strong>the</strong> wellbore,from Figure 3(a), we see that <strong>the</strong> temperaturegradient near <strong>the</strong> wellbore is very high, although itdecreases with time. This may lead to a reductionin pore pressure to below <strong>the</strong> reservoir pressuresince <strong>the</strong> contraction <strong>of</strong> cooling water results in a227


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>volume decrease <strong>of</strong> <strong>the</strong> pore fluid.The pore pressure and temperature induced by<strong>the</strong> anti-symmetrical loading is displayed in Figure2(b) and Figure 3(b). We see that, even though<strong>the</strong> <strong>the</strong>rmal effect has been taken into account,<strong>the</strong> pore pressure curves from <strong>the</strong> <strong>the</strong>rmo-poroelasticsolutions show little difference compared to<strong>the</strong> poro-elastic solutions. This confirms, asexpected, that <strong>the</strong> shear deformation induced by<strong>the</strong> anti-symmetric loading does not causesignificant temperature change, as shown inFigure 3(b). For <strong>the</strong> present case, <strong>the</strong> antisymmetricstress S 0 is 20 MPa, from Figure 3(b)<strong>the</strong> temperature change is in <strong>the</strong> order <strong>of</strong> 1ºC.Figure 2(c) is superposition <strong>of</strong> Figure 2(a) and (b),where <strong>the</strong> <strong>the</strong>rmal effect on <strong>the</strong> pore pressure canbe strongly <strong>of</strong>fset by <strong>the</strong> pressure change fromshear loading.Thermal effect on stressesIn mode II, <strong>the</strong> radial stress is not sensitive to <strong>the</strong>temperature difference between <strong>the</strong> well and <strong>the</strong>far field, as show Figure 4(b). But <strong>the</strong> radial stressdepends on <strong>the</strong> wellbore temperature, since <strong>the</strong><strong>the</strong>rmal responses and volumetric change areboth significant. At a certain distance to <strong>the</strong> wall <strong>of</strong><strong>the</strong> well, <strong>the</strong> radial stress level is elevated by acooler injection fluid as indicated in Fig. 4(c).However, <strong>the</strong> radial stress on <strong>the</strong> well wall isimposed by <strong>the</strong> boundary condition.Figures 5(a)-(d) display <strong>the</strong> hoop stress evolutionfor two different well temperatures. Figure 5(b)shows that <strong>the</strong> hoop stresses induced by mode IIloading follow <strong>the</strong> poroelastic solutions closelyexcept at early time and near <strong>the</strong> wellbore.Figures 5(c) and 5(d) indicate that <strong>the</strong> cooler <strong>the</strong>well, <strong>the</strong> higher <strong>the</strong> hoop stress in tension.Moreover, <strong>the</strong> hoop stress at <strong>the</strong> wall, although itdoes not change with time, can be increased byimposing a cooler well condition. The hoop stresscontours at different wellbore temperatures(T * w =373 K and 423 K) are shown in Figure 6.These plots clearly demonstrate <strong>the</strong> positionalong <strong>the</strong> maximum tectonic stress directionexperiences <strong>the</strong> lowest compressive hoop stress.In Figure 7, <strong>the</strong> vertical stress evolution isprovided. When <strong>the</strong> wellbore temperature is equalto <strong>the</strong> far-field rock temperature shown in Figure7(A), <strong>the</strong> vertical stress contours appearunchanged because <strong>of</strong> <strong>the</strong> very small temperaturegradient in <strong>the</strong> whole domain.However, when <strong>the</strong> wellbore is at a lowertemperature (Figure 7(B)), <strong>the</strong> vertical stresschange is also enhanced. The maximum tensilestress change in <strong>the</strong> vertical direction also existsat <strong>the</strong> position along <strong>the</strong> maximum tectonic stress.Moreover, if <strong>the</strong> vertical stress becomes less than<strong>the</strong> borehole pressure, a horizontal openingfracture may well be formed at this corner. Theplane strain assumption adopted here is expectedto produce <strong>the</strong> strongest estimate for change in<strong>the</strong> vertical stress because <strong>of</strong> <strong>the</strong> built-inassumption <strong>of</strong> zero strain in <strong>the</strong> axial direction.P/|S0|P/|S0|P/|S 0 |4.14.03.93.83.70.0-0.2-0.4-0.6-0.8-1.0-1.24.24.03.83.63.43.23.02.82.6(a)2 4 6 8 10r/r w(b)2 4 6 8 10r/r w(c)2 4 6 8 10r/r wFigure 2: Pore pressure for (a) mode I, (b) mode II and (c)mode I+II for θ=0.Temperature T/TR*Temperature T/TR *1.000.950.900.850.800.750.0000-0.0001-0.0002-0.0003(a)t=0.9 st=1.5 minst=2.5 hrst=10.4 dayst=2.85 years2 4 6 8 10r/r w(b)t=0.9 st=1.5 minst=2.5 hrst=10.4 dayst=2.85 years2 4 6 8 10r/r wFigure 3: Temperature for (a) mode I and (b) mode II at θ=0228


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>-4-7-5-8(a)(a) r/|S0 |-6 /|S 0|-9-7-10-82 4 6 8 10r/r w-114.02 4 6 8 10r/r w0.43.5 r/|S0 |0.20.0-0.2-0.4(b) /|S 0|3.02.52.0(b)-0.61.5-0.8-1.0-42 4 6 8 10r/r w1.0-5.01.0 1.2 1.4 1.6 1.8 2.0r/r w-5.5-5(c)-6.0(c) r/|S0 |-6 |S 0|-6.5-7-7.0-7.5-8-42 4 6 8 10r/r w-5.02 4 6 8 10r/r w-5.5-5(d)-6.0(d) r/|S0 |-6 |S 0|-6.5-7-7.0-82 4 6 8 10r/r wFigure 4: Radial stresses at θ=0 for (a) mode I, (b) mode IIand (c) mode I+II at Tw * =373 K; (d) mode I+II at Tw * =423 K.Thermal effects on wellbore stabilityWellbore breakdownThe hoop stress on <strong>the</strong> wall <strong>of</strong> <strong>the</strong> well can becalculated <strong>the</strong>oretically. Based on rock strength<strong>the</strong>ory, <strong>the</strong> breakdown pressure is obtained asfollows (Wu et al. 2009)* *6 GK ( T T)*B B R WT2R0 2PR4S0KB 4 G/3pb2(1 )where σ T is <strong>the</strong> tensile strength. When S 0 0, θ is taken as /2 toobtain <strong>the</strong> minimum pressure.,-7.52 4 6 8 10r/r wFigure 5: Hoop stresses at θ=0 for (a) mode I, (b) mode IIand (c) mode I+II at Tw * =373 K; (d) mode I+II at Tw * =423 K.Wellbore shear failureThe Mohr Coulomb strength criterion is used toassess wellbore shear failure risk based on <strong>the</strong>solutions for σ r , σ θ , σ rθ and σ z . In terms <strong>of</strong> principaleffective stresses, <strong>the</strong> criterion may be written as: (1sin ) / (1sin )''1 s3where σ s and are <strong>the</strong> unconfined compressivestrength and <strong>the</strong> internal friction angle’respectively. The stresses σ 1 ’ and σ 3 are <strong>the</strong>maximum and minimum principal effectivestresses based on Terzaghi’s definition. A safetyfactor for shear failure is defined based on <strong>the</strong>Mohr-Coulomb strength criterion as' 'SF (1 ssin ) / (1 sin ) 3 / 1.229


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>SF>1 indicates that <strong>the</strong> effective stress state isbelow <strong>the</strong> shear strength envelope and <strong>the</strong>reforesafe from shear failure, whilst SF


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>can be reduced in magnitude if <strong>the</strong> well becomescooler. This may lead to <strong>the</strong> formation <strong>of</strong> openingfracture from <strong>the</strong> borehole.3. The breakdown pressure is reformulated toinclude <strong>the</strong> <strong>the</strong>rmal effect.4. In addition to <strong>the</strong> shear failure in <strong>the</strong> minimumhorizontal stress direction <strong>of</strong>ten observed as widebreakout, shear failure can also occur in <strong>the</strong>maximum horizontal stress direction d ue to <strong>the</strong>wellbore cooling effect. However, <strong>the</strong> later isdependent on <strong>the</strong> plane strain assumption.(A)(B)Figure 8: Safety factor for different wellbore temperature.ConclusionsIn this paper, <strong>the</strong> semi-analytical solutions for <strong>the</strong>temperature, pore pressure and stress around awellbore are obtained. By comparing <strong>the</strong> resultswith those from <strong>the</strong> poroelastic solutions, <strong>the</strong>following interesting results are drawn:1. The <strong>the</strong>rmal effect can affect <strong>the</strong> pore pressureat small times and in <strong>the</strong> near-well region, but thisinfluence decays with time.2. The <strong>the</strong>rmal effects can elevate not only <strong>the</strong>radial stress but also <strong>the</strong> hoop stress. This effectbecomes more important with time and for acooler well. It is also found that <strong>the</strong> vertical stressReferencesRice, J.R. and Cleary, M.P., 1976, Some basicstress diffusion solutions for fluid saturated elasticporous media with compressible constituents,Rev. Geophys and Space Physics, v.14, no.2,p.227-241.Detournay, E. and Cheng, A. H-D., 1988,Poroelastic response <strong>of</strong> a borehole in a nonhydrostaticstress field, Int. J. Rock Mech. Min.Sci. & Geomech. Abstr., v.25, no.3, p.171-182.Ekbote, S., Abousleiman, Y., Cui, L. and Zaman,M., 2004, Analyses <strong>of</strong> inclined boreholes inporoelastic media, Int. J. Geomech., v.4, no.3,p.178-190.Rajapakse, R.D.. 1993, Stress analysis <strong>of</strong>borehole in poroelastic medium, J. <strong>of</strong> Eng. Mech.v.119,no.6, p.1205–1227.Biot, M.A., 1941, General <strong>the</strong>ory <strong>of</strong> three-M., 1989, A <strong>the</strong>rmoelastic <strong>the</strong>ory <strong>of</strong>dimensional consolidation, J. Appl. Phys., v.12,no.2, p.154-164.McTigue, D.F., 1986, Thermoelastic reponse <strong>of</strong>fluid-saturated porous rock, J. Geophys. Res.,v.91 (B9), p.9533-9542.Kurashige,fluid-filled porous materials, Int. J. Solids Struct.,v.25, no.9, p.1039-1052.Coussy, O. 1989, A general <strong>the</strong>ory <strong>of</strong><strong>the</strong>rmoporoelastoplasticity for saturated porousmaterials, Journal Transport in Porous Media, v.4,no.3, p.281-293.Wang, Y. L. and Papamichos, E., 1994,Conductive heat flow and <strong>the</strong>rmally induced fluidflow around a wellbore in a poroelastic medium,Water Resour. Res., v.30, p.3375-3384.Li, X., Cui, L., and Roegiers, J.C., 1998,Thermoporoelastic analyses <strong>of</strong> inclined boreholes,In SPE/ISRM Rock Mechanics in PetroleumEngineering, Trondheim, Norway, p.443-451.Wu, B., Zhang, X. and Jeffrey, R. G., 2009,CSIRO internal report.231


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>3D Geological Modelling for Geo<strong>the</strong>rmal Exploration in <strong>the</strong> TorrensHinge ZoneMat<strong>the</strong>w Zengerer 1 *, Chris Mat<strong>the</strong>ws 2, Jerome Randabel 3 .1 10 Holland St, Thebarton, SA, 5031.2 6 Hollywood Way, Glenalta, SA, 5052.3 Torrens <strong>Energy</strong> Limited. PO Box 506, Unley, SA, 5035.* Corresponding author: mzengerer@hotmail.comThis paper d escribes 2D/3 DGeophysical/Geological M odelling undertaken by<strong>the</strong> autho r f or T orrens E nergy i n 20 09, for <strong>the</strong>purpose <strong>of</strong> establi shing 3D Geol ogical Models o f<strong>the</strong> uppe r crust within th eir Torren s Hinge Zonetenements in South Australia. Geolo gical Mo delsare a re quirement for a ny Geo<strong>the</strong> rmal <strong>Energy</strong>explorer sea rching for Hot Dry Ro ck or HotSedimentary Aquifer targets. T hese Geol ogicalModels are assigne d <strong>the</strong>rmal parametersdetermined by field and laborato ry measurementsbased on th e litholo gies included in t he mo del.Heat resources m ay <strong>the</strong>n be computed for th egiven volume based on <strong>the</strong> geological model and<strong>the</strong>rmal rock prope rties. Whil st <strong>the</strong> studie s we recarried out for <strong>the</strong> purp ose <strong>of</strong> cre atingtemperature model s an d geoth ermal resou rceestimates, this document will di scuss <strong>the</strong>geological models, geophysical investigations andtectonic impl ications ge nerated by <strong>the</strong> stu dy.Examples <strong>of</strong> Geological M odels are sh own from<strong>the</strong> Torren s <strong>Energy</strong> Po rt Augusta, Y adlamalkaand Pa rachilna G eo<strong>the</strong>rmal Pro spects, ba sedover <strong>the</strong>ir GELs 230, 234, 235, 285 and 501.Keywords: South Aust ralia, 3 D GeologicalModelling, Geophy sical Modellin g, Heat Flow,Stratigraphy, Torren s Hinge Zo ne, Adelaid eGeosyncline, Magneti cs, Euler Deconvolution,Geo<strong>the</strong>rmal <strong>Energy</strong>.Introduction and Geological SettingThe principle behind 3D Geological Modelling is tointegrate existing geological and drillinginformation with ge ophysical data such a sseismic, gravity and magneti cs, in a 3 Denvironment which will simulate <strong>the</strong> 3D geology <strong>of</strong><strong>the</strong> region <strong>of</strong> interest by creating a 3D geologicalmodel which ca n <strong>the</strong> n b e u sed a s a n inp ut fo r<strong>the</strong>rmal modelling.The Torrens Hinge Zone is a lo ng but narrow (upto 40 km wide) geological transition zone between<strong>the</strong> relativel y stable Eastern Ga wler Craton“Olympic Do main” to <strong>the</strong> west an d <strong>the</strong> folde dsedimentary ba sin known a s th e Adelaid eGeosyncline to <strong>the</strong> e ast (Drexel et al, 1993). TheTHZ is essentially a region <strong>of</strong> overlap between <strong>the</strong>Gawler Craton and Adelaide Geosyncline (Figure1). In <strong>the</strong> study areas <strong>of</strong> <strong>the</strong> T HZ, <strong>the</strong> Adelaideanand Camb rian se dimentary seq uences areunderlain at depths between 2,000 and 7,000m byPaleoproterozoic to Meso proterozoic Ga wlerCraton Olym pic Domain rocks (Matth ews andGodsmark, 2009).Heat flo w va lues <strong>of</strong> over 90 m W/m 2 have bee nrecorded in several wells drilled in <strong>the</strong> THZ. Withseveral kilometres th ickness <strong>of</strong> mode rateconductivity sedim ents o verlying <strong>the</strong> crystallin ebasement in this re gion, predicted te mperaturesat 5000 m are u p to 3 00 o C in some are as(Mat<strong>the</strong>ws and Godsmark, 2009).Data and MethodologyAvailable ge ological data inclu ded hi storic an dTorrens En ergy d rillholes and South <strong>Australian</strong>(SA) geol ogical map ping. Geophy sical datacomprised SA magnetic and Bouguer Gravity dataalong with recently acquired Torrens <strong>Energy</strong> andGeoscience Australi a 2D de pth-convertedSeismic. Ro ck <strong>the</strong>rmal p roperties were de rivedfrom lab oratory mea surements pe rfomed byTorrens En ergy an d top and downhol etemperatures measured from drilling.The Intrepid 3D Geo modeller suite wa s used tobuild <strong>the</strong> 3D Ge ological Mo del. The 3 DGeomodeller s<strong>of</strong>tware interp olates bet weengeological b oundaries, orientatio n data an ddrillholes to g enerate a 3D geologi cal model thatis flexible an d rea dily ad aptable with addition algeological information. Geomodeller also supportsfaults and fo ld informatio n into its interpol ation.The final ou tput can be discretised into a 3D“voxel” mod el <strong>of</strong> desired resolution to use in 3 DGeo<strong>the</strong>rmal Modelling.232


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Figure 1. Map <strong>of</strong> Central South Australia showing tectonic elements and study areas toge<strong>the</strong>r with Torrens <strong>Energy</strong>wells, seismic lines and prospects233


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Basic Modelling requirementsThe follo wing method ology wa s a pplied toconstruct a 3 D Geological model. It relies he avilyon inte rpretation and inte gration <strong>of</strong> m any datatypes, as well as some cr eative th inking an dintuition. All 3D geol ogical mod els built byGeomodeller begin with 4 pieces <strong>of</strong> information.The first is a defined 3D volume <strong>of</strong> interest, set b yrectangular coordinates <strong>of</strong> <strong>the</strong> target area, and asuitable dept h dimen sion which will encom pass(preferably) <strong>the</strong> heat source, basin thickness andtopography. For both Parachil na and PortAugusta a d epth belo w Mean Sea L evel <strong>of</strong> 7kmand a maximum <strong>of</strong> 1.5km above MSL to clear <strong>the</strong>range topo graphy was deemed sufficient, givingan 8.5km thi ck mo del. T he are a cov ered in <strong>the</strong>Parachilna model wa s 50x45 km, and 50x80kmover Port Augusta/Yadlamalka.A surface topography is re quired for <strong>the</strong> model tocompute th e interse ctions <strong>of</strong> <strong>the</strong> geologicalinterfaces at su rface, ie to have an initial 2 Dsection at which to i nput geolo gical i nformationand have it reproduced by <strong>the</strong> model computationfor validation. Topog raphy was imp orted into <strong>the</strong>models from SRTM DEM grids at 90 m resolutionclipped to <strong>the</strong> Area Of Interest (AOI), Figure1.The third and fourth requirements are <strong>the</strong> definedgeology in <strong>the</strong> form <strong>of</strong> lith ological inte rfaces an dassociated stru ctural orie ntations, and astratigraphic pile whi ch defines th e re lationshipsbetween <strong>the</strong> lithologies. T he latter is particularlyimportant as contacts need to have rel ationshipsdefined a s ei <strong>the</strong>r Onl apping or Ero sional, as thisdetermines whe<strong>the</strong>r interface isolines intersect orremain ap art with repe ct to on e ano<strong>the</strong> r.Sequences <strong>of</strong> geolo gical units such a s fou nd i nsedimentary ba sins m ay also be grouped inonlapping se ries, whe reas intrusives are alwayserosional a nd ap pear where requi red in th estratigraphic pile to best sati sfy conta ctrelationships. In st rongly deform ed regi ons,structural requirements may imply that lithologie smust o bey o nlapping rath er tha n e rosional rules.A simplificati on <strong>of</strong> <strong>the</strong> stratig raphy wa s alsocreated fo r e ase <strong>of</strong> mode lling (Fig ure 2), whi chessentially has g rouped <strong>the</strong> Cam brian a ndNeoproterozoic sequences i nto t heir m ajortectono-stratigraphic units.Figure 2. Simplified Parachilna Stratigraphy.Geological i nformation a t surfa ce came fromimporting simplified or grouped shapefiles derivedfrom State 100k geol ogy polygons, and assigning<strong>the</strong>se to <strong>the</strong> sim plified stratigraphic f ormations.Likewise ori entation dat a, whe re known fro mmapping, have been supplied where possible andassigned to specific fo rmations. T orrens Ene rgyand historic diamond drillhole data have providedconstraint in <strong>the</strong> 3 rd dimensio n. Once again <strong>the</strong>geological logs <strong>of</strong> <strong>the</strong>se d rillholes were simplifiedto <strong>the</strong> stratigrap hy and <strong>the</strong> drillhole s importe dusing <strong>the</strong> import tools in Geomodeller (figure 3).Figure 3. Port Augusta 3D Interface Points and Drillholes inGeomodeller project.Supplementing Geology with GeophysicsUnless <strong>the</strong> re is a complete cove rage o f mappe dgeological information at surface, it is u nlikely thatreliable mode ls ma y b e d erived fr om s urfacemapping alo ne. To sup plement <strong>the</strong> existinggeological i nformation, interp retation <strong>of</strong> four 2 Ddepth-converted seismic lines, (two f rom th eParachilna area and two from <strong>the</strong> Port234


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Figure 4. 2D Magnetics Model across Parachilna , showing main basin elements, possible magnetic intrusives andshallow fault-related magnetic bodiesFigure 5. Persepective view <strong>of</strong> 3D Bodies derived from 2.5D Magnetic modelling within Augusta/Yadlamalka acrossParachilna , including dykes, possible magnetic intrusives and sheet-like layers, probably thrusted Beda Volcanics.Figure 6. Depths to Base Sturtian, ie top Beda Volcanics, derived from Euler Deconvolution <strong>of</strong> Magnetics. Showntoge<strong>the</strong>r with drillholes from Augusta/Yadlamalka prospects.235


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Augusta/Yadlamalka a rea), was performed (se eAppendix 1). These were con strained whereverpossible by drilling and outcrop i nformation.These seismic sections w ere im ported int oGeomodeller as im age backdrops alo ng verti calsections through <strong>the</strong> model and <strong>the</strong> interpretationtransformed into interfac es within <strong>the</strong>se vertic alsections.The inte rpretation alon g <strong>the</strong>se sections wasaugmented f ur<strong>the</strong>r in <strong>the</strong> Para chlina AOI by 2Dmodelling <strong>of</strong> state mag netic data al ong two line sadjacent to <strong>the</strong> 09TE-01 seismic line (figure 4). In<strong>the</strong> Port Augusta re gion, 2D mag netic modellingwas also performed in order to obtain estimates <strong>of</strong>basement de pth and mag netic bo dy shape s an dlocations (figure 5). In each case images or actual3D data poi nts from <strong>the</strong> result s we re importe dback into Geomodeller.Euler Deconvolution <strong>of</strong> magnetic d ata wa s alsoused in this area to pro vide spot estimates <strong>of</strong>depth to sh allow-dipping volca nic u nits, implyinglocal e stimates to <strong>the</strong> top <strong>of</strong> Willouran -age Bed aVolcanics (figure 6 ). Ad ditional scans u sing alarger window size revealed information about <strong>the</strong>shape and size <strong>of</strong> de eper magnetic bodies whichcorrelate well with 2D magnetic modelling results.Finally, structural interpretation <strong>of</strong> both gravity andmagnetic d ata wa s used t o define fault traces inGeomodeller (see Appendix 2).3D Geological ModelsComputation time <strong>of</strong> th e two 3D Geologicalmodels is dependent on <strong>the</strong> amou nt <strong>of</strong> datasupplied. Re sults which are strongly biased toorientation data were trea ted with ca ution. Someadditional inference <strong>of</strong> contacts and o rientationswas requi red to en sure geological co nsistency,especially near faults. Additional se ctions lin kingdrillholes p rovided strong er cro ss-correlation <strong>of</strong>geological i nterfaces, especially in <strong>the</strong> PortAugusta/Yadlamalka area where data was wid elyspaced. Although in some ca ses actu al outcro pgeology was fur<strong>the</strong>r from <strong>the</strong> area <strong>of</strong> interest thanrequired, it was incl uded to provide geologicalreality and well-defined constraints on modelling.relatively flat-lying in <strong>the</strong> west to mod erately eastdippingat <strong>the</strong> Ediacara fault contact.Figure 7a. Projected section view <strong>of</strong> Parachilna 3D GeologyModel, view SE. Vertical. exaggeration= 2:1The Edia cara fault zone chan ges in characte rfrom south to north. Our m odelling shows it to bea ste eply west-dipping fe ature, u pthrown on th eeastern side, whi ch evolves i n <strong>the</strong> south from arelatively si mple antiform, to a complex horststructure inv olving seve ral faults an d possiblybasement o r diapiri c mat erial fro m <strong>the</strong> cent re <strong>of</strong><strong>the</strong> Para chilna AOI to its nor<strong>the</strong> rn edg e.Basement depths in <strong>the</strong> far west are predicted torange from 2km depth in t he north to 5 km in <strong>the</strong>south. In <strong>the</strong> vicinity <strong>of</strong> <strong>the</strong> Ediacara Fault footwallbasement depth reaches 6km, but this decreasesto 2.5-3km i n <strong>the</strong> fa r north. In <strong>the</strong> fa ulted h orstblocks <strong>of</strong> <strong>the</strong> Ediacara Fa ult region ba sement ordiapiric material may reach depths <strong>of</strong> 2km. East <strong>of</strong><strong>the</strong> Ediaca ra Fault in <strong>the</strong> central and sou<strong>the</strong> rnareas is a moderately folded di sturbed regi onleading eastward into a very d eep synclinal basinwithin <strong>the</strong> Cambri an – Adelaide an seq uencesadjacent to <strong>the</strong> ran ge fro nt fault. To <strong>the</strong> north <strong>of</strong>this are a <strong>the</strong> model pre dicts le ss inten se foldin gwith flatter basi n sequences, but still basinthicknesses <strong>of</strong> > 7km.As faults also require orientation information to becomputed in <strong>the</strong> modelling, <strong>the</strong>ir direction, dip andapparent mo vement was estimated e i<strong>the</strong>r fromseismic ima ges or ge ological an d geophysicalimages.ParachilnaEmphasis on interpretatio n an d m odelling in th eParachilna area focu ssed on area s west <strong>of</strong> <strong>the</strong>Ediacara fault (Figure 7a, 7b, Appendix 2) where<strong>the</strong>re is sim pler geology according to <strong>the</strong> seismicdata. In this area we se e from modelling that <strong>the</strong>Early Camb rian to A delaidean ro cks transit f romFigure 7b. Interfaces and Faults, Parachilna 3D. View NE,VE=3:1236


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Cainozoic erosional unit s ten d to range inthickness f rom 300 -400m and thi n o ut in <strong>the</strong>vicinity <strong>of</strong> <strong>the</strong> Ediacara Fa ult hangi ng wall. Earlyto Middle Cambri an unit s <strong>of</strong> <strong>the</strong> La ke Frome,Unnamed, and Ha wker Groups h ave beenconfirmed b y deep drilli ng, whil st Adelaid eanrocks <strong>of</strong> Mari noan to Sturt ian age s a re expecte dto lie b eneath <strong>the</strong> se based on <strong>the</strong>ir p resence in<strong>the</strong> Edia cara Hill s to <strong>the</strong> north in th e fault zo neand outcrops <strong>of</strong> <strong>the</strong> se units to <strong>the</strong> we st on <strong>the</strong>Stuart Shelf. Inference <strong>of</strong> Torrensian to Willouranrocks is ba sed on <strong>the</strong> apparent p resence <strong>of</strong>diapirs to <strong>the</strong> south an d east, although <strong>the</strong>serocks are expected to thi n out somewhere in thi sregion. Torre nsian ro cks in parti cular may notappear anywhere west <strong>of</strong> <strong>the</strong> Edi acara F aultsystem. Basem ent has b een largel yundifferentiated in <strong>the</strong> Pa rachilna 3 D model wit h<strong>the</strong> exception <strong>of</strong> what are inferred to be two largemagnetic intrus ives in <strong>the</strong> c entral parts andnorthwest.Port Augusta/YadlamalkaA very large area has been modelled in this study,which naturally implie s a greater amount <strong>of</strong> b othinference and uncertainty. To complement this i smore complex geology and more drilling data, aswell a s mu ch more dive rse ma gnetic sign aturesand seismic imagery.The final 3D model is shown as sections andsurfaces in Figures 8a and 8b. In general <strong>the</strong>stratigraphy is identical to that used at Parachilna,with <strong>the</strong> addition <strong>of</strong> several intrusive basementunits <strong>of</strong> varying magnetic signature and a split <strong>of</strong><strong>the</strong> Willouran-age rocks into BedaVolcanics/Backy Point Formation, generalWillouran – age rocks and several thrustedWillouran – age slices. The overall trendsmodelled show an eastward – thickening wedge<strong>of</strong> sediments toward <strong>the</strong> range front, with possibledown-thrown rift basins evolving closer to <strong>the</strong>range. To <strong>the</strong> nor<strong>the</strong>ast thrust faults occur subparallelto <strong>the</strong> Gairdner Dyke Swarm before <strong>the</strong>range front and are possibly facilitated byCallanna group evaporitic units and/or diapirism.To <strong>the</strong> east <strong>of</strong> <strong>the</strong>se significant thrusts, closer to<strong>the</strong> range fault, sediments begin to dip morestrongly or are deformed. Some deformation isalso present immediately west <strong>of</strong> <strong>the</strong> thrusts on<strong>the</strong> footwall side, but this peters out as sedimentsbecome more flat-lying to <strong>the</strong> west.In <strong>the</strong> south and south central areas in <strong>the</strong> vicinity<strong>of</strong> Port Augusta, <strong>the</strong> model predicts gently dippingAdelaidean rocks <strong>of</strong> 800 – 1200m thickness,overlying granitic or metamorphic basement,crossing a significant north-nor<strong>the</strong>ast trendingbasin-defining fault approximately 10km northwest<strong>of</strong> Port Augusta, coincident with <strong>the</strong> onset <strong>of</strong> asignificant gravity low and a step in <strong>the</strong> magneticsand seismic images. Here <strong>the</strong> basin thicknessincreases to at least 2000m, dropping awaygradually to 3000m approximately 9km west <strong>of</strong><strong>the</strong> range front, before dipping away more steeplyto 4500m at <strong>the</strong> base <strong>of</strong> <strong>the</strong> range fault. Deeperreflectors in <strong>the</strong> Augusta seismic section areenigmatic but <strong>the</strong>ir pattern is suggestive <strong>of</strong> rifting,<strong>the</strong> timing <strong>of</strong> which should be investigated fur<strong>the</strong>r,if proven (see Discussion). Modelling resultsbased on historical drilling near Wilkatana (centralsou<strong>the</strong>rn Yadlamalka prospect) demonstratelocalised basins containing Cambrian sediments.The interpretation on <strong>the</strong> seismic lines 09TE-02(Augusta) and 08GA-01 (Arrowie) is still <strong>the</strong>subject <strong>of</strong> some debate, until such time as somespecific drilling is performed along <strong>the</strong> lines andstratigraphic correlations are performed. Theinterpretation has been made through carefulcross-comparison <strong>of</strong> nearby drillholes usingGeomodeller as a guide, using logged depths tospecific units and comparing how <strong>the</strong>y aredistributed across <strong>the</strong> area, and existinggeological mapping.Inferences have been made on <strong>the</strong> nature anddistribution <strong>of</strong> <strong>the</strong> Willouran and Torrensian agerocks in a fashion similar to <strong>the</strong> interpretation atParachilna, as well as deeper Proterozoicbasement units. These inferences will bediscussed in <strong>the</strong> next section.Figure 8a 3D volume model <strong>of</strong> Augusta/Yadlamalka. ViewNE, VE=3:1.The nor<strong>the</strong>rn parts <strong>of</strong> <strong>the</strong> model, described asYadlamalka after <strong>the</strong> name <strong>of</strong> <strong>the</strong> stationsou<strong>the</strong>ast <strong>of</strong> Lake Torrens near a major thrustzone, has similar gently dipping Adelaideanstratigraphy ranging from 600m thickness in <strong>the</strong>far west to 2300m before encountering asignificant thrust fault which displaces Willouranvolcanics close to surface, as evidenced by <strong>the</strong>Arrowie seismic section, drilling and magnetics.Unlike <strong>the</strong> more obvious extensional faultingregime exhibited far<strong>the</strong>r south, basin units appearless disturbed, but a very marked angularunconformity exists between <strong>the</strong>sedimentary/volcanic pile and <strong>the</strong> basement,which comprises a series <strong>of</strong> west-dippingreflectors. East <strong>of</strong> <strong>the</strong> Yadlamalka thrust <strong>the</strong>237


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>sedimentary pile is moderately folded and <strong>of</strong>unclear composition and thickness. What is clearis that thrusting and compressional deformationhas disturbed <strong>the</strong> Adelaidean sequences in morethan one location. It is also speculated thatWillouran/Callanna Group salt formations mayagain be principally involved.Figure 8b 3D section view <strong>of</strong> Augusta/Yadlamalka. View NW,VE=3:1.In <strong>the</strong> nor<strong>the</strong>rn part <strong>of</strong> <strong>the</strong> model magneticmodelling has suggested that a number <strong>of</strong>magnetic intrusives are present, along with slices<strong>of</strong> Willouran age volcanics. These have beenemplaced into <strong>the</strong> model where most likely, but<strong>the</strong> remainder <strong>of</strong> <strong>the</strong> basement has beenundifferentiated.Partial modelling <strong>of</strong> <strong>the</strong> range to <strong>the</strong> east hasbeen included to add both strratigraphic andstructural control, but has been performed at arepresentative level only. Cainozoic strata alsoappear relatively thin in this region but have beenincluded as a thin uppermost layer where evident.Overall, <strong>the</strong> Early Cambrian to Neoproterozoicbasin succession throughout <strong>the</strong> area remainsrelatively simple. Sequences dip gently eastwardand thicken before <strong>the</strong> onset <strong>of</strong> thrusting, folding,or extensional faulting. Roughly midway across<strong>the</strong> model Torrensian lithologies are inferred toappear (see Discussion).DiscussionResults and some <strong>of</strong> <strong>the</strong> methodology used in <strong>the</strong>Port Augusta/Yadlamalka area require somediscussion due to inferences being made and <strong>the</strong>tectonic consequences <strong>of</strong> <strong>the</strong> modelledrelationshipsThese inferences particularly concern <strong>the</strong> nature<strong>of</strong> <strong>the</strong> rocks within <strong>the</strong> basin sequences west <strong>of</strong><strong>the</strong> range front fault. Torrensian/Burra Grouprocks are not known to occur west <strong>of</strong> this structureor anywhere on <strong>the</strong> Stuart Shelf, however wehave inferred from <strong>the</strong> seismic that Torrensianrocks pinch out or fault out fairly consistently 20-30km west <strong>of</strong> <strong>the</strong> range front, mainly at depthsdeeper than what has been currently encounteredin drill holes. The implication from this is thatTorrensian sedimentation is controlled by asecond onset <strong>of</strong> strong rift-related extensioncloser to <strong>the</strong> Central Flinders Zone.Willouran age/Callanna Group rocks have longbeen enigmatic in terms <strong>of</strong> <strong>the</strong>ir relationship too<strong>the</strong>r rocks <strong>of</strong> <strong>the</strong> Adelaide Fold Belt and <strong>the</strong>Gawler Craton, but inferences on <strong>the</strong>ir distributionand geology have implications for understanding<strong>the</strong> early evolution <strong>of</strong> <strong>the</strong> rift zone and laterdeformation. Basaltic rocks <strong>of</strong> <strong>the</strong> Beda Volcanicshave been encountered in many drillholes on <strong>the</strong>Stuart Shelf, mostly at shallow depths, but alsomay have been confused with older GawlerRange Volcanics (GRV) in some holes. Theserocks and associated intertonguing sediments <strong>of</strong><strong>the</strong> Backy Point Formation are thought to form <strong>the</strong>basal units <strong>of</strong> <strong>the</strong> Adelaide Fold Belt rift sequence.Exactly how thick <strong>the</strong>se units are, and whe<strong>the</strong>radditional sediments lie beneath <strong>the</strong> volcanics, isunknown, however drillhole information suggeststhat <strong>the</strong> Beda Volcanics are probably only a fewhundred metres thick, and <strong>the</strong>ir flat-lying naturesuggests that <strong>the</strong>y should form a good reflector inseismic data.Both seismic lines in <strong>the</strong> area show good deepcontinuous reflectors just above or not far above<strong>the</strong> basement, but in places drillholes appear tohave intersected Beda Volcanics well above <strong>the</strong>suspected top basement horizon, at ano<strong>the</strong>rreflector. The Port Augusta seismic line evenappears to show what may be ano<strong>the</strong>r rift grabenwell beneath what is interpreted as Willouran, butuntil this is confimed by fur<strong>the</strong>r studies we haveassumed it to be basement, or at least GRV orsimilar age sediments. Elsewhere we haveinferred that <strong>the</strong> Beda Volcanics are reasonablythick or probably have much larger proportions <strong>of</strong>Backy Point Formation beneath <strong>the</strong>m for <strong>the</strong>purpose <strong>of</strong> modelling. The unmodelled o<strong>the</strong>rpossibilities are that beneath <strong>the</strong> Beda/BackyPoint rocks lie reasonable thicknesses <strong>of</strong>Mesoproterozoic rocks such as <strong>the</strong> PandurraFormation and Gawler Range Volcanics (GRV), orthat Torrensian and Sturtian rocks increasedramatically in thickness midway across <strong>the</strong>model, or both.Fur<strong>the</strong>r information was derived from <strong>the</strong>magnetics. Petrophysically, <strong>the</strong> Beda Volcanicsare known to be moderately magnetic, but <strong>the</strong>irflat-lying nature and probable magnetisationpattern means that unless <strong>the</strong>y are tipped on <strong>the</strong>irsides, <strong>the</strong> net effect is only to add a regional dcshift to <strong>the</strong> overall magnetic signal. High pass andanalytic signal filtering <strong>of</strong> <strong>the</strong> state magnetics,however, has revealed where Beda Volcanicshave been tipped on <strong>the</strong>ir sides and thrust tosurface at <strong>the</strong> Yadlamalka thrust and Depot Creekon <strong>the</strong> range front, where <strong>the</strong>y have been238


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>intersected at surface or in drillholes, with <strong>the</strong>thrust also visible in <strong>the</strong> Arrowie seismic section.Euler Deconvolution <strong>of</strong> magnetics is basedaround automated scanning <strong>of</strong> changes in <strong>the</strong>magnetic signal in windows across a grid, withdepth estimates to magnetic sources dependenton <strong>the</strong> size, intensity, and shape <strong>of</strong> bodies, andwindow size. Two different window sizes wereused, <strong>the</strong> first scanning to depths <strong>of</strong> 2km and <strong>the</strong>o<strong>the</strong>r to 8km. The results <strong>of</strong> <strong>the</strong> shallower windowtargeted mainly <strong>the</strong> tops <strong>of</strong> <strong>the</strong> Gairdner DykeSwarm, which are known to be Beda Volcanicequivalent ages. These are <strong>the</strong>refore byimplication minimum depths to <strong>the</strong> base <strong>of</strong>Sturtian Adelaidean rocks in <strong>the</strong> west, whereTorrensian rocks are not present, and base <strong>of</strong>Torrensian rocks in <strong>the</strong> east where <strong>the</strong> methoddetected thrusted Beda Volcanics. These resultswere statistically culled for reasonableness andproximity to dykes, thrusted volcanics orcloseness to interception in drillholes.The remarkable consistency <strong>of</strong> Euler depth trendsin <strong>the</strong> west for <strong>the</strong> shallow scan gives credence to<strong>the</strong> notion that Beda Volcanics overlie deepersediments and/or volcanics. The idea that GawlerRange Volcanics lie below <strong>the</strong> obvious basementunconformity seen in <strong>the</strong> Arrowie seismic is notsupported by this model, unless east <strong>of</strong> <strong>the</strong> majorvolcanic flows on <strong>the</strong> Gawler Craton <strong>the</strong> GRVwere deformed along with Hiltaba suite anderoded prior to ei<strong>the</strong>r Mesoproterozoic clasticdeposition or Willouran rifting. Similar notionsapply in <strong>the</strong> Port Augusta area.The deeper window targeted magnetic intrusions,by implication a maximum depth to basementacross <strong>the</strong> area. Again <strong>the</strong>se results werestatistically culled and sorted by proximity to <strong>the</strong>inferred “tops” <strong>of</strong> magnetic body depths. Theseresults, along with results <strong>of</strong> 2D magneticmodelling were interpreted to be from deepmagnetic intrusives, possibly even Iron OxideCopper Gold – bearing intrusives lying in <strong>the</strong>centre <strong>of</strong> <strong>the</strong> region (though perhaps too deep fordrilling), ra<strong>the</strong>r than belonging to metasediments,GRV or younger volcanics. Fur<strong>the</strong>r support forthis notion came from examination <strong>of</strong> filteredmagnetic grid images as described above.Values from <strong>the</strong> deeper Euler and 2D magneticmodelling were input back into Geomodeller as<strong>the</strong> basis for intrusive 3D body shapes.Results <strong>of</strong> 3D modelling in <strong>the</strong> Parachilna areaare currently considered less contentious. Theprincipal features for discussion are <strong>the</strong> nature <strong>of</strong><strong>the</strong> magnetic anomalies, whe<strong>the</strong>r <strong>the</strong>y indeedcorrespond to deep intrusives, or are related todiapirism bringing basement magnetic material tocloser to surface, or a combination. The stronggravity anomaly running through <strong>the</strong> centre <strong>of</strong> <strong>the</strong>region suggests it is more likely to be basementreactivated along <strong>the</strong> Ediacara Fault. Once again<strong>the</strong> o<strong>the</strong>r major issue for consideration is <strong>the</strong>presence and distribution <strong>of</strong> Torrensian andWillouran rocks.ConclusionTwo large 3D Geological models have been made<strong>of</strong> se ctions o f <strong>the</strong> Torren s Hing e Zon e in SouthAustralia. Th e north ern model n ear Parachilnashows mo derately di pping Cambrian t oAdelaidean sediments <strong>of</strong> thickne sses between2000 and 4000m overlying unknown basement in<strong>the</strong> we st. A modern a ctive fault system, <strong>the</strong>Ediacara Fault, has uplifte d basement locally an dforms <strong>the</strong> boundary <strong>of</strong> a d eep, moderatelydeformed n orth-south b asin a djacent to <strong>the</strong>Flinders Range front.The sou<strong>the</strong> rn model bet ween La ke T orrens a ndPort Augu sta sho ws tra nsitions bet ween ge ntlydipping Adel aidean sequ ences <strong>of</strong> up to 2300 mthickness with thrus ted, deformed bas ins to <strong>the</strong>north a nd d eeper rifted basi ns to <strong>the</strong> so uth.Evidence fro m sei smic a nd ma gnetics suggests<strong>the</strong> presen ce <strong>of</strong> sub stantial sedim entary o rvolcanic sequences lying beneath Willouran BedaVolcanics and overlying deformed metamorphic orgranitic basement with sharp unconformity.ReferencesMat<strong>the</strong>ws, C. G. & God smark, B., 2009.Geo<strong>the</strong>rmal <strong>Energy</strong> Prospectivity <strong>of</strong> <strong>the</strong> TorrensHinge Zone: Evidence from New Heat Flow Data.AGEG 2009 <strong>Conference</strong> Extended Abstracts.Drexel J. F. Preiss W. V. & Parker A. J. eds.1993. The Geology <strong>of</strong> South Australia, GeologicalSurvey <strong>of</strong> South Australia Bulletin 54239


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Appendix 1: Seismic Surveys and Results (after Mat<strong>the</strong>ws and Godsmark, 2009)Parachilna Seismic Survey, completed January 2009Interpretation belowCambrianBase CainozoicNeoproterozoicEdiacara FaultMesoproterozoicAnd Older Basement240


Port Augusta Seismic Survey, completed May 2009<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Base CainozoicNeoproterozoicMesoproterozoicAnd Older BasementRangeFrontFault241


Appendix 2: Fault Interpretation from Magnetics<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Fault Interpretation (blue and yellow lines) <strong>of</strong> SA Magnetics in <strong>the</strong> Port Augusta/Yadlamalka area.Image is a Tilt Angle filter draped over Analytical Signal Amplitude. Torrens <strong>Energy</strong> GELs in black.MGA Zone 53.242


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Numerical simulation <strong>of</strong> geo<strong>the</strong>rmal reservoir systems withmultiphase fluidsZhang, J. 1 *, Xing, H.L. 11 Earth Systems Science Computational Centre, School <strong>of</strong> Earth Sciences, The University <strong>of</strong> Queensland, QLD 4072*Corresponding author: ji.zhang@uq.edu.auThis p aper descri bes a modula r framework forsimulating geo<strong>the</strong> rmal well and reservoi rperformance. The numerical model i s able toaccount for transient, three-dimensional, single- ortwo-phase flu id flow in normal hete rogeneous o rfractured-matrix formation s. Both cond uctive andconvective heat flow are accou nted for and fluidstates in <strong>the</strong> reservoi r ca n ran ge bet ween liquidphase, two -phase ste am-water mi xtures tosuperheated steam. Both short term well reactionand lo ng te rm reservoi r perfo rmance ca n bemonitored as dynamic ma ss/heat flow processes.Equations-<strong>of</strong>-state (E OS) for wate r an d CO 2 areintegrated as p art <strong>of</strong> <strong>the</strong> fully-cou pled nonlinearfinite element simulator. In this paper, <strong>the</strong> code hasbeen ap plied for use in geotechnical riskassessments for mine develop ments ingeo<strong>the</strong>rmal a reas. Com parison <strong>of</strong> EGS-CO 2 andEGS-water i s dem onstrated in <strong>the</strong> paper a ndresults show that <strong>the</strong> simulat orPANDAS/ThermoFluid ca n be u sed for bothconventional geo<strong>the</strong>rmal fields and enhance dgeo<strong>the</strong>rmal systems.Keywords: Nume rical simulatio n, Enhan cedgeo<strong>the</strong>rmal system, EG S, Geotech nical ri skassessment, Carbon dioxideIntroductionGeo<strong>the</strong>rmal energy is regarded a s a renewable,clean, co st effective ene rgy source, whi ch i sbecoming increasingly attractive, espe cially since<strong>the</strong> enhanced geo<strong>the</strong>rmal system (EGS) has beenproposed and applied as a new type <strong>of</strong> geo<strong>the</strong>rmalpower technology. Geo<strong>the</strong>rmal reservoir modelinghas been played an import ant role as a n integralpart <strong>of</strong> reservoir assessment and ma nagement in<strong>the</strong> p ast few de cades. Although compute rmodeling is routinely applied in hydro<strong>the</strong> rmalreservoir e ngineering, <strong>the</strong> re are severa l asp ectsthat continually need improvement:(1) Two-phase flow phenomenology. This includes<strong>the</strong> impleme ntation an d calibration <strong>of</strong> relativepermeability and capillary pre ssure, t wo-phaseflow in fra ctures an d m ass tran sfer betwe enphases (evaporation and condensation);(2) Non-equilibrium models. To relax assumption s<strong>of</strong> local <strong>the</strong>rmodynami c equilibri um, severalnon-equilibrium model s h ave bee n d eveloped,including double porosity models (Warren & Root,1963), explicit fracture treatment (fo r sp arselyfractured systems) an d st atistical models(“MINC”-TYPE, Pruess & Narasimhan, 1985) (fordensely fractured systems);(3) Natural-state modelin g. Fur<strong>the</strong>r vali dation <strong>of</strong><strong>the</strong> co mputed natu ral st ate against e arlyexploration well data is required;(4) Cons titutive repres entations. Res ervoir fluidswith dissol ved solid s (i.e. Na Cl) a ndnon-condensable ga ses are no w available inseveral si mulators. Mo deling <strong>of</strong> fluid un derextremely high tempe rature and pressu re(supercritical state) is already being conducted butnot in <strong>the</strong> geo<strong>the</strong>rmal modeling arena;(5) Coupled reservoir chemistry. There are a fewcalculations that have been reported incorporatingreactive che mistry, coupled with flui d flow bydissolution and precipitation <strong>of</strong> solids (creation anddestruction <strong>of</strong> porosity and permeability), however,this area still provides a challen ge to g eo<strong>the</strong>rmalmodeling;(6) Autom atic inv ersion te chniques. In versemodeling uses an ite rative inversion procedure todrive co nventional forward reservoi r model s(treated as sub routines). With <strong>the</strong> increa se inmodel complexity and de grees <strong>of</strong> fre edom, <strong>the</strong>computational cost is extremely high.In conclusion, fur<strong>the</strong>r computational modeling andcode development is u rgently needed t o improveour understanding <strong>of</strong> geo<strong>the</strong>rmal reservoir and <strong>the</strong>relevant nature. It is also needed for <strong>the</strong> enhancedevolution such a s <strong>of</strong> enhanced g eo<strong>the</strong>rmalreservoir sy stem, and a chieves a m ore accurateand comp rehensive rep resentation <strong>of</strong> rese rvoirprocesses in more details. It also help s to redu ce<strong>the</strong> unce rtainties in model s, and to enhan ce <strong>the</strong>practical utility and reliability <strong>of</strong> reservoir simulationas a basis for field development and management.This p aper will focus on our research ef fortstowards <strong>the</strong> simulation <strong>of</strong> enha nced g eo<strong>the</strong>rmalreservoir systems with multiphase fluids.PANDAS/ThermoFluidPANDAS (Parallel Adaptive Nonlinear DeformationAnalysis S<strong>of</strong> tware) i s a m odular sy stem <strong>of</strong> finiteelement met hod ba sed modules. Cu rrently, itincludes <strong>the</strong> following four key components:• ESyS_Crustal for <strong>the</strong> interac ting fault sys temsimulation;• PANDAS/Fluid for simulati ng <strong>the</strong> fluid flow infractured porous media;• PANDAS/Thermo for <strong>the</strong> <strong>the</strong>rm al analysis <strong>of</strong>metals and fractured porous media;243


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>• PANDAS/Pre and P ANDAS/Post forconceptual modelin g, mesh g eneration andvisualization.All <strong>of</strong> <strong>the</strong> abo ve modules can be u sed individuallyor togeth er to simulat e phe nomena su ch asinteracting fa ult system dynamics, hea t flow andfluid flow with or without coupling effects.PANDAS/ThermoFluid (<strong>the</strong> fully coupl ed modules<strong>of</strong> PANDAS/Thermo and PANDAS/Fluid) is a finiteelement method based module for sim ulating <strong>the</strong>fluid and heat flow in a fra ctured porous media bysolving <strong>the</strong> conservation equations <strong>of</strong> macroscopicproperties numerically.The mass and energy conservation equations fortransient two-pha se water/steam couple dheat/fluid flow in porous medium used in PANDASare given in Equations (1) and (2):[ ( Sw w Ss s)] tKkrw(1)[w Pw wgZ]wKkrs[ s Ps sgZ]q ms[ ( Sw wuw Ss sus) (1 ) rcr] tKk(2)rw[ whw Pw wgZ]wKkrs[ shs Ps sgZ]( T)qesTo compl ete <strong>the</strong> governing eq uations, it isassumed th at Darcy’ s Law a pplies to <strong>the</strong>movement <strong>of</strong> each phase (momentum balance):Kkrwvw Pw wgZ(3)wKkrsvs Ps sgZ(4)swhere P is fluid pre ssure [Pa]; is <strong>the</strong> poro sity; Sis <strong>the</strong> phas e s aturation, with S w +S s =1; is <strong>the</strong>density [kg/m 3 ]; K is th e intrinsi c permeabilitytensor <strong>of</strong> <strong>the</strong> porous medium [m 2 ], k r is <strong>the</strong> relativepermeability <strong>of</strong> <strong>the</strong> phase; μ is <strong>the</strong> dynamicviscosity [kg/m·s]; g is gravity, Z is <strong>the</strong> depth; u andh are specific internal energy and specific enthalpyrespectively [kJ/ kg]; is <strong>the</strong> <strong>the</strong>rmal condu ctivitytensor <strong>of</strong> th e po rous m edium [ W/m·K]; T istemperature [℃]; q m and q e are source/sink terms<strong>of</strong> <strong>the</strong> total mass and energy respectively [kg/m3·s,kJ/m3·s]; v is <strong>the</strong> fluid veloc ity vector in [m/s]; <strong>the</strong>subscript w, s an d r denote wate r, ste am ph aseand rock matrix respectively.Thermodynamic p roperties <strong>of</strong> reservoir fluid s(such as water and CO 2 ) are <strong>of</strong> vital importance tounderstand <strong>the</strong> subsurface physical-chemical andgeological processes. The most acce ptedIAPWS-95 formulation (Wagner & Prub , 2002) fo rwater equation-<strong>of</strong>-state (EOS) is integ rated in oursimulator, which allows us to retrieve basicphysical parameters such as density and dynamicviscosity, as well as <strong>the</strong> saturated properties forphase transition modeling. SWEOS, an EOS forCO 2 which was o riginally developed by Span andWagner (1 996) ba sed on <strong>the</strong>ir algo rithm <strong>of</strong> anempirical representation <strong>of</strong> <strong>the</strong> fundam entalequation <strong>of</strong> Helmholtz e nergy, ha s also be enimplemented into our simulator to model EGS-CO 2processes.For more details <strong>of</strong> PANDAS, please refer to Xing& Makinouchi (2002), Xing et al. (2006a , b, 2007,2008, <strong>2010</strong> ). Model va lidation <strong>of</strong> PANDAS/ThermoFluid code is reported in Xing et al. (2008,2009).PANDAS/ThermoFluid application inGeotechnical risk assessments formine developments in geo<strong>the</strong>rmalareasTo demonstrate <strong>the</strong> feasibility and value <strong>of</strong>multi-phase fluid flow modeling as a pit design tooland for risk analysis <strong>of</strong> geo<strong>the</strong>rmal hazards duringmining in ho t ground, a numerical model wa sdeveloped f or a gold mine site usin g <strong>the</strong>PANDAS/ThermoFluid model code .PANDAS/ThermoFluid was used for sim ulation <strong>of</strong>temperature, pressure an d steam dist ribution in<strong>the</strong> se awall and fou ndation <strong>of</strong> <strong>the</strong> da m along anorth-nor<strong>the</strong>ast to south -southwest oriented crosssection.(a) Stage 1(b) Stage 2(c) Stage 3Steam Zone Mixed Zone LiquidWater ZoneFigure 1: PANDAS/ThermoFluid results <strong>of</strong> <strong>the</strong> cross sectionmodel <strong>of</strong> pit excavation for three development stages.For dem onstration pu rpose, three pit excavationstages were simulated. The first to a depth <strong>of</strong> 90m,<strong>the</strong> second reaching <strong>the</strong> t op <strong>of</strong> <strong>the</strong> b oiling zone at180m and <strong>the</strong> third down to 270m below surface.2


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>It was found that after <strong>the</strong> first stage <strong>of</strong> excavationto 90m stea m did not d evelop throu ghout <strong>the</strong>model domain despite temperatures computed tobe p artly sig nificant a bove 100º C. Thi s is due tohigh hyd rostatic pre ssures preventin g water f romboiling at this stage. The simulation results for <strong>the</strong>second and third develo pment st ages predi ctedboiling to occur below <strong>the</strong> pit floor and in <strong>the</strong> lowerbenches <strong>of</strong> <strong>the</strong> seawall.Short-term/long-term modeling <strong>of</strong>fracture dominated EGS-water andEGS-CO 2Operating e nhanced geo<strong>the</strong>rmal sy stems (E GS)with CO 2 instead <strong>of</strong> water as a heat tra nsmissionfluid is a new attra ctive concept wit h severalbenefits incl uding: The lowe r visco sity <strong>of</strong> CO 2would yield large r flow velocities for a givenpressure gra dient; less p ower con sumption forfluid circulati on system s due to buoyancy ef fectsand geologic storage <strong>of</strong> green house gases as anancillary benefit (Brown, 2000, Pruess, 2006). Thefollowing se ction demon strates simulations u singEGS-water and EGS-CO 2 under typica lgeo<strong>the</strong>rmal field situatio ns to compare th eefficiency and longevity <strong>of</strong> both systems as well as<strong>the</strong> estimation amount <strong>of</strong> geologic storage <strong>of</strong> CO 2 .Pruess (2006) has compared <strong>the</strong> <strong>the</strong>rm odynamicproperties <strong>of</strong> CO 2 and water under typical reservoirconditions. A five-spot well pattern geo<strong>the</strong>rmal fieldwas model ed by T OUGH2 (Prue ss, 20 06) an d aseries <strong>of</strong> co mparisons betwee n EGS-CO 2 andEGS-water h as dem onstrated <strong>the</strong> advant ages <strong>of</strong>using EGS -CO 2 su ch as <strong>the</strong> long-te rmperformance (up to 36 ye ars) heat exaction rate,mass flow rate and pressure/temperature field.In <strong>the</strong> deve lopment <strong>of</strong> enhanced g eo<strong>the</strong>rmalsystems, greater focus is shifted to <strong>the</strong> short-termdynamic response <strong>of</strong> well tests. A number <strong>of</strong> tests(with o r with out tracers) need to b e run betwee n<strong>the</strong> injectio n and p roduction well s bef ore p owergeneration to assess <strong>the</strong> ability <strong>of</strong> prod uction andcirculation within an EGS. Here, a simplified500x200m fracture domi nated geoth ermal field(Figure 2) is modeled by PANDAS/ThermoFluid tocompare b oth long -term an d short-termperformance <strong>of</strong> EGS-CO 2 and EGS-water.Figure 3 sho ws <strong>the</strong> fluid ve locity evolution at anearly st age <strong>of</strong> <strong>the</strong> well test. With <strong>the</strong> sam epressure drop between injection well an dproduction well, CO 2 ha s highe r flow rates th anwater (2.5×10 -3 m/s for CO 2 to 8.7 ×10 -4 m/s forwater at its stable stage). It can also be seen thatCO 2 takes about 81 hours to reach <strong>the</strong> stable state,while water takes less than 50 hours. The reasonfor <strong>the</strong> longer stabalization time for CO 2 is becauseit has a la rger ratio <strong>of</strong> fluid den sity to viscosity(Pruess, 2006) and a larg er compressibility (about8 times <strong>of</strong> water) than water under reservoi rpressure/temperatures.Figure 3: Fluid velocity evolution at early stage <strong>of</strong> well test.Injection well pressure is 44MPa, constant pressure drop <strong>of</strong>10MPa is set between <strong>the</strong> injection well and production well.Figure 4 shows a long term temperaturedistribution along <strong>the</strong> f racture zone. For thi sparticular case, it t akes l ess than 10 years forEGS-CO 2 to redu ce temperature within <strong>the</strong> entireregion to und er 200℃, while EGS-water requiresmore tha n 2 0 years befo re temperature dro ps to200℃. This is due to CO 2 ’s higher heat extractionrate which was suggested by Pruess (2006).Figure 2: A fracture dominated geo<strong>the</strong>rmal field. L=500m,D=100m, H=0.1m. Permeability <strong>of</strong> <strong>the</strong> fracture zone is 5×10 -14 m 2 . Rock density is 2.65×10 3 kg/m 3 , specific heat is1kJ/(kgK), <strong>the</strong>rmal conductivity is 2.1W/(mK). Initialtemperature <strong>of</strong> entire region is 250℃, <strong>the</strong> Injection fluid is 90℃.Figure 4: Comparison <strong>of</strong> fracture zone temperature atdifferent years. Constant pressure drop <strong>of</strong> 10MPa is setbetween <strong>the</strong> injection well and production well. With <strong>the</strong>fracture space <strong>of</strong> 100m, flow rate for water and CO2 are7.3kg/s and 10.8kg/s, respectively.ConclusionsComputer modeling <strong>of</strong> g eo<strong>the</strong>rmal systems ha sbeen widely used i n indu stry. Fur<strong>the</strong> rcomputational modeling and code development isurgently needed to impro ve our unde rstanding <strong>of</strong>


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong> 22kkgeo<strong>the</strong>rmal reservoir and <strong>the</strong> relevant nature. It isalso needed for <strong>the</strong> enhanced evolution such as <strong>of</strong>enhanced g eo<strong>the</strong>rmal rese rvoir system, andachieves a more a ccurate and com prehensiverepresentation <strong>of</strong> re servoir processe s in mo redetails. It also hel ps to reduce <strong>the</strong> uncertainties inmodels, and to enhance <strong>the</strong> pra ctical utility andreliability <strong>of</strong> reservoir simulation as a basis for fielddevelopment and man agement. This p aperintroduced a simul ator ‘PANDAS/ThermoFluid’ tomodel <strong>the</strong> transi ent, non-iso<strong>the</strong> rmal, multipha sefluid flow in hetero geneous o r fra ctured-matrixformations for simul ating geo<strong>the</strong>rm al well andreservoir performance. It was applied for use in ageotechnical risk a ssessment <strong>of</strong> a n open pitmining site si tuated in hot ground. As well as tolook at sho rt-term/long-term modelin g <strong>of</strong> fractu redominated e nhanced geo <strong>the</strong>rmal systems (EGS )with wate r and CO 2 as h eat transmi ssion fluid s,PANDAS/ThermoFluid ha s p roven t o be avaluable to ol to su pport <strong>the</strong> develo pment a ndimplementation <strong>of</strong> g eo<strong>the</strong>rmal risk managementstrategies to combat geo<strong>the</strong>rmal hazards. Resultsalso sh ow its ef ficiency and usefu lness insimulating both conventional geo<strong>the</strong>rmal fields andenhanced g eo<strong>the</strong>rmal sy stems with multiphasefluids.AcknowledgementsSupport is gratefully ackno wledged by <strong>the</strong><strong>Australian</strong> Rese arch Council an d Ge odynamicsLimited thro ugh <strong>the</strong> A RC Linkage proje ctLP0560932.ReferencesBrown, D.W ., 2000, A Hot Dry Rock g eo<strong>the</strong>rmalenergy concept utilizing su percritical CO 2 instead<strong>of</strong> wate r: Proceedi ngs <strong>of</strong> <strong>the</strong> T wenty-FifthWorkshop on Geo<strong>the</strong>rmal Reservoir Engineering,p. 233–238.Pruess K., and Narasimhan T . N. , 1985, APractical Method for Modeling Fluid and Heat Flowin Fractured Porous Media: Society <strong>of</strong> PetroleumEngineers Journal, v. 25, no. 1, p. 14-26.Pruess K., 2 006, Enha nced ge o<strong>the</strong>rmal syste ms(EGS) us ing C O 2 a s worki ng fluid - A novelapproach for generatin g rene wable e nergy withsimultaneous sequ estration <strong>of</strong> carbon:Geo<strong>the</strong>rmics, v. 35, p. 351–367.Span, R., and W agner, W., 1996, A new equatio n<strong>of</strong> state for carbon dioxide covering <strong>the</strong> fluid regionfrom <strong>the</strong> triple-p oint temperature to 1 100K atpressures up to 800 MPa: Journal <strong>of</strong> Physical andChemical Reference Data, v . 25, no. 6, p.1509–1596.Wagner W., and Pru b, A., 2002, The IAPWS for<strong>the</strong> <strong>the</strong>rm odynamic prope rties <strong>of</strong> o rdinary watersubstance for general and scientific use: Journal <strong>of</strong>Physical and Chemical Reference Data, v. 31, no.2, p. 387–535.Warren, J. E., and Root, P. J., 1963, The behavior<strong>of</strong> naturally frac tured reservoirs : SPE J ., v. 3, p.245-255.Xing, H.L., and Ma kinouchi, A., 2002, Thre edimensional finite element mo delling <strong>of</strong><strong>the</strong>rmomechanical frictional contact between finitedeformation bodies u sing R-mi nimum strate gy:Computer M ethods in Applied Me chanics andEngineering, v. 191, p. 4193-4214.Xing, H.L., Mora, P., and Makinouchi, A., 2006a, Aunified frictio nal descri ption and it s ap plication to<strong>the</strong> simulation <strong>of</strong> frictional instability using <strong>the</strong> finiteelement m ethod: Philo sophical Mag azine, v . 86,no. 21-22, p. 3453-3475.Xing, H.L., Mora, P ., 2006b, Co nstruction <strong>of</strong> anintraplate fa ult system mo del <strong>of</strong> South Australi a,and simulation tool for <strong>the</strong> iSER VO institute see dproject: Pure and Ap plied Geop hysics, v. 163, p.2297-2316. DOI 10.1007/s00024-006-0127-x.Xing, H.L., Makin ouchi, A. and Mora , P ., 2007,Finite element modeling <strong>of</strong> interacting fault system:Physics <strong>of</strong> <strong>the</strong> Earth and Planetary Interiors, v. 163,p. 106-121. doi:10.1016/j.pepi.2007.05.006.Xing, H.L. 2008, Progress Report: SupercomputerSimulation o f Hot Fra ctured Rock G eo<strong>the</strong>rmalReservoir S ystems: E SSCC/ACcESS T echnicalReport, The University <strong>of</strong> Queensland, p.1-48.Xing, H.L., Gao J., Zha ng J. and Li u Y., <strong>2010</strong>,Towards An Integrated Si mulator F or EnhancedGeo<strong>the</strong>rmal Re servoirs: Proce edings WorldGeo<strong>the</strong>rmal Cong ress <strong>2010</strong>. Bali, Indonesi a,25-29 April <strong>2010</strong>.246


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Development <strong>of</strong> Hydraulic Fractures and Conductivity near a WellboreXi Zhang and Robert G. Jeffrey*CSIRO Earth Science and Resource Engineering, Melbourne VIC, AustraliaABSTRACTHydraulic fra ctures play an imp ortant role i nestablishing a hi gh co nductive path wayconnecting <strong>the</strong> wellbore and reservoir. The n earwellborefracture develo pment is cru cial to <strong>the</strong>efficiency <strong>of</strong> a fractu re t reatment a s a smoothfracture path will redu ce <strong>the</strong> flow imp edance. Anumerical model is u sed to sim ulate <strong>the</strong>propagation pathway s followed by hydrauli cfractures, in <strong>the</strong> presen ce <strong>of</strong> a p ressurised welland natural fractures. By including <strong>the</strong> coupling <strong>of</strong>viscous fluid flow and rock defo rmation in <strong>the</strong>analysis, we find that th e non-uniform pre ssuredistribution along <strong>the</strong> fractures and <strong>the</strong> removal <strong>of</strong>near-well fra cture closure result in growth <strong>of</strong> afracture with less curvature (a me asure o ftortuosity) i n its path. More over, th e fractu recurvature ca n be cha racterised b y tw odimensionless pa rameters. If multiple fractu rescoexist, fracture lin kage is po ssible due t omechanical i nteraction between fra ctures, p reexistingnatural f ractures a nd th e well bore.Natural fract ures can alte r <strong>the</strong> hydraulic fra cturepropagation direction, can <strong>of</strong>fset <strong>the</strong> fra cture pathand can p rovide sites for new fracture growth. In<strong>the</strong> case <strong>of</strong> two hydraulic fractures initially growingin op posite directions from <strong>the</strong> well bore, <strong>the</strong>interaction with a natu ral f racture on o ne si de <strong>of</strong><strong>the</strong> well will result in <strong>the</strong> o<strong>the</strong>r fract ure wingpropagating faster. Th e complexity <strong>of</strong> <strong>the</strong> nearwellboref racture ge ometry can b e st udied with<strong>the</strong> aid <strong>of</strong> our numerical model.Keywords: Near-well fracture tortuos ity, c ouplingmechanisms, naturally fractu red reservoi r,numerical modellingINTRODUCTIONMultiple sub parallel fra ctures can b e gene ratednear th e wel lbore because <strong>of</strong> fractu re initiationfrom pe rforations spaced alon g an d pha sedaround <strong>the</strong> wellbore o r from natural fra ctures andflaws that are usually not aligned with <strong>the</strong> far-fieldstress di rection. Fractu res initiate d from <strong>the</strong> sedefects will reo rient th emselves to a pl aneperpendicular to <strong>the</strong> minimum far-field stre ssdirection a s <strong>the</strong>y grow a way from <strong>the</strong> wellbo re.The ove rall result <strong>of</strong> su ch a f racture initiationprocess produces ne ar-wellbore fractu retortuosity. As a consequ ence, <strong>the</strong> net pressu rerequired to extend <strong>the</strong> fractu res is i ncreasedconsiderably. Beca use <strong>of</strong> its imp ortance tooptimisation <strong>of</strong> fra cture treatments, th e stu dy onthis subject has continu ed for several de cades(Hamison a nd Fairhurst, 1970; Daneshy, 1973;Weng, 199 3; Soliman et al. 2008; Cherny et al .2009).Geomechanical models are <strong>of</strong> significant value i ntreating <strong>the</strong> se sort s <strong>of</strong> problems that rel ate tocompeting f racture growth, incl uding l ocal wi dthrestrictions and in creased viscou s frictionalpressure loss. Base d on such geo mechanicalanalyses, various operational remedial techniqueshave bee n p roposed to overco me or avoid <strong>the</strong>near-wellbore effects, su ch a s usi ng highe rinjection rates, higher viscosity fluids and orientingslots o r p erforations for fractu re initiation(Manrique and Venkitaraman, 2001; Abass, et al.,2009). However, most studies were based on <strong>the</strong>uniform p ressurization assumptio n so that <strong>the</strong>fracture p roblem ca n be treated by conventionalfracture m echanics meth ods. In pa rticular, th efracture turn ing pro cesses, duri ng which <strong>the</strong>fracture reorients as it grows fro m a wellbore tobecome perpendicular to <strong>the</strong> minim um prin cipalstress di rection, involve s viscous fluid flow andfrictional slip. In addition, a moving bound aryexists associated with b oth <strong>the</strong> fluid flow and th efracture tip. The se aspects <strong>of</strong> th e proble mincrease its compl exity, b ut must be inclu ded i nany realistic model.In this pape r, we will e mploy a 2D numeri calmethod th at can model h ydraulic fra cture growthfrom a borehole. The 2D plane strai n assumptionis justified if <strong>the</strong> h eight <strong>of</strong> a slot or natural flaw islarge compared to <strong>the</strong> well radius. Moreover, <strong>the</strong>method can dire ctly co pe with <strong>the</strong> fractureinteraction with <strong>the</strong> wellbore and natural fractures.Although <strong>the</strong> <strong>the</strong>rmal effect is not yet considered,<strong>the</strong> re sults provide i nsights into fractu redevelopment around <strong>the</strong> wellbore in a hot dry rockreservoir.PROBLEM STATEMENTSThe pro perties used in <strong>the</strong> model for <strong>the</strong> rock,fluid and fra ctures a re a s follows. T he ela sticproperties for <strong>the</strong> intact rock are Young’s modulus(E), Pois son’s ratio ( ) and <strong>the</strong> Mode I fractu retoughness i s K IC. The injecte d fluid isincompressible and has a Ne wtonian visco sitygiven by . T he sum <strong>of</strong> a ll injection rates <strong>of</strong>fracture b ranches g rowing from th e well isassumed to be constant and is denoted as Q in. Itmust be noted that <strong>the</strong> injected fluid rate into eachfracture varies in time because <strong>of</strong> <strong>the</strong> differentgrowth rate s <strong>of</strong> each fr acture. The total rate247


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Q ininjected, , is sp ecified as co nstant andrepresents <strong>the</strong> rate fluid is injected into <strong>the</strong> well.In addition, <strong>the</strong> volume change (compressibility) <strong>of</strong><strong>the</strong> bo rehole fluid an d ro ck system is n otaccounted for in determining <strong>the</strong> injection rate.LFigure 1 Fractures around a wellbore, in-situ stress andcoordinate system. The origin <strong>of</strong> <strong>the</strong> coordinate system is at<strong>the</strong> wellbore centre.The two sides <strong>of</strong> a fra cture may come intocontact, espe cially ne ar th e well bore. T he mo delallows for contact stresses to develop and uses acohesionless Coulomb friction criteri on for slip onsurfaces in contact ( n p ) (1)f HP wywhere is <strong>the</strong> she ar stress along th e clo sedfractures, nis <strong>the</strong> n ormal stress a cting acro ss<strong>the</strong>m, pfis th e fluid pressure and is <strong>the</strong>coefficient <strong>of</strong> friction.In addition to <strong>the</strong> tange ntial di splacementdiscontinuity (DD), v, associated with slip alon g<strong>the</strong> clo sed fractu re segments, <strong>the</strong>re exi stsopening displacement w along th e opene dhydraulic fra ctures, which contri butes to fractu reconductivity. All <strong>of</strong> <strong>the</strong>se elastic di splacementsgive rise to changes in <strong>the</strong> rock stress or changesin <strong>the</strong> tractions acting along <strong>the</strong> fracture surfaces.The g overning eq uations for stresses, flui dpressure and displacements are given in Zhang etal. (200 7, 2 009), a nd a re given i n terms <strong>of</strong>Green’s fu nctions. We e mploy <strong>the</strong> di splacementdiscontinuity method (DDM) fo r <strong>the</strong> simulation <strong>of</strong>rock deformation in a 2D h omogeneous a ndisotropic el astic mate rial, on which a uniformstress is applied at infinity.The governi ng equatio ns for fluid flow in <strong>the</strong>fracture channel are given by Zhang et al. (2009).There are t wo type <strong>of</strong> fluid migra tion alongfractures. The fluid not only can diffuse along <strong>the</strong>closed fractu res without a ny mech anical openi ng<strong>of</strong> <strong>the</strong> fracture, but also can flow through an openchannel a s a result <strong>of</strong> openin g mode hydrauli cxFlaw hWellborefracturing processes. In <strong>the</strong> latter case, <strong>the</strong> fluidpressure is b alanced by <strong>the</strong> co mpressive stre sscaused by rock ela stic deformation , that is,n pf. We use Reynolds’ equation to describefluid movem ent insi de t he op ened hydra ulicfractures:(w ) ( w ) [ts3pf] (2)swhere w is <strong>the</strong> mechanical opening and vanishesfor th e closed s egments, is <strong>the</strong> pre-existinghydraulic aperture arising from surface roughnessand microstructures and . 12However, it must be me ntioned that effectivestress cha nges in <strong>the</strong> fluid-infiltra ted andpressurised fracture portion can produce changes<strong>of</strong> <strong>the</strong> hydra ulic ap erture without fully openin g afracture. The dilatation can s lightly affec t <strong>the</strong>internal p ressure di stributions si nce th e re sultingfluid cond uctivity varies in location an d time. Asstated a bove, <strong>the</strong> hydr aulic aperture at <strong>the</strong>beginning is assigned an initial value for eachclosed fra cture se gment. The evolution <strong>of</strong>obeys a no nlinear spring model in response toany in crements <strong>of</strong> <strong>the</strong> internal pressure. Inparticular, an equation g overning <strong>the</strong> hydrauli caperture change associated with pressure changeis given as follows,d / dP f (3)where is a small constant with a value <strong>of</strong>per Pa in <strong>the</strong> model. A pressure diffusion equationis applie d to calcul ate <strong>the</strong> fluid flow inside aclosed natural fracture (Zhang et al., 2009)pftw 0 p2 f c ( ) 0(4)ssw 010 8where c 1/(12). This cal culation applies toall clo sed p ortions <strong>of</strong> fract ures, wh e<strong>the</strong>r <strong>the</strong>y areundergoing or have undergone slip or not.To complete <strong>the</strong> problem formul ation, we n eedboundary and initial conditions fo r t he ab ovegoverning equatio ns. Initially, all fracturesegments are assumed to be evacu ated and <strong>the</strong>rock mass is stationary. Rock failure cri terion willbe given bel ow, as well as <strong>the</strong> metho d use d forhandling fracture intersection and a ssociated fluxredistribution. For <strong>the</strong> f ractures connected to <strong>the</strong>borehole, <strong>the</strong> sum <strong>of</strong> <strong>the</strong> fluid flux entering <strong>the</strong>m isequal to <strong>the</strong> injection rate, that is,N qi(0, t) Qin (5)i1where N is t he num ber o f fractures andq i<strong>the</strong>248


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>fluid volumetric flux into fracture i.At <strong>the</strong> fracture tip, <strong>the</strong> ope ning and shearing DDsare zero, that is,w ( l) v(l) 0 (6)and <strong>the</strong> fracture opening pr<strong>of</strong>ile near <strong>the</strong> crack tippossesses a square root shape with distance from<strong>the</strong> tip as p redicted by Linea r Elasti c Fra ctureMechanics (LEFM) <strong>the</strong>ory.When <strong>the</strong> stress intensity factor at <strong>the</strong> f racture tipreaches <strong>the</strong> fracture toughn ess <strong>of</strong> <strong>the</strong> rock,fracture growth occurs. In general, <strong>the</strong> frac turepropagation direction may change as dictated by<strong>the</strong> ne ar-tip stress fiel d ch aracterised by <strong>the</strong>Stress Intensity Fac tors (SIFs). In part icular, <strong>the</strong>mixed-mode fracture crite rion is used fo rdetermining f racture g rowth in <strong>the</strong> model. Thissame approach h as been use d by a number <strong>of</strong>researchers (e.g. Mogilevskaya et al., 2000).The co upled fluid flow (to obtain pre ssure) an drock d eformation (to ob tain fractu re openin g)problem is solved in an implicit m anner byincorporating <strong>the</strong> ela sticity equation into th eReynolds’ equation. Th e resp onses obt ained arehistory dependent because <strong>of</strong> <strong>the</strong> irreversible fluidflow and fri ctional sliding processes. Additionally,<strong>the</strong>re are th ree m oving fronts i nherent in <strong>the</strong>problem, namely <strong>the</strong> slip front, <strong>the</strong> fluid front an d<strong>the</strong> fractu re opening (cra ck tip ) front. The re aderis refe rred t o Zhan g et al. (200 7, 2 009) fo r adetailed d escription <strong>of</strong> <strong>the</strong> num erical solutio nmethods applied in modelling <strong>the</strong>se processes. At<strong>the</strong> borehole, <strong>the</strong> fracture entry pressures must beequal to <strong>the</strong> borehole pressure. T his condition i senforced through an it eration sch eme. Thefracture entry and bo rehole pressure s a reconstrained to be equal by enforcing Eq. (5). Theinjection rate into each fracture is found based on<strong>the</strong> specified current borehole pressure, using <strong>the</strong>method described in our previous work applied t<strong>of</strong>racture j unctions (Zhang et al., 2 007). In th ecalculation, <strong>the</strong> conve rgence <strong>of</strong> <strong>the</strong> solution i svery sen sitive to <strong>the</strong> time step and <strong>the</strong>convergence error tol erance. T o rapi dly find aconverged wellbore pre ssure, a relaxa tion factoris used in updating <strong>the</strong> borehole pressure at eachiteration step. A tolera nce (< 10 4 ) is set for <strong>the</strong>relative erro r betwee n <strong>the</strong> wellb ore a nd fra ctureentry pressures. Therefore, in <strong>the</strong> program, a newiteration loo p is introd uced for o btaining aconverged b orehole a nd fracture e ntry pre ssuresolution.The nume rical method h as bee n verif ied, in ourprevious pa pers, by co mparison to publish edsolutions to a range <strong>of</strong> problems; see Zhang et al.(2009). However, to treat p roblems that include aborehole, th e prog ram was modifie d to allowcorrect treat ment <strong>of</strong> <strong>the</strong> interior and exterio rproblems g enerated when th e b orehole i sdiscretised usin g <strong>the</strong> DD (DisplacementDiscontinuity) method. Di scretising th e well boreusing conve ntional DD elements results in th eformation <strong>of</strong> a disc <strong>of</strong> ro ck insi de <strong>the</strong> wellbore,which can move rigidly. It must be mentioned that<strong>the</strong> resulting DDs along <strong>the</strong> wellbore boundary arefictitious alt hough <strong>the</strong>y are ne cessary forcalculating p ressure a nd displa cement at <strong>the</strong>borehole wall and alon g <strong>the</strong> fractu res. The sefictitious DDs do n ot h ave a literal physi calinterpretation as DDs, bu t ra<strong>the</strong> r a re needed t oobtain <strong>the</strong> stress and di splacement everywhere in<strong>the</strong> e xterior pa rt o f th e pr oblem. Mor eover, s ince<strong>the</strong> inte rior di sc is fre e to move a s a rigid b ody,<strong>the</strong> direct u se <strong>of</strong> a co nventional DDM is notpossible without sup pressing <strong>the</strong> rigid -bodymotion <strong>of</strong> this disc.A simple m ethod to suppress <strong>the</strong> se rigid -bodymotions is as follows. Two additional elements aredefined inside <strong>the</strong> borehole and assigned fictitiousDDs. Then we cal culate <strong>the</strong> displacement on <strong>the</strong>negative sid e <strong>of</strong> an el ement ba sed on <strong>the</strong>fundamental elastic solutions. After th at <strong>the</strong> fou rdisplacements at <strong>the</strong>se two additio nal element sare set to zero, in orde r to co nstruct a cl osed,well-posed problem s for all DDs. T hedisplacements on <strong>the</strong> negative si de <strong>of</strong> <strong>the</strong>elements are given as Eq. (5.6.1) in Crou ch andStarfield (19 83) fo r both normal and tange ntialdisplacement components.The ela sticity equation s for <strong>the</strong> n ormal andtangential DDs ( ukinclude s w an d v.) at <strong>the</strong>middle <strong>of</strong> ea ch element a long th e bo rehole an d<strong>the</strong> fractures and for <strong>the</strong> t wo additional elementsare, respectively,K u P k n,s (7)ijk k f ij ijM u 0 k n,s(8)ijkkwhere Kijkand Mijkare <strong>the</strong> coefficient matricesderived from <strong>the</strong> fundamental elastic solution as isdone i n conv entional boundary el ement method s(see detail s in Cro uch an d Starfield, 1983); an d ijare <strong>the</strong> resultant stresse s alon g <strong>the</strong> fracturesurface arising from far-field (in situ) stresses.The above first equation enforces equilibrium atDD elements along <strong>the</strong> fractures and <strong>the</strong> wellbore,and <strong>the</strong> second one enforces <strong>the</strong> con straint thateliminates rigid body motion <strong>of</strong> <strong>the</strong> interior disc byrequiring zero di splacements at two additio nalinterior ele ments. The above si multaneousequations (Eqns (7) and (8)) are solved for normaland shear DDs <strong>of</strong> all elements along <strong>the</strong> borehole,<strong>the</strong> fractu res and <strong>of</strong> <strong>the</strong> two addition al elements,once <strong>the</strong> flui d pressu re i s kno wn. T he DDs thatare obtained can <strong>the</strong>n be used to calculate stressor displacement at any ot her point inside <strong>the</strong> rockmass.249


NUMERICAL RESULTSSingle hydraulic fractureWe first co mpare <strong>the</strong> o pening and path for ahydraulic fracture driven by a uniform p ressure orby injection o f a viscou s fluid. A uniform pre ssurecondition in a hydra ulic f racture i s eq uivalent tousing an i nviscid fluid (Detou rnay, 2 004). T hepressure ma gnitude is ad justed at e ach fra cturegrowth step to satis fy <strong>the</strong> fra cture extensi oncriterion at <strong>the</strong> fractu re tip. Fractu re reorientationis cle arly sh own in Fi g. 2 for both uniformlypressurised and viscous fluid flow cases. For zeroviscosity fluids as shown in Fig. 2(a), <strong>the</strong> portionadjacent to <strong>the</strong> well wall is in conta ct. In thisregion, fluid flow will be restricted and frictionalslip condition must be imp osed. For ge nerality <strong>of</strong>results, Mogil evskaya et al. (2000 ) sho wed tha t<strong>the</strong> fractu re path is controlled by <strong>the</strong> followingdimensionless parameter,( Hh)R (9)Ky(m)y(m)0.40.30.20.10-0.1IC0.1 mm16.9 MPa4.22MPa-0.2-0.3 -0.2 -0.1 0 0.1 0.2 0.3x(m)0.40.30.20.10-0.10.1 mm(a)16.9 MPaTime=0.072 second4.22MPa-0.2-0.3 -0.2 -0.1 0 0.1 0.2 0.3x(m)(b)<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>y(m)0.40.30.20.10-0.110 MPa16.9 MPaTime=0.072 second4.22MPa-0.2-0.3 -0.2 -0.1 0 0.1 0.2 0.3x(m)(c)Figure 2 Fracture trajectory, opening DD for uniformlypressurised fractures (a); opening DD (b) and internal fluidpressure (c) for fluid-driven fracture growth in <strong>the</strong> case <strong>of</strong> <strong>the</strong>borehole radius =0.1 m and crack starting angle <strong>of</strong> 170degree.If <strong>the</strong> fluid vi scosity is 0.01 Pa s and <strong>the</strong> injectionrate is specified as 0.0 004 m 2 /s, <strong>the</strong> frac turepathway an d asso ciated openi ng DD a ndpressure distributions are given in Figs. 2(b) and(c). The fra cture closure d oes n ot app ear in thiscase, but a high fluid pressure results as <strong>the</strong> fluidenters <strong>the</strong> n arrow fra cture an d op ens it again st<strong>the</strong> high er normal stresses a cting alo ng its nearwell extent F ig. 2(c). Mo reover, a flui d lag zonedevelops wh en viscous dissipatio n cannot b eneglected an d is rep resented in Fig. 2(c) a s th eunpressurised region <strong>of</strong> <strong>the</strong> fra cture near <strong>the</strong> tip.This is o ne manifestation <strong>of</strong> <strong>the</strong> coupl ed flow anddeformation pro cess interacting with a movingboundary.To ch aracterize th e effect <strong>of</strong> fluid visco usdissipation on fractu re path s, we intro duceano<strong>the</strong>r p arameter which provid es an appa rentfracture to ughness arising from viscou sdissipation, a s given in Jeffrey(1989), ba sed onan earlier somewhat different formulation given bySettari an d Price (1984), a nd as given byDetournay (2 004) i n <strong>the</strong> case <strong>of</strong> zero lag. Thisapparent toughness, when substituted for <strong>the</strong> rockfracture tou ghness in Eqn. 9 provide s adimensionless pa rameter, given by Eq n. 10, thatwe hypo<strong>the</strong>size will control <strong>the</strong> curvi ng <strong>of</strong> aviscosity do minated hyd raulic fra cture gro wingfrom a wellbore (Zhang et al. <strong>2010</strong>),( Hh)RF3 1/4( QE)in(10)where E is th e plan e-strain modul us. I n thisformula, <strong>the</strong> product <strong>of</strong> injection rate and fluidQ in250


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>viscosity are parameters that can be controlledby a fracturing engineer.The above t wo parameters given by Eqs. (9 ) and(10) ca n fully cha racterise <strong>the</strong> fractu re path an drelated p ressure evolutio n for a singl e hydrauli cfracture g rowing from a wellbore. Z hang et al.(<strong>2010</strong>) provide numerical examples demonstratingthat <strong>the</strong>se parameters control <strong>the</strong> curvature in <strong>the</strong>hydraulic fra cture path as it g rows from a nuncased wellbore.Two winged hydraulic fracturesfractures at angle 30° and 210°, do extend but toa shorter distance. These two fractures propagatetowards <strong>the</strong> long er f ractures afte r le aving th einfluence region around <strong>the</strong> borehole and a sharpkink is evident in Fig. 4. Th e tendency for fracturelinkage is a lso c lear. T he s lowly g rowing andpartially su ppressed fra ctures p ropagate towards<strong>the</strong> domin ant gro wing fractures and m ay link-upwith <strong>the</strong>m a s previo usly f ound by We ng (199 3).These results sugg est that initiation <strong>of</strong> severalfractures from a wellbore subject to a larger stressratio favou rs intera ctions leadin g to link-up a sargued by Daneshy (1973).0.5 100 MPa0.450 MPaTime=0.165 second0.40.350 MPaTime=0.0846 second0.30.2100 MPa80 MPay(m)0.280 MPay(m)0.10.100-0.1-0.1-0.2-0.4 -0.3 -0.2 -0.1 0 0.1 0.2 0.3 0.4x(m)Figure 3 A pair <strong>of</strong> fractures growing from a wellbore: fracturetrajectory and internal fluid pressure for high-angle fractureinitiation. The fluid viscosity is 0.01 Pa s and <strong>the</strong> injectionrate is specified as 0.0004 m 2 /s.We n ext consi der t wo fractu res that gro wsimultaneously to form a single bi-win g fractu regeometry as shown in Fi g. 3. The pre ssure lo ssnear <strong>the</strong> wellbore wall is l ess evident and fracturerotation to align with <strong>the</strong> maximum principal stressoccurs in a very smooth way. This symmetri cgeometry is found in m any field obse rvations a sdescribed by Wen g (199 3) a nd Cherny et al.(2009).Multiple hydraulic fracturesThe m ore co mplicated init ial co ndition consisting<strong>of</strong> six starte r fractu res that are a rranged aroun d<strong>the</strong> wellb ore is con sidered next. The starte rfractures h ave an un even ang ular di stribution to<strong>the</strong> x-axis <strong>of</strong> 30°, 120°, 150°, 210°, 240° and 330°,as shown in Fig. 4. Th e fractu res at angle s <strong>of</strong>120° and 24 0° a re in a more compressive i nitialstress state, whi ch cau ses th eir gro wth to becompletely suppresse d co mpared with o<strong>the</strong>r fou rfractures. The remaining four starter fractures areall subjected to <strong>the</strong> same stress levels, except for<strong>the</strong> shear stress directions. The fra cture at angl e150° is can extend more easily because it ha s aslightly long er initial fra cture l ength. As th efractures grow and turn to align with <strong>the</strong> horizontalx direction, <strong>the</strong> fractures at <strong>the</strong> a ngle <strong>of</strong> 150° and330° become more d ominant and form a bi -wingfracture configuration. Ho wever, <strong>the</strong> o<strong>the</strong>r two-0.2-0.4 -0.3 -0.2 -0.1 0 0.1 0.2 0.3 0.4x(m)Figure 4 Fracture trajectory and internal fluid pressure in <strong>the</strong>presence <strong>of</strong> six initial flaws around <strong>the</strong> wellbore, where <strong>the</strong>fluid viscosity is 0.005 Pa s and <strong>the</strong> injection rate is specifiedas 0.0012 m 2 /s. The flaw alignment angles are 30°, 120°,150°, 210°, 240° and 330°.Effects <strong>of</strong> natural fracturesIf <strong>the</strong>re i s a natu ral f racture in th e fra cturepropagation pathway, fluid will e nter it after ahydraulic fra cture interse cts it. Th e e xistence <strong>of</strong>natural fract ure will affect <strong>the</strong> growth <strong>of</strong> <strong>the</strong>hydraulic fra cture an d <strong>the</strong> inflation <strong>of</strong> <strong>the</strong> naturalfracture caused by <strong>the</strong> fluid pre ssure can indu ceslip alo ng t he natu ral fracture an d fractu rereinitiation from <strong>the</strong> end s <strong>of</strong> a finite-size natu ralfracture. The example fra cture geometry is give nin Fig. 5(a).y(m)0.30.20.10-0.180 MPa100 MPa50 MPaTime=0.16069 second-0.2 -0.1 0 0.1 0.2 0.3 0.4x(m)(a)251


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>y(m)0.30.20.10-0.180 MPa100 MPa50 MPaTime=0.14715 second-0.4 -0.3 -0.2 -0.1 0 0.1 0.2 0.3x(m)(b)Figure 5 Fracture trajectory and internal fluid pressure in <strong>the</strong>presence <strong>of</strong> a natural fracture that has finite length and aninclination angle <strong>of</strong> 135 degree with respect to <strong>the</strong> x-axis.The coefficient <strong>of</strong> friction <strong>of</strong> <strong>the</strong> natural fracture is 0.3. Thefluid viscosity is 0.01 Pa s and <strong>the</strong> injection rate is specifiedas 0.0004 m 2 /s.The a rrest <strong>of</strong> one fra cture will faci litate <strong>the</strong>propagation <strong>of</strong> a second win g <strong>of</strong> a t wo-wingedfracture, as shown in Fig. 5(b). The left-hand sidefracture p ropagates at a lower p ressure, takin gmost <strong>of</strong> injected fluid and growing much faster.ReferencesAbass, H. H., Soliman, M. Y., Tahi ni, A. M.,Surjaatmadja, J., Meadows, D. L., Sierra, L.,2009, Ori ented fractu ring: A new tech nology tohydraulically fractu re op enhole ho rizontal well ,SPE 124483, Proceedi ngs <strong>of</strong> <strong>the</strong> 2009 SPEAnnual Technical <strong>Conference</strong> and Exhibition, NewOrleans, Louisiana, October 4-7 2009Cherny, S., Chirkov, D., Lapin, V., Muran ov, A.,Bannkov, D., Miller, M., Willberg, D., Medvedev ,O. and Aleksee nko, O., 2009, Two-di mensionalmodelling <strong>of</strong> <strong>the</strong> near-well bore fracture tortuosityeffect, Int. J. Rock Mech. & Mining Sci. 46, p. 992-1000.Crouch, S. L. and Starfield, A. M., 1990, BoundaryElement Me thod in Sol id Me chanics, Un winHyman, BostonDaneshy, A. A., 1973, A stu dy <strong>of</strong> incli nedhydraulic fractures, SPE J 13: p. 61-68.Detournay, E., 2004, Prop agation regime <strong>of</strong> flui d-driven fractu res in imp ermeable ro cks, Int. J.Geomechanics 4, p. 35-45.Detournay, E. and Jeffrey, R., 19 86, Stre ssconditions for initiation o f seconda ry fractu resfrom a fract ured b orehole, proceedi ngs <strong>of</strong> <strong>the</strong>international symposium on ro ck stress and rockstress me asurements, St ockholm, S weden, 1 -3,September, 1986.Hamison, B. and Fai rhurst C., 1970 In-situ stressdetermination at gre at depth by means <strong>of</strong>hydraulic fra cturing, in Ro ck M echanics—Theoryand Pra ctice, (ed.) W. H. Somerton, Am. Inst.Mining Engrg., 559–584, 1970Jeffrey, R. G., 1989 The combi ned effect <strong>of</strong> fluidlag and f racture tou ghness on hydraulic fra cturepropagation, SPE 18957, Pr oceedings <strong>of</strong> SPEJoint Rocky Mountain Regional/ Low PermeabilityReservoirs S ymposium a nd Exhibition , Denve r,Colorado, March 6-8, 1989.Manrique, J. F. and Ven kitaraman, A., 2001,Oriented fra cturing – A pra ctical te chnique forproduction optimization, <strong>Proceedings</strong> <strong>of</strong> <strong>the</strong> 2001SPE Annual Technical <strong>Conference</strong> and Exhibitionheld in New Orleans, Louisiana, 30 Se ptember–3October 2001Mogilevskaya, S. G., Ro<strong>the</strong> nburg, L. an dDusseault, M. B., 2000, Growth <strong>of</strong> pressu reinducedfra ctures in <strong>the</strong> vicinity <strong>of</strong> a wellbo re,International Journal <strong>of</strong> Fracture 104, p. L25-L30.Settari, A. and H. S. Pri ce., 19 84, Si mulation <strong>of</strong>hydraulic fracturing in low-permeability reservoirs,SPEJ April 1984, p. 141-152.Soliman, M. Y., East, L. and Ad ams, D., 2008,Geomechanics aspects <strong>of</strong> multiple fracturi ng <strong>of</strong>horizontal and vertical wells, SPE 86889, SPEDrilling and Completion, Sept. 2008, 217-228.Weng, X., 1993, Fracture Initiation andPropagation from Deviated Well bores, SPE26597, pre sented at <strong>the</strong> 1993 AT CE, Hou ston,TX, 3-6 October, 1993.Zhang, X. Jeffrey, R. G. an d Thiercelin, M., 2007,Deflection <strong>of</strong> fluid-driven fractures a t beddin ginterfaces: A numerical investigation, J. StructuralGeology 29, p. 396-410.Zhang, X. Jeffrey, R. G. an d Thiercelin, M., 2009,Mechanics <strong>of</strong> fluid-drive n fra cture growth i nnaturally fractured reservoirs with si mple networkgeometries, J. Ge ophysical Research -S olidEarth, 114, B12406.Zhang, X. Jeffrey, R.G ., Bunger, A.P. andThiercelin, M., <strong>2010</strong> Initia tion and growth <strong>of</strong> ahydraulic fracture from a boreho le unde rtoughness- or visco sity- domin ated conditions,44 th US Ro ck Me chanics Symposiu m and 5 thU.S.-Canada R ock Me chanics Symp osium, Sa ltLake City, UT June 27–30, <strong>2010</strong>.252


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Economics <strong>of</strong> geo<strong>the</strong>rmal feedwater heating for steam Rankine cyclesDavid L. Battye * , Peter J. Ashman, Gus J. NathanCentre for <strong>Energy</strong> TechnologyUniversity <strong>of</strong> Adelaide, SA 5005.* Corresponding author: david.battye@adelaide.edu.auWe have investigated <strong>the</strong> economics <strong>of</strong>geo<strong>the</strong>rmal feedwater heating (GFWH) in a steamRankine cycle with base capacity <strong>of</strong> 583 MW(gross). The capital cost per kW geo<strong>the</strong>rmalpower (before ge<strong>of</strong>luid pumping) is compared withthose <strong>of</strong> stand-alone geo<strong>the</strong>rmal plants <strong>of</strong> equalpower. The economic benefits <strong>of</strong> GFWH overstand-alone plants for enhanced geo<strong>the</strong>rmalsystems are, in order <strong>of</strong> importance:• 67% less operating and maintenance cost• 28% less capital cost• 30-35% less ge<strong>of</strong>luid pumping loadsThe reduction in levelised geo<strong>the</strong>rmal energy costis estimated to be 48%.Keywords: geo<strong>the</strong>rmal power, cost, economics,hybrid.IntroductionIn steam Rankine cycles, boiler feedwater mustbe heated from a low temperature at <strong>the</strong>condenser outlet (typically ~40 C) totemperatures <strong>of</strong> typically 250 C before entering<strong>the</strong> boiler. In “regenerative” steam cycles, this isaccomplished in a series <strong>of</strong> feedwater heaters,which use steam extracted from various stages in<strong>the</strong> turbine. One feedwater heater is a deaerator,in which extracted steam and feedwater are indirect contact, liberating oxygen and o<strong>the</strong>r gasesin <strong>the</strong> feedwater for venting to atmosphere. Theo<strong>the</strong>r feedwater heaters are shell-and-tube heatexchangers where feedwater flows in <strong>the</strong> tubesand steam condenses on <strong>the</strong> outside.If feedwater heating can be accomplished usinggeo<strong>the</strong>rmal heat, <strong>the</strong> steam normally extracted forfeedwater heating can instead generate power in<strong>the</strong> turbine. The extra power generated bygeo<strong>the</strong>rmal feedwater heating (GFWH) <strong>of</strong>fers <strong>the</strong>following potential benefits:• Existing plants may be retr<strong>of</strong>itted toaccommodate a proportion <strong>of</strong> geo<strong>the</strong>rmalpower• Geo<strong>the</strong>rmal power may be generated morecheaply than in a stand-alone plant• Steam cycles may be adapted for GFWH withno novel technology required.GFWH is suitable for coal, gas, solar-<strong>the</strong>rmal andnuclear-fuelled boiler plants, but not combinedcyclegas turbine plants. The latter plants use hotexhaust gas for feedwater heating in <strong>the</strong> Rankinecycle section.Interest in geo<strong>the</strong>rmal feedwater heating hasexisted since <strong>the</strong> 1970s, when it was investigatedfor application at sites in California and Utah(Parsons, 1978). It has been recently studied byBruhn (2002), Buchta (2009) and Borsukiewicz-Gozdur (<strong>2010</strong>). All studies agree that geo<strong>the</strong>rmalpower generation by GFWH is significantly moreefficient <strong>the</strong>rmodynamically than in conventionalstand-alone plants. However, to <strong>the</strong> authors'knowledge, no previous comparison has beenreported <strong>of</strong> <strong>the</strong> economic benefits <strong>of</strong> GFWH overstand alone geo<strong>the</strong>rmal power generation. Weseek to provide such a comparison, specificallywith respect to power generation from enhancedgeo<strong>the</strong>rmal systems.Condensate tocondenserFWH 1FWH 2FWH 3FWH 4FWH 5(deaerator)FWH 6FWH 7Feedwater from condenser49 C, 386 kg/sSteam72 C, 12 kg/s67 C88 CSteam132 C, 23 kg/s125 CSteam147 C, 10 kg/s140 CSteam186 C, 29 kg/s188 CSteam222 C, 22 kg/s218 CFeedwater to boiler251 C, 470 kg/sSteam94 C, 13 kg/sSteam255 C, 33 kg/sFigure 1: Feedwater heating section in a conventional 583MW (gross) steam Rankine cycle. Steam flows extractedfrom turbine stages are shown at right. These steam flowsmay be replaced by a single flow <strong>of</strong> hot water from ageo<strong>the</strong>rmal reservoir.253


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>MethodologyFor our economic analysis we consider <strong>the</strong> casethat GFWH is being used to provide extracapacity for a new Rankine steam cycle plant.This scenario is in contrast to <strong>the</strong> retr<strong>of</strong>it <strong>of</strong> anexisting plant, where <strong>the</strong> capacity is typically fixed.The basis for analysis is a 583 MW (gross)subcritical steam cycle with single reheat, forwhich design specifications and cost estimateshave been reported (NETL, 2007). A processflow diagram <strong>of</strong> <strong>the</strong> feedwater heating section isshown in Figure 1. In <strong>the</strong> proposed GFWHscenario, feedwater is heated by ge<strong>of</strong>luid instead<strong>of</strong> steam extracted from turbine stages. Theo<strong>the</strong>rwise extracted steam flows are <strong>the</strong>navailable for power generation in <strong>the</strong> turbine.The temperature to which <strong>the</strong> feedwater is heatedby <strong>the</strong> ge<strong>of</strong>luid, T GFWH, is a variable in <strong>the</strong>analysis. Above this temperature, we assumethat feedwater heating is achieved byconventional heaters as per normal. However,<strong>the</strong> deaerator must be retained in <strong>the</strong> cycle, andmay have to operate at higher temperatures thannormal. We assume that <strong>the</strong> upper limit <strong>of</strong> GFWHinput is one where feedwater is heated to 220 Cby ge<strong>of</strong>luid, and a deaerator heats feedwater from220 C to 251 C.To estimate <strong>the</strong> increased costs <strong>of</strong> equipment inGFWH cases, <strong>the</strong> reported costs <strong>of</strong> componentsare increased in proportion to turbine exhauststeam flow (turbine, condenser, steam piping, andcooling system) or gross power (generator,accessory electrical plant, instrumentation andcontrol).The cost <strong>of</strong> feedwater heaters (apart from <strong>the</strong>deaerator) is proportional to <strong>the</strong> heat transfersurface area, which varies with <strong>the</strong> overall heattransfer coefficient, U, and mean temperaturedifference between ge<strong>of</strong>luid and feedwaterstreams, MTD. We estimate that U is decreasedby ~30% in GFWH, since <strong>the</strong> high film coefficientsassociated with condensing steam are absent.MTD is about 15 K on average in conventionalfeedwater heaters. In GFWH cases MTD is avariable. The resulting multiplier applied to <strong>the</strong>conventional feedwater heater train cost is: TGFWH 38 21 f 1 1 213 MTD Ge<strong>of</strong>luid costs are estimated assuming:• Flow <strong>of</strong> 80 kg/s per well drilled• Drilling costs vary exponentially with depthaccording to:C drill 0.5e0.0001491d$M, 2000 US• O<strong>the</strong>r costs (stimulation, ge<strong>of</strong>luid pumps andpiping) are 20 % <strong>of</strong> drilling costs.Ge<strong>of</strong>luid costs (2009 US dollars) versus ge<strong>of</strong>luidtemperature are shown in Figure 2 for <strong>the</strong>rmalgradients <strong>of</strong> 40 and 50 K/km.Ge<strong>of</strong>luid cost, $K per kg/s2502001501005050 K/km40 K/km050 100 150 200 250 300Ge<strong>of</strong>luid temperature, CFigure 2: Ge<strong>of</strong>luid cost versus ge<strong>of</strong>luid temperature for<strong>the</strong>rmal gradients <strong>of</strong> 40 and 50 K/km.Estimates <strong>of</strong> <strong>the</strong> cost and performance <strong>of</strong> standalonegeo<strong>the</strong>rmal power plants are based on datain <strong>the</strong> Next Generation Geo<strong>the</strong>rmal Power Plantsreport (Brugman et al., 1995 and CE Holt, 2006)and documentation for <strong>the</strong> Geo<strong>the</strong>rmal ElectricTechnologies Evaluation Model (GETEM)(Entingh, 2006).All plants in <strong>the</strong> analysis are water-cooled and usea cooling tower.The costs determined from <strong>the</strong> literature havebeen updated to 2009 US dollars using <strong>the</strong>Chemical Engineering Plant Cost Index.Results and discussionFigure 3 shows percentage extra gross power andexhaust steam flow versus T GFWH. The effectivegeo<strong>the</strong>rmal power output (before ge<strong>of</strong>luidpumping) ranges from 9.6 MW at 100 C to 61MW at 220 C.Figure 4 shows <strong>the</strong> consumption <strong>of</strong> ge<strong>of</strong>luid perunit geo<strong>the</strong>rmal energy generated (net beforege<strong>of</strong>luid pumping) versus ge<strong>of</strong>luid temperature.The GFWH plants require significantly lessge<strong>of</strong>luid than <strong>the</strong> stand-alone plants, typically 30-35% less above 200 C. The explanation for thislies in <strong>the</strong> fact that <strong>the</strong> GFWH plants minimise<strong>the</strong>rmodynamic inefficiency associated with heattransfer from <strong>the</strong> ge<strong>of</strong>luid. The lower <strong>the</strong> MTD,<strong>the</strong> greater <strong>the</strong> <strong>the</strong>rmodynamic benefit, but at <strong>the</strong>expense <strong>of</strong> higher heat exchanger costs.(Entingh, 2006), where d is depth in feet.254


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>% extra power or steam flow35302520151050Exhaust steam flowGross power50 100 150 200 250T GFWH , CPlant cost, $/kW4000300020001000ORCDouble flashGFWH, MTD = 30 KGFWH, MTD = 20 K0100 150 200 250Ge<strong>of</strong>luid temperature, CFigure 3: Percentage extra gross power and turbine exhauststeam flow versus geo<strong>the</strong>rmal feedwater heatingtemperature.0.1Figure 5: Plant cost versus ge<strong>of</strong>luid temperature for equalpower outputs. GFWH plant costs correspond to <strong>the</strong>increment on base plant cost.6000Ge<strong>of</strong>luid consumption, kg/kJ0.080.060.040.020ORCDouble flashGFWH, MTD = 30 KGFWH, MTD = 20 KCapital cost, $/kW500040003000200010000ORCDouble flashGFWH100 150 200 250Ge<strong>of</strong>luid temperature, C100 150 200 250Ge<strong>of</strong>luid temperature, CFigure 4: Ge<strong>of</strong>luid consumption per unit geo<strong>the</strong>rmal energygenerated (net before ge<strong>of</strong>luid pumping) versus ge<strong>of</strong>luidtemperature.Figure 5 compares plant costs for GFWH andstand-alone plants, ie. Organic Rankine Cycles(ORC) and double flash steam plants. Increasingge<strong>of</strong>luid temperature reduces <strong>the</strong> cost <strong>of</strong> all plantsdue to improving <strong>the</strong>rmal efficiency. However, <strong>the</strong>stand-alone plant cost also decreases due toeconomies <strong>of</strong> scale. GFWH plant costscorrespond to <strong>the</strong> increment on base plant cost.Since <strong>the</strong> base plant capacity is already manytimes greater than for <strong>the</strong> stand-alone plants,GFWH plant costs are much lower on averageover <strong>the</strong> ge<strong>of</strong>luid temperature range. At <strong>the</strong> upperge<strong>of</strong>luid temperatures in Figure 5, <strong>the</strong> GFWHplant costs are 15-25 % lower than for a doubleflash plant.Figure 6: Capital cost versus ge<strong>of</strong>luid temperature for<strong>the</strong>rmal gradient <strong>of</strong> 50 K/km.Capital cost, $/kW60005000400030002000ORC1000 Double flashGFWH0100 150 200 250Ge<strong>of</strong>luid temperature, CFigure 7: Capital cost versus ge<strong>of</strong>luid temperature for<strong>the</strong>rmal gradient <strong>of</strong> 40 K/km.Total capital costs are shown in Figures 6 and 7for <strong>the</strong>rmal gradients <strong>of</strong> 50 K/m and 40 K/mrespectively. Note that <strong>the</strong> $/kW value is forgeo<strong>the</strong>rmal power before ge<strong>of</strong>luid pumping. The255


value <strong>of</strong> MTD is optimised in each case: 30 K for50 K/km and 20 K for 40 K/km. The following isobserved:• Optimal ge<strong>of</strong>luid temperatures are 220 C orgreater.• Optimal GFWH plants reduce total cost by28% relative to optimal stand-alone plants inboth cases.• GFWH with a 40 K/km <strong>the</strong>rmal gradient cangenerate power at <strong>the</strong> same cost as a standaloneplant with a 50 K/km gradient.• GFWH can generate power at <strong>the</strong> same costas optimal stand-alone plants, but at ge<strong>of</strong>luidtemperatures <strong>of</strong> only 120-150 C as opposedto 220 C.Relative to stand-alone plants, GFWH has <strong>the</strong>additional benefit <strong>of</strong> incurring less ge<strong>of</strong>luidpumping power loads, which are not accountedfor in <strong>the</strong> preceding analysis. Since GFWHconsumes 30-35 % less ge<strong>of</strong>luid above 200 C,pumping loads are reduced by <strong>the</strong> same amountrelative to stand-alone plants.Ano<strong>the</strong>r economic benefit is that geo<strong>the</strong>rmaloperating and maintenance costs are drasticallyreduced by GFWH. For example, O&M costs in a61 MW stand-alone geo<strong>the</strong>rmal plant areestimated at 7.3 $M/year (Sanyal, 2004) whereas61 MW generated by GFWH only incurs 10 % <strong>of</strong><strong>the</strong> annual O&M costs <strong>of</strong> <strong>the</strong> whole plant, ie. 2.4$M/year (NETL, 2007), a saving <strong>of</strong> 67%.A simple estimate <strong>of</strong> <strong>the</strong> reduction in <strong>the</strong> levelisedcost <strong>of</strong> geo<strong>the</strong>rmal energy can be made usingfigures reported by Sanyal (2007) for EGS power.Table 1 illustrates how <strong>the</strong> estimate is made andsuggests a reduction in total levelised costapproximating 48%.Table 1: Estimate <strong>of</strong> reduction in levelised cost <strong>of</strong> geo<strong>the</strong>rmalenergy by GFHW, based on estimates <strong>of</strong> Sanyal (2007) andpreceding analysis.Levelised costfor standaloneplant,¢/kWh(US, 2007)Reductionby GFWHGFWHlevelisedcost,¢/kWh(US, 2007)O&M 2.75 1.84 (67%) 0.91Capital andcost <strong>of</strong>money2.68 0.75 (28%) 1.93Total 5.43 2.59 (48%) 2.84<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Concluding remarksThe economic analysis has shown geo<strong>the</strong>rmalfeedwater heating in a purpose-built steamRankine cycle to have economic merit. Giventhat good solar and EGS resources in Australiaare generally co-located, solar-geo<strong>the</strong>rmal hybridsusing GFWH are possible. Fur<strong>the</strong>r work willinvestigate <strong>the</strong> economics <strong>of</strong> retr<strong>of</strong>itting existingsteam Rankine cycle plants for GFWH.ReferencesBorsukiewicz-Gozdur, A., <strong>2010</strong>, Dual-fluid-hybridpower plant co-powered by low-temperaturegeo<strong>the</strong>rmal water, Geo<strong>the</strong>rmics, 39, 170-176.Brugman, J., Hattar, M., Nichols, K. and Esaki, Y.,1995, Next Generation Geo<strong>the</strong>rmal Power Plants,Electric Power Research Institute (EPRI) ReportNo. EPRI/RP 3657-01.Bruhn, M., 2002, Hybrid geo<strong>the</strong>rmal–fossilelectricity generation from low enthalpygeo<strong>the</strong>rmal resources: geo<strong>the</strong>rmal feedwaterpreheating in conventional power plants, <strong>Energy</strong>,27, 329–346Buchta, J., 2009, Green power from conventionalsteam power plant combined with geo<strong>the</strong>rmalwell, <strong>Proceedings</strong> <strong>of</strong> <strong>the</strong> IEEE International<strong>Conference</strong> on Industrial Technology , Article No.4939553.CE Holt Consulting Firm, 2006, NGGPP processdata for binary cycle plants, Document for U.S.Dept. <strong>of</strong> <strong>Energy</strong>.Entingh, D.J., 2006, US Dept. <strong>of</strong> <strong>Energy</strong> (DOE)Geo<strong>the</strong>rmal Electricity Technology EvaluationModel (GETEM): Volume I – Technical ReferenceManual.National <strong>Energy</strong> Technology Laboratory (NETL),2007, Cost and Performance Baseline for Fossil<strong>Energy</strong> Plants, Volume 1: Bituminous Coal andNatural Gas to Electricity Final Report, ReportNo. DOE/NETL-2007/1281.Parsons, R.M., 1978, System design verification<strong>of</strong> a hybrid geo<strong>the</strong>rmal/coal fired power plant, City<strong>of</strong> Burbank and Ralph M. Parsons Company; USDept. <strong>of</strong> <strong>Energy</strong> (DOE), Report No. SAN-1572-T2.Sanyal, S.K., 2004, Cost <strong>of</strong> geo<strong>the</strong>rmal power andfactors that affect it, <strong>Proceedings</strong> <strong>of</strong> <strong>the</strong> Twenty-Ninth Workshop on Geo<strong>the</strong>rmal ReservoirEngineering, Stanford University, Stanford,California, Jan. 26-28, SGP-TR-175.Sanyal, S.K., 2007, Cost <strong>of</strong> electricity fromenhanced geo<strong>the</strong>rmal systems, <strong>Proceedings</strong> <strong>of</strong><strong>the</strong> Thrity-Second Workshop on Geo<strong>the</strong>rmalReservoir Engineering, Stanford University,Stanford, California, Jan. 22-24, SGP-TR-175.256


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>A Protocol for Estimating and Mapping Global EGS PotentialGraeme Beardsmore 1* , Ladislaus Rybach 2 , David Blackwell 3 and Charles Baron 41. Hot Dry Rocks PL, PO Box 251, South Yarra VIC 3141, Australia2. Geowatt AG, Dohlenweg 28, CH-8050 Zürich, Switzerland3. Sou<strong>the</strong>rn Methodist University, Dallas, TX 75275, USA4. Google.org, 1600 Amphi<strong>the</strong>atre Parkway, Mountain View, CA 94043, USA* Corresponding author: graeme.beardsmore@hotdryrocks.comAbstractWe present a Protocol to estimate and map <strong>the</strong>Theoretical and Technical potential forEngineered Geo<strong>the</strong>rmal Systems (EGS) in aglobally self-consistent manner compatible withcurrent public geo<strong>the</strong>rmal Reporting Codes. Thegoal <strong>of</strong> <strong>the</strong> Protocol is to standardise <strong>the</strong>production <strong>of</strong> regional estimates and maps <strong>of</strong>EGS potential so that <strong>the</strong>y are directlycomparable to one ano<strong>the</strong>r globally.The Protocol is divided into five stages:1. Model <strong>the</strong> temperature, heat flow and availableheat <strong>of</strong> <strong>the</strong> Earth’s crust to a depth <strong>of</strong> 10,000 m2. Estimate <strong>the</strong> Theoretical Potential for EGSpower in <strong>the</strong> crust to a depth <strong>of</strong> 10,000 m3. Estimate <strong>the</strong> Technical Potential that can berealized with current technology, and consideringgeographic, ecologic, legal and regulatoryrestrictions4. Define a level <strong>of</strong> confidence in <strong>the</strong> estimatedTechnical Potential at each location, consistentwith public Reporting Codes5. Present results using KML visualization anddata architectureThe maps, estimates and source dataunderpinning <strong>the</strong> estimates and maps will bemade freely available for public use andpresented in <strong>the</strong> Keyhole Markup Language(KML) for Google Earth.Keywords:Engineered Geo<strong>the</strong>rmal Systems; EGS resourceestimation; Global geo<strong>the</strong>rmal resource inventory;Google Earth; Keyhole Markup Language; KMLIntroductionEngineered Geo<strong>the</strong>rmal Systems‘Engineered Geo<strong>the</strong>rmal Systems (EGS)’ is ageneric term for <strong>the</strong> process whereby heat isextracted from <strong>the</strong> Earth’s crust by circulatingwater through an artificially engineered set <strong>of</strong>permeable fractures in hot rocks (Figure 1).Although significant engineering and financialhurdles remain, EGS plants hold <strong>the</strong> promise <strong>of</strong>nearly ubiquitous, low to zero CO 2 emission,secure, base-load power for millennia to come. In<strong>the</strong>ory, EGS plants may be constructed anywherethat <strong>the</strong> mechanical limits <strong>of</strong> drilling and fractureengineering allow. Fur<strong>the</strong>rmore, geo<strong>the</strong>rmalsystems have <strong>the</strong> second lowest land footprint <strong>of</strong>all electrical generating technologies (McDonaldet al., 2009). These attributes make EGS anattractive potential major contributor to worldenergy supplies.Figure 1. Conceptual EGS power plant design (from MIT,2006)For EGS to play a material role in <strong>the</strong> globalenergy mix, improving public awareness anddispersing knowledge <strong>of</strong> <strong>the</strong> global potential andits regional distribution is a vital precursor toinformed R&D, energy policy making, and broadscalecommercial deployment.A Protocol for estimating and mapping globalEGS potentialThis paper summarises a Protocol to estimateand map <strong>the</strong> Theoretical Potential and TechnicalPotential (as defined by Rybach, <strong>2010</strong>) for EGS ina globally self-consistent manner. Any estimate ormap <strong>of</strong> EGS potential in a region involves anumber <strong>of</strong> inputs about geology, <strong>the</strong>rmalproperties, recovery factors, power conversionefficiencies, ambient temperatures and so on. Itfollows that an inventory <strong>of</strong> <strong>the</strong> global EGSpotential requires a globally consistentmethodology and a globally consistent set <strong>of</strong>assumptions to fall back on when real data arenot available.The Protocol does not seek to provide a uniquepicture <strong>of</strong> <strong>the</strong> magnitude and distribution <strong>of</strong> <strong>the</strong>world’s EGS potential. Alternative approaches toestimating EGS potential may be more relevant inparticular locations and more robust analyses will257


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>certainly be required to assess <strong>the</strong> commercialviability <strong>of</strong> EGS at specific sites. The Protocol will,however, provide consistent methodologies andassumptions that will ultimately allow a selfconsistentinventory and map <strong>of</strong> EGS potentialaround <strong>the</strong> world.The Protocol will provide utility for academia,policy makers and commercial entities bystandardizing technical language, improvingunderstanding <strong>of</strong> EGS generation potential,providing a consistent visualization platform, andfacilitating international commercialization efforts.The basis for <strong>the</strong> ProtocolThe Protocol closely follows <strong>the</strong> methodsunderpinning a report by <strong>the</strong> MassachusettsInstitute <strong>of</strong> Technology, which concluded in 2006that EGS could provide 100,000 MW <strong>of</strong> electricalgenerating capacity to <strong>the</strong> United States by 2050(MIT, 2006). An integral component <strong>of</strong> that studywas a review <strong>of</strong> <strong>the</strong> heat resource within <strong>the</strong> top10,000 m <strong>of</strong> <strong>the</strong> crust by Pr<strong>of</strong>essor DavidBlackwell and his team at Sou<strong>the</strong>rn MethodistUniversity (SMU; Blackwell et al., 2007). SMUassumed that conduction is <strong>the</strong> primary heattransfer mechanism in <strong>the</strong> crust, and that <strong>the</strong>upper crust can be broadly divided into sections <strong>of</strong>‘sediment’ and ‘basement’, each with its ownphysical properties <strong>of</strong> <strong>the</strong>rmal conductivity andinternal heat generation.In 2008, <strong>the</strong> SMU team and Google.org converted<strong>the</strong> MIT findings into KML format for visualizationon <strong>the</strong> Google Earth platform (Figure 2). Thelayers are available for free download and viewingfrom www.google.org/egs/.Figure 2. Screen capture <strong>of</strong> a Google Earth layer depicting<strong>the</strong> predicted temperature at 5.5 km and <strong>the</strong> EGS Potentialbase for Nevada, USA.Theoretical and Technical PotentialThe Protocol calls for an initial estimate <strong>of</strong> <strong>the</strong>‘Theoretical Potential’ for EGS across a region,following <strong>the</strong> terminology <strong>of</strong> Rybach (<strong>2010</strong>).Theoretical Potential is “defined solely by <strong>the</strong>physical limits <strong>of</strong> use and thus marks <strong>the</strong> upperlimit <strong>of</strong> <strong>the</strong> <strong>the</strong>oretically realizable energy supplycontribution.” From <strong>the</strong> Theoretical Potential, <strong>the</strong>Protocol provides guidelines to estimate <strong>the</strong>‘Technical Potential’, or “<strong>the</strong> fraction <strong>of</strong> <strong>the</strong><strong>the</strong>oretical potential that can be used under <strong>the</strong>existing technical restrictions…structural andecologic restrictions as well as legal andregulatory allowances” (Rybach, <strong>2010</strong>). Theserestrictions vary greatly with geology, location andtime, providing some flexibility to modify TechnicalPotential based on current local conditions.Geo<strong>the</strong>rmal Resource reporting codesCodes for <strong>the</strong> reporting <strong>of</strong> Geo<strong>the</strong>rmal Resourceestimates exist for Australia and Canada. TheProtocol aims to conform to those reportingCodes in so far as respecting <strong>the</strong>ir underlyingprinciples <strong>of</strong> ‘transparency’, ‘materiality’ and‘competence’. These principles will be honouredthrough <strong>the</strong> inclusion <strong>of</strong> all relevant information(generally as metadata) with each set <strong>of</strong> mapsand tables produced, and by including <strong>the</strong>personal endorsement <strong>of</strong> one or more‘Competent’ or ‘Qualified’ Persons. The Protocolproposes <strong>the</strong> following minimum level <strong>of</strong>information to comply with <strong>the</strong>se principles:1. A statement that <strong>the</strong> data should not be reliedon to inform commercial investment decisions2. Sources <strong>of</strong> all data utilized for <strong>the</strong> estimates <strong>of</strong>EGS potential3. A brief description <strong>of</strong> <strong>the</strong> modelling technique4. Assumed ambient temperatures, recoveryfactors, and conversion efficiencies5. Assumed lifespan <strong>of</strong> power generation6. Statement <strong>of</strong> relative accuracy / confidence7. The name(s) <strong>of</strong> <strong>the</strong> Competent or QualifiedPerson(s) who accept(s) responsibility for <strong>the</strong>Resource estimate.MethodologyThe Protocol assumes that pure verticalconduction dominates heat transport through <strong>the</strong>crust, and that a simple two-layer geologicalmodel (‘sediment’ on ‘basement’) approximates<strong>the</strong> top 10,000 m <strong>of</strong> crust in all continental areas.A region is divided into a grid-work <strong>of</strong> ‘cells’, and<strong>the</strong> simple two-layer model is used to estimate <strong>the</strong>local <strong>the</strong>rmal structure in each cell. The EGSTheoretical Potential (relative to a defined ‘basetemperature’) is <strong>the</strong>n tallied over differentdepth/volume intervals by assuming density andspecific heat values for <strong>the</strong> rocks in question, andassuming a uniform heat–electricity conversionpathway. The discrete estimates <strong>of</strong> each cell maybe summed to estimate <strong>the</strong> total EGS potentialover <strong>the</strong> region or depth interval.In practice, <strong>the</strong> process is divided into five stages:1. Model temperature, heat flow and heat in <strong>the</strong>Earth’s crust down to a depth <strong>of</strong> 10,000 m258


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>2. Estimate <strong>the</strong> Theoretical Potential <strong>of</strong> EGSpower in <strong>the</strong> crust down to a depth <strong>of</strong> 10,000 m3. Estimate <strong>the</strong> Technical Potential given currenttechnology, geographic, ecologic, legal andregulatory restrictions4. Define a level <strong>of</strong> confidence in <strong>the</strong> estimatedTechnical Potential at each location, consistentwith public Reporting Codes5. Present results using common visualization anddata architectureModel temperature, heat flow and heat in <strong>the</strong>Earth’s crust down to a depth <strong>of</strong> 10,000 mThe temperature in <strong>the</strong> crust can be estimatedusing a ‘top down’ approach, where surface heatflow (Q 0 ) is assumed to extend downwards,gradually decreasing with increasing depth due to<strong>the</strong> distribution <strong>of</strong> heat generation in <strong>the</strong> rocks.Average <strong>the</strong>rmal gradient can be estimated overany depth interval from <strong>the</strong> heat flow and <strong>the</strong>rmalproperties <strong>of</strong> <strong>the</strong> rocks. The Protocol recommendsestimating <strong>the</strong> temperature pr<strong>of</strong>ile through <strong>the</strong> top10,000 m <strong>of</strong> crust using a ‘top down’ approach.Figure 3 provides a flow chart for a process thatcan be applied for any location.The next step is to chart <strong>the</strong> average thickness <strong>of</strong>‘sediment’ overlying ‘basement’ in each 5’ x 5’cell—in effect, develop a ‘depth to basement’ mapfor <strong>the</strong> region <strong>of</strong> interest. For Australia, <strong>the</strong>SEEBASE TM database provides a first passestimate <strong>of</strong> <strong>the</strong> thickness <strong>of</strong> Phanerozoic basinsacross <strong>the</strong> continent (Figure 4), and can be freelydownloaded over <strong>the</strong> Internet. SEEBASE is aregistered trademark <strong>of</strong> FrOG Tech Pty Limited inAustralia, and stands for Structurally Enhancedview <strong>of</strong> Economic BASEment.Figure 4. A visualization <strong>of</strong> <strong>the</strong> SEEBASE TM database.Figure 3. General process for estimating <strong>the</strong> temperaturepr<strong>of</strong>ile <strong>of</strong> <strong>the</strong> crust to 10,000 m depth. See Glossary forsymbol definitions.The region under investigation is first divided intoa regular grid. 5’ x 5’ graticules are recommendedas <strong>the</strong> basic ‘cell’ size. A region such as Australia(7.6 million square kilometres at an averagelatitude <strong>of</strong> around 25°S) requires ~100,000 cells.Temperature can be predicted at any arbitrarydepth for a given surface heat flow (Q 0 ), <strong>the</strong>rmalconductivity and heat generation (A) structure.The temperature prediction process requires that<strong>the</strong> sediment and basement sections <strong>of</strong> each cellbe individually characterised with values <strong>of</strong><strong>the</strong>rmal conductivity (K S and K B for sediment andbasement, respectively) and heat generation (A Sand A B , respectively). To maintain consistencywith Blackwell et al. (2007), <strong>the</strong> Protocol assumesthat <strong>the</strong> <strong>the</strong>rmal conductivity <strong>of</strong> sediment deeperthan 4,000 m is <strong>the</strong> same as <strong>the</strong> basement (K B ).Mean surface temperature (T 0 ) is an importantboundary condition for models <strong>of</strong> undergroundtemperature and for estimates <strong>of</strong> EGS potential.The Protocol assumes that mean surface rocktemperature is approximately equal to meansurface air temperature.Temperatures at depth are estimated in twosteps. The first step is to estimate <strong>the</strong> temperatureat <strong>the</strong> sediment–basement interface (T S ). T S isderived using one or both <strong>of</strong> <strong>the</strong> followingformulae, depending on whe<strong>the</strong>r sedimentthickness (S) is greater than or less than 4,000 m.If S < 4,000 m:T S = T 0 + [(Q 0 x S) / K S ] - A S x [S 2 / (2 x K S )]Eq 1259


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>If S > 4,000 m, <strong>the</strong> conductivity <strong>of</strong> that portion <strong>of</strong>sediment deeper than 4,000 m is K B . In this case,first calculate T 4km using S = 4000 in Eq 1, <strong>the</strong>n:T S = T 4km + [(Q 0 - 4000.A S ) x (S - 4000) / K B ] - A S x[(S - 4000) 2 / (2 x K B )] Eq 2Heat flow at <strong>the</strong> sediment–basement interface(Q S ) becomes <strong>the</strong> ‘surface heat flow’ forestimation <strong>of</strong> temperature at deeper levels. Q S isderived by subtracting <strong>the</strong> total contribution <strong>of</strong>sedimentary heat from Q 0 :Q S = Q 0 - S x A S Eq 3The second step is to estimate temperature atdepth (X) in <strong>the</strong> basement (T X ):T X = T S + [(Q S x (X-S)) / K B ] - A B x [(X-S) 2 / (2xK B )]Eq 4At <strong>the</strong> completion <strong>of</strong> this step, a mean predictedtemperature pr<strong>of</strong>ile to 10,000 m depth should beavailable for each 5’ x 5’ cell.Estimate <strong>the</strong> Theoretical Potential <strong>of</strong> EGS powerin <strong>the</strong> crust down to a depth <strong>of</strong> 10,000 mThe heat stored within a volume <strong>of</strong> rock isproportional to <strong>the</strong> temperature, heat capacity,density and volume <strong>of</strong> <strong>the</strong> rock. In addition, it canonly be estimated relative to a ‘base temperature’.Estimates <strong>of</strong> EGS potential, <strong>the</strong>refore, requirevalues for each <strong>of</strong> <strong>the</strong>se parameters. Figure 5provides a flow chart <strong>of</strong> <strong>the</strong> recommended fivestepprocess for estimating <strong>the</strong> TheoreticalPotential for EGS in <strong>the</strong> top 10,000 m <strong>of</strong> crust inany location.Figure 5. General process for estimating stored heat energyand <strong>the</strong>oretical power generation potential. See Glossary forsymbol definitions.Crustal temperature is <strong>the</strong> key determinant <strong>of</strong>Theoretical Potential for EGS at any specificlocation. Equation 4 provides this value for anyspecific depth. To relate temperature to heatcontent in a particular volume <strong>of</strong> crust, we need toassign a density (ρ) and specific heat (C p ) valuefor <strong>the</strong> volume <strong>of</strong> interest.Each depth interval beneath a surface cell willcontain a different amount <strong>of</strong> <strong>the</strong>rmal energy. Thetotal available heat in exajoules (H) in a volume <strong>of</strong>crust (V c ) is a function <strong>of</strong> <strong>the</strong> temperature, density,specific heat, and a ‘base temperature’ (T r ):H = ρ x C p x V c x (T X - T r ) x 10 -18 Eq 5The base temperature is <strong>the</strong> temperature to which<strong>the</strong> crust can <strong>the</strong>oretically be reduced throughutilization <strong>of</strong> geo<strong>the</strong>rmal heat. The Protocolproposes following <strong>the</strong> lead <strong>of</strong> <strong>the</strong> USGS in arecent assessment <strong>of</strong> geo<strong>the</strong>rmal potential in <strong>the</strong>USA (Williams et al., 2008), in which <strong>the</strong> USGSassumed approximately T r = T 0 + 80°C.Again following <strong>the</strong> lead <strong>of</strong> <strong>the</strong> USGS (Williams etal., 2008), Theoretical Potential power generationis derived using <strong>the</strong> following assumptions:1. All heat (H) above <strong>the</strong> base temperature is<strong>the</strong>oretically recoverable in all locations2. 30 years life span <strong>of</strong> power generation3. Cycle <strong>the</strong>rmal efficiency, η th , is a function <strong>of</strong>resource temperature as per MIT (2006):η th = 0.00052 x T + 0.032 Eq 6Note that <strong>the</strong> temperature appropriate for Eq 6 is<strong>the</strong> average <strong>of</strong> <strong>the</strong> initial rock temperature and <strong>the</strong>base temperature:T = (T X + T r ) / 2 Eq 7The potential power generation, P (MW e ), from avolume <strong>of</strong> rock with available heat, H, is:P = H x 10 12 x η th / 9.46x10 8 Eq 8Theoretical Potential power generation can becollated and tabulated for specific depth andtemperature intervals.Estimate <strong>the</strong> Technical Potential given currenttechnology, geographic, ecologic, legal andregulatory restrictionsIt is impossible to realize <strong>the</strong> entire TheoreticalPotential for EGS power in any location. Following<strong>the</strong> terminology <strong>of</strong> Rybach (<strong>2010</strong>), <strong>the</strong> ‘TechnicalPotential’ is that part <strong>of</strong> <strong>the</strong> Theoretical Potentialthat can be extracted after consideration <strong>of</strong>currently ‘insurmountable’ technical limitations.‘Technical’ is defined in its broadest sense,including factors such as land access, rock type,drilling technology, fracture density, stressorientation, regulatory framework, powerconversion technology and availability <strong>of</strong> water.Rybach (<strong>2010</strong>) argues that “<strong>the</strong> EGS potentialcannot yet be termed ‘technical’”, but <strong>the</strong> Protocolproposes a set <strong>of</strong> assumptions for deriving anestimate <strong>of</strong> Technical Potential. The steps areillustrated in Figure 6.National parks, conservation areas, denselypopulated areas, mountains, large lakes andswamps, militarized zones, deserts with noavailable water resources, and o<strong>the</strong>r areas maybe excluded from EGS development. Theproportion <strong>of</strong> each cell that is accessible andavailable for EGS (R av ) is a value between 0–1.260


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Figure 6. General process for estimating Technical Potential<strong>of</strong> EGS from <strong>the</strong> Theoretical Potential. See Glossary forsymbol definitions.The Protocol recommends limiting estimates <strong>of</strong>Technical Potential for EGS to <strong>the</strong> top 6,500 m.This may change if <strong>the</strong>re are significant advancesin hard-rock drilling technology.Recoverability factor (R) is <strong>the</strong> proportion <strong>of</strong> heatthat can ultimately be recovered from a volume <strong>of</strong>rock. The Protocol suggests estimates <strong>of</strong> potentialbe based on a range <strong>of</strong> R values representing <strong>the</strong>expected minimum, maximum and mean values.This Protocol proposes 0.02 as <strong>the</strong> minimum R,following <strong>the</strong> precedent <strong>of</strong> MIT (2006), and 0.14and 0.20 as <strong>the</strong> mean and maximum R,respectively, following <strong>the</strong> findings <strong>of</strong> Williams etal. (2008). These values are based on <strong>the</strong> results<strong>of</strong> numerical modelling. While <strong>the</strong>y fulfil <strong>the</strong> aim <strong>of</strong><strong>the</strong> Protocol to provide a globally consistent set <strong>of</strong>assumptions, estimates <strong>of</strong> Technical Potentialusing this Protocol should only be viewed aspreliminary until such time as practical experienceprovides real data on recoverability.There is a practical limit to <strong>the</strong> temperaturedrawdown a power plant can withstand before itwill no longer operate effectively. This Protocolrecommends following <strong>the</strong> methodology <strong>of</strong> MIT(2006) by assuming a maximum allowabletemperature drawdown <strong>of</strong> 10°C. This effectivelyintroduces a ‘temperature drawdown’recoverability factor (R TD ) defined by:R TD = 10 / (T X - T r ) Eq 9The Technical Potential (P T ) is that part <strong>of</strong> <strong>the</strong>Theoretical Potential accessible from <strong>the</strong> surface,shallower than 6,500 m, accessible via fracturenetworks, and available with


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Thirdly, <strong>the</strong> Protocol extends <strong>the</strong> methodologydescribed by MIT (2006) and Blackwell et al.(2007) to apply in areas where real data arescarce or non-existent.Fourthly, <strong>the</strong> Protocol recommends assessingEGS potential relative to a base temperature <strong>of</strong> T 0+ 80°C, ra<strong>the</strong>r than relative to T 0 .ConclusionsEstimates <strong>of</strong> EGS potential derived using <strong>the</strong>Protocol will not be ‘final’. They will continue to berefined as more relevant data become available.Theoretical Potential will be refined as newgeological and geophysical data improve ourunderstanding <strong>of</strong> <strong>the</strong> <strong>the</strong>rmal structure <strong>of</strong> <strong>the</strong>crust. Refinements here are expected to begradual. Technical Potential will be refined astechnological advancements in drilling, powerconversion and legal regimes allow greateramounts <strong>of</strong> <strong>the</strong> Theoretical Potential to berealized. Changes here are expected to besudden and dramatic.Application <strong>of</strong> <strong>the</strong> Protocol will undoubtedly revealgaps and uncertainties that will require <strong>the</strong>Protocol itself to be refined through time. TheProtocol will, <strong>the</strong>refore, be a ‘living document’.The authors hope that <strong>the</strong> EGS potential <strong>of</strong> most<strong>of</strong> <strong>the</strong> world’s continental surface will eventuallybe assessed and charted following <strong>the</strong> guidelines<strong>of</strong> <strong>the</strong> Protocol, allowing for <strong>the</strong> first time acoherent view <strong>of</strong> <strong>the</strong> size and distribution <strong>of</strong> <strong>the</strong>‘hidden’ energy stored in <strong>the</strong> rocks <strong>of</strong> <strong>the</strong> top10,000 m <strong>of</strong> <strong>the</strong> Earth’s crust.AcknowledgementsThe development <strong>of</strong> <strong>the</strong> Protocol was madepossible by <strong>the</strong> financial support <strong>of</strong> Google.orgthrough its ‘Renewable <strong>Energy</strong> Cheaper thanCoal’ initiative (RE


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Changes to Geo<strong>the</strong>rmal Reporting Code andGuidelines on Company ReportingBeardsmore, G. 1 , Budd, A. 2 , Goldstein, B. 3 , Holgate, F. 4 , Jeffress, G. 5 , Larking, A. 6 , Lawless, J. 7 , Libby J. 8 , Middleton,M. 9 , Reid, P. 10*, Stafford, C. 11 , Ward, M. 12 , Williams, A. 131Hot Dry Rocks Pty Ltd, PO Box 251, South Yarra, VIC 3141; 2 Geoscience Australia, GPO Box 378, CanberraACT 2601; 3 Primary Industries and Resources, PO Box 277, Adelaide SA; 4 KUTh <strong>Energy</strong> Ltd, 35 Smith Street,North Hobart, TAS 7000; 5 CSA Global, PO Box 139, Burswood, WA 6100; 6 Green Rock <strong>Energy</strong>, PO Box1177,WestPerth, WA 6872; 7 Sinclair Knight Merz, PO Box 9806, Newmarket , Auckland NZ; 8 New World <strong>Energy</strong>, Level 3, 46Ord St, West Perth, WA 6005; 9 WA Department <strong>of</strong> Mines and Petroleum, 100 Plain Street, East Perth, WA 6004; 10Petra<strong>the</strong>rm Limited, 129 Greenhill Rd, Unley 5061, South Australia; 11 Granite Power Limited, Level 6, 9 Barrack St,Sydney NSW 2000; 12 Geo<strong>the</strong>rmal Advisory Pty Ltd, PO Box 150, Richmond Tas 7025; 13 Geodynamics Limited, POBox 2046, Milton, Qld 4064* Corresponding Author: preid@petra<strong>the</strong>rm.com.auWith <strong>the</strong> launch <strong>of</strong> <strong>the</strong> First Edition <strong>of</strong> <strong>the</strong>Geo<strong>the</strong>rmal Reporting Code in August 2008,Members <strong>of</strong> <strong>the</strong> <strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong>Association (AGEA) agreed to report <strong>the</strong>irExploration Results, Geo<strong>the</strong>rmal Resources andGeo<strong>the</strong>rmal Reserves in accordance with <strong>the</strong>Geo<strong>the</strong>rmal Reporting Code. In its first year <strong>of</strong>operation, a number <strong>of</strong> issues became apparentin <strong>the</strong> use and interpretation <strong>of</strong> <strong>the</strong> Geo<strong>the</strong>rmalReporting Code. Most significant amongst <strong>the</strong>sewere: That <strong>the</strong> definition <strong>of</strong> an InferredGeo<strong>the</strong>rmal Resource was allowing largeestimates <strong>of</strong> stored heat to be reported.Whilst derived by legitimatemethodologies, it was perceived that<strong>the</strong>se large figures may not be properlyunderstood by non-technical people andmay result in a diminution <strong>of</strong> credibility <strong>of</strong><strong>the</strong> industry;Person sign-<strong>of</strong>f on public reports ando<strong>the</strong>r company announcements.The Geo<strong>the</strong>rmal Reporting Code Committeeconsulted with industry and received feedbackfrom companies and practitioners both in Australiaand overseas. The Second Edition <strong>of</strong> <strong>the</strong>Geo<strong>the</strong>rmal Reporting Code addresses <strong>the</strong> issuesidentified above. In some cases definitions andmeanings have been changed (for example, <strong>the</strong>re-defining <strong>of</strong> Geo<strong>the</strong>rmal Resources asrecoverable energy, ra<strong>the</strong>r than energy in place)whilst in o<strong>the</strong>rs, aspects <strong>of</strong> <strong>the</strong> Geo<strong>the</strong>rmalReporting Code that were already in place havebeen made more explicit (for example, <strong>the</strong>obligations in respect <strong>of</strong> Competent Person sign<strong>of</strong>fs).This presentation outlines <strong>the</strong> key changesto <strong>the</strong> Second Edition <strong>of</strong> <strong>the</strong> <strong>Australian</strong>Geo<strong>the</strong>rmal Reporting Code, and providesclarification on <strong>the</strong> public reporting requirements<strong>of</strong> Companies.The units <strong>of</strong> energy described in <strong>the</strong> FirstEdition were not always consistent orpractical; andCompanies were misunderstanding <strong>the</strong>circumstances requiring a CompetentKeywords: Geo<strong>the</strong>rmal <strong>Energy</strong>, ResourceEstimation, AustraliaReferencesThe <strong>Australian</strong> Geo<strong>the</strong>rmal Code Committee,2008. “<strong>Australian</strong> Code for Reporting <strong>of</strong>Exploration Results, Geo<strong>the</strong>rmal Resources andGeo<strong>the</strong>rmal Reserves; The Geo<strong>the</strong>rmal Reporting263


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Code 2008 Edition” <strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong>Group and <strong>the</strong> <strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong>Association.The <strong>Australian</strong> Geo<strong>the</strong>rmal Code Committee,<strong>2010</strong>. “<strong>Australian</strong> Code for Reporting <strong>of</strong>Exploration Results, Geo<strong>the</strong>rmal Resources andGeo<strong>the</strong>rmal Reserves; The Geo<strong>the</strong>rmal ReportingCode <strong>2010</strong> Edition” <strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong>Group and <strong>the</strong> <strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong>Association.264


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>3D analysis <strong>of</strong> induced micro-seismic event records compared withgeology and structure: Preliminary results <strong>of</strong> a Cooper Basin projectChloé Bonet 1,2 , Stewart Hore 1 , Desmond FitzGerald 1 , Michel Rosener 3 ,Helen J. Gibson 1 and David Jepsen 41 Intrepid Geophysics, Unit 2, 1 Male Street, Brighton, Victoria, 3186, Australia.2Institut de Physique du Globe de Paris <strong>of</strong> Earth's Geophysics, Paris, France.3Geodynamics Limited, Level 2, 23 Graham Street, Milton, Queensland, 4064, Australia.4Geoscience Australia, Cnr Jerrabomberra Avenue & Hindmarsh Drive, Symonston, ACT, 2609, Australia.* Corresponding author: chloe@intrepid-geophysics.comAbstractThe concept <strong>of</strong> an EGS geo<strong>the</strong>rmal prospect isbased on fracture network permeability enhancedby hydraulic stimulation. Characterisation <strong>of</strong>fracture/fault mechanisms and geometries are<strong>the</strong>refore an important part <strong>of</strong> prospectdevelopment.In this study, building a prospect-scale 3Dgeology and structure model <strong>of</strong> <strong>the</strong> Cooper Basingeo<strong>the</strong>rmal field has assisted prospect explorationand evaluation, but even greater advantage willcome from <strong>the</strong> ability to integrate (in <strong>the</strong> sameworkspace) information from induced seismicevents records such as location, magnitude,timing, focal mechanism, and shear planeorientation.Keywords: Induced seismicity, fracture/fault networks,clustering, focal mechanisms, 3D geology models.IntroductionThe Cooper Basin geo<strong>the</strong>rmal field is located near<strong>the</strong> common borders <strong>of</strong> Queensland and SouthAustralia. Since geo<strong>the</strong>rmal exploration began in2002, 4 wells have been drilled into <strong>the</strong> underlyinggranite, with final depths around 4300 metres. Of<strong>the</strong>se, <strong>the</strong> designated injection well, Habanero-1was hydraulically stimulated in 2003 and again in2005. Both stimulations induced detectable microseismicitycentred on TD <strong>of</strong> Habanero-1 (4421 m).Detailed studies by Geodynamics, GeoscienceAustralia, and Q-Con (Baisch et al, 2006)concluded that <strong>the</strong> hydraulic stimulationssuccessfully enhanced hydraulic permeabilitybetween <strong>the</strong> injection well (Habanero-1) and one<strong>of</strong> <strong>the</strong> production wells (Habanero-2). Comparedwith <strong>the</strong> earlier stimulations, those in 2005extended <strong>the</strong> previous stimulated reservoir, aswell as fur<strong>the</strong>r enhancing permeability.Beyond <strong>the</strong> goal <strong>of</strong> increased permeability,hydraulic stimulations also provide an opportunityto ga<strong>the</strong>r induced seismicity event records whichenable studies on: Fracture / fault mechanism and geometrycharacterization, andlikelihood <strong>of</strong> seismic risk to infrastructure fromgeo<strong>the</strong>rmal reservoir activities.Joint R&D project outlineSince March 1 st <strong>2010</strong>, Intrepid Geophysics andGeodynamics have been engaged in acollaborative project with <strong>the</strong> following goals:1. Develop a 3D micro-seismic time recordsviewer so that new knowledge about faultgeometries and fault mechanisms can evolve andbe integrated in <strong>the</strong> context <strong>of</strong> all availablegeology and geoscience observations.2. Investigate clustering or condensing <strong>of</strong> <strong>the</strong>event records in a manner that is coherent withgeological and geomechanical principals, with <strong>the</strong>aid <strong>of</strong> filtering capabilities.3. Characterize focal mechanisms in a suitableviewing format, e.g., triangular state diagram.4. Syn<strong>the</strong>size and integrate o<strong>the</strong>r disparateobservations <strong>of</strong> <strong>the</strong> geo<strong>the</strong>rmal field in a 3Dworkspace, such as: tectonic stress, well fracturerecords, and rock velocity data. The aim here is t<strong>of</strong>acilitate creation <strong>of</strong> workable 3D velocity models,and hence to improve <strong>the</strong> accuracy <strong>of</strong> locating <strong>the</strong>hypocenters <strong>of</strong> micro-seismic events.Induced Seismicity DatabaseThe primary database underpinning this project is<strong>the</strong> induced seismicity events records from <strong>the</strong>mid-September 2005 hydraulic re-stimulation <strong>of</strong>Habanero-1. Over a period <strong>of</strong> 13 days 22,500m 3<strong>of</strong> water was injected into 4421 m. (For details <strong>of</strong><strong>the</strong> injection flow rate and wellhead pressure, seeBaisch et al., 2009.)In April 2005 a continuous seismic monitoringsystem was installed at <strong>the</strong> Cooper Basingeo<strong>the</strong>rmal field, and this captured <strong>the</strong> events <strong>of</strong><strong>the</strong> September 2005 re-stimulation. The seismicstation network includes instruments at depthsvarying from surface, to shallow depths (80-370m)265


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>and one deep station at 1780m. (See Baisch 2009for details.)During <strong>the</strong> mid-September 2005 injection <strong>of</strong>Habanero-1, approximately 16,000 detectableseismic events were recorded. From this total, Q-Con determined absolute hypocentre locations for8886 events, that is, events for which at least fiveP-phase and three S-phase onsets could beidentified (Baisch et al. 2009).The data processed by Q-con (containinghypocenter locations, magnitudes and focalmechanism data for 8886 micro-seismic events)was selected for use in <strong>the</strong> joint R&D project,ahead <strong>of</strong> an alternative dataset available from aJapanese processing team.3D model <strong>of</strong> <strong>the</strong> Copper Basingeo<strong>the</strong>rmal fieldA preliminary 3D geology model <strong>of</strong> <strong>the</strong> CooperBasin geo<strong>the</strong>rmal field site has been constructedin 1 3D GeoModeller s<strong>of</strong>tware (e.g., see Calcagnoet al, 2008) using formation tops data from <strong>the</strong>three Habanero wells, and McLeod-1 drilled in1983 on a site approximately 440 m east-nor<strong>the</strong>ast<strong>of</strong> Habanero-1 (Table 1).WellsnamesLatitude Longitude Depths(m)DipDateFigure 1. Stratigraphic pile for <strong>the</strong> Cooper and EromangaBasins, within <strong>the</strong> geo<strong>the</strong>rmal field (excluding Cainozoic EyreFm), as used in <strong>the</strong> geology model shown in Figure 2, below.Habanero1Habanero227°48’57.0’’ 140°45’15.9’’ 4420.82 90° 14/10/0327°49’9.7’’ 140°45’4.9’’ 4357.73 90° 31/03/05Habanero327°48’43.3’’ 140°45’28.9’’ 4221.48 90° 05/02/08McLeod 1 27°48’53.2’’ 140°45’31.3’’ 3806.34 - 08/10/83Table 1. Location and description <strong>of</strong> <strong>the</strong> Habanero-1, -2, -3,and McLeod-1 wells.The geological model was also constrained byformation tops data derived from interpretedconventional seismic lines.The preliminary geological model has extents <strong>of</strong>10 x 10 x 6.5 km, and incorporates <strong>the</strong>stratigraphic successions <strong>of</strong> <strong>the</strong> Cooper andoverlying Eromanga Basin (Fig 1). The mainlyTriassic-aged basin fill, has an average beddingangle around horizontal, and top <strong>of</strong> <strong>the</strong> graniticbedrock lies between 3500 and 4200 m (Fig 2).Figure 2.Preliminary geologicalmodel for <strong>the</strong> CooperBasin geo<strong>the</strong>rmal field(view to <strong>the</strong> nor<strong>the</strong>ast).Exaggerated drill holeintersects arehighlighted forHabanero-1, -2 and -3,and for McLeod-1 (at<strong>the</strong> rear). Hypocentrelocations estimated byQ-Con for 8886 microseismiceventsinduced during <strong>the</strong>September 2005hydraulic simulation <strong>of</strong>Habanero-1 are shownby <strong>the</strong> cloud <strong>of</strong> whitesymbols.266


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Interpreted basement fault characterizationAs viewed in Figure 2, <strong>the</strong> hypocentre locationsestimated by Q-Con for 8886 micro-seismicevents induced during <strong>the</strong> September 2005hydraulic simulation <strong>of</strong> Habanero-1 are localisedin a zone approximately 3200 m x 1800 mhorizontally (long-axis oriented NNE) and within600 m vertically, centred on TD <strong>of</strong> Habanero-1(4421 m).Analysis <strong>of</strong> <strong>the</strong>se event locations by Q-Consuggests induced seismicity aligns along a single,reactivated sub-horizontal fracture system (Baischet al, 2009; Ro<strong>the</strong>rt & Baisch, <strong>2010</strong>). Indeed, abest-fit plane to <strong>the</strong> seismic cloud supports thisinterpretation.Pre-existence <strong>of</strong> this sub-horizontal fracture andit’s primary tectonic origin, is evidenced by loggingdata acquired before any reservoir tests began(D. Wyborn unpublished data, in: Baisch et al,2009).Viewing focal mechanism informationGoal number 3 <strong>of</strong> <strong>the</strong> joint R&D project beingundertaken by Geodynamics and IntrepidGeophysics is <strong>the</strong> ability to visualize focalmechanism information about faults at <strong>the</strong>hypocentres <strong>of</strong> induced seismicity. Plots createdon-<strong>the</strong>-fly from a whole or filtered database arerequired in order to differentiate discrete faults /fractures activated during hydraulic stimulation,and to determine <strong>the</strong>ir stress state, orientation,and slip direction, etc. This requires a preprocesseddataset to be loaded, and demandssophisticated plotting and visualization options.Plotting <strong>of</strong> triangular state diagrams is likely to beimplemented. These will allow groups <strong>of</strong> seismicevents representing similar focal mechanisms, tobe identified, and conclusions about <strong>the</strong> presence<strong>of</strong> single or multiple structures to be made. Foreach diagram, <strong>the</strong> 3 poles will represent an endmembersense <strong>of</strong> movement on a fault: normal,thrust, or strike-slip. Two complete triangular statediagrams are required: one each containingdextral strike-slip and sinistral strike-slip sense.Fracture orientations in <strong>the</strong> Cooper Basingeo<strong>the</strong>rmal fieldAs above, focal mechanism information for 8886micro-seismic events recorded during <strong>the</strong>September 2005 stimulation <strong>of</strong> Habanero-1 wasprocessed by Q-con, and provided for this R&Dproject by Geodynamics. From this information,we imported <strong>the</strong> fracture orientations <strong>of</strong> all seismicevents, noting (on a first-pass) <strong>the</strong> existence <strong>of</strong>two distinct populations <strong>of</strong> fracture orientations:a) 96% <strong>of</strong> fractures orientations are similarlyoriented, with a mean dip <strong>of</strong> 9° towards247° (pale blue discs in Fig 3)b) 3% <strong>of</strong> fractures orientations are similarlyoriented with a mean dip <strong>of</strong> 20° towards164° (red discs in Fig 3)c) 1% <strong>of</strong> fracture orientations are not definedas belonging to any population.Figure 3. Visualisation in 3D GeoModeller <strong>of</strong> fractureorientations <strong>of</strong> <strong>the</strong> seismic cloud captured during <strong>the</strong> 2005hydraulic stimulation <strong>of</strong> Habanero-1. One dominant and oneminor population constitute <strong>the</strong> dataset. (See text.)Figure 4 Enlargement <strong>of</strong> part <strong>of</strong> <strong>the</strong> seismic cloud from Fig 3,to highlight <strong>the</strong> variations in orientations.Compared with <strong>the</strong> simple analysis visualised inFigs 3 and 4, <strong>the</strong> ability to fur<strong>the</strong>r filter and sort<strong>the</strong> fracture orientation dataset is required, so thatindividual faults and fault-families can be tagged,assisting <strong>the</strong> interpreter to trial scenarios <strong>of</strong>possible fault network interpretations – whileworking with superimposed representations <strong>of</strong>prior knowledge <strong>of</strong> geology and structure, ando<strong>the</strong>r independent data.267


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Micro-seismic event magnitudeAdditionally, for <strong>the</strong> Cooper Basin geo<strong>the</strong>rmal fieldwe have facilitated visualization <strong>of</strong> variablemagnitudes <strong>of</strong> micro-seismic event records from<strong>the</strong> 2005 stimulation <strong>of</strong> Habanero-1 (Fig 5). Again<strong>the</strong>se data were made available through <strong>the</strong>processed dataset <strong>of</strong> Q-con which includes focalmechanism information.geological and geoscientific knowledge. In turn,improved knowledge on fault / fracture locations,orientations and connectivity will lead to a betterunderstanding <strong>of</strong> <strong>the</strong> overall behaviour <strong>of</strong> areservoir in terms <strong>of</strong> mechanics, and alsohydraulics.Acknowledgements1 3D GeoModeller is a commercial s<strong>of</strong>twaredeveloped by BRGM and Intrepid Geophysics.ReferencesBaisch S, Vörös R, Weidler R And Wyborn D(2009). Investigation <strong>of</strong> fault mechanisms duringgeo<strong>the</strong>rmal reservoir stimulation experiments in<strong>the</strong> cooper basin, Australia, Bulletin <strong>of</strong> <strong>the</strong>Seismological Society <strong>of</strong> America, 99, 148-158Baisch, S.; Weidler, R; Voros, R; Wyborn, D. Andde Graaf, L. (2006). Induced seismicity during <strong>the</strong>stimulation <strong>of</strong> a geo<strong>the</strong>rmal HFR reservoir in <strong>the</strong>Cooper Basin, Australia. Bulletin <strong>of</strong> <strong>the</strong>Seismological Society <strong>of</strong> America, 96, 2242-2256Calcagno, P., Chiles J., Courrioux, G. and Guillen,A. (2008) Geological modelling from field data andgeological knowledge. Phys. Earth Planet.Interiors, doi: 10.1016 / j.pepi.2008.06.013Ro<strong>the</strong>rt E And Baisch S (<strong>2010</strong>). Passive seismicmonitoring: Mapping enhanced permeability,Proceeding world geo<strong>the</strong>rmal congress <strong>2010</strong>.Figure 5. Oblique view to <strong>the</strong> nor<strong>the</strong>ast, through hypocentrelocations for micro-seismic events <strong>of</strong> <strong>the</strong> 2005 stimulation <strong>of</strong>Habanero-1, including enlarged well traces for Habanero-1(lower), Habanero-3 (middle) and McLeod-1 (upper). Thevariations <strong>of</strong> event magnitude range from +2.9 to -1.0(Moment Magnitude Scale), with highest magnitudes in red,mid-scale in yellow, and lowest in blue.Concluding NoteBeyond customised objectives and early accessto <strong>the</strong> project results for Geodynamics Ltd, a keyobjective <strong>of</strong> this joint R&D project is to develop amicro-seismic time records viewer capability in1 3D GeoModeller. As described above, <strong>the</strong> viewerwill also have <strong>the</strong> ability to filter and sort recordsbased on attributes such as timing, magnitudeand focal mechanism.These improvements will give reservoir engineersa tool to directly interpret <strong>the</strong> micro-seismic eventrecord against <strong>the</strong> background <strong>of</strong> <strong>the</strong> prior268


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Geo<strong>the</strong>rmal <strong>Energy</strong>'s Transition from Resource to Power: LegalChallengesAnna Collyer*, Nadia Harrison and Natasha McNamaraAllens Arthur Robinson.Level 27, 530 Collins Street, Melbourne, 3000.* Corresponding author: Anna.Collyer@aar.com.auGrowth and development in <strong>the</strong> geo<strong>the</strong>rmalenergy sector will require <strong>the</strong> industry tounderstand and comply with several forms <strong>of</strong>regulation. The geo<strong>the</strong>rmal energy sector hasmuch in common with mining <strong>of</strong> petroleum andminerals, and is regulated as such. However,because geo<strong>the</strong>rmal will ultimately serve as asource <strong>of</strong> electricity, it is equally important tounderstand <strong>the</strong> legal regime that governs <strong>the</strong>national electricity market and <strong>the</strong> sector's entryinto <strong>the</strong> electricity market. Differences in Stateand Territory regulation <strong>of</strong> geo<strong>the</strong>rmal projectsmean that <strong>the</strong> sector will have different obligationswith which to comply in different jurisdictions.Different approaches to allocating priority amongholders <strong>of</strong> overlapping tenements are taken under<strong>the</strong> various State and Territory regimes. Thegeo<strong>the</strong>rmal energy sector's engagement with <strong>the</strong>Scale Efficient Network Extension (SENE)framework and <strong>the</strong> National Electricity Marketestablished by <strong>the</strong> National Electricity Law will becrucial if it is to have a significant role in electricityproduction.Keywords: geo<strong>the</strong>rmal; regulation; overlappingtenements; National Electricity Market; ScaleEfficient Network ExtensionsRegulation <strong>of</strong> geo<strong>the</strong>rmal resourcesState and Territory Regulatory RegimesThe geo<strong>the</strong>rmal sector must come to terms with<strong>the</strong> different systems regulating geo<strong>the</strong>rmalprojects in each State and <strong>the</strong> Nor<strong>the</strong>rn Territory.Each legislative scheme imposes differentobligations, and <strong>the</strong> differing classifications <strong>of</strong>geo<strong>the</strong>rmal resources have implications that willaffect project development. In South Australiaand Western Australia, petroleum legislation wasamended so that it now regulates both petroleumand geo<strong>the</strong>rmal energy. In Queensland, Victoriaand <strong>the</strong> Nor<strong>the</strong>rn Territory, geo<strong>the</strong>rmal energy isregulated by a dedicated Act. In New SouthWales and Tasmania, a geo<strong>the</strong>rmal resource isdefined as a mineral and is regulated undermining legislation.In <strong>the</strong> <strong>Australian</strong> Geo<strong>the</strong>rmal IndustryDevelopment Framework, which was published by<strong>the</strong> Federal Department <strong>of</strong> Resources, <strong>Energy</strong>and Tourism in 2008, concern was expressed thatthat differences in legislative schemes have <strong>the</strong>potential to affect investment decision-making.Investment decisions may be influenced by <strong>the</strong>number <strong>of</strong> hurdles to exploration and exploitationa particular legislative scheme imposes and <strong>the</strong>degree <strong>of</strong> certainty it provides. Thus, decisionsthat should be based on <strong>the</strong> potential <strong>of</strong> <strong>the</strong>geo<strong>the</strong>rmal resource may be influenced bydifferences in regulation <strong>of</strong> <strong>the</strong> industry. One <strong>of</strong><strong>the</strong> objectives outlined in <strong>the</strong> framework is to'harmonise <strong>the</strong> framework governing <strong>the</strong> industryacross Australia.' Given <strong>the</strong> existence <strong>of</strong> sevendifferent schemes for <strong>the</strong> regulation <strong>of</strong> geo<strong>the</strong>rmalenergy, this objective will be difficult to achieve.The practical implications <strong>of</strong> <strong>the</strong> differinglegislative regimes must be understood. Twoexamples serve to illustrate this. First, in SouthAustralia activity may only be conducted if <strong>the</strong>region or land concerned is covered by aStatement <strong>of</strong> Environmental Objectives that hasbeen approved by <strong>the</strong> Minister. Geo<strong>the</strong>rmal andpetroleum activities are governed by <strong>the</strong> same Actin South Australia, so Statements <strong>of</strong>Environmental Objectives developed forpetroleum activities can be adopted forgeo<strong>the</strong>rmal operations.Second, native title negotiations must beapproached based on <strong>the</strong> different regulatorytreatment <strong>of</strong> geo<strong>the</strong>rmal energy in eachjurisdiction. In South Australia, <strong>the</strong> Governmenthas made a determination that geo<strong>the</strong>rmalactivities are not mining activities. This meansthat holders <strong>of</strong> South <strong>Australian</strong> geo<strong>the</strong>rmallicenses are not subject to <strong>the</strong> additional criteriaunder <strong>the</strong> right to negotiate process associatedwith holding mining leases. In Queensland andWestern Australia, holders <strong>of</strong> geo<strong>the</strong>rmaltenements are subject to <strong>the</strong> more stringent rightto negotiate procedure. In Victoria and <strong>the</strong>Nor<strong>the</strong>rn Territory, native title is dealt wi<strong>the</strong>xplicitly under geo<strong>the</strong>rmal legislation. In Victoria,native title holders must be compensated for anyloss or damage sustained in relation to <strong>the</strong>irinterests as a result <strong>of</strong> geo<strong>the</strong>rmal activity. In <strong>the</strong>Nor<strong>the</strong>rn Territory, <strong>the</strong> Minister must be satisfied<strong>the</strong> native title holder's consent has been obtainedand <strong>the</strong> federal Native Title Act proceduresfollowed before granting <strong>the</strong> geo<strong>the</strong>rmal authorityapplied for.Overlapping tenementsTenements granted for <strong>the</strong> purpose <strong>of</strong>development <strong>of</strong> geo<strong>the</strong>rmal resources mayoverlap with o<strong>the</strong>r mineral or petroleum269


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>tenements. For example, <strong>the</strong> Cooper Basin is <strong>the</strong>site <strong>of</strong> a geo<strong>the</strong>rmal resource and significant gasand oil reserves. The legislative regimes resolve<strong>the</strong> question <strong>of</strong> prioritisation <strong>of</strong> interests indifferent ways. The approach to overlappingtenements taken in each jurisdiction is linked toclassification <strong>of</strong> geo<strong>the</strong>rmal energy and <strong>the</strong> mode<strong>of</strong> regulation <strong>of</strong> geo<strong>the</strong>rmal energy adopted ineach state.In South Australia and Western Australia,geo<strong>the</strong>rmal tenements and petroleum tenementsmay subsist in <strong>the</strong> same area. Governed under<strong>the</strong> same legislation in <strong>the</strong>se states, geo<strong>the</strong>rmaland petroleum resources are treated equally.However, prior to <strong>the</strong> grant <strong>of</strong> <strong>the</strong> secondtenement (geo<strong>the</strong>rmal or petroleum), <strong>the</strong> Ministermust consult <strong>the</strong> existing tenement holder. Thus,in both <strong>of</strong> <strong>the</strong>se jurisdictions, <strong>the</strong> Minister has aresponsibility to hear and take into account <strong>the</strong>concerns <strong>of</strong> <strong>the</strong> existing tenement holder.In Queensland, a more prescriptive approach istaken. Geo<strong>the</strong>rmal exploration cannot beundertaken to <strong>the</strong> extent that it adversely affectsactivity under a mineral or petroleum tenementthat has already started. Conversely, activity ontenements granted under <strong>the</strong> mineral andpetroleum legislation cannot be undertaken to <strong>the</strong>extent that it adversely affects activity under ageo<strong>the</strong>rmal tenement that is already underdevelopment. This approach clearly gives priorityto <strong>the</strong> holder <strong>of</strong> <strong>the</strong> tenement that was obtainedfirst, whereas in Western Australia and SouthAustralia <strong>the</strong> existing tenement holder need onlybe consulted before <strong>the</strong> Minister grants <strong>the</strong>second interest. Although one <strong>of</strong> <strong>the</strong> purposes <strong>of</strong><strong>the</strong> Queensland Act is to facilitate consultationwith and compensation for persons adverselyaffected by geo<strong>the</strong>rmal exploration, <strong>the</strong> Actprovides no guidance as to how to determinewhe<strong>the</strong>r a project is 'adversely affected' by ageo<strong>the</strong>rmal project. The Queensland legislationdictates that a project that is first in time andadversely affected by a second proposed activityon <strong>the</strong> same land has priority. However, discretionin relation to what constitutes an 'adverse effect'remains. The question <strong>of</strong> whe<strong>the</strong>r <strong>the</strong> first activitywill be 'adversely affected' by <strong>the</strong> second is amatter that will require resolution in each case <strong>of</strong>overlapping tenements.In New South Wales and Tasmania, geo<strong>the</strong>rmalresources have <strong>the</strong> same status as o<strong>the</strong>rminerals. In New South Wales, an overlappingtenement may not be granted without <strong>the</strong> consent<strong>of</strong> <strong>the</strong> existing tenement holder. As in SouthAustralia and Western Australia, <strong>the</strong> Minister hasa role to play: disputes between <strong>the</strong> overlappingtenement holders are referred to <strong>the</strong> Minister fordetermination. In Tasmania, an explorationlicense or mining lease cannot be granted overland that is already <strong>the</strong> subject <strong>of</strong> a tenement.Because geo<strong>the</strong>rmal resources are notdistinguished from o<strong>the</strong>r minerals in <strong>the</strong>se states,<strong>the</strong> approach taken to overlapping tenements ismore rigid.The Victorian Act is silent on <strong>the</strong> question <strong>of</strong>overlapping tenements. However, <strong>the</strong> OperationPlan that is submitted to <strong>the</strong> Minister prior to <strong>the</strong>carrying out <strong>of</strong> <strong>the</strong> geo<strong>the</strong>rmal operation mustdetail <strong>the</strong> risk <strong>of</strong> injury to land users in <strong>the</strong> vicinity<strong>of</strong> <strong>the</strong> operation.As well as describing <strong>the</strong>se differing regulatoryregimes in <strong>the</strong> abstract, analysis <strong>of</strong> <strong>the</strong>practicalities associated with attempts to complywith <strong>the</strong>m will also be provided.In <strong>the</strong> Nor<strong>the</strong>rn Territory, <strong>the</strong> holder <strong>of</strong> ageo<strong>the</strong>rmal tenement must consult <strong>the</strong> holder <strong>of</strong>an existing mining right or petroleum interestabout <strong>the</strong> proposed geo<strong>the</strong>rmal activities. Unlike<strong>the</strong> Queensland legislation, <strong>the</strong> Nor<strong>the</strong>rnTerritory's Geo<strong>the</strong>rmal <strong>Energy</strong> Act does notprovide that holders <strong>of</strong> mining rights andpetroleum interests must consult with holders <strong>of</strong>existing geo<strong>the</strong>rmal tenements. Unlike <strong>the</strong> South<strong>Australian</strong> and Western <strong>Australian</strong> requirementthat existing tenement holders be consulted priorto <strong>the</strong> grant <strong>of</strong> an overlapping tenement,geo<strong>the</strong>rmal tenement holders need only consult<strong>the</strong> holder <strong>of</strong> an existing right or petroleuminterest before conducting geo<strong>the</strong>rmal activities.The resolution <strong>of</strong> issues associated withoverlapping tenements <strong>of</strong>ten rely on <strong>the</strong> exercise<strong>of</strong> Ministerial jurisdiction, ei<strong>the</strong>r at <strong>the</strong> time when<strong>the</strong> tenement is granted, or in <strong>the</strong> event <strong>of</strong> adispute. The exercise <strong>of</strong> Ministerial discretionmay be influenced by political considerations.Holders <strong>of</strong> overlapping tenements may benefitfrom using contract to overcome uncertainty as tohow <strong>the</strong>ir interests will be prioritised. Ano<strong>the</strong>rsituation in which contractual negotiation andagreement may also benefit <strong>the</strong> development <strong>of</strong><strong>the</strong> project is where tenements over a singlegeo<strong>the</strong>rmal resource are granted to differentparties. In some jurisdictions, cooperation can bemandated. In Western Australia, license holderscan be required to enter into an agreement if <strong>the</strong>Minister is <strong>of</strong> <strong>the</strong> view that unit development <strong>of</strong> <strong>the</strong>geo<strong>the</strong>rmal resources area would secure moreeffective recovery <strong>of</strong> geo<strong>the</strong>rmal energy. Similarlyin Victoria, <strong>the</strong> Minister may require holders <strong>of</strong>extraction licences that cover adjacent areas toenter into cooperative agreements for <strong>the</strong>extraction <strong>of</strong> geo<strong>the</strong>rmal energy. Fur<strong>the</strong>r insightswill be provided into how contracts are likely tooperate as a practical tool. Our analysis will drawfrom contexts which share importantcharacteristics with <strong>the</strong> geo<strong>the</strong>rmal energy sector,including experiences <strong>of</strong> <strong>the</strong> wind power sector.Regulation <strong>of</strong> geo<strong>the</strong>rmal energyWhile geo<strong>the</strong>rmal remains a young andunderdeveloped industry in Australia, <strong>the</strong>re will be270


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>a tendency for industry participants to focus onregulatory systems governing preliminary issuessuch as exploration, prospecting and valuation.As geo<strong>the</strong>rmal resources are developed tobecome sources <strong>of</strong> power, parties with an interestin geo<strong>the</strong>rmal projects will need to becomefamiliar with <strong>the</strong> requirements and peculiarities <strong>of</strong><strong>the</strong> National Electricity Market (NEM) and <strong>the</strong>rules which apply to it.The NEM: an overviewAn outline <strong>of</strong> how <strong>the</strong> NEM operates and some <strong>of</strong><strong>the</strong> key principles underpinning <strong>the</strong> NationalElectricity Law and <strong>the</strong> NEM will be provided.This will be distinguished from <strong>the</strong> system whichoperates in <strong>the</strong> Nor<strong>the</strong>rn Territory and WesternAustralia. A brief description <strong>of</strong> <strong>the</strong> rules andstandards likely to be particularly important forgeo<strong>the</strong>rmal projects will also be provided.Entry into <strong>the</strong> NEM and ContractingElectricity prices in respect <strong>of</strong> base load powerare determined according to bids placed bygenerators at five minute intervals. In thiscompetitive environment, <strong>the</strong> capacity to sellelectricity at a specified price cannot be taken forgranted.ContractingThe production <strong>of</strong> geo<strong>the</strong>rmal energy requiressignificant capital investment when compared witho<strong>the</strong>r electricity generation methods. TheMassachusetts Institute <strong>of</strong> Technology citesCalifornian research indicating that capitalreimbursement and interest charges account for65% <strong>of</strong> <strong>the</strong> total cost <strong>of</strong> geo<strong>the</strong>rmal power. Thiscan be compared to combined-cycle natural gasplants for example, for which equivalent costsaccount for approximately 22%. In each case <strong>the</strong>remaining costs cover items including fuel (egwater), labour and access charges.There will <strong>the</strong>refore be an understandable desireamong industry participants to obtain somesecurity regarding electricity sales and prices.Generators may seek to negotiate longer termunderlying contracts to give <strong>the</strong>mselves, <strong>the</strong>irfinanciers and <strong>the</strong>ir investors certainty. Suchcontracts are commonly relied upon within <strong>the</strong>current market. The NEM structure means thatderivatives are <strong>of</strong>ten used for this purpose,although a PPA may also be appropriate incertain circumstances.As RECs will support <strong>the</strong> economic viability <strong>of</strong>geo<strong>the</strong>rmal projects under <strong>the</strong> Renewable <strong>Energy</strong>(Electricity) Act 2000 (Cth), it is likely thatproponents will sell a bundled product comprisingelectricity ('black') and RECs ('green').An outline <strong>of</strong> <strong>the</strong> operation <strong>of</strong> such contractswithin <strong>the</strong> electricity market currently, includingsome practical tips on contract drafting,negotiation and key risks will be provided.Scale Efficient Network Extensions(SENE)In order to promote development <strong>of</strong> <strong>the</strong>infrastructure needed to transfer electricity from(<strong>of</strong>ten remote) energy generation sites to <strong>the</strong>electricity grid, <strong>the</strong> <strong>Australian</strong> <strong>Energy</strong> MarketCommission has drafted proposed amendmentsto <strong>the</strong> National Electricity Rules which wouldfacilitate <strong>the</strong> construction <strong>of</strong> SENEs between newelectricity generators and existing infrastructure.While <strong>the</strong> extensions will be available to varioustypes <strong>of</strong> energy producers, <strong>the</strong>y are likely to beparticularly important for <strong>the</strong> renewable energysector.According to <strong>the</strong> current proposal, SENEs wouldbe developed by Network Service Providers withGenerators paying for <strong>the</strong> right to transmit energythrough an SENE and <strong>the</strong> cost <strong>of</strong> any shortfallbeing passed through to customers. Customershere are those registered with AEMO ascustomers and <strong>the</strong>refore would include retailersra<strong>the</strong>r than end use customers. Customers arehowever expected to benefit from <strong>the</strong> prevention<strong>of</strong> costly duplication which could result ifcompanies were left to each construct <strong>the</strong>ir owninfrastructure in order to connect to <strong>the</strong> network.Outlined below is a sample <strong>of</strong> some <strong>of</strong> <strong>the</strong> issuesraised by <strong>the</strong> draft amendment which are likely topresent challenges.CapacityThe fact that geo<strong>the</strong>rmal sites in any particularregion are likely to develop in a staggered mannermakes <strong>the</strong> determination <strong>of</strong> suitable capacity forSENEs particularly difficult. Clearly, <strong>the</strong>re shouldbe enough to enable geo<strong>the</strong>rmal and o<strong>the</strong>rgenerators to transmit electricity to <strong>the</strong> market. At<strong>the</strong> same time, a potential over-sizing or 'assetstranding' would be paid for by electricitycustomers and would likely be passed through to<strong>the</strong>ir end-use consumers in <strong>the</strong> form <strong>of</strong> higherelectricity costs.As <strong>the</strong> Network Service Providers responsible fordeveloping SENEs will be able to recover <strong>the</strong>ircosts entirely from generators and customers, <strong>the</strong>AEMC notes that <strong>the</strong> incentives may favour oversizing(and excessive capacity) ra<strong>the</strong>r than undersizing(and inadequate capacity).Notwithstanding, geo<strong>the</strong>rmal industry participantsconsidering investing in reliance on transmissionservices <strong>of</strong>fered through an SENE should notconsider this to constitute a capacity guarantee.The draft rules prescribe that <strong>the</strong> AER maydisallow proposed SENE projects. Moreover, aNetwork Service Provider will only be required tocommence <strong>the</strong> SENE planning procedure if <strong>the</strong>reis a reasonable likelihood <strong>of</strong> o<strong>the</strong>r generators271


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>connecting to <strong>the</strong> proposed SENE and itsdevelopment is likely to <strong>of</strong>fer material scaleefficiencies. In <strong>the</strong> event that <strong>the</strong>re is inadequatecapacity, <strong>the</strong> draft rule provides that <strong>the</strong> generatorwhose requirements cannot be met is required t<strong>of</strong>und an augmentation to <strong>the</strong> SENE. If <strong>the</strong>generator does not agree to fund such anaugmentation and its generation (in excess <strong>of</strong> itsagreed power transfer capability) has 'constrained<strong>of</strong>f' ano<strong>the</strong>r generator connected to <strong>the</strong> SENE, <strong>the</strong>fist generator will be required to pay <strong>the</strong> o<strong>the</strong>rcompensation. Importantly, compensation iscalculated with reference to a formula which willnot necessarily result in recovery <strong>of</strong> <strong>the</strong> 'trueeconomic cost <strong>of</strong> connection'.Relationship with shared networkDepending on <strong>the</strong> way in which <strong>the</strong> SENEinfrastructure develops, its interaction with <strong>the</strong>shared network could present challenges. Where<strong>the</strong> SENE generates benefits and/or costs forusers <strong>of</strong> <strong>the</strong> shared network, <strong>the</strong>re is limitedallowance in <strong>the</strong> rules for <strong>the</strong>ir allocation. Theremay also be practical difficulties associated with<strong>the</strong> fact that <strong>the</strong> shared network operates throughan open access system whereas after <strong>the</strong>introduction <strong>of</strong> <strong>the</strong> SENE, generators will beallocated a specific agreed power transfercapability.Infrastructure development efficiencyThe Clean <strong>Energy</strong> Council has noted that <strong>the</strong>Network System Operators responsible fordeveloping SENEs have few incentives to avoidcost blow outs.ReferencesApproval Process for EGS Projects (includingInduced Seismicity), Workshop on Geo<strong>the</strong>rmalReservoir Engineering, 35 th , Stanford University,Abstract.Gove-White, G., and Frederiks, P., June <strong>2010</strong>,Geodynamics - The Opportunity.Hedge, J., 2006, Recent Developments:Geo<strong>the</strong>rmal <strong>Energy</strong> Heating Up, AMPLA Limited13 th Annual <strong>Conference</strong>, Melbourne.Lund, J. W., 2007, Characteristics, Developmentand Utilization <strong>of</strong> Geo<strong>the</strong>rmal Resources, p. 1-3,7-9.Massachusetts Institute <strong>of</strong> Technology, 2006,The Future <strong>of</strong> Geo<strong>the</strong>rmal <strong>Energy</strong>: Impact <strong>of</strong>Enhanced Geo<strong>the</strong>rmal Systems (EGS) on <strong>the</strong>United States in <strong>the</strong> 21st Century, Ch. 8-9.Steol Rives LLP Attorneys at Law,McKinsey, J.A., 2009, The Law <strong>of</strong> Lava, p. 10-17.Mineral Resources Development Act 1995 (Tas).Mining Act 1992 (NSW).Mining Regulation 2003 (NSW).Native Title Act 1993 (Cth).Petroleum and Geo<strong>the</strong>rmal <strong>Energy</strong> Act 2000 (SA).Petroleum and Geo<strong>the</strong>rmal <strong>Energy</strong> Resources Act1967 (WA).Geo<strong>the</strong>rmal Exploration Act 2004 (Qld).The authors have also relied on various internalresearch resources owned by Allens ArthurRobinson.<strong>Australian</strong> <strong>Energy</strong> Market Commission, <strong>2010</strong>,Consultation Paper National ElectricityAmendment (Scale Efficient Network Extensions)Rule <strong>2010</strong>.<strong>Australian</strong> <strong>Energy</strong> Market Operator, <strong>2010</strong>,AEMO's Submission to <strong>the</strong> AEMC's ConsultationPaper on Scale Efficient Network Extensions, Ch.1, 6, 7, 9, 10.Bartlett, R. H., Native Title in Australia, 2004.Blodgett, L., Holm, A., Jennejohn, D. and Gawell,K., May <strong>2010</strong>, Geo<strong>the</strong>rmal <strong>Energy</strong>: InternationalMarket Update, p. 4-10, 51-52.Department <strong>of</strong> Resources, <strong>Energy</strong> and Tourism,2008, <strong>Australian</strong> Geo<strong>the</strong>rmal IndustryDevelopment Framework.Geo<strong>the</strong>rmal <strong>Energy</strong> Resources Act 2005 (Vic).Geo<strong>the</strong>rmal Exploration Act 2004 (NT).Goldstein, B., Malavazos, M., Long, A., Bendall,B., Hill, T., and Alexander, E., <strong>2010</strong>, TheRegulator's Perspective – Best Practice Activity272


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Trusted Regulation for Geo<strong>the</strong>rmal Resource Development (IncludingInduced Seismicity Associated with EGS Operations)Barry Goldstein, Betina Bendall, Alexandra Long, Michael Malavazos, David Cockshell and David LovePrimary Industries & Resources South Australia (PIRSA), GPO Box 1671, Adelaide, South Australia, 5001AbstractOperations need be managed to reduce materialrisks to acceptable levels and as low asreasonably practical to meet communityexpectations. Public trust in both industry andregulators to deliver safe outcomes fostersinvestment and enables efficient land access andactivity approvals. These principles and practicesare especially important for EngineeredGeo<strong>the</strong>rmal System development which maypose uncertain risks from induced seismicityThe objective based, one-stop-shop, regulatoryframework in South Australia (Petroleum andGeo<strong>the</strong>rmal <strong>Energy</strong> Act 2000) and <strong>the</strong> behaviour<strong>of</strong> <strong>the</strong> regulator, Primary Industries andResources – South Australia (PIRSA) arerecognized as “a relatively straightforwardregulatory system, which could be considered abenchmark for o<strong>the</strong>r jurisdictions” (<strong>Australian</strong>Productivity Commission, 2009).The regulatory instruments that deliver trust andefficiency in South Australia are: non-prescriptive;allow for innovation while ensuring that operatorsdemonstrate <strong>the</strong>ir ability to manage all possiblerisks to an acceptable level; and entail extensivestakeholder consultation to set standards whichare aligned with community expectations.Operations in South Australia includeinternationally significant Enhanced Geo<strong>the</strong>rmalSystems (EGS) developments. Recognizing EGSis (at least to <strong>the</strong> public) a new technology withuncertain risks, PIRSA has taken account <strong>of</strong>international developments, commissionedresearch and is supporting national cooperation toincrease certainty in relation to risk managementfor EGS operations.This paper describes practices and technologiesthat can help to inform activity approvals for EGSoperations anywhere.Efficient Co-regulation through Statements<strong>of</strong> Environmental Objectives (SEOs) andEnvironmental Impact Reports (EIRs)The South <strong>Australian</strong> geo<strong>the</strong>rmal licenses shownin figure 1 are governed by <strong>the</strong> Petroleum andGeo<strong>the</strong>rmal <strong>Energy</strong> Act 2000 (P&GE Act).In <strong>the</strong> context <strong>of</strong> <strong>the</strong> P&GE Act, <strong>the</strong> legalstandards set for <strong>the</strong> protection <strong>of</strong> natural, social,heritage and economic environments are agreedthrough a robust, open and transparent researchand consultation process that culminates in P&GEAct license operators owning and abiding bySEOs and associated EIRs (Laws, et al, 2002).EIRs detail potential impacts <strong>of</strong> proposedoperations and specify strategies to mitigate risksto as low as reasonably practical (ALARP).SEOs set standards for area and operationspecific compliance with co-regulatory objectivesfor <strong>the</strong> sustainability <strong>of</strong> natural, social, heritageand economic environments. Hence, SEOsenable PIRSA to act as a first-line, one-stop-shopfor co-regulation for <strong>the</strong> full-cycle <strong>of</strong> geo<strong>the</strong>rmal,upstream petroleum, high pressure pipelines andgas storage operations in <strong>the</strong> State <strong>of</strong> SouthAustralia.Figure 1: Figure 1.Geo<strong>the</strong>rmal licenses in South Australia and <strong>the</strong> South<strong>Australian</strong> Heat Flow Anomaly (adapted from Neumann, et al 2000)Trust Underpins Efficient Co-regulationEmbedding relevant local, State and Federalobjectives and standards into SEOs make abreach <strong>of</strong> co-regulatory standards a breach <strong>of</strong> <strong>the</strong>P&GE Act.Stakeholders are engaged during <strong>the</strong>development <strong>of</strong> EIRs and draft SEOs and usuallyin a staged process that entails face-to-facemeetings. The process for SEO consultation withstakeholders can take 3 months or moredepending on <strong>the</strong> level <strong>of</strong> impact <strong>of</strong> <strong>the</strong> activity,and stakeholder consultation requirements. Givenpotential for relatively low environmental impactsand sufficient prior publicly developed anddisclosed criteria, <strong>the</strong> Minister (who is an electedParliamentarian) may agree public consultationmay be restricted to a time after a relevant SEO isfully developed for consideration. Publicconsultation is undertaken for <strong>the</strong> development <strong>of</strong>o<strong>the</strong>r EIRs and draft SEOs.273


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Final SEOs, final EIRs and annual statements <strong>of</strong>licensees’ performance against SEOs and <strong>the</strong>Minister's determinations <strong>of</strong> <strong>the</strong> level <strong>of</strong>environmental impact <strong>of</strong> proposals are freelyavailable to <strong>the</strong> public on PIRSA’s website. PIRSAalso proactively participates in public forums toenable well-informed consideration <strong>of</strong> riskmanagement strategies put in place to protectnatural, social and economic environments.This openness and transparency underpins trustin PIRSA’s roles as first-line regulator for: <strong>the</strong>integrity <strong>of</strong> plant and equipment; <strong>the</strong> protection <strong>of</strong>:water; air; flora; fauna; landscape; heritage; native(aboriginal) title; and as an interlocutor fordisputes between P&GE Act licensees andstakeholders in multiple land use. In addition to<strong>the</strong> first-line roles listed above, PIRSA also worksclosely with South Australia’s lead agency for <strong>the</strong>regulation <strong>of</strong> occupational health, safety andwelfare (SafeWorkSA) matters.Formal agreements and policies explicate mutualexpectations and underpin both <strong>the</strong> efficiency andeffectiveness <strong>of</strong> co-regulation. Hence, licenseeshave a one-stop-shop for regulation.Australia’s Productivity Commission (2009) reviewconcludes that PIRSA “has a clear mandate, clearregulatory responsibilities, good processes toengage with o<strong>the</strong>r agencies, and checks andbalances that apply in high risk situations” and “iswidely seen as a model for o<strong>the</strong>r jurisdictions toemulate”.Geo<strong>the</strong>rmal SEOs and EIRsThe P&GE Act requires that any activity can onlybe conducted if it is covered by an approved SEOfor <strong>the</strong> region and/or land system within which itwill be carried out. Hence, geo<strong>the</strong>rmal operatorsmust develop appropriate EIRs and SEOs orconclude a bridging assessment to make plain <strong>the</strong>practicality <strong>of</strong> adopting and <strong>the</strong>n abiding by preexistingSEOs for analogous operations inanalogous areas. When adopting pre-existingSEOs, <strong>the</strong> bridging assessment must satisfyrelevant co-regulators that location-specific risksare adequately covered in adopted SEOs. Iflocation-specific risks are not already adequatelycovered, <strong>the</strong>n a new relevant SEO is drafted by<strong>the</strong> operator for stakeholder consultation. In someinstances, SEOs developed for petroleum licenseactivities are adopted for analogous geo<strong>the</strong>rmaloperations.EIRs underpin <strong>the</strong> relevance and contents <strong>of</strong>SEOs. All licensed field activities must be coveredby an SEO approved by relevant Minister(s).When considering EIRs, PIRSA makes adetermination whe<strong>the</strong>r proposed activities shouldbe characterized as low-, medium or high-levelenvironmental impact. For activities characterizedas:• Low-impact – PIRSA consults with relevant coregulatorygovernment agencies.• Medium impact – PIRSA undertakes publicconsultation with support from <strong>the</strong> operator;and• High impact – an Environmental ImpactStatement process is instigated under SouthAustralia’s Development Act 1993.In this way – final SEOs cover all materialconcerns raised by stakeholders.Licensees are required to report annually and byexception on <strong>the</strong>ir performance against SEOs.Five-yearly reviews consider <strong>the</strong> efficacy <strong>of</strong> SEOsand, following <strong>the</strong> principle <strong>of</strong> transparency, <strong>the</strong>sereports are available to <strong>the</strong> public from PIRSA’swebsite.Table 1 provides examples <strong>of</strong> EIRs and SEOsthat illuminate potential risks, strategies tomitigate risks to as low as reasonably practicaland standards for outcomes for geophysicalsurvey and well operations (including drilling)used to date for deep geo<strong>the</strong>rmal well operations.Table 1. Examples <strong>of</strong> EnvironmentalImpact Reports and Statements <strong>of</strong>Environmental Objectives (SEOs)Geophysical Surveys State-wide EIR for non-seismic geophysical surveyswww.pir.sa.gov.au/__data/assets/pdf_file/0003/50844/EIR_GeoOps_NonSeis.pdf State-wide SEO for non-seismic geophysical surveyswww.pir.sa.gov.au/__data/assets/pdf_file/0004/50845/SEO_GeoOps_NonSeis.pdf Cooper Basin EIR for geophysical operationswww.pir.sa.gov.au/__data/assets/pdf_file/0011/27398/cooper_basin_geophysical_operations_eir.pdf Cooper Basin SEO for geophysical operationswww.pir.sa.gov.au/__data/assets/pdf_file/0010/27397/cooper_basin_geophysical_operations_seo.pdfDrilling and Well OperationsCooper Basin EIR for drilling and well operationswww.pir.sa.gov.au/__data/assets/pdf_file/0004/27409/drilling_and_well_operations_eir_february_2003.pdf5-Year Review <strong>of</strong> Operations, Addendum to CooperBasin EIR for drilling and well operationswww.pir.sa.gov.au/__data/assets/pdf_file/0009/123030/Santos_-_Drilling__and__Well_Ops_EIR_Addendum_-_November_2009_Final.pdfCooper Basin SEO for drilling and well operationswww.pir.sa.gov.au/__data/assets/pdf_file/0010/123031/Santos_-_Drilling_and_Well_Operations_SEO_-_November_2009_Final.pdfHabanero Well Operations EIRwww.pir.sa.gov.au/__data/assets/pdf_file/0018/27441/habanero1_eir_sept2002.pdfHabanero EIR and SEO for circulationwww.pir.sa.gov.au/__data/assets/pdf_file/0007/27439/habanero_circulation_eir_seo_oct2004.pdfJacaranda Ridge 2 EIRwww.pir.sa.gov.au/__data/assets/pdf_file/0010/52588/Adelaide_<strong>Energy</strong>_PEL_255_Region_EIR.pdfJacaranda Ridge 2 SEOwww.pir.sa.gov.au/__data/assets/pdf_file/0010/52597/Final_Adelaide_<strong>Energy</strong>_PEL_255_SEO.pdfGeodynamics demonstrated <strong>the</strong> existing CooperBasin SEO for drilling and well operations wasrelevant, and adopted that SEO for its operationsin <strong>the</strong> Habanero, Jolokia and Savina wells.Petra<strong>the</strong>rm also adopted <strong>the</strong> Cooper Basin SEOfor its Paralana 2 drilling and well operations.Panax Geo<strong>the</strong>rmal has adopted <strong>the</strong> Otway Basin(Jacaranda Ridge) SEO for its Salamander 1drilling and well operations.Responsible Operator’s Needto Know Best (Practice)274


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>P&GE Act’s non-prescriptive requirements for riskmanagement enable experienced geo<strong>the</strong>rmaloperators to easily deploy <strong>the</strong>ir existing corporategovernance standards for risk management foruse in South Australia. New entrants togeo<strong>the</strong>rmal operations do sometimes express asense <strong>of</strong> uncertainty while documenting <strong>the</strong>ir ownstandard operating (including risk management)procedures. This uncertainty leads some relativelynew entrants to ask to be told how to operate, asa perceived easier path to attaining competencein managing operational risks. In such cases,PIRSA willingly (and <strong>of</strong>ten does) ‘hold-<strong>the</strong>-hand’<strong>of</strong> new entrant operators ascending learningcurves that result in licence-holders adopting ordeveloping <strong>the</strong>ir own activity- and area-specificSEOs and EIRs. Operator ownership <strong>of</strong> activityoutcomes (and potential liabilities) also satisfies<strong>the</strong> government’s policy objective that <strong>the</strong> public isprotected from insufficiently managed risks.Additionally, South Australia’s non-prescriptiveapproach allows operators to innovate andmanage risks so efficiently as practical to attainstandards set for outcomes. Sustainableoperations and benign outcomes elicit communitytrust in both <strong>the</strong> regulator and industry. This is avirtuous cycle.Activity ApprovalsLocal issues for particular field operations areaddressed case-by-case during activity approvalprocesses. In <strong>the</strong> activity approval process,PIRSA reviews: operator capabilities; fitness-forpurpose<strong>of</strong> plant and equipment; riskassessments concluded by licensees; and sitespecific environmental impacts. License operatorswho have demonstrated capabilities thatconsistently achieve regulatory compliancerequire low-level surveillance and only need tonotify <strong>the</strong> regulator <strong>of</strong> activities, ra<strong>the</strong>r thanseeking case-by-case activity approval.Advance Notice <strong>of</strong> EntryLicense operators must provide 21 days notice inwriting to users <strong>of</strong> <strong>the</strong> land that may be affectedby specific regulated activities to relevantstakeholders, including PIRSA. Land users have14 days to raise access-related concerns with <strong>the</strong>license operator and have <strong>the</strong> option <strong>of</strong> raising <strong>the</strong>concern directly with <strong>the</strong> regulator, and <strong>the</strong> finaldispute resolution is a Warden’s Courtproceeding.Induced Micro-seismicityThe most advanced engineered geo<strong>the</strong>rmalsystem (EGS) projects in Australia are remotefrom population centers, so experience inAustralia will be gained while potential risks <strong>of</strong>induced micro-seismicity are effectively managed.This experience will be <strong>of</strong> great value in showing<strong>the</strong> extent and magnitude <strong>of</strong> induced microseismicity,<strong>the</strong> reliability <strong>of</strong> pre-stimulationforecasts, and providing a logical basis forpredicting safe distances from fracture stimulationoperations in built-up areas.Regulatory Research for EGS OperationsMany <strong>of</strong> <strong>the</strong> geo<strong>the</strong>rmal resources in SouthAustralia are expected to be hydraulically fracturestimulatedto achieve optimum (high) rates <strong>of</strong> heatflow from well-bores. Fracture stimulation <strong>of</strong>reservoirs inevitably induces seismic events <strong>of</strong>some measurable magnitude. Proper planningand management <strong>of</strong> EGS operations can ensurethat risks to people, buildings and infrastructureare reduced to as low as reasonably practical andacceptable levels.To inform regulation, mitigate potential risks andaddress concerns raised by stakeholders, in2005, PIRSA contracted University <strong>of</strong> Adelaideresearchers to address a critical uncertaintyshared by all geo<strong>the</strong>rmal licensees planning todemonstrate EGS in South Australia. Thatresearch (Hunt and Morelli, 2006) assessedinduced seismicity within <strong>the</strong> context <strong>of</strong> localgeologic conditions in <strong>the</strong> Innamincka area <strong>of</strong> <strong>the</strong>Cooper Basin, and concluded:• Granite basement in <strong>the</strong> Cooper Basin inSouth Australia is ideally suited to EGSactivities in terms <strong>of</strong> its compressive stressregime (prone to sub-horizontal fracturepropagation), low levels <strong>of</strong> natural backgroundseismicity and <strong>the</strong> availability <strong>of</strong> extensive highquality reflection seismic to illuminate faultsand fracture trends;• Reactivation <strong>of</strong> faults in <strong>the</strong> vicinity <strong>of</strong> <strong>the</strong>Habanero site is unlikely. This is due to <strong>the</strong>nearby faults being beyond <strong>the</strong> reach <strong>of</strong> <strong>the</strong>induced seismicity associated with EGSactivity.• Induced seismic events at <strong>the</strong> Habanero wellsite in <strong>the</strong> Cooper Basin could reasonably beexpected to fall below a ground acceleration <strong>of</strong>0.05 g, which is a safe level for <strong>the</strong> Habanerolocation and its surrounds.These findings informed <strong>the</strong> regulator andstakeholders that <strong>the</strong> fracture stimulation <strong>of</strong>geo<strong>the</strong>rmal wells in <strong>the</strong> Innamincka area <strong>of</strong> <strong>the</strong>Cooper Basin could be safely managed so thatmicro-seismic events induced during <strong>the</strong> fracturestimulation:• would be well below potentially damaginglevels;• were unlikely to induce slip and consequent,larger seismic events on larger geologicalfaults; and• were unlikely to create hydrauliccommunication between <strong>the</strong> stimulated granite(basement) zones below 4,000 metres and <strong>the</strong>overlying sedimentary Cooper Basin above3,700 metres.This last finding is based on:• <strong>the</strong> prevailing, natural, highly compressivestress regime acting to constrain fracturepropagation to sub-horizontal intervals;• acceleration attenuation is at least one order <strong>of</strong>magnitude greater in s<strong>of</strong>t rocks and soils thanin crystalline rocks; and• high frequency motion is attenuated morequickly with distance than low frequency275


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>motion and <strong>the</strong> seismic events induced duringfracture stimulation and pumping into HotFractured Rocks (HFR) are characteristicallyhigh frequency (100–500 Hz).Indeed, fracture stimulation and injectionprograms in Geodynamics’ Cooper BasinHabanero wells were both conducted safely andwere successful in <strong>the</strong> enhancement and flowtesting <strong>of</strong> EGS reservoirs.Risk Management for Induced SeismicityGiven <strong>the</strong> results in <strong>the</strong> Cooper Basin, and lookingforward to many additional EGS projects inAustralia (and South Australia, in particular),PIRSA commissioned <strong>the</strong> development <strong>of</strong> riskmanagement protocols for induced seismicityassociated with EGS reservoir development in2007. The findings (Morelli and Malavazos 2008)are fully consistent with <strong>the</strong> findings <strong>of</strong> Majer,Baria and Stark (2008) and are summarized inTable 2.Running Ahead <strong>of</strong> <strong>the</strong> Frac CrewAn informed risk assessment for EGS operationsstarts with an analysis <strong>of</strong>:• historical (monitored) earth movementsmagnitude and location; and• geophysical survey data to relate earthmovements to faults and fracture trends.The adequacy <strong>of</strong> seismic monitoring arrays has abearing <strong>of</strong> <strong>the</strong> certainty <strong>of</strong> seismic eventmagnitudes, locations and sense <strong>of</strong> motion, andhence <strong>the</strong> usefulness <strong>of</strong> recorded (historical)base-line information. Equipment capable <strong>of</strong>sensing seismicity (detectability) may only providecomplete records <strong>of</strong> all movements at a higherlevel (completeness), because instrumentationmaybe insufficient to detect many small events.The seismic monitoring stations in South Australiaare depicted in Figure 2. Additional seismicmonitoring stations are located in adjacentjurisdictions. The locations <strong>of</strong> four additionalstations in South Australia have been agreedbetween State and Federal Government agencies(as shown in Figure 2) and <strong>the</strong> equipment to bedeployed will enhance both <strong>the</strong> completeness andaccuracy <strong>of</strong> measuring seismic events.The detection limits <strong>of</strong> <strong>the</strong> existing seismographnetwork in and around South Australia is variable(as shown in Figure 2, based on Dent, 2009), andthis array is reliably locating all events aboveRichter magnitudes <strong>of</strong> 3.5 (e.g. recording iscomplete for events >3.5) and is more resolute(complete for events above Richter magnitudes <strong>of</strong>2.0) for settled areas. This is considered sufficientto manage public safety under currentcircumstances. If required, existing networks canbe augmented to provide higher resolution <strong>of</strong> <strong>the</strong>location and depth <strong>of</strong> hypocentres.Table 2 Information that can most help to inform activityapprovals (or o<strong>the</strong>rwise) for <strong>the</strong> fracture stimulation <strong>of</strong>geo<strong>the</strong>rmal reservoirs includes: Characterization <strong>of</strong> <strong>the</strong> local environment,infrastructure and population for vulnerability toground movements and loss modeling (taking account<strong>of</strong> design standards) High-quality records <strong>of</strong> seismicity waveforms,magnitude and location; Thickness and shear velocity <strong>of</strong> soil and wea<strong>the</strong>redcover over bedrock. Measuring shear velocities to 30metres depth is a generalized suggestion; Reservoir data for characterization – including:- Orientation and magnitude <strong>of</strong> stress fields;- Location, extent <strong>of</strong> faults and fracture trends;- Mechanical, <strong>the</strong>rmal and chemical rock properties, and- Hydrologic parameters (extent, pressure, chemistry andnature <strong>of</strong> confining aquitards) Conclude loss modeling (taking account <strong>of</strong> designstandards and infrastructure that pre-dates designstandards)Non-exhaustive protocols for credible risk management forgeo<strong>the</strong>rmal operations that may induce seismicity Apply national or international standards for riskmanagement Proponent to demonstrate adequate assessment <strong>of</strong>potential consequence <strong>of</strong> induced seismicity for sitesselected for hydraulic stimulation or large scaleinjection. Stakeholder engagement to start as soon as is practical If required, augment <strong>the</strong> existing seismic monitoringnetwork to detect and ga<strong>the</strong>r seismic events <strong>of</strong>magnitudes (Richter scale) less than 3. It will beadvantageous to deploy seismic monitoring stations to:- Continuous digital high sample frequency (≥ 100 htz)recording;- Attain adequate network to accurately locate seismicevents and measure attenuation; and- Geophysical surveys to calibrate regolith responsemodels at EGS locations. Maintain <strong>the</strong> seismic monitoring network for <strong>the</strong> life <strong>of</strong><strong>the</strong> project. As practical, deploy at least one sub-surface seismicmonitoring station (below regolith if possible) prior tohydraulic stimulation or large scale injection. Deploy down-hole and near surface monitoring stationsto determine attenuation and regolith amplification. Sustain an evergreen watching brief so new informationis assessed and considered for induced seismicity riskmanagement.The location and magnitude <strong>of</strong> historical, recordedearth movements in South Australia are depictedin Figure 3. This map does not express <strong>the</strong>uncertainty <strong>of</strong> epicenter locations, but thisuncertainty is a factor considered when assessingpotential risks posed by EGS operations.The most advanced EGS projects in Australia arethose <strong>of</strong> Geodynamics (Habanero, Jolokia andSavina wells – see figure 1) and Petra<strong>the</strong>rm(Paralana 2 – see figure 1). Only Habanero wellshave been fracture stimulated by year-end 2009.High resolution seismic monitoring arrays havebeen installed at Habanero and Paralana to bettermeasure both background seismicity andseismicity induced during stimulation, productionand circulation operations. The array positioned atHabanero can detect and locate events as low as-2.5 (Richter scale) at a depth <strong>of</strong> 5 km, with a 3D276


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>locational accuracy <strong>of</strong> about 30metres, but <strong>the</strong>completeness <strong>of</strong> accurately computing all eventsis probably limited to -1 (Richter scale). Networkscan be augmented as required to provide greaterresolution and completeness <strong>of</strong> <strong>the</strong> epicenterlocations.Hot Sedimentary Aquifer projects that do notrequire fracture stimulation and entail welloperations largely analogous to petroleum welloperations do not necessarily need to deployseismic monitoring arrays.Reflection seismic is useful to optimize drillinglocations for EGS targets. Figure 4 depicts vastareas in <strong>the</strong> South <strong>Australian</strong> Heat Flow Anomalythat are remote from population centers, andcovered with at least some modern reflectionseismic information.Figure 2. Locations and approximate capability <strong>of</strong> seismographnetwork in South Australia (including use <strong>of</strong> seismographs inadjacent States and <strong>the</strong> Nor<strong>the</strong>rn Territory. Adapted fromDent, 2009. The South <strong>Australian</strong> Heat Flow Anomaly is alsoshown (adapted from Neumann, et al 2000).• <strong>the</strong> <strong>Australian</strong> Building Code AS 1170.4 -(1993) characterizes this region as having a10% chance in 50 years <strong>of</strong> experiencing apeak ground acceleration <strong>of</strong> 0.05g, and• <strong>the</strong> calculated maximum peak groundacceleration from EGS operations in <strong>the</strong>Habanero wells is 0.041g, which for thislocation.Figure 3 Location and magnitude <strong>of</strong> historical earth movementepicenters in South Australia. The South <strong>Australian</strong> Heat FlowAnomaly is also shown (adapted from Neumann, et al 2000).Figure 4. Reflection seismic lines (2D and 3D surveys)onshore South Australia. The South <strong>Australian</strong> Heat FlowAnomaly is also shown (adapted from Neumann, et al 2000)Tools <strong>of</strong> Trade in AssessingAttenuationStandards for attenuation for induced seismicityneed be locally appropriate. The largest recordedmagnitude seismic event associated with EGSoperations at Habanero in <strong>the</strong> Cooper Basindetermined to be <strong>of</strong> magnitude 3.7 on <strong>the</strong> Richterscale e.g. an event felt but one that would rarelycause damage, and which had no significantnegative impacts on local social, natural oreconomic environments.Analysis <strong>of</strong> natural and induced seismicity(associated with EGS operations in <strong>the</strong> term2003-5) in <strong>the</strong> Innamincka region in <strong>the</strong> CooperBasin, Hunt and Morelli (2006) found:• natural seismicity can be expected to rangebetween Richter magnitudes <strong>of</strong> 3.5 and 4.0once every 50 to 167 years;• <strong>the</strong> largest event in <strong>the</strong> area prior to 2003 wasin 1979 with magnitude 2.9;Using Toro’s (1997) relationships, Hunt andMorelli (2006) mapped <strong>the</strong> attenuation distance <strong>of</strong>peak ground acceleration in units <strong>of</strong> gravity (g)and distance (in kms) from <strong>the</strong> Habanero site asredisplayed here in figure 5.Figure 5. Toro (1997) relationship calculation <strong>of</strong> attenuationdistance <strong>of</strong> peak ground acceleration in units <strong>of</strong> gravity (g) and277


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>distance (in kms) generated at <strong>the</strong> Habanero well locationsnear Innamincka in <strong>the</strong> Cooper Basin. From fig.8 in Hunt andMorelli, 2006)Figure 6. Estimated attenuation <strong>of</strong> earth movement intensity <strong>of</strong>a Richter scale 3.7 magnitude seismic event with distancefrom an event hypocenter in nor<strong>the</strong>ast South Australia.Modified Mercalli Intensity ScaleAttenuation Distance from Hypocenters basedon Greenhalgh, et al (1990) function for Australia876543210 100Hypocentral Distance (Km )Ano<strong>the</strong>r approach is illustrated with Figure 6,which is output from a spreadsheet tooldeveloped by PIRSA (Love, 2009) that usesestimates <strong>of</strong> earth movement (seismic wave)velocities to forecast modified Mercalli scaleintensity attenuation with distance fromhypocentres. This spreadsheet tool estimatesintensity attenuation based on five functionspublished in: Bierbaum, et al, 1994; Gaull, et al1990; Greenhalgh, et al, 1990; and Greenhalgh,et al 1994. The Greenhalgh, et al (1994) functionfor Australia is considered <strong>the</strong> best approximation<strong>of</strong> <strong>the</strong>se five correlations to characteriseseismicity induced during EGS operations in <strong>the</strong>Cooper Basin in South Australia. More detailedanalyses (akin to <strong>the</strong> analysis illustrated in figure5) are expected to be concluded by EGSoperators to optimise fracture stimulationprograms, assess potential hazards, and underpinconsultation with stakeholders. Based on thiscorrelation (figure 6), <strong>the</strong> maximum (3.7 on <strong>the</strong>Richter scale) recorded event at Habanero ischaracterised as having attenuated to a modifiedMercalli scale intensity <strong>of</strong> 4.8 at 10 km distancefrom <strong>the</strong> hypocenter and diminished to a slightintensity at a distance 20 km from <strong>the</strong> hypocentere.g.


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Figure 7. Intensity map <strong>of</strong> <strong>the</strong> Beachport (South Australia)earthquake <strong>of</strong> 10 May 1897 based on print media reports fromhttp://www.pir.sa.gov.au/minerals/earthquakes/major_earthquakes_in_south_australia.Better Baseline DataA unique opportunity arises for cooperation toefficiently meet multiple objectives for publicsafety, and exploration for EGS, unconventionalgas reservoir sweet-spots and geosequestration.This would entail cooperation <strong>of</strong>: governmentagencies responsible for assessing geo-hazardsassociated with earth movements; proponents <strong>of</strong>developing fractured reservoirs for <strong>the</strong> production<strong>of</strong> heat energy (e.g. EGS); proponents <strong>of</strong>developing coal bed methane, shale gas and tightgas reservoirs; and proponents <strong>of</strong> subsurfacegreenhouse gas storageIn particular – it will be advantageous forcompanies exploring for reservoir sweet-spotsrelated to tensile rock fabrics and seismicallyquiescent storage reservoirs and relevantgovernment agencies to coordinate plans in <strong>the</strong>context <strong>of</strong>:• publically managed seismic monitoringnetworks, so those networks are augmentedwith multiple objectives in mind;• privately installed monitoring stations becomepublic assets, post-decommissioning <strong>of</strong>industry’s projects; and• national and international forums to fosterinteroperability <strong>of</strong> databases and s<strong>of</strong>twareapplications (input and output).Cooperation will advance both knowledge <strong>of</strong>induced seismicity risks and reservoirdevelopment opportunities.Conclusions1. Co-regulatory efficiency and effectiveness forgeo<strong>the</strong>rmal operations can be delivered withan objective-based and transparent one-stopshopapproach as applied in South Australia.2. PIRSA’s research into potential risks posed byEGS operations has informed regulatoryapprovals for fracture stimulation operations ingeo<strong>the</strong>rmal wells in areas that are remote frompopulation centers.3. The magnitude and extent <strong>of</strong> micro-movementinduced by fracture stimulation and injection atHabanero in <strong>the</strong> Cooper Basin were largely aspredicted e.g. EGS reservoirs were createdand circulated without adverse impacts.4. Calibration <strong>of</strong> predictive models for <strong>the</strong> riskmanagement <strong>of</strong> induced seismicity in remotelocations will provide benchmarks for <strong>the</strong>regulation <strong>of</strong> EGS projects nearer to populatedlocations.5. Australia is becoming a globally importantlaboratory for EGS operations.6. Given enough experience – risk managementstrategies for fracture stimulating and injectinginto geo<strong>the</strong>rmal reservoirs are expected toevolve and EGS operations are expected tobecome predictably pr<strong>of</strong>itable and reliablysafe. The outcome will be wide-spreadcommunity and investor trust in EGSdevelopment.References<strong>Australian</strong> Building Code AS 1170.4 (1993),Minimum design loads on structures. Part 4Earthquake Loads. The <strong>Australian</strong> Standard wasprepared by Committee BD/6, Loading onStructures. It was approved on behalf <strong>of</strong> <strong>the</strong>Council <strong>of</strong> Standards Australia on 21 April 1993and published on 16 August 1993. A 2007 update<strong>of</strong> this reference is available for purchase from <strong>the</strong>sales agent for Standards – Australia from:http://infostore.saiglobal.com/store2/Details.aspx?ProductID=215710.Bierbaum, S. J, 1994. Earthquake hazard andmicro-tremor analysis, South Australia” HonoursThesis, Flinders University <strong>of</strong> South Australia,Australia. Quotes formula used in Love (2009)that was developed by K. Malpas.Dent, V. F., 2009. Seismic network capability andmagnitude completeness maps, 1960 – 2005 forWest Australia, South Australia and <strong>the</strong> Nor<strong>the</strong>rnTerritory, proceedings from <strong>the</strong> <strong>Australian</strong>Earthquake Engineering, Society <strong>Conference</strong>,Newcastle, NSW, Australia, 11-13 December2009 (see:http://www.aees.org.au/<strong>Proceedings</strong>/<strong>Proceedings</strong>.html).Gaull, B. A., Michael-Leiba, M. O., and Ryan, J.M. W., 1990; Probabilistic earthquake risk maps<strong>of</strong> Australia, <strong>Australian</strong> Journal <strong>of</strong> Earth Sciencesv 37 pp 169-187.Greenhalgh S. A., and McDougall, R. M. 1990.Earthquake Risk in South Australia, <strong>Australian</strong>Civil Engineering Transactions v 32 no 3.Greenhalgh S. A., Love, D., Malpas, K., andMcDougall, R. M. 1994. South <strong>Australian</strong>earthquake, 1980-92, <strong>Australian</strong> Journal <strong>of</strong> EarthSciences v 41 pp 483-495.Hunt, S.P. and Morelli, C., 2006. Cooper BasinHDR hazard evaluation: predictive modelling <strong>of</strong>local stress changes due to HFR geo<strong>the</strong>rmalenergy operations in South Australia. SouthAustralia Department <strong>of</strong> Primary, Industries andResources. Report Book 2006/16.279


Laws, R. A., Aust, T. and Malavazos, M., 2002.Environmental regulation <strong>of</strong> <strong>the</strong> upstreampetroleum industry in South Australia. The APPEAJournal, 42 (1), 683–96.Love, D., 2009. unpublished spreadsheet tocalculate intensity attenuation with distance fromhypocentres, Primary Industries & Resources –South Australia.Majer, E., Baria, R., Stark, M., Smith, B., Oates,S., Bommer, J., and Asanuma, H. (2006). InducedSeismicity Associated with Enhanced Geo<strong>the</strong>rmalSystems. Available at: http://www.ieagia.org/documents/ISWPf1MajerWebsecure20Sep06.docMajer, E., Baria, R. and Stark, M. (2008). Protocolfor induced seismicity associated with enhancedgeo<strong>the</strong>rmal systems. Report produced in Task DAnnex I (9 April 2008), International <strong>Energy</strong>Agency-Geo<strong>the</strong>rmal Implementing Agreement(incorporating comments by: C. Bromley, W.Cumming, A. Jelacic and L. Rybach). Available at:http://www.iea-gia.org/publications.asp.Morelli, C., and Malavazos, M. (2008), “Analysisand Management <strong>of</strong> Seismic Risks AssociatedWith Engineered Geo<strong>the</strong>rmal System Operationsin South Australia, in Gurgenci, H. and Budd, A.R. (editors), <strong>Proceedings</strong> <strong>of</strong> <strong>the</strong> Sir Mark OliphantInternational Frontiers <strong>of</strong> Science and Technology<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong> <strong>Conference</strong>,Geoscience Australia, Record 2008/18, pp 113-116. Download fromhttp://www.ga.gov.au/image_cache/GA11825.pdfNeumann, N., M. Sandiford, J. Foden, 2000.Regional geochemistry and continental heat flow:implications for <strong>the</strong> origin <strong>of</strong> <strong>the</strong> South <strong>Australian</strong>heat flow anomaly Earth and Planetary ScienceLetters, 183 pp. 107-120.Productivity Commission, 2009, Review <strong>of</strong>Regulatory Burden on <strong>the</strong> Upstream Petroleum(Oil and Gas) Sector, Research Report, April2009, Melbourne, Australia. Published by <strong>the</strong>Commonwealth <strong>of</strong> Australia. Download from:http://www.pc.gov.au/__data/assets/pdf_file/0011/87923/upstream-petroleum.pdfSouth <strong>Australian</strong> Government (2009), Petroleumand Geo<strong>the</strong>rmal <strong>Energy</strong> Act 2000, as amended inDecember 2009. Download from:http://www.legislation.sa.gov.au/LZ/C/A/PETROLEUM%20AND%20GEOTHERMAL%20ENERGY%20ACT%202000.aspx.Toro, G.R., N.A. Abrahamson and J.F. Schneider(1997). A Model <strong>of</strong> Strong GroundMotions from Earthquakes in Central and EasternNorth America: Best Estimates andUncertainties. Seismological Research Letters,v.68, no. 1, pp. 41-57.USGS, 2009. The Modified Mercalli IntensityScale. Abridged from The Severity <strong>of</strong> anEarthquake, USGS General Interest Publication1989-288-913. Webpage updated 27 October2009 at:www.earthquake.usgs.gov/learn/topics/mercalli.php<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>AcknowledgmentsThe authors thank Ladsi Rybach (GeoWatt), RoyBaria (EGS-<strong>Energy</strong>) and PIRSA colleagues for<strong>the</strong>ir kind inputs, especially James Coda, BelindaHayter Carice Holland, Peter Hough, and ShaneFarrelly.Keywords: geo<strong>the</strong>rmal, EGS, induced seismicity,attenuation distance, one-stop-shop regulation,geohazards280


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>GREAT EXPECTATIONS FOR GEOTHERMAL ENERGY – FORECAST TO 2100Goldstein, B.A., Hiriart, G., Tester, J.,. B., Bertani, R., Bromley, Gutierrez-Negrin, L.,C.JHuenges, E., H, Ragnarsson, A., Mongillo, M.A. Muraoka, and V. I. Zui,INTRODUCTIONGeo<strong>the</strong>rmal energy systems have: a modest environmental footprint; compared to many renewableand conventional alternatives ; will not be impacted by climate change; and have potential to become<strong>the</strong> world’s lowest cost source <strong>of</strong> sustainable <strong>the</strong>rmal fuel for zero-emission, base-load direct use andpower generation. Displacement <strong>of</strong> more emissive fossil energy supplies with geo<strong>the</strong>rmal energy canalso be expected to play a key role in climate change mitigation strategies.In this context, sharedchallenges on <strong>the</strong> road to a global portfolio <strong>of</strong> safe, secure, competitively priced energy supplies aredrivers for international cooperation in research, exploration, pilot demonstration and pre-competitivedevelopment <strong>of</strong> geo<strong>the</strong>rmal energy resources and technologies.The intellectual and financial inputs for international, pre-competitive initiatives are coming from publicand private investors with aspirations for low emissions, affordable, and globally deployable 24/7energy supplies. It is reasonable to conclude that <strong>the</strong> outcomes (improved technologies and methods)<strong>of</strong> <strong>the</strong>se collective efforts over <strong>the</strong> next 20 years will underpin great expectations for widespread,pr<strong>of</strong>itable and environmentally sustainable use <strong>of</strong> geo<strong>the</strong>rmal energy for centuries to come. This paperprovides a synopsis <strong>of</strong> recent findings and current objectives <strong>of</strong> notable international fora enablingcooperation to reduce impediments to widespread use <strong>of</strong> geo<strong>the</strong>rmal energy.SHARING OF PRE-COMPETITIVE KNOWLEDGEThe co-authors <strong>of</strong> this paper have supported one or more <strong>of</strong> <strong>the</strong> international geo<strong>the</strong>rmal energy foralisted in Table 1.Table 1. Names and websites <strong>of</strong> 10 key international geo<strong>the</strong>rmal energy foraInternational <strong>Energy</strong> Agency’s Geo<strong>the</strong>rmal Implementing Agreement(IEA GIA)International Geo<strong>the</strong>rmal Association (IGA) and its World Geo<strong>the</strong>rmalCongress (WGC) (a)International Partnership for Geo<strong>the</strong>rmal Technologies (IPGT) (a)Geo<strong>the</strong>rmal Engineering Integrating Mitigation <strong>of</strong> Induced Seismicityin Reservoirs (GEISER)ENhanced Geo<strong>the</strong>rmal Innovative Network for Europe (ENGINE)European <strong>Energy</strong> Research Alliance Joint Programme on Geo<strong>the</strong>rmal<strong>Energy</strong> (EERA JPGE)European Geo<strong>the</strong>rmal <strong>Energy</strong> Council (EGEC)Geo<strong>the</strong>rmal Resource Council (GRC) and its annual conference inparticularGeo<strong>the</strong>rmal Resource Association (GEA)Stanford University Geo<strong>the</strong>rmal WorkshopsInternational Panel for Climate Change (IPCC) Working Group III –Special Report on Renewable <strong>Energy</strong> (and in particular Chapter 4 –Geo<strong>the</strong>rmal)http://www.iea-gia.org/http://www.geo<strong>the</strong>rmal-energy.org/http://internationalgeo<strong>the</strong>rmal.org/http://www.geiser-fp7.eu/default.aspxhttp://engine.brgm.fr/http://www.eera-set.eu/index.php?index=36http://www.egec.org/http://www.geo<strong>the</strong>rmal.org/http://www.geo-energy.org/http://pangea.stanford.edu/ERE/research/geoth/conference/workshop.htmlhttp://www.ipcc-wg3.de/publications/specialreports/special-report-renewable-energy-sourcesSHARED CHALLENGES BEGET COMPLEMENTARY ACTIONImproved, evermore reliable, cost-effective methods to enhance <strong>the</strong> productivity <strong>of</strong> geo<strong>the</strong>rmalsystems will be essential to <strong>the</strong> competitiveness <strong>of</strong> geo<strong>the</strong>rmal resource in energy markets. Inparticular, <strong>the</strong> commercialisation <strong>of</strong> fracture and/or chemical stimulation methods to reliably createEngineered Geo<strong>the</strong>rmal Systems (EGS) will be one key milestone on <strong>the</strong> road to great expectationsfor widespread economic use <strong>of</strong> geo<strong>the</strong>rmal energy. A scan <strong>of</strong> <strong>the</strong> objectives <strong>of</strong> <strong>the</strong> internationalgeo<strong>the</strong>rmal energy fora define <strong>the</strong> high priorities summarized in Table 2.281


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Table 2. Twenty key priorities for international geo<strong>the</strong>rmal energy fora. This is an update priorities presented inGoldstein et al., 2009.1. Openness to cooperation to engender complementary researchand <strong>the</strong> sharing <strong>of</strong> knowledge2. Informing industry experts, government policy makers and<strong>the</strong> public at large through presentations, publications,websites, submissions to enquiries and <strong>the</strong> convening <strong>of</strong>conferences, workshops and courses3. Creating effective standards for reporting geo<strong>the</strong>rmal4. For EGS, improved hard rock drill equipmentoperations, resources and reserves5. Predictive reservoir performance modelling 6. For EGS, improved multiple zone isolation7. Predictive stress field characterisation 8. For deep EGS, reliable submersible pumps9. For EGS, mitigate induced seismicity 10. Longevity <strong>of</strong> well cement and casing11. Condensers for high ambient-surface temperatures 12. For EGS: Optimum fracture stimulation methods13. Use <strong>of</strong> CO 2 as a circulating fluid 14. High temperature logging tools and sensors15. Improve power plant design 16. High temperature flow survey tools17. Technologies & methods to minimise water use 18. High temperature fluid flow tracers19. Predict heat flow and reservoirs ahead <strong>of</strong> <strong>the</strong> bit 20. Mitigation <strong>of</strong> formation damage, scale and corrosionUnited States3094 MWFrance16 MWPortugal29 MWIceland575 MWGermany6.6 MWAustria1.4 MWItaly843 MWTurkey82 MWEthiopia7.3 MWKenya167 MWChina24 MWRussia82 MWMexico958 MWJapan536 MWGuatemala52 MWPhilippines1904MWEl Salvador204 MWPapua‐N. G.56 MWNicaragua88 MWN. Zealand628 MWCosta Rica166 MWTotal : 10,715 MWeThailand0.3 MWIndonesia1197 MWAustralia1.1 MWFigure 1 Geo<strong>the</strong>rmal-electric installed capacity by country in 2009. Figure shows worldwide average heat flow in mW/m 2 and tectonic plates boundaries(illustration adapted from a figure in Hamza et al., 2008 with data from Bertani, <strong>2010</strong>).This map <strong>of</strong> heat flow does not reconcile all geo<strong>the</strong>rmal information.The delineation <strong>of</strong> geo<strong>the</strong>rmal resources will be improved by integrating temperature gradient, heat flow and reservoir data.INFORMING POLICY MAKERS AND THE PUBLIC AT LARGEWORLD REPORT - GEOTHERMAL ENERGY USEGeo<strong>the</strong>rmal energy supplies are currently used to generate base-load electricity in 24 countries withan installed capacity <strong>of</strong> 11 gigawatts <strong>of</strong> electricity (GWe) and a global average capacity factor <strong>of</strong> 71%,with newer installations above 90%, providing 10% to 30% <strong>of</strong> <strong>the</strong>ir electricity demand in six countries(Bertani, <strong>2010</strong>). Figure 1 is a map <strong>of</strong> estimated heat flow in milliwatts per square metre (Wx10 -6 /m -2 )annotated with geo<strong>the</strong>rmal electricity generation capacity by country. Geo<strong>the</strong>rmal energy supplies arealso used for direct use applications in 78 countries, accounting for 50 GW <strong>the</strong>rmal including district(space) heating and cooling and ground-source (geo<strong>the</strong>rmal) heat pumps (GHPs), which haveachieved significant market penetration worldwide (Lund et al.,<strong>2010</strong>).282


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>BUILD (INNOVATE) AND MARKET BETTER MOUSE-TRAPSThe obvious generalised impediments to massive, global geo<strong>the</strong>rmal energy use are: currently insufficiently predictable reliability <strong>of</strong> geo<strong>the</strong>rmal reservoir performance (and in particular,<strong>the</strong> predicable reliability <strong>of</strong> engineered geo<strong>the</strong>rmal system reservoirs); and current costs <strong>of</strong> geo<strong>the</strong>rmal well deliverability (and in particular, fluid production levels fromstimulated engineered geo<strong>the</strong>rmal systems and <strong>the</strong> high costs <strong>of</strong> drilling deep wellsHence, <strong>the</strong> over-arching common and well justified objectives <strong>of</strong> global government initiatives are tostimulate technologic and learn-while-doing breakthroughs that will lead to a point where <strong>the</strong> cost <strong>of</strong>geo<strong>the</strong>rmal energy use is reliably cost-competitive and comparatively advantageous within markets.MARKET (COMMUNICATE!)Geo<strong>the</strong>rmal resources contain <strong>the</strong>rmal energy that can be produced, stored and exchanged (flowed)in rock, gas (steam) and liquids (mostly water) in <strong>the</strong> subsurface <strong>of</strong> <strong>the</strong> earth.With proper management practice, geo<strong>the</strong>rmal resources are sustainable and renewable overreasonable time periods. As stored <strong>the</strong>rmal energy is extracted from local regions in an activereservoir, it is continuously restored by natural conduction and convection from surrounding hotterregions, and <strong>the</strong> extracted geo<strong>the</strong>rmal fluids are replenished by natural recharge and by reinjection <strong>of</strong><strong>the</strong> exhausted fluids. Additionally: geo<strong>the</strong>rmal plants have low- to emissions-free operations and relatively modest land footprints. Theaverage direct emissions yield <strong>of</strong> partially open cycle, hydro<strong>the</strong>rmal flash and direct steam electricpower plants yield is about 120 g CO 2 /kWhe 1 . Current binary cycle plants with total reinjection yieldless than 1 g CO 2 /kWhe in direct emissions. Emissions from direct use applications are even lower(Fridleifsson et al., 2008). Over its full life-cycle (including <strong>the</strong> manufacture and transport <strong>of</strong>materials and equipment), CO 2 -equivalent emissions range from 23-80 g/kWhe for binary plants(based on Frick et al. <strong>2010</strong> and Nill, 2004) and 14-202 g/kWht for district heating systems andGHPs (based on Kaltschmitt, 2000). This means geo<strong>the</strong>rmal resources are environmentallyadvantageous and <strong>the</strong> net energy supplied more than <strong>of</strong>fsets <strong>the</strong> environmental impacts <strong>of</strong> human,energy and material inputs; geo<strong>the</strong>rmal electric power plants have characteristically high capacity factors; <strong>the</strong> average forpower generation in 2009 is71% (67,246 GWh electrical used from installed capacity <strong>of</strong> 10.714GW electrical based on Bertani, <strong>2010</strong>), and modern geo<strong>the</strong>rmal power plants exhibit capacity factorsgreater than 90%. This makes geo<strong>the</strong>rmal energy well suited for base-load (24/7), dispatchableenergy use; <strong>the</strong> average estimated 27.5% capacity factor for direct use in 2009 (121.7 TWh <strong>the</strong>rmal used frominstalled capacity <strong>of</strong> 50.6 GW <strong>the</strong>rmal based on Lund, et al., <strong>2010</strong>) can be improved with smart grids(as for domestic and industrial solar energy generation), by employing combined heat and powersystems, by using geo<strong>the</strong>rmal heat absorptive and vapour compression cooling technology, and byexpanding <strong>the</strong> distributed use <strong>of</strong> ground source heat pump energy generation; and properly managed geo<strong>the</strong>rmal reservoir systems are sustainable for very long term operation,comparable to or exceeding <strong>the</strong> foreseeable design-life <strong>of</strong> associated surface plant and equipment.CHARACTERISING GEOTHERMAL RESOURCES, RESERVES AND SUPPLIESThe <strong>the</strong>oretical global geo<strong>the</strong>rmal resource base corresponds to <strong>the</strong> <strong>the</strong>rmal energy stored in <strong>the</strong>Earth’s crust. The technical (prospective) global geo<strong>the</strong>rmal resource is <strong>the</strong> fraction <strong>of</strong> <strong>the</strong> earth’sstored heat that is accessible and extractable for use with foreseeable technologies, without regard toeconomics. Technical resources can be subdivided into three categories in order <strong>of</strong> increasinggeological confidence: inferred, indicated and measured (AGEG-AGEA, 2009), with measuredgeo<strong>the</strong>rmal resources evidenced with subsurface information to demonstrate it is useable. Geo<strong>the</strong>rmalreserves are <strong>the</strong> portion <strong>of</strong> geo<strong>the</strong>rmal resources that can confidently be used for economic purposes.Geo<strong>the</strong>rmal reserves developed and connected to markets are energy supplies. Accessiblegeo<strong>the</strong>rmal resources are enormous as detailed in Figure 2. Resources size is clearly not a limitingfactor for global geo<strong>the</strong>rmal energy development.1 This is <strong>the</strong> weighted average <strong>of</strong> 85% <strong>of</strong> <strong>the</strong> world power plant capacity, according to Bertani and Thain, 2002,and Bloomfield et al., 2003283


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Figure 2. Potential geo<strong>the</strong>rmal energy resources split into categories e.g. <strong>the</strong>oretical, technical, economic, developable and existing supplies for powergeneration and direct use. All categories for power generation assume a 71% capacity factor and 8.1% average efficiency for converting <strong>the</strong>rmal intoelectrical energy, though both factors will likely improve (increase) in future. All direct use estimates assume an average 31% capacity factor, somewhathigher than <strong>the</strong> average (27.5%) in 2009. Adapted from a figure developed by Ladsi Rybach and published in <strong>the</strong> <strong>Proceedings</strong> <strong>of</strong> <strong>the</strong> Joint IEA-GIA~IGAWorkshop: Geo<strong>the</strong>rmal <strong>Energy</strong> Global Development Potential and Contribution to Mitigation <strong>of</strong> Climate Change, 5-6 May 2009, Madrid, Spain, edited byM.A. Mongillo, 20 March <strong>2010</strong>FAQ: WHAT IS GEOTHERMAL ENERGY AND HOW DOES IT WORK? (COMMUNICATE!)Geo<strong>the</strong>rmal energy is <strong>the</strong> terrestrial heat stored in, or discharged from rocks and fluids (water, brines,gases) saturated pore space (including fractures), and is widely harnessed in two ways: for power(electricity) generation; and for direct use e.g. heating, cooling, aquaculture, horticulture, spas and avariety <strong>of</strong> industrial processes, including drying. The use <strong>of</strong> energy extracted from <strong>the</strong> constanttemperatures <strong>of</strong> <strong>the</strong> earth at shallow depth by means <strong>of</strong> ground source heat pumps (GSHP) is acommon form <strong>of</strong> geo<strong>the</strong>rmal energy use. The direct use <strong>of</strong> natural flows <strong>of</strong> geo<strong>the</strong>rmally heated watersto surface have been practised at least since <strong>the</strong> Middle Palaeolithic (Cataldi, 1999), and industrialutilisation began in Italy by exploiting boric acid from <strong>the</strong> geo<strong>the</strong>rmal zone <strong>of</strong> Larderello, where in 1904<strong>the</strong> first kilowatts <strong>of</strong> electric energy (kWe) were generated and in 1913 <strong>the</strong> first 250-kWe commercialgeo<strong>the</strong>rmal power plant was installed (Burgassi, 1999).Where very high temperature fluids (> 180 C) flow naturally to surface (e.g. where heat transfer byconduction dominates), geo<strong>the</strong>rmal resources are <strong>the</strong> manifestation <strong>of</strong> two factors: a geologic heat source to replenish <strong>the</strong>rmal energy; and a hydro<strong>the</strong>rmal reservoir that can be tapped to flow geo<strong>the</strong>rmal fluids for its direct use and/or forgenerating electricity.Elsewhere, a third geologic factor, <strong>the</strong> insulating capacity <strong>of</strong> rocks (acting <strong>the</strong>rmal blankets) is anadditional necessary natural ingredient in <strong>the</strong> process <strong>of</strong> accumulating usable, stored heat energy ingeologic reservoirs that can be tapped to flow heat energy, and replenished by convective, conductiveand radiated heat flow from sources <strong>of</strong> geo<strong>the</strong>rmal energy.284


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Usable geo<strong>the</strong>rmal systems occur in a variety <strong>of</strong> geological settings. These are frequently categorizedas follows: 1. High-temperature (>180°C) systems at depths above (approximately) 3.5 km aregenerally associated with recent volcanic activity and mantle hot spot anomalies.. O<strong>the</strong>r hightemperature geo<strong>the</strong>rmal systems below (approximately) 3.5 km are associated with anomalously highheat producing crustal rocks, mostly granites. 2. Intermediate temperature systems (100-180°C) and3. Low temperature ( 180C) fluids to surface. Indeed, temperatures above 1000°C can occurat less than 10 km depth in areas <strong>of</strong> magma intrusion. Given <strong>the</strong> global average land area surfacetemperature <strong>of</strong> (about) 15C and an approximate global geo<strong>the</strong>rmal temperature gradient for landareas outside volcanic settings <strong>of</strong> (about) 30C, <strong>the</strong> same high temperature (> 180C) can be reached(on average) at a depth <strong>of</strong> about 5.5 km below ground level.The main types <strong>of</strong> geo<strong>the</strong>rmal power plants use direct steam (<strong>of</strong>ten called dry steam), flashed steamand binary cycles.Power plants that use dry and/or flashed steam to spin turbines are <strong>the</strong> most commonly deployed form<strong>of</strong> geo<strong>the</strong>rmal electricity generation. These plants use <strong>the</strong> heat energy contained in water and steamflowed from geo<strong>the</strong>rmal wells to spin turbines, converting <strong>the</strong>rmal and kinetic energy to electricalenergy.Organic Rankine power plants employing secondary working fluids are increasingly being used forgeo<strong>the</strong>rmal power generation. These so-called binary closed-loop power plants do not flow producedgeo<strong>the</strong>rmal fluids directly into turbines. Thermal energy contained in water and/or steam producedfrom geo<strong>the</strong>rmal wells is transferred to a secondary working fluid using a heat exchanger (hence <strong>the</strong>term binary closed-loop). Organic compounds with lower boiling points than water (such as propanethat boils at about 28 degrees C are <strong>of</strong>ten used as working fluids. The heat energy in <strong>the</strong> geo<strong>the</strong>rmalfluid boils <strong>the</strong> working fluid changing it from a liquid to a pressurized gas within <strong>the</strong> closed-loop, whichcan <strong>the</strong>n be expanded in a turbine to spins a generator. The exhausted working fluid is cooled,condensed back into a liquid, pressurized and <strong>the</strong>n recycled into <strong>the</strong> heat exchanger to complete <strong>the</strong>cycle.285


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Table 1 Estimated global long term forecasts <strong>of</strong> installed capacity for geo<strong>the</strong>rmal power and direct uses (heat) and <strong>of</strong> electricand direct uses (heat) generation from Bertani, <strong>2010</strong> and Authors, <strong>2010</strong>.Expected World UseExpected global useDirect(GWt)2020 2030 2050 2100Electric(GWe)Direct(GWt)Electric(GWe)Direct(GWt)Electric(GWe)Capacity 160.5 25.9 380.1 51.0 831.1 160.6Direct(GWt)1,367 to5,906Electric(GWe)264 to1,141TWh t /y TWh e /y TWh t /y TWh e /y TWh t /y TWh e /y TWh t /y TWh e /y421.9 181.8 998.8 380.0 2184.0 1266.43,592to15,5212,083to9,000EJ/y EJ/y EJ/y EJ/y EJ/y EJ/y EJ/y EJ/y12.9 to 7.5 to1.52 0.65 3.60 1.37 7.86 4.5655.9 32.4HOW BIG WILL GEOTHERMAL BE? (COMMUNICATE!)The extent or accessibility <strong>of</strong> geo<strong>the</strong>rmal resources will not be a limiting factor for deployment. Tables1 and 2 summarise <strong>the</strong> conclusions reached by <strong>the</strong> co-authors in <strong>2010</strong>). These forecasts assumeimprovements in capacity factors power generation from <strong>the</strong> current average 71% to 90% by 2050, alevel already attained in efficient, existing geo<strong>the</strong>rmal power generation plants. Earlier estimates fordeployment beyond <strong>2010</strong> that were considered in developing forecasts in Table 1 include: IPCC,2007; IEA, 2008; and EREC, 2008.Table 2 World installed capacity, electricity production and capacity factor <strong>of</strong> geo<strong>the</strong>rmal power plants 1995-<strong>2010</strong>, forecastsfor 2015-2050 (adapted from data from Bertani, <strong>2010</strong> and Authors, <strong>2010</strong>) and forecasts for 2100 based on 1% and 4%average annual growth for 50 years from 2050.YearInstalled Capacity (GWe) Electricity Production (GWh/y) Capacity FactorActual or mean forecast Actual or mean forecast(%)1995 6.8 38,035 642000 8.0 49,261 712005 8.9 56,786 73<strong>2010</strong> 10.7 67,246 712015 18.5 121,600 752020 25.9 181,800 802030 51.0 380,000 852040 90.5 698,000 882050 160.6 1,266,400 902100 264 to 1,141 2,082,762 to 8,999,904 90+NEXT STEPS IN GLOBAL RESOURCE ASSESSMENTSA fur<strong>the</strong>r global geo<strong>the</strong>rmal resource assessment is planned under an existing IEA GIA researchannex. This will include a probabilistic range <strong>of</strong> estimates, for example, assuming that a log normaldistribution adequately describes <strong>the</strong> range <strong>of</strong> recovery <strong>of</strong> stored heat from a minimum <strong>of</strong> 0.5% at a99% probability to a maximum <strong>of</strong> 40% <strong>of</strong> stored heat at a 1% probability. This implies: a low-siderecovery <strong>of</strong> 1.34% <strong>of</strong> stored (90% probability); a mid-range recovery <strong>of</strong> 4.47% <strong>of</strong> stored heat (50%probability); a Swanson’s mean 2 recovery <strong>of</strong> 6.68% <strong>of</strong> stored heat; and a high-side recovery <strong>of</strong>14.95% <strong>of</strong> stored heat (10% probability).CONCLUSIONS REGARDING DEPLOYMENT BY 2100Current global trends and regional research underpin credible expectations for great growth in <strong>the</strong>global use <strong>of</strong> geo<strong>the</strong>rmal energy over <strong>the</strong> next 90 years. Great expectations are:Power generation with binary plants and total re-injection will become common-place in countrieswithout high-temperature resources.2 Swanson’s mean is <strong>the</strong> weighted approximation for a log-normal distribution equal to <strong>the</strong> summation <strong>of</strong> 30% <strong>of</strong><strong>the</strong> 90% probability value, 30% <strong>of</strong> <strong>the</strong> 10% probability value, and 40% <strong>of</strong> <strong>the</strong> 50% probability value e.g. (P90 x0.3) + (P10 x 0.3) + (P50 x 0.4) equals <strong>the</strong> Swanson’s mean value286


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Geo<strong>the</strong>rmal energy utilization from conventional hydro<strong>the</strong>rmal resources continues to accelerateand <strong>the</strong> advent <strong>of</strong> EGS is expected to rapidly increase growth after 10 to 15 years puttinggeo<strong>the</strong>rmal on <strong>the</strong> path to provide an expected generation global supply <strong>of</strong> 4.56 EJ per year(~160 GWe) by 2050, and between 7.5 EJ per year (with 1% growth per year) and 32.4 EJ peryear (with 4% growth per year) by 2100.In addition to <strong>the</strong> widespread deployment <strong>of</strong> EGS, <strong>the</strong> practicality <strong>of</strong> using supercriticaltemperatures and <strong>of</strong>fshore resources is expected to be tested with experimental deployment <strong>of</strong>one or both a possibility by 2100.Direct use <strong>of</strong> geo<strong>the</strong>rmal energy for heating and cooling, including geo<strong>the</strong>rmal heat pumps(GHPs) is expected to increase to 7.86 EJ /year (~815 GWt) by 2050 and between 12.9 EJ peryear (with 1% growth per year) and 55.9 EJ per year (with 4% growth per year)by 2100.Marketing and multiple internationally competitive supply chains will underpin this growth. Thisexpectation is supported information published by Rybach, 2005Geo<strong>the</strong>rmal energy is expected to meet between 2.5% and 4.1% <strong>of</strong> <strong>the</strong> total global demand forelectricity by 2050 and potentially more than 10% by 2100. It is also expected to provide about5% <strong>of</strong> <strong>the</strong> global demand for heating and cooling in by 2050 and potentially, more than 10% by2100. Geo<strong>the</strong>rmal energy will be a dominant source <strong>of</strong> base-load renewable energy in manycountries in <strong>the</strong> next century.With its natural <strong>the</strong>rmal storage capacity, geo<strong>the</strong>rmal is especially suitable for supplying bothbase-load electric power generation and for fully dispatchable heating and cooling applications inbuildings, and thus is uniquely positioned to play a key role in climate change mitigationstrategies (Bromley, et al., <strong>2010</strong>).ACKNOWLEDGEMENTSThe authors thank <strong>the</strong>ir international colleagues who have contributed so much <strong>of</strong> <strong>the</strong>ir pr<strong>of</strong>essionallives and time to provide improved understanding <strong>of</strong> geo<strong>the</strong>rmal systems. We are especially gratefulto: John Lund, Ladsi Rybach, Mike Mongillo, Ken Williamson, David Newell, Trevor Demayo, ArthurLee, Subir Sanyal, Roland Horne, David Blackwell, and Doone Wyborn.REFERENCESAGEG-AGEA, 2009, <strong>Australian</strong> Code for Reporting <strong>of</strong> Exploration Results, Geo<strong>the</strong>rmal Resources andGeo<strong>the</strong>rmal Reserves, prepared by <strong>the</strong> Prepared by: The <strong>Australian</strong> Geo<strong>the</strong>rmal Code Committee - acommittee <strong>of</strong> <strong>the</strong> <strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong> Group (AGEG) and <strong>the</strong> <strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong>Association (AGEA). Download fromhttp://www.pir.sa.gov.au/geo<strong>the</strong>rmal/ageg/geo<strong>the</strong>rmal_reporting_codeAuthors (<strong>of</strong> this report), <strong>2010</strong>. Unpublished correspondence leading to tabulations <strong>of</strong> expectations forgeo<strong>the</strong>rmal energy deployment from resources below 3,500 metres in 2020, 2030 and 2050. Bertani,R. and Tester, J. were instrumental in developing <strong>the</strong>se estimates.Bertani, R., <strong>2010</strong>. World Update on Geo<strong>the</strong>rmal Electric Power Generation 2005-2009. <strong>Proceedings</strong>World Geo<strong>the</strong>rmal Congress <strong>2010</strong>, Bali, Indonesia, April 25-30, <strong>2010</strong>.Bertani, R., and I. Thain, 2002. Geo<strong>the</strong>rmal power generating plant CO 2 emission survey. IGA News,49, pp. 1-3. (ISSN: 0160-7782)Bloomfield, K.K., J.N. Moore, and R.N. Neilson, 2003. Geo<strong>the</strong>rmal energy reduces greenhouse gases.Geo<strong>the</strong>rmal Resources Council Bulletin, Vol. 32, No. 2, pp. 77-79. (ISSN 01607782)Bromley, C.J., M.A. Mongillo, B. Goldstein, G. Hiriart, R. Bertani, E. Huenges, H. Muraoka, A.Ragnarsson, J. Tester, and V. Zui, <strong>2010</strong>. IPCC Renewable <strong>Energy</strong> Report: <strong>the</strong> Potential Contribution<strong>of</strong> Geo<strong>the</strong>rmal <strong>Energy</strong> to Climate Change Mitigation. <strong>Proceedings</strong> World Geo<strong>the</strong>rmal Congress <strong>2010</strong>,Bali, Indonesia, April 25-30, <strong>2010</strong>.Burgassi, P.D., 1999. Historical Outline <strong>of</strong> Geo<strong>the</strong>rmal Technology in <strong>the</strong> Larderello Region to <strong>the</strong>Middle <strong>of</strong> <strong>the</strong> 20th Century. In: Stories from a Heated Earth, R. Cataldi, S. Hodgson, J.W. Lund eds.,Geo<strong>the</strong>rmal Resources Council, Sacramento, CA. pp. 195-219. (ISBN: 0934412197)Cataldi, R., 1999. The Year Zero <strong>of</strong> Geo<strong>the</strong>rmics. In: Stories from a Heated Earth, R. Cataldi, S.Hodgson, J.W. Lund eds., Geo<strong>the</strong>rmal Resources Council, Sacramento, CA. pp. 7-17. (ISBN:0934412197)287


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Dickson, M.H., and M. Fanelli, 2003. Geo<strong>the</strong>rmal energy: Utilization and technology. Publication <strong>of</strong>UNESCO, New York, 205 pp. (ISBN: 9231039156)Electric Power Research Institute (EPRI), 1978. Geo<strong>the</strong>rmal energy prospects for <strong>the</strong> next 50 years.ER-611-SR, Special Report for <strong>the</strong> World <strong>Energy</strong> <strong>Conference</strong> 1978.Frick, S., G. Schröder, and M. Kaltschmitt, <strong>2010</strong>. Life cycle analysis <strong>of</strong> geo<strong>the</strong>rmal binary power plantsusing enhanced low temperature reservoirs. <strong>Energy</strong>, Vol. 35, Issue 5, pp. 2281-2294. (ISSN: 0360-5442)Fridleifsson, I.B., R. Bertani, E. Huenges, J.W. Lund, A. Ragnarsson, and L. Rybach, 2008. ThePossible Role and Contribution <strong>of</strong> Geo<strong>the</strong>rmal <strong>Energy</strong> to <strong>the</strong> Mitigation <strong>of</strong> Climate Change. IPCCScoping Meeting on Renewable <strong>Energy</strong> Sources, Luebeck, Germany 21-25 January 2008. 36 p.Available at: http://www.ipcc.ch/pdf/supporting-material/proc-renewables-lubeck.pdfHamza, V.1; Cardoso, R.; and Ponte Neto, C., 2008. Spherical harmonic analysis <strong>of</strong> earth'sconductive heat flow, International Journal <strong>of</strong> Earth Sciences, Volume 97, Number 2, April 2008, pp.205-226(22), Publisher: SpringerIPCC 2007, Climate Change 2007, Fourth Assessment Report <strong>of</strong> <strong>the</strong> Intergovernmental Panel onClimate Change, Working Group III: Mitigation <strong>of</strong> Climate Change, Chapter 4 - Geo<strong>the</strong>rmal, Section4.3.3.4International <strong>Energy</strong> Agency (IEA), 2008, World <strong>Energy</strong> Outlook 2008, download fromhttp://www.iea.org/textbase/nppdf/free/2008/weo2008.pdfEuropean Renewable <strong>Energy</strong> Council (EREC) and Greenpeace International (GPI), 2008, <strong>Energy</strong>[R]evolution – A sustainable Global <strong>Energy</strong> Outlook (EREC-GPI-08). Download from:http://www.greenpeace.org/raw/content/international/press/reports/energyrevolutionreport.pdfGoldstein, B.A., Hill, A.J., Long, A., Budd, A. R., Holgate, F., and Malavazos, M., 2009. Hot RockGeo<strong>the</strong>rmal <strong>Energy</strong> Plays in Australia, <strong>Proceedings</strong> <strong>of</strong> <strong>the</strong> 34 th Workshop on Geo<strong>the</strong>rmal ReservoirEngineering, Stanford University, Stanford, California, February 9-11, 2009, SGP-TR-187Hiriart, G., R.M. Prol-Ledesma, S. Alcocer and G. Espíndola, <strong>2010</strong>. Submarine Geo<strong>the</strong>rmics:Hydro<strong>the</strong>rmal Vents and Electricity Generation. <strong>Proceedings</strong> World Geo<strong>the</strong>rmal Congress <strong>2010</strong>, Bali,Indonesia, 25-29 April, <strong>2010</strong>.Kaltschmitt, M., 2000. Environmental effects <strong>of</strong> heat provision from geo<strong>the</strong>rmal energy in comparisonto o<strong>the</strong>r resources <strong>of</strong> energy. <strong>Proceedings</strong> World Geo<strong>the</strong>rmal Congress 2000, Kyushu-Tohoku, Japan,May 28-June 10, 2000. (ISBN: 0473068117)Krewitt, W., K. Nienhaus, C. Klebmann, C. Capone, E. Stricker, W. Grauss, M. Hoggwijk, N.Supersberger, U. Von Winterfeld, and S. Samadi, 2009. Role and potential <strong>of</strong> renewable energy andenergy efficiency for global energy supply. Climate Change, 18, December 2009, 344 pp. (ISSN:1862-4359)Lund, J. W., Freeston, D.H. and Boyd, T.L <strong>2010</strong>. Direct Utilization <strong>of</strong> Geo<strong>the</strong>rmal <strong>Energy</strong> <strong>2010</strong>Worldwide Review. <strong>Proceedings</strong> World Geo<strong>the</strong>rmal Congress <strong>2010</strong>, Bali, Indonesia, 25-30 April <strong>2010</strong>.Mongillo, M.A., <strong>2010</strong>, <strong>Proceedings</strong> <strong>of</strong> <strong>the</strong> Joint GIA-IGA Workshop - Geo<strong>the</strong>rmal <strong>Energy</strong> GlobalDevelopment Potential and Contribution to Mitigation <strong>of</strong> Climate Change, 5-6 May 2009, Madrid,Spain. Download from http://www.ieagia.org/documents/ProcGIA_IGAWorkshopMadridFinalprepress22Mar10_000.pdfNill, M., 2004. Die zukünftige Entwicklung von Stromerzeugungstechniken, Eine ökologische Analysevor dem Hintergrund technischer und ökonomischer Zusammenhänge, Fortschritt-Berichte VDI Nr.518. Düsseldorf, D: VDI-Verlag, 346 (in German). (ISSN: 0178-9414)Rybach, L., 2005. The advance <strong>of</strong> geo<strong>the</strong>rmal heat pumps world-wide. IEA Heat Pump CentreNewsletter, 23, pp. 13-18. (ISSN: 0724-7028)Sims, R.E.H., R.N. Schock, A. Adegbululgbe, J. Fenhann, I. Konstantinaviciute, W. Moomaw, H.B.Nimir, B. Schlamadinger, J. Torres-Martínez, C. Turner, Y. Uchiyama, S.J.V. Vuori, N. Wamukonya, X.Zhang, 2007. <strong>Energy</strong> supply. In Climate Change 2007: Mitigation. Contribution <strong>of</strong> Working Group III to<strong>the</strong> Fourth Assessment Report <strong>of</strong> <strong>the</strong> Intergovernmental Panel on Climate Change [B. Metz, O.R.288


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Davidson, P.R. Bosch, R. Dave, L.A. Meyer (eds)], Cambridge University Press, Cambridge, UnitedKingdom and New York, NY, USA. (ISBN-13: 9780521705981)Tester, J.W., E.M. Drake, M.W. Golay, M.J. Driscoll, and W.A. Peters, 2005. Sustainable <strong>Energy</strong> –Choosing Among Options, MIT Press, Cambridge, MA, 850 pp.Tester, J.W., B.J. Anderson, A.S. Batchelor, D.D. Blackwell, R. DiPippo, and E.M. Drake (eds.), 2006.The Future <strong>of</strong> Geo<strong>the</strong>rmal <strong>Energy</strong> Impact <strong>of</strong> Enhanced Geo<strong>the</strong>rmal Systems on <strong>the</strong> United States in<strong>the</strong> 21st century. Prepared by <strong>the</strong> Massachusetts Institute <strong>of</strong> Technology, under Idaho NationalLaboratory Subcontract No. 63 00019 for <strong>the</strong> U.S. Department <strong>of</strong> <strong>Energy</strong>, Assistant Secretary for<strong>Energy</strong> Efficiency and Renewable <strong>Energy</strong>, Office <strong>of</strong> Geo<strong>the</strong>rmal Technologies. 358 p. (ISBN-10:0486477711, ISBN-13: 978-0486477718)289


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>New Design Concepts for Natural Draft Dry Cooling TowersHal Gurgenci* and Zhiqiang GuanThe Queensland Geo<strong>the</strong>rmal <strong>Energy</strong> Centre <strong>of</strong> Excellence (QGECE), <strong>the</strong> University <strong>of</strong> Queensland, St Lucia,Brisbane, Qld 4072*Corresponding author: h.gurgenci@uq.edu.auDesign <strong>of</strong> efficient natural draft dry cooling systemis essential for <strong>Australian</strong> geo<strong>the</strong>rmal power plantapplications. In fact, dry cooling may be <strong>the</strong> onlyoption for most geo<strong>the</strong>rmal power plants plannedto be established in Australia since <strong>the</strong>se areashave limited access to water resource.Natural draft cooling towers in coal-fired andnuclear power plants have been mainly <strong>of</strong>concrete construction. It has been reported that<strong>the</strong> highest concrete cooling tower in <strong>the</strong> world <strong>of</strong>200 meters high has been built at <strong>the</strong> RWE powerstation at Niederaussem (Busch et al, 2002). Dueto <strong>the</strong> lower <strong>the</strong>rmal efficiencies <strong>of</strong> geo<strong>the</strong>rmalpower plants, <strong>the</strong> heat rejection per kWh(e) <strong>of</strong> netgeneration from <strong>the</strong>se plants will be four or moretimes as great as from fossil fuelled plants (Kröger2004), which will require a much larger coolingtower for a geo<strong>the</strong>rmal power plant <strong>of</strong> comparedto a coal-fired power plant <strong>of</strong> similar capacity. Thedesign and construction <strong>of</strong> such a large concretecooling tower is extremely expensive and takes along time to build. The tower structure is heavyand requires substantial foundation.The Queensland Geo<strong>the</strong>rmal <strong>Energy</strong> Centre <strong>of</strong>Excellence (QGECE) is to explore new conceptsfor natural draft dry cooling technologies forgeo<strong>the</strong>rmal power plants. The aims for <strong>the</strong> newdesign concepts are to increase <strong>the</strong> performance<strong>of</strong> <strong>the</strong> cooling tower and reduce <strong>the</strong> overall cost.Two alternative designs are proposed: low costair-lift mobile cooling tower (Gurgenci and Guan,2009) and solar cooling tower.The design concept for air-lift mobile coolingtower is as follow: <strong>the</strong> tower is built as a flexibleshroud and is held in place in tension by <strong>the</strong>buoyancy force provided by a lighter-than-air gas.One benefit for <strong>the</strong> air-lift cooling tower is that <strong>the</strong>industry can construct very tall cooling towers atan acceptable cost. O<strong>the</strong>r benefits includeconstructing such towers with a minimum <strong>of</strong> timeand expense, which are <strong>of</strong> relatively light weightand which are not subject to frequent repairs. Thetowers are mobile and can be disassembled andmoved to a new geo<strong>the</strong>rmal plant site with aminimum <strong>of</strong> time and effort.The design concept for solar cooling towerincludes a solar energy system which is used topreheat <strong>the</strong> air inside <strong>the</strong> cooling tower toincrease <strong>the</strong> buoyancy <strong>of</strong> <strong>the</strong> natural draft coolingtower. The enhanced buoyancy enable <strong>the</strong>cooling tower be constructed with ei<strong>the</strong>r reducedsize or with increased tower performance, whichis especially beneficial during hottest time periodin a day.Keywords: Geo<strong>the</strong>rmal energy, Cooling tower andheat exchanger, natural draft coolingtechnologies.Natural Draft Dry Cooling TowersA natural draft dry cooling tower is a heat rejectiondevice that creates <strong>the</strong> flow <strong>of</strong> air through <strong>the</strong>bundles <strong>of</strong> finned tube heat exchangers by means<strong>of</strong> buoyancy effects. Buoyancy occurs due to adifference in air density before and after heatexchanger resulting from temperature andmoisture differences. The greater <strong>the</strong> <strong>the</strong>rmaldifference and <strong>the</strong> height <strong>of</strong> <strong>the</strong> tower structure,<strong>the</strong> greater <strong>the</strong> buoyancy force. Therefore, <strong>the</strong>volume flow rate <strong>of</strong> air across <strong>the</strong> heat exchangerbundle is directly proportional to <strong>the</strong> height <strong>of</strong> <strong>the</strong>cooling tower.Natural draft dry cooling towers are particularlyattractive as a cost-saving solution for largerpower plants where water resource is limited andexpensive. The unique economic advantage <strong>of</strong>natural draft cooling towers lies in <strong>the</strong>ir very lowelectric energy requirement. Fan cost andsubstantial amount <strong>of</strong> fan power are saved in thissystem. The operating costs are minimal.Natural cooling towers have been designed invarious ways. However, reinforced concretestructures have become standard to handle <strong>the</strong>high cooling water flow rates in large powerplants.Fig.1 shows a configuration <strong>of</strong> natural draft drycooling tower used by <strong>the</strong> <strong>the</strong>rmal power plants.Fig.2 is a photo taken from Yangchen powerplant <strong>of</strong> China.Fig.1 Natural draft dry cooling [GEA Aircooled Systems]290


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>concrete tower used in most coal-fired andnuclear power plants). The tension cables areconnected to <strong>the</strong> stiffening rings to add strengthand hold <strong>the</strong> shroud in place by tension. Thesealing skin can be made <strong>of</strong> light materials andcan be attached to <strong>the</strong> stiffening rings quickly andeconomically in site. The flexible shroud can havedurability for wind load and wea<strong>the</strong>r resistance.Fig.2 Yangchen Natural Draft Cooling TowerNew Design ConceptsThree design concepts are proposed in thispaper. The first concept relies on a conventionalsteel construction design. The second concept,<strong>the</strong> air-lifted tower, is a radical invention thatproposes <strong>the</strong> use <strong>of</strong> helium-filled toroidal rings toprovide <strong>the</strong> tower structure. The third concept is anovel combination <strong>of</strong> <strong>the</strong> solar chimney idea withnatural draft dry cooling towers.Steel Towers with Advanced Heat ExchangersOne <strong>of</strong> <strong>the</strong> reasons behind <strong>the</strong> use <strong>of</strong> reinforcedconcrete construction as a method <strong>of</strong> buildingnatural draft dry cooling towers in coal-fired powerplants is <strong>the</strong> concern about corrosion caused byexposure to some <strong>of</strong> <strong>the</strong> elements in <strong>the</strong> fluegases in combination with <strong>the</strong> ambient effects.These concerns do not apply to a binarygeo<strong>the</strong>rmal plant. Therefore, <strong>the</strong> use <strong>of</strong> steeltowers is allowable in geo<strong>the</strong>rmal plants and thischoice may <strong>of</strong>fer new options that are notavailable to fossil fuel power plant designers. Acombination <strong>of</strong> steel construction methods withsome <strong>of</strong> <strong>the</strong> advanced heat exchanger optionsthat deliver high heat exchange rate/ pressuredrop ratios could <strong>the</strong>n be a viable option. A steeltower design will be presented that will have <strong>the</strong>capability to power air-cooled condensers for acommercial geo<strong>the</strong>rmal power plant subject toambient conditions typical <strong>of</strong> <strong>the</strong> <strong>Australian</strong>outback.Air-lifted natural draft cooling towerIn this design, a flexible shroud is <strong>the</strong> main body<strong>of</strong> <strong>the</strong> tower structure and is held in place intension by <strong>the</strong> buoyancy force. This flexibleshroud includes stiffening rings, sealing skin andtensioning cables as shown in Figure 3. Theshroud can be divided into several sections andprefabricated in factory and assembled/installedquickly in site.The stiffening rings are made <strong>of</strong> differentdiameters and placed periodically to form <strong>the</strong>desired shape required (such as hyperbolicFig.3 Proposed structure flexible shroudTo provide lifting force to <strong>the</strong> flexible shroud,stacked helium-filled toroidal vessels areconnected directly to stiffening rings separately asindicated in Figure 4 to provide adequate liftingforce. Each inflatable donut can pull ei<strong>the</strong>r asingle stiffening ring or several rings toge<strong>the</strong>r.Each inflatable donut can have its own air inletand can be pneumatically controlled. Redundancyis desirable in order to ensure that <strong>the</strong> towerintegrity can be maintained during <strong>the</strong>maintenance and to facilitate repair <strong>of</strong> leakingdonuts.Not all donuts will need helium or lighter than airgas. Normal air can be pumped into some donuts,probably those towards <strong>the</strong> bottom, withpredefined pressure to provide supporting forcefor <strong>the</strong> shroud. The donuts can be fur<strong>the</strong>r dividedinto several sections vertically along <strong>the</strong> shroud(such as four or eight sections). Each verticalsection can be individual controlled pneumatically.291


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Fig.4 Design <strong>of</strong> donut-shaped air-lifted cooling towerSolar enhanced natural draft cooling towerIn this design, based on <strong>the</strong> principal <strong>of</strong> solarchimney, a solar collector is placed at <strong>the</strong> base <strong>of</strong>a natural draft cooling tower between <strong>the</strong> towerand <strong>the</strong> vertically arranged heat exchanger.Heating <strong>of</strong> <strong>the</strong> air behind <strong>the</strong> heat exchanger(inside <strong>the</strong> tower) will enhance convection, andhence more airflow through <strong>the</strong> heat exchanger.The cooling ability <strong>of</strong> this tower depends primarilyon two factors: <strong>the</strong> size <strong>of</strong> <strong>the</strong> solar collector areaand tower height. With a larger solar collectorarea, a greater volume <strong>of</strong> air is warmed to flow up<strong>the</strong> tower. With a larger tower height, <strong>the</strong> pressuredifference increases <strong>the</strong> buoyancy effect.Figure 5 shows schematic drawing <strong>of</strong> proposeddesign <strong>of</strong> solar enhanced natural draft coolingtower. In this design, heat exchanger bundles areplaced circumferential at <strong>the</strong> base <strong>of</strong> <strong>the</strong> tower. Asolar collector is added between <strong>the</strong> heatexchanger bundles and <strong>the</strong> cooling tower to heat<strong>the</strong> air below. Due to <strong>the</strong> upstream airtemperature <strong>of</strong> <strong>the</strong> heat exchanger has beenheated and much higher than <strong>the</strong> downstream airtemperature, <strong>the</strong> flow rate <strong>of</strong> <strong>the</strong> air through <strong>the</strong>heat exchanger increase, which results ei<strong>the</strong>r <strong>the</strong>tower size can be reduced (for fixed heat sink) or<strong>the</strong> performance <strong>of</strong> <strong>the</strong> tower increases (for fixedtower size).The cooling tower structure can be a standardconcrete tower used in power plant or it can be achimney shape as shown in figure 5. The air-liftcooling tower can also be used in this design.Fig.5 Schematic <strong>of</strong> solar natural draft cooling towerAir-Lifted Tower ConstructionTo erect <strong>the</strong> air-lift cooling tower shown in Figure4, <strong>the</strong> stiffening rings are placed first around <strong>the</strong>bases in order and <strong>the</strong> top stiffening ring isconnected to <strong>the</strong> first donut shape vessel and <strong>the</strong>top end <strong>of</strong> <strong>the</strong> tension cables. Helium is <strong>the</strong>npumped into <strong>the</strong> top donut vessel which lifts <strong>the</strong>first stiffening ring and part <strong>of</strong> <strong>the</strong> tension cables.After <strong>the</strong> first ring has been raised to a desiredposition above <strong>the</strong> ground, <strong>the</strong> second top ringcan be connected to <strong>the</strong> tension cables in <strong>the</strong>same way. The ascending height <strong>of</strong> <strong>the</strong>assembled rings is controlled by <strong>the</strong> release <strong>of</strong>tension cables. The sealing skin can be formedand fixed to <strong>the</strong> already assembled stiffening ringswith various fixing mechanisms.With <strong>the</strong> same process repeated as above, <strong>the</strong>controlled upward motion <strong>of</strong> <strong>the</strong> lifting donutvessels result in a corresponding advance <strong>of</strong> <strong>the</strong>cooling tower shroud. The intermediate advance<strong>of</strong> <strong>the</strong> installation <strong>of</strong> <strong>the</strong> cooling tower is shown inFigure 6.Once <strong>the</strong> bottom ring has been assembled andraised to desired position, <strong>the</strong> tension cables are<strong>the</strong>n secured to <strong>the</strong>ir respective anchors.292


Future WorkFig.6 Intermediate position <strong>of</strong> installationAn engineering feasibility study on <strong>the</strong> above newdesign concepts will be carried first based on <strong>the</strong>environmental conditions in <strong>the</strong> proposedgeo<strong>the</strong>rmal power plant sites.Should <strong>the</strong> feasibility study favour <strong>the</strong> air-liftcooling tower concepts, a detailed design <strong>of</strong> suchcooling tower for a planned 50MW geo<strong>the</strong>rmalpower plant will be conducted. A 3D model is tobe built to predict tower deformation and itsperformance under various wind conditions.Simulation and modelling <strong>of</strong> <strong>the</strong> solar natural draftcooling tower will be carried out by <strong>the</strong> PhDstudent Zeng Zhang who started his study inMarch <strong>2010</strong>.Full economic study needs to be performed forboth conventional concrete cooling tower and <strong>the</strong>new design concepts as proposed in this paper.Once <strong>the</strong> study favours air-lift option, a scaledphysical model will be built and tested in ourmobile plant. Different wind loads will besimulated and <strong>the</strong> best stabilizing controlledmechanism will be identified. All modelling andsimulating results will also be confirmed by <strong>the</strong>laboratory testing results.Materials for <strong>the</strong> toroidal vessels, sealing skin andstiffening rings <strong>of</strong> <strong>the</strong> shroud play important rolesin cost reduction and durability <strong>of</strong> <strong>the</strong> tower. It is<strong>the</strong>refore required to search, identify and testdifferent materials suitable for <strong>the</strong> shroud andvessels.Optimisation <strong>of</strong> <strong>the</strong> area <strong>of</strong> solar collector and size<strong>of</strong> <strong>the</strong> tower for solar enhanced natural coolingtower will be carried in future by a PhD student.Stress analysis for tower structure for new designconcepts will be done to determine <strong>the</strong> strength <strong>of</strong><strong>the</strong> structure.<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>ConclusionsAir-lift cooling towers provide an alternative to <strong>the</strong>widely used concrete cooling tower used in powerindustries. This alternative will achieve aconstruction with minimum <strong>of</strong> time and expense.Since materials <strong>of</strong> <strong>the</strong> tower can be made <strong>of</strong>nonferrous and light materials, <strong>the</strong> resulting towerwill <strong>the</strong>refore be corrosion free and it will belightweight allowing quick installation with <strong>the</strong>advantages <strong>of</strong> easy disassembly and mobilisationat a minimum <strong>of</strong> time and effort. The whole towercan be reused in a new site.The inflatable donuts (cells) can be divided intoportions which are so arranged that malfunction <strong>of</strong>one or more <strong>of</strong> <strong>the</strong>m will not interfere withoperation <strong>of</strong> <strong>the</strong> tower as a whole. Suchredundancy provides reliable maintenance andrepair.The shroud is made <strong>of</strong> light material and can befactory manufactured in segments or as a whole.This provides for a quick and easy fieldinstallation. Since <strong>the</strong>re is less material (weight) tobe transported to <strong>the</strong> construction site, it willreduce <strong>the</strong> cost <strong>of</strong> transportation which may havesignificant impact when <strong>the</strong> site is located in aremote area.The most serious concern on air-lift cooling toweris its deformation and stabilization under strongwind which could affect <strong>the</strong> performance <strong>of</strong> <strong>the</strong>tower. Mechanism for improving design andcontrol will be identified.By adding solar collector to preheat <strong>the</strong> upstreamair temperature <strong>of</strong> <strong>the</strong> heat exchanger, it results amore air flow rate through <strong>the</strong> heat exchanger dueto a much higher buoyancy effect. This can ei<strong>the</strong>rreduce <strong>the</strong> tower size (for fixed heat sinking) orincrease <strong>the</strong> performance <strong>of</strong> <strong>the</strong> tower (for fixedtower size).A comparative life cycle cost analysis for bothconventional and <strong>the</strong> new design concepts <strong>of</strong>natural draft dry cooling tower is necessary infuture work.ReferencesBusch D., Harte R., Kra¨tzig W.B. and Montag U.2002, New natural draft cooling tower <strong>of</strong> 200 m <strong>of</strong>height, Engineering Structures 24 (2002) 1509–1521.Kröger, D.G. 2004, Air-Cooled Heat Exchangersand Cooling Towers, Penwell Corp., Tulsa, USA.Gurgenci, H., and Guan, Z. 2009, Dirigible naturaldraft cooling tower in geo<strong>the</strong>rmal and solar powerplant applications, 14th IAHR Cooling Tower andAir-cooled Heat Exchanger <strong>Conference</strong>, 1 to 3December 2009, Stellenbosch, South Africa.293


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>QGECE Research on Heat Exchangers and Air-Cooled CondensersKamel HoomanQueensland Geo<strong>the</strong>rmal <strong>Energy</strong> Centre <strong>of</strong> Excellence,The University <strong>of</strong> Queensland, Brisbane, Australiak.hooman@uq.edu.auAbstractThe aim <strong>of</strong> this paper is to give an overview <strong>of</strong> <strong>the</strong>research conducted at Queensland Geo<strong>the</strong>rmal<strong>Energy</strong> Centre <strong>of</strong> Excellence (QGECE) on aircooledcondensers for application in geo<strong>the</strong>rmalpower plants. The application <strong>of</strong> metal foam heatexchangers in Natural Draft Dry Cooling Towers(NDDCTs) has also been studied in detail.Samples <strong>of</strong> <strong>the</strong> numerical and experimentalresults are presented. These findings are <strong>the</strong>nbacked up by <strong>the</strong>oretical modelling that enablesus to run parametric studies which are sensible todifferent working/environmental conditions.Keywords: Air-cooled condensers, NDDCT, heatexchangers, <strong>the</strong>oretical, experimental, CFDIntroductionAustralia’s current policy targets an annualrenewable energy generation <strong>of</strong> 45,000 GWh by2020. Geo<strong>the</strong>rmal energy systems have <strong>the</strong>potential to produce a base load generationcapacity capable <strong>of</strong> replacing existing coal-firedplants. However, <strong>the</strong>re are some technicalchallenges to be overcome first. One <strong>of</strong> <strong>the</strong> majortechnical difficulties is <strong>the</strong> cooling system.Although wet cooling is more efficient than drycooling, water shortages and harsh environmentalconditions in areas such as <strong>the</strong> <strong>Australian</strong> deserthave forced designers to consider less efficientand more expensive air-cooled systems, or drycoolingas it is <strong>of</strong>ten termed.Air-cooled plants <strong>of</strong>fer potential economicadvantages due to plant sitting flexibility. Bothnatural draft and mechanical draft dry-coolingtowers, equipped with air-cooled heat exchangers(almost always with extended airside surfacearea), are used. The fan-driven systems can bebuilt quickly and at relatively low cost but <strong>the</strong>iroperating costs are higher due to <strong>the</strong>ir highermaintenance requirements and <strong>the</strong> parasiticlosses associated with running <strong>the</strong> fans. Thecooling system is a significant cost item in <strong>the</strong>power plant and affects <strong>the</strong> performance <strong>of</strong> <strong>the</strong>entire power cycle. If <strong>the</strong> cooling system does notprovide adequate cooling, <strong>the</strong> overall plantefficiency plunges with serious economicconsequences (e.g. decreased electricityproduction).It has been reported that approximately 0.3 GWh(per year) <strong>of</strong> electricity generation in <strong>the</strong> UnitedStates is lost because <strong>of</strong> cooling towers operatingbelow <strong>the</strong>ir design efficiency. This corresponds toan economic penalty <strong>of</strong> around 20 million USdollars per year [1]. It is <strong>the</strong>refore, very importantto design and analyse highly efficient dry coolingsystems for power plants.Though air-cooled condensers are not verypopular, <strong>the</strong>ir application to power industry is nota new practice. Interestingly, a hyperboloidcooling tower was patented in 1918. The reasonfor <strong>the</strong> renewed interest in air-cooled condensersis scarcity <strong>of</strong> water or high humidity [2]. In ei<strong>the</strong>rcase fan-cooled systems can lead to highparasitic losses. This makes <strong>the</strong> NDDCT an idealoption for such cases. The reason for QGECE’sinterest in NDDCT is obvious. Most <strong>of</strong> ourgeo<strong>the</strong>rmal resources are located where <strong>the</strong>re isno water. Besides, <strong>the</strong> <strong>the</strong>rmal efficiency <strong>of</strong> ourbinary power plants is already so low that wecannot afford parasitic losses (fans).MethodologyIn view <strong>of</strong> <strong>the</strong> above, QGECE has been lookinginto applying efficient heat exchangers to reduce<strong>the</strong> cost <strong>of</strong> towers. This would have beenimpossible unless a proper test bed is provided. Indoing so, a 2m height cooling tower is built and isoperational at our QGECE lab, see Figure 1.Figure 1: The QGECE lab scale model for a NDDCT.294


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>The tower has a square cross-section with1.4x1.4 m 2 base area and 0.9167x0.9167 m 2tower exit area. The heating elements are fourelectrically heated copper bars <strong>of</strong> 10 mmdiameter. At <strong>the</strong> same time, a numerical model isbuilt, as depicted by Figure 2, so that parametricstudy <strong>of</strong> <strong>the</strong> problem is possible [3]fluid flowing in <strong>the</strong> tubes undergoes phasechange. The same test section is used to collectdata for a finned-tube <strong>of</strong> 30 mm OD with (197 fins<strong>of</strong> 0.6 mm thickness per meter). This is a typicaldesign for an air-cooled condenser; similar to <strong>the</strong>ASPEN design one analysed in [3].Figure 2: The computational QGECE lab scale model for aNDDCT.Parallel to <strong>the</strong>se tests and simulations a<strong>the</strong>oretical model is developed to shed some lighton <strong>the</strong> scaling <strong>of</strong> such NDDCTs under no windconditions [4].A new design for tubes in air-cooled condensersis currently being examined at QGECE. The ideais to replace <strong>the</strong> fins by a layer <strong>of</strong> metal foams,see Figure 3, to increase <strong>the</strong> heat transfer areaand, hence, reduce <strong>the</strong> total tube numbers andheat exchanger size/cost [2]. This can significantlyreduce <strong>the</strong> cost as an efficient heat exchanger willlead to a less expensive (and shorter) coolingtower.Figure 4: The low speed wind tunnel test facility; <strong>the</strong> hotwater circulator and data acquisition system (sitting on <strong>the</strong>desk).Results and discussionCooling tower resultsExperiments are conducted to evaluate <strong>the</strong> towerfrictional (shape) resistance, i.e. by excluding <strong>the</strong>heat exchanger resistances. A total <strong>of</strong> 25 datapointswere used to measure <strong>the</strong> air temperatureat <strong>the</strong> exit from <strong>the</strong> tower, as depicted by Figure 5.The results are <strong>the</strong>n compared to numerical and<strong>the</strong>oretical predictions. The result from <strong>the</strong>temperature measurements involves <strong>the</strong>uncertainty <strong>of</strong> measurements which is estimatedby using a basic uncertainty analysis [6]. Themeasured air velocity at <strong>the</strong> exit is 0.543±0.064m/s which is very close to both <strong>the</strong>oretical (0.515m/s) and numerical (0.515 m/s) predictions.Figure 3: The metal foam-wrapped tube used in QGECE labsto conduct experiments on air-cooled condensers.Theoretical and numerical analysis <strong>of</strong> such foamwrappedtubes in air-cooled condensers havebeen reported in an earlier study [5]. Thus,experimental analysis followed initial high-level<strong>the</strong>oretical investigations. Figure 4 illustrates aphoto <strong>of</strong> our test section where air is forced (by asuction fan) to flow over a heated metal foamwrappedtube. The tube surface temperature iskept constant by using a circulation heater thatpumps water (at adjustable flow rates) through <strong>the</strong>tube to keep <strong>the</strong> tube surface temperature uniformand constant similar to a condenser where <strong>the</strong>Figure 5: The location <strong>of</strong> <strong>the</strong> <strong>the</strong>rmocouples to measure <strong>the</strong>air temperature at <strong>the</strong> exit from <strong>the</strong> tower.295


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>The following formula [4] has been used to predict<strong>the</strong> tower inlet velocity, U, for <strong>the</strong> empty towerheat transfer to pressure drop ratio) <strong>of</strong> <strong>the</strong> foamheat exchanger is higher than that <strong>of</strong> an ASPENdesigned finned- tube one; see Figure 7.(1)and for <strong>the</strong> case where heat exchangers introducea resistance to flow(2)with k, g, K, H, t, C F , and Δρ being <strong>the</strong> frictionalloss coefficient, gravitational acceleration, bundlepermeability, <strong>the</strong> tower height, <strong>the</strong> bundlethickness, form drag coefficient, <strong>the</strong> inlet-outlet airdensity difference, respectively.Figure 6 illustrates <strong>the</strong> results <strong>of</strong> numericalsimulations compared to <strong>the</strong>oretical predictionsfor taller cooling towers where <strong>the</strong> bundle velocityis plotted versus <strong>the</strong> tower height on a log-logscale. The 200m tower is designed to dump 283MW <strong>of</strong> heat for a power plant that generates50MWe [3]. The volumetric heat generation ratesfor shorter towers are <strong>the</strong>n scaled down andimplemented as inputs to our CFD simulations. Asseen, <strong>the</strong> developed <strong>the</strong>ory in [4] is capable <strong>of</strong>predicting <strong>the</strong> <strong>the</strong>rmohydraulic performance <strong>of</strong> aNDDCT under no wind conditions. However, aswind can dramatically affect <strong>the</strong> performance <strong>of</strong> aNDDCT [7-12], QGECE is focusing on betterunderstanding <strong>of</strong> <strong>the</strong> effects <strong>of</strong> cross-wind onscaling <strong>of</strong> <strong>the</strong> cooling towers.Bundle Velocity (m/s)4.13.83.53.22.92.62.32Theoretical PredictionNumerical (CFD)1.720 50 80 110 140 170 200Tower Height (m)Figure 6: Numerical and <strong>the</strong>oretical prediction <strong>of</strong> bundlevelocity for towers <strong>of</strong> different heights.Metal foam resultsIn our last year report at <strong>Australian</strong> Geo<strong>the</strong>rmal<strong>Conference</strong>, it was numerically shown that <strong>the</strong>metal foams can be used in air-cooledcondensers with a potential to reduce <strong>the</strong> size andcost <strong>of</strong> <strong>the</strong> condensers [13]. It has been arguedthat <strong>the</strong> area goodness factor (j/f; dimensionlessFigure 7: Normalized area goodness factor versus porouslayer thickness for different samples and free streamvelocities (samples 2-7 refer to commercially available ERGmetal foam samples).[13]Figure 8 illustrates a sample <strong>of</strong> our recentlycollected experimental data. This figure showsplot <strong>of</strong> heat transfer ratio versus <strong>the</strong> approachingair velocity.Foam/fin heat transfer ratio32.82.62.42.221.81.61.41.211 3 5 7 9 11Face Velocity (m/s)Figure 8: Heat transfer ratio (foam-wrapped tube divided byfinned-tube) versus face velocity. Finned-tube is designed byASPEN where tubes are 30 mm OD with 197 fins per meter.Fin diameter is 60 mm and <strong>the</strong> fin plate thickness is 0.6 mm;see [3] for more details.Interestingly, with <strong>the</strong> same pressure drop, <strong>the</strong>heat transfer from a foam-wrapped tube is always296


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>higher than that <strong>of</strong> a finned tube. The ratio canfigure out at 2.6 at high velocities which can leadto more compact tube bundles and thus results indecreasing <strong>the</strong> capital cost. This gain for fancooledsystems can lead to significantly reducedparasitic loses as with new design <strong>the</strong> number <strong>of</strong>bundles is almost halved (so are <strong>the</strong> parasiticlosses). Fur<strong>the</strong>rmore, <strong>the</strong> pressure drop in <strong>the</strong> aircooled condenser is reduced as <strong>the</strong> number <strong>of</strong> <strong>the</strong>bundles is almost halved. Ano<strong>the</strong>r point in favour<strong>of</strong> such compact systems is <strong>the</strong> lower tube-sidepressure drops because <strong>of</strong> <strong>the</strong> elimination <strong>of</strong> alarge number <strong>of</strong> <strong>the</strong> tubes in <strong>the</strong> condenser.Concluding remarksAn accurate model, compared to experimentaland CFD results, is developed to predict <strong>the</strong> heatand fluid flow through NDDCTs. Metal foam heatexchangers are tested and found to be superior t<strong>of</strong>ins for air-cooled condensers. Fur<strong>the</strong>r research isplanned at QGECE to examine different workingand environmental conditions.References[1] North American Electric ReliabilityCouncil, Generating Availability Data SystemReport, Princeton, NJ, 1986.[2] Hooman K, Gurgenci H. Different heatexchanger options for natural draft cooling towers.World Geo<strong>the</strong>rmal Congress Nusa Dua, Bali,Indonesia <strong>2010</strong>: Paper # 2633.[3] Hooman K, Gurgenci H. Porous mediummodelling <strong>of</strong> air-cooled condensers. Transport inPorous Media 84 (<strong>2010</strong>): 257-273.[4] Hooman K. Dry cooling towers ascondensers for geo<strong>the</strong>rmal power plants.International Communications in Heat and MassTransfer <strong>2010</strong>;in press.[5] Odabaee M, Hooman K, Gurgenci H.Metal foam heat exchangers for heat transferaugmentation from a cylinder in cross-flow.Transport in Porous Media <strong>2010</strong>;in press.[6] Mee DJ. Uncertainty analysis <strong>of</strong>Conditions in <strong>the</strong> test section <strong>of</strong> <strong>the</strong> T4 shocktunnel, Department Research Report # 1993/4,Division <strong>of</strong> Mechanical Engineering, TheUniversity <strong>of</strong> Queensland, Brisbane, Australia,1993.[7] Kroger DG. Air-cooled heat exchangersand cooling towers. Pennwell Corp., 2004.[8] Al-Waked R, Behnia M. The Effect <strong>of</strong>Windbreak Walls on <strong>the</strong> Thermal Performance <strong>of</strong>Natural Draft Dry Cooling Towers. Heat TransferEngineering 26(2005): 50-62.[9] Zhai Z, Fu S. Improving cooling efficiency<strong>of</strong> dry-cooling towers under cross-wind conditionsby using wind-break methods. Applied ThermalEngineering 26 (2006): 1008-1017.[10] Sabbagh-Yazdi SR, Goudarzi MA,Mastorakis N. Solution <strong>of</strong> Internal and ExternalWind Induced Pressure for a Single CoolingTower in Kazerun Power Plant (IRAN), in: S.H.Sohrab, H.J. Catrakis, N. Kobasko, S. Necasova,N. Markatos (Eds.), 6th IASME/WSEASInternational <strong>Conference</strong> on Fluid Mechanics andAerodynamics; 2008 Aug 20–22, World Scientificand Engineering Academy and Society, Rhodes,Greece.[11] Liu BM. Numerical Prediction for <strong>the</strong>Performance <strong>of</strong> a Natural Draft Cooling Towerwith Comparison to <strong>the</strong> Field Test Data, in: G.F.Hewitt (Ed.), 10th International Heat Transfer<strong>Conference</strong>; 1994 Aug 14–18, Institute <strong>of</strong>Chemical Engineers, Brighton, England.[12] Iovino G, Mattoni H, Mazzocchi L, SenisR, Vanzan R. Optimal Sizing <strong>of</strong> Natural Draft, DryCooling Towers for ENEL Combined CyclePower-Plants, in: S.S. Stecco, M.J. Moran (Eds.),Florence World <strong>Energy</strong> Research Symp; 1990May 28–Jun 01, Pergamon Press Ltd, Florence,Italy.[13] Odabaee M, Hooman K, Gurgenci H.Comparing <strong>the</strong> tube fin heat exchangers to metalfoam heat exchangers. <strong>Australian</strong> Geo<strong>the</strong>rmal<strong>Energy</strong> <strong>Conference</strong>, Brisbane, Australia,November 11-13, 2009.297


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Equation-Free Summary <strong>of</strong> <strong>the</strong> <strong>2010</strong> Ma<strong>the</strong>matics in Industry StudyGroup on Geo<strong>the</strong>rmal Data Analysis and OptimizationRobert McKibbin 1 ,*Franklin G. Horowitz 2,3 , Neville Fowkes 4 , Brendan Florio 41 Massey University Institute <strong>of</strong> Information & Ma<strong>the</strong>matical Sciences2 Western <strong>Australian</strong> Geo<strong>the</strong>rmal Centre <strong>of</strong> Excellence,The University <strong>of</strong> Western Australia 3 School <strong>of</strong> Earth & Environment and 4 School <strong>of</strong> Ma<strong>the</strong>matics & Statistics,AbstractThe Australia and New Zealand Industrial andApplied Ma<strong>the</strong>matics (ANZIAM) division <strong>of</strong> <strong>the</strong><strong>Australian</strong> Ma<strong>the</strong>matical Society (AustMS) held itsannual Ma<strong>the</strong>matics and Statistics-in-IndustryStudy Group (MISG) both at RMIT in Melbourne,and via telepresence at UWA using <strong>the</strong> accessgrid from <strong>the</strong> 7 th through <strong>the</strong> 12 th <strong>of</strong> February<strong>2010</strong>. The Geo<strong>the</strong>rmal Working Group attracted atotal <strong>of</strong> 18 academic, pr<strong>of</strong>essional, post-doctoral,and post-graduate applied ma<strong>the</strong>maticians ando<strong>the</strong>rs to study problems <strong>of</strong> potential interest to<strong>the</strong> geo<strong>the</strong>rmal projects in <strong>the</strong> Perth Basin HotSedimentary Aquifer plays. In <strong>the</strong> interests <strong>of</strong>attracting <strong>the</strong> wider AGEC community’s attentionto <strong>the</strong> annual MISG efforts, reproduced below is<strong>the</strong> “Equation Free Summary” <strong>of</strong> <strong>the</strong> week-longintensive effort. The detailed summary paper andseveral flow-on papers are currently beingprepared for publication. The author list <strong>of</strong> thiscurrent document are comprised <strong>of</strong> <strong>the</strong> so-called“Industry Representative”, <strong>the</strong> “ProjectModerators”, and “Student Moderator”. A full list <strong>of</strong><strong>the</strong> participants in <strong>the</strong> geo<strong>the</strong>rmal study group arefound in Appendix 1.Equation-Free SummaryThe aim <strong>of</strong> this project was to assess <strong>the</strong>economic feasibility <strong>of</strong> extracting geo<strong>the</strong>rmalenergy from <strong>the</strong> deep sedimentary Perth Basin inWestern Australia. The WA Geo<strong>the</strong>rmal Centre <strong>of</strong>Excellence (WAGCoE), based in UWA, has beencollecting data from (groundwater and oil)boreholes in <strong>the</strong> area as well as examiningremotely-sensed observational data <strong>of</strong> groundsurface temperatures. The question was how tointerpret <strong>the</strong> available data to gain information on<strong>the</strong> modes <strong>of</strong> <strong>the</strong>rmally-driven convective flows, ifany, in <strong>the</strong> groundwater aquifers, <strong>the</strong>rebydetermining which parts <strong>of</strong> <strong>the</strong> system would bemost economical to use for energy extraction.The <strong>2010</strong> MISG "Geo<strong>the</strong>rmal" study groupconcentrated on problems <strong>of</strong> advective transport<strong>of</strong> heat in stratified geological units appropriate for<strong>the</strong> conditions found in <strong>the</strong> Perth Basin <strong>of</strong> WesternAustralia. The main hypo<strong>the</strong>sis examined – forseveral different sub-problems – is that advectivetransport <strong>of</strong> heat is an important contribution to<strong>the</strong> overall heat transport. Measuredtemperatures in <strong>the</strong> system indicate anapproximate temperature increase through <strong>the</strong>main aquifers from about 40 ˚C to 80 ˚C. Clearly,conductive heat transport is present (aselsewhere over <strong>the</strong> Earth's surface), but wedesired to find out whe<strong>the</strong>r <strong>the</strong> system issusceptible to "unforced" or natural convection.There is a well-developed <strong>the</strong>ory in <strong>the</strong> fluidmechanics/porous media literature about <strong>the</strong>conditions required for convective instability innon-homogeneous permeable systems that areheated from below. The criterion manifests itselfin a dimensionless combination <strong>of</strong> <strong>the</strong>rmodynamicand rock matrix parameters known as <strong>the</strong>Rayleigh number, denoted Ra. This was seen asrelevant for our study, so we concentrated onusing <strong>the</strong> available field data to determinewhe<strong>the</strong>r or not conditions in <strong>the</strong> Perth Basin wouldbe right or not.It is likely <strong>the</strong>re is also an advective transportcomponent due to a hydraulic gradient from arecharge zone assumed to be at an elevatedheight in <strong>the</strong> Darling escarpment to <strong>the</strong> east,westwards to a discharge zone assumed to be<strong>of</strong>fshore. However, for <strong>the</strong> purposes <strong>of</strong> most <strong>of</strong>our sub-problems, we neglected <strong>the</strong> hydraulicgradient effects.The geological backgroundRocks <strong>of</strong> <strong>the</strong> Perth Basin consist <strong>of</strong> multiple layers<strong>of</strong> sedimentary strata, where matrix (as opposedto fracture) hydraulic permeability is expected tobe dominant. Immediately below <strong>the</strong> groundsurface, <strong>the</strong>re is an unconfined aquifer consisting<strong>of</strong> rocks geologically known as <strong>the</strong> "superficial"formations. These rocks are underlain by variousshallow confined aquifers consisting <strong>of</strong> rocks <strong>of</strong><strong>the</strong> Kings Park Formation (locally), <strong>the</strong> LeedervilleFormation, and <strong>the</strong> South Perth Formation. For<strong>the</strong> study group's convenience, since <strong>the</strong>se rocksare not in hydraulic communication with <strong>the</strong>deeper and hotter aquifers, we lumped all <strong>of</strong> <strong>the</strong>seaquifers toge<strong>the</strong>r into a group we labelled(perhaps confusingly to people familiar with <strong>the</strong>stratigraphy) as <strong>the</strong> "superficial" units andbasically ignored <strong>the</strong>m (o<strong>the</strong>r than <strong>the</strong> boundaryconditions <strong>the</strong>y provide) in our models.At a depth assumed for our purposes to be about600 m we find <strong>the</strong> top <strong>of</strong> a confined aquiferconsisting <strong>of</strong> rocks from <strong>the</strong> Gage Formation.Those rocks are assumed to be about 200 mthick, with uniform physical properties. Below <strong>the</strong>Gage, but in hydraulic communication with it, wefind rocks <strong>of</strong> <strong>the</strong> Yarragadee Formation. Thecontact between <strong>the</strong> two formations is anerosional unconformity, so <strong>the</strong> thicknesses <strong>of</strong> <strong>the</strong>two units vary with map position. The rocks <strong>of</strong> <strong>the</strong>Yarragadee are assumed to be about 1000 mthick, also with uniform physical properties.298


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>(These assumptions <strong>of</strong> uniform rock propertieswere relaxed in various ways in several <strong>of</strong> oursub-problems.) Below <strong>the</strong> Yarragadee lie <strong>the</strong>rocks <strong>of</strong> <strong>the</strong> Cadda Formation, about 600 m thick,also in hydraulic communication with <strong>the</strong>Yarragadee. Indeed, in <strong>the</strong> groundwatercommunity, rocks <strong>of</strong> all three formations (Gage,Yarragadee, and Cadda) are <strong>of</strong>ten called <strong>the</strong>"Yarragadee Aquifer".Below <strong>the</strong> Cadda Formation lie rocks <strong>of</strong> <strong>the</strong>Cattamarra Coal Measures. These rocks aredominantly shales, with interbedded sandstonelayers. Hence, we treat <strong>the</strong> basal contact <strong>of</strong> <strong>the</strong>Cadda with <strong>the</strong> Cattamarra as being a hydraulicseal.The result is our basic model <strong>of</strong> three stratifiedlayers, with physical properties internally uniform,all participating in a single hydraulically connectedsystem.Well Log constraintsThe closest deep borehole to <strong>the</strong> sites <strong>of</strong>WAGCoE's proposed exploitation systems is <strong>the</strong>Cockburn Number 1 oil well. Cockburn 1 wasdrilled in 1967, to a total depth <strong>of</strong> 10,020 feet(3054 m), with cores recovered from severaldiscrete sites within <strong>the</strong> bore. Results <strong>of</strong>laboratory measurements <strong>of</strong> porosity, permeabilityand o<strong>the</strong>r physical parameters from <strong>the</strong>se coresare found in <strong>the</strong> well completion report. Such welllogs have been used to try to determine a relationbetween porosity and permeability from <strong>the</strong> coremeasurements; it yielded two different estimates<strong>of</strong> <strong>the</strong> vertical distribution <strong>of</strong> permeability.Statistics from <strong>the</strong>se estimates were used in <strong>the</strong>sub-problem concerned with estimating Rayleighnumbers and critical values <strong>the</strong>re<strong>of</strong> for our PerthBasin problem.Ma<strong>the</strong>matical modellingThe usual modelling paradigm for such problemsis to use a spatially averaged continuumapproximation for <strong>the</strong> rock matrix and fluidcomponents <strong>of</strong> <strong>the</strong> system. Standard fluid mass,fluid momentum (Darcy's law in this case) and<strong>the</strong>rmal energy conservation laws enable a set <strong>of</strong>differential equations to be formulated. Withappropriate geometric and <strong>the</strong>rmal boundaryconditions, <strong>the</strong> ma<strong>the</strong>matical problem may besolved; usually this has to be completed usingnumerical techniques since <strong>the</strong> equations and <strong>the</strong><strong>the</strong>rmodynamic parameters are non-linear.However, with simplified geometry and certainassumptions, <strong>the</strong> ma<strong>the</strong>matical problem istractable using analytic methods.Some numbersTo get an idea <strong>of</strong> <strong>the</strong> times and fluid speedsinvolved, we estimated that a water particledescending into <strong>the</strong> aquifer in <strong>the</strong> Darling Rangewould flow underground to <strong>the</strong> west at a speed <strong>of</strong>about 3.5 m year –1 , and take about 8,500 years tocomplete <strong>the</strong> 30 km journey.If "waste" fluid from a geo<strong>the</strong>rmal energyinstallation was pumped into <strong>the</strong> aquifer at a rate<strong>of</strong> 100 l s –1 , after 1 year <strong>the</strong> injected fluid wouldhave penetrated to a radius <strong>of</strong> about 100 m, with<strong>the</strong> fluid speed at <strong>the</strong> cylindrical front being about50 m year –1 at that time. This speed issignificantly greater than <strong>the</strong> estimated naturalflow above, so <strong>the</strong> injected fluid would be likely topenetrate <strong>the</strong> aquifers "upstream" against <strong>the</strong>natural slow current.Convective instabilitySome effort was spent in attempting to determinewhe<strong>the</strong>r <strong>the</strong> system was prone to convectiveinstability; this would, according to <strong>the</strong>ory andexperiment, result in large-scale convective "rolls"<strong>of</strong> fluid motion that sought to augment <strong>the</strong>conductive heat transport. A series <strong>of</strong> alignedrolls, each in counter-rotation to its neighbours,would induce hot spots or alignments near <strong>the</strong>ground surface, as well as cooler areas near <strong>the</strong>downflows. A consequent question was: Could<strong>the</strong> associated perturbed iso<strong>the</strong>rm patterns andnon-uniform surface heat flux actually bemeasured? Even if <strong>the</strong>re was convection, howwould we know <strong>the</strong> pattern?Figure 1 shows a simple idealized model <strong>of</strong> aporous slab that has a base maintained at auniform constant temperature that is higher thanthat at <strong>the</strong> top. The hotter fluid near <strong>the</strong> bottom isless dense than <strong>the</strong> cooler fluid near <strong>the</strong> top.Provided <strong>the</strong> net buoyancy force can overcomeviscous resistance everywhere, convective motionis induced. The most unstable mode is a set <strong>of</strong>longitudinal "rolls".Figure 1: Idealized set-up for a permeable slab subjected toa vertical temperature gradient.Linear perturbation <strong>the</strong>ory for <strong>the</strong>rmal convectionin this idealized porous medium that is laterallyunconfined determines that, for a uniform matrix,<strong>the</strong> critical value <strong>of</strong> <strong>the</strong> Rayleigh number is Ra crit =4 2 , with <strong>the</strong> most unstable mode being horizontalrolls with square cross-sectional boundaries. If<strong>the</strong> temperature gradient in <strong>the</strong> system is toosmall, so that Ra has a sub-critical value, <strong>the</strong>n <strong>the</strong>heat transfer mechanism is conductive only.Above critical, heat transfer is by conduction andconvection. The simplified <strong>the</strong>ory assumes a299


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>linearization <strong>of</strong> <strong>the</strong>rmodynamic parametersaround a certain temperature.When <strong>the</strong> iso<strong>the</strong>rmal bounding surface above is atground level some distance above <strong>the</strong> porousregion, <strong>the</strong> above results are modified. Theiso<strong>the</strong>rms near <strong>the</strong> top <strong>of</strong> <strong>the</strong> convection regionare <strong>the</strong>n not horizontal. This is shownschematically in Figure 2, which also indicates <strong>the</strong>general form <strong>of</strong> <strong>the</strong> convective rolls.Figure 2: Schematic <strong>of</strong> longitudinal rolls in <strong>the</strong> permeableaquifer beneath a confining stratum, with an exampleperturbed iso<strong>the</strong>rm near <strong>the</strong> top <strong>of</strong> <strong>the</strong> convection region.Associated with supercritical conditions is anenhancement <strong>of</strong> <strong>the</strong> heat transfer. This increaseswith temperature gradient; <strong>the</strong> general trend <strong>of</strong> <strong>the</strong>so-called Nusselt number Nu, defined as <strong>the</strong> ratio<strong>of</strong> heat transferred by conduction plus convectionto that transferred by conduction alone, is shownin Figure 3.Figure 3: Trend <strong>of</strong> Nusselt number Nu with Rayleighnumber Ra; compilation <strong>of</strong> results from various <strong>the</strong>oreticaland experimental studies (from Nield & Bejan, 2006).First we considered a homogenized matrix systemwhere <strong>the</strong> rock parameters were assumeduniform with somewhat arbitrarily-averagedvalues from <strong>the</strong> borehole core values. Thecalculated values <strong>of</strong> Ra exceeded <strong>the</strong> criticalvalue only for high enough (and perhapsunrealistic) values <strong>of</strong> <strong>the</strong> datum. However, <strong>the</strong>lack <strong>of</strong> euphoria was briefly tempered by <strong>the</strong>thought that <strong>the</strong> layering <strong>of</strong> <strong>the</strong> system mayinfluence <strong>the</strong> calculation. It was fur<strong>the</strong>rdetermined from <strong>the</strong> <strong>the</strong>ory that anisotropy <strong>of</strong><strong>the</strong>rmal conductivity and permeability <strong>of</strong> <strong>the</strong> matrixproduces an estimate <strong>of</strong> <strong>the</strong> critical Rayleighnumber that is different from that for ahomogeneous system.Anisotropy in <strong>the</strong> <strong>the</strong>rmal conductivity <strong>the</strong>oreticallyincreases <strong>the</strong> critical Rayleigh number; however,<strong>the</strong> conductivity <strong>of</strong> rocks varies very little, so <strong>the</strong>anisotropy in that parameter is negligibly differentfrom unity (measured data gave a value <strong>of</strong> around1.06). Anisotropy in permeability is induced bymaterial layering. Geological strata necessarilyinduce a permeability that is averagely greater in<strong>the</strong> bedding plane than perpendicular to it. Whatis more, such anisotropy generally reduces <strong>the</strong>(<strong>the</strong>oretical) critical Rayleigh number!Amidst some excitement, an assessment <strong>of</strong> thisanisotropy, from a ra<strong>the</strong>r complicated set <strong>of</strong> rockcore measurements and well logs, was made as astratum-thickness weighted average <strong>of</strong> intrinsicrock permeabilities, with <strong>the</strong> result that <strong>the</strong>horizontal value is about 4.6 times that in <strong>the</strong>vertical. These estimates reduced <strong>the</strong> criticalRayleigh number to 21.6, about half thatcomputed from <strong>the</strong> homogenized parameters.Immediately, it became possible that conditionsfor convection may be met, even using <strong>the</strong>linearised <strong>the</strong>ory with <strong>the</strong> lowest datumtemperature (40 ˚C) for <strong>the</strong> linearised calculations.Convective rolls and heat transferIn optimistic anticipation <strong>of</strong> such a result, a smallgroup had been working on how enhanced heattransfer in <strong>the</strong> Yaragadee Aquifer would manifestitself in <strong>the</strong> temperature distribution in <strong>the</strong> nearsurfacesuperficial formations. This is a fairlystandard problem in heat transfer, and quickprogress was made. However, it was shown that<strong>the</strong>re would be a very small signature at groundsurface level, and instrumentation would have tobe sensitive and widespread to obtain significantmeasurements. So, this encapsulated <strong>the</strong>problem overall: Even if <strong>the</strong>re was a convectiveprocess at work, how would measurements beable to be made to detect <strong>the</strong> upflow anddownflow regions? So, how could advantage betaken <strong>of</strong> <strong>the</strong> convection even if <strong>the</strong> Ra estimateswere correct?The UWA GroupiesOver in WA, <strong>the</strong> small "at home" group wasworking; with <strong>the</strong> assumption that convection wasoccurring, <strong>the</strong>y trawled <strong>the</strong> literature forinformation about <strong>the</strong>oretical work on layeringeffects on cell-size, and <strong>the</strong> stability <strong>of</strong> suchconvection cells. The idea was that significant300


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>sub-layering caused by thick differentlypermeablestrata might produce vertically-alignedbut largely separated co-rotating cells that, intandem, would advect heat from <strong>the</strong> hot base to<strong>the</strong> surface. At <strong>the</strong> end <strong>of</strong> <strong>the</strong> week, no firmconclusions had been able to be made.SimulationDriven by concern that <strong>the</strong> <strong>the</strong>rmodynamicproperties <strong>of</strong> water were being approximated tooseverely in <strong>the</strong> linear stability <strong>the</strong>ory, a numericalsimulation <strong>of</strong> 2-D rolls was made using acommercial computer package. This allowedmore accurate values for <strong>the</strong> water's temperaturedependentdensity, viscosity, etc. to be used.While <strong>the</strong> simulations were completed post-MISG,it turned out that <strong>the</strong>re were only small qualitativedifferences in <strong>the</strong> flow patterns.Slope-induced <strong>the</strong>rmal convectionA late idea resulted from current work by one <strong>of</strong><strong>the</strong> group members; it considers <strong>the</strong> possibilitythat longitudinal convection may be induced in asloping aquifer by a near-vertical temperaturegradient. The warmer fluid near <strong>the</strong> bottom wouldmove up-slope (in this case, towards <strong>the</strong> east)while <strong>the</strong> returning cooler fluid near <strong>the</strong> top movesdown-slope. It was not clear how this would affect<strong>the</strong> possible exploitation, because <strong>the</strong>temperature pr<strong>of</strong>ile would remain conductive, andonly be altered by convective rolls as werealready considered above.A small group <strong>of</strong> postgraduate students from <strong>the</strong>group seized upon some aspects <strong>of</strong> this, and <strong>the</strong>irefforts will be rewarded by co-authorship <strong>of</strong> apaper to be submitted later in <strong>the</strong> year. A moregeneral case will be considered, where inducedconvection in a layered sloping aquifer isinvestigated for optimal net convective heattransport by such a mechanism, as well as <strong>the</strong>stability <strong>of</strong> such motion to longitudinal rolls. Theenthusiasm to participate in this way reinforces<strong>the</strong> benefits <strong>of</strong> MISG to engagement <strong>of</strong> postgradsin ma<strong>the</strong>matical enquiry into useful applications.SummaryThe problem was tractable, but depended onsuitable estimates <strong>of</strong> rock matrix properties fromdrill cores and well logs which were ra<strong>the</strong>rcomplex in structure. It also depended on goodestimates <strong>of</strong> aquifer temperatures; <strong>the</strong> deepervalues were elusive, and had to be deduced fromextrapolations <strong>of</strong> shallow well measurements.However, by <strong>the</strong> end <strong>of</strong> <strong>the</strong> study week, <strong>the</strong>re wasa good increase <strong>of</strong> understanding <strong>of</strong> <strong>the</strong> problem,<strong>the</strong> issues to be resolved, and possiblemechanisms at work in <strong>the</strong> Perth Basin.Geo<strong>the</strong>rmal systems are complicated geologicalgeophysical-<strong>the</strong>rmodynamicalentities. A multidisciplinaryapproach to understanding <strong>the</strong>m isnecessary. However, <strong>the</strong> quantification <strong>of</strong> <strong>the</strong>irattributes is well-handled by ma<strong>the</strong>matically-ablescientists and <strong>the</strong> MISG proved a suitable venueto tackle <strong>the</strong> WAGCoE problem.Keywords: Convection, Hot SedimentaryAquifers, AnisotropyReferenceNield, D. A., & Bejan, A. (2006). Convection inPorous Media . Springer, 3rd ed.AppendixParticipants in <strong>the</strong> <strong>2010</strong> MISG Geo<strong>the</strong>rmal StudyGroup (alphabetically by surname):Nurul Syaza Abdul Latif, Massey University NZManarah Eraki, (Affiliation Missing)Brendan Florio, University <strong>of</strong> Western AustraliaNeville Fowkes, University <strong>of</strong> Western AustraliaLuke Fullard, Massey University, NZTony Gibb, Consultant, South AustraliaNick Hale, Oxford University, UKDes Hill, University <strong>of</strong> Western AustraliaFrank Horowitz, University <strong>of</strong> Western AustraliaGrant Keady, University <strong>of</strong> Western AustraliaThiansiri (Pat) Luangwilai, ADFA, AustraliaFleur McDonald, Massey University, NZRobert McKibbin, Massey University, NZMelanie Roberts, University <strong>of</strong> Western AustraliaThomas Stemler, University <strong>of</strong> Western AustraliaRob Style, Oxford University, UKChristian Thomas, University <strong>of</strong> Western AustraliaNicole Walters, Victoria University <strong>of</strong> Wellington,NZ301


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Status <strong>of</strong> Compliance With The Geo<strong>the</strong>rmal Reporting CodeJim Lawless*, Graeme Beardsmore, Malcolm Ward, Fiona Holgate and Graham Jeffress*SKM PO Box 9806 Newmarket, Auckland, NZJLawless@skm.co.nzAbstractThe <strong>Australian</strong> Geo<strong>the</strong>rmal Reporting Code hasnow been in operation since late 2008. The Codecurrently operates on a voluntary basis and as yethas no legal status or sanctions. However, in late2008 AGEA members agreed that its use inPublic Reports would be mandatory for <strong>the</strong>m anda Compliance Subcommittee (currentlycomprising <strong>the</strong> above authors) was established.The Subcommittee has since reviewed all PublicReports that we have become aware <strong>of</strong> to checkfor compliance. This paper presents an analysis<strong>of</strong> instances <strong>of</strong> non-compliance broken intoseveral categories but without identification <strong>of</strong> <strong>the</strong>companies concerned. In each case <strong>the</strong>company concerned was informally notified about<strong>the</strong> issue. In general <strong>the</strong>re has been a high level<strong>of</strong> willingness to comply with <strong>the</strong> Code andcompanies have responded positively to anyissues raised. Most instances <strong>of</strong> non-compliancehave been <strong>of</strong> a procedural nature such as omittingto include Competent Person statements in publicpresentations which include resource estimates.The experience gained has been valuable andhas been taken into account in drawing up <strong>the</strong>Second Edition <strong>of</strong> <strong>the</strong> Code and its accompanyingLexicon. O<strong>the</strong>r jurisdictions have been studying<strong>the</strong> <strong>Australian</strong> Code which has led to an almostidentical Code being established in Canada. It iscurrently understood that consideration is alsobeing given to equivalent Codes in <strong>the</strong> USA andEurope. The benefits <strong>of</strong> <strong>the</strong> <strong>Australian</strong> Code arebeing appreciated even in countries where it hasno formal standing and Code compliant reportshave recently been produced on resources inChile and Indonesia.Keywords: Geo<strong>the</strong>rmal, resources, reserves,compliance, Australiapaper presents an analysis <strong>of</strong> instances <strong>of</strong> noncompliance,broken into several categories, butwithout identification <strong>of</strong> <strong>the</strong> companies concerned.AnalysisMost instances <strong>of</strong> non-compliance have been <strong>of</strong> aprocedural nature such as omitting to includeCompetent Person (CP) statements in publicpresentations which include resource estimates.It is safe to say that <strong>the</strong>re has been no case <strong>of</strong> anapparent intention to issue misleadinginformation, though a few statements have vergedon <strong>the</strong> over-enthusiastic at times.Figure 1 shows <strong>the</strong> number <strong>of</strong> reports reviewedand number <strong>of</strong> companies concerned againsttime. As is to be expected, <strong>the</strong> number hasincreased with time but has fluctuated dependingon <strong>the</strong> quarterly and annual reporting cycle aswell as <strong>the</strong> frequency <strong>of</strong> reviews. The latestreview has shown a drop in <strong>the</strong> number <strong>of</strong> reportsand several companies which have previouslyreported have not done so, which perhaps reflects<strong>the</strong> generally static state <strong>of</strong> <strong>the</strong> industry at thistime.IntroductionThe <strong>Australian</strong> Geo<strong>the</strong>rmal Reporting Code hasnow been in operation since late 2008. The Codecurrently operates on a voluntary basis and as yethas no legal status. However, in late 2008 AGEAmembers agreed that its use in Public Reportswould be mandatory for <strong>the</strong>m and a ComplianceSubcommittee (currently comprising <strong>the</strong> aboveauthors) was established under <strong>the</strong> Joint<strong>Australian</strong> Geo<strong>the</strong>rmal Reporting CodeCommittee (JAGRCC). The Subcommittee hassince reviewed all Public Reports that we havebecome aware <strong>of</strong> to check for compliance. ThisFigure 1: Reports reviewed and number <strong>of</strong> companies withtimeFigure 2 show <strong>the</strong> percentage <strong>of</strong> reports whichhave been considered fully compliant. Although<strong>the</strong>re is still significant room for improvement, it ispleasing to see this increasing with time.Fur<strong>the</strong>rmore, a simple percentage does not reflectthat <strong>the</strong> initial instances <strong>of</strong> non-compliance weregenerally more significant and those recently havegenerally been <strong>of</strong> a less serious nature. Thecompanies have clearly embraced <strong>the</strong> reportingprocess and learned from it. It would also be fair302


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>to say that <strong>the</strong> Compliance Sub-committee hasalso refined <strong>the</strong>ir understanding and criteria overtime.investors, is a Public Report under <strong>the</strong> Code, so<strong>the</strong> fundamental principle <strong>of</strong> requiring a CPstatement has been adhered to. In reaching thisconclusion <strong>the</strong> JAGRCC has adhered to astanding practice <strong>of</strong> consistency with <strong>the</strong> Joint OreReserve Committee (JORC) Code for mineralsresource statements on which <strong>the</strong> Geo<strong>the</strong>rmalCode was originally modelled.Wrong terminology. This has largely been amatter <strong>of</strong> companies coming to terms with <strong>the</strong>resource and reserve categories, and <strong>the</strong>re arenow few problems with <strong>the</strong> latest reports.Figure 2: Percentage <strong>of</strong> fully compliant reports with timeInadequate detail. This has been a muchdebatedissue, as <strong>the</strong>re is a tension betweenproviding so much information as to make reportstoo complex for <strong>the</strong> average investor while at <strong>the</strong>same time fulfilling <strong>the</strong> requirements formateriality. The issue has been dealt with in partby allowing relatively brief Public Reports, but withmore detailed back up being available. A number<strong>of</strong> example reports have also been produced toprovide guidance.No reference to Code. This is an issue that hasdecreased with time, although <strong>the</strong>re has been asteady stream <strong>of</strong> new companies coming on to<strong>the</strong> market who have had to be informed about<strong>the</strong> Code. Responses have been positive.Figure 3: Break down <strong>of</strong> non-compliance by typeIn Figure 3, <strong>the</strong> instance <strong>of</strong> non- compliance arebroken down by category. Discussing each <strong>of</strong><strong>the</strong>se in turn:No (or incorrect) Competent Personstatement. This has generally speaking been <strong>the</strong>most common issue and one that has provensomewhat intractable with time in that instancesare still occurring. The usual situation is that acompliant resource estimate has been preparedwhich includes a CP statement, but <strong>the</strong>n that issummarised down to a brief ASX announcement,conference or shareholder presentation in which<strong>the</strong> CP statement is omitted.It is noteworthy that in <strong>the</strong> Canadian geo<strong>the</strong>rmalreporting Code, which in most instances is basedon and identical to <strong>the</strong> <strong>Australian</strong> Code, strictcompliance in terms <strong>of</strong> including a CP statementin every Public Report is not required. However,this issue has been debated by <strong>the</strong> JAGRCC, andit is considered that every public announcementwhich refers to reserves or resources, and whichcould be deemed to provide information toMiscellaneous issues include items such asinappropriate aggregation <strong>of</strong> resources andconversion <strong>of</strong> heat-in-place to barrels <strong>of</strong> oilequivalent, delivered electricity or numbers <strong>of</strong>households that could potentially be supplied,without stating <strong>the</strong> assumptions involved. Therehas sometimes been a degree <strong>of</strong> over-enthusiasmin making such claims. The Code is notprescriptive as to methodology in such instancesbut <strong>the</strong>y remain matters <strong>of</strong> concern.ReactionIn each case on perceived non-compliance <strong>the</strong>company concerned has been informally notifiedabout <strong>the</strong> issue. In general <strong>the</strong>re has been a highlevel <strong>of</strong> willingness to comply with <strong>the</strong> Code andcompanies have responded positively to anyissues raised.The Way ForwardThe experience gained in reviewing reports hasbeen valuable and has been taken into account indrawing up <strong>the</strong> Second Edition <strong>of</strong> <strong>the</strong> Code andLexicon which, at <strong>the</strong> time <strong>of</strong> writing, have beenfinalised and which should be released at thisconference. O<strong>the</strong>r jurisdictions have beenstudying <strong>the</strong> <strong>Australian</strong> Code which has led to an303


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>almost identical Code being established inCanada, and it is understood that consideration isalso being given to Codes in <strong>the</strong> USA andEurope. The benefits <strong>of</strong> <strong>the</strong> <strong>Australian</strong> Code arebeing appreciated even in counties where it hasno formal standing and Code compliant reportshave recently been produced on resources inChile and Indonesia, as is described in acompanion paper.304


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Application <strong>of</strong> <strong>the</strong> <strong>Australian</strong> Geo<strong>the</strong>rmal Reporting Code to“Conventional” Geo<strong>the</strong>rmal ProjectsJim Lawless*, Zim Aunzo and Jose Seastres, JrAbstractThe Geo<strong>the</strong>rmal Reserves and ResourcesReporting Code was developed in Australia with<strong>the</strong> intention <strong>of</strong> it being principally applied to<strong>Australian</strong> geo<strong>the</strong>rmal projects, though it wasframed in such a way as to apply to geo<strong>the</strong>rmalprojects <strong>of</strong> all types. Recently, SKM has applied<strong>the</strong> Code to a number <strong>of</strong> “conventional” hightemperature magmatic-related geo<strong>the</strong>rmalprojects outside Australia. This paper describeshow <strong>the</strong> Code principles and <strong>the</strong> underlyingresource estimation methodology have beenapplied in those cases. Some <strong>of</strong> <strong>the</strong> major issueswhich had to be addressed included:• What conversion efficiencies are applicablewhen <strong>the</strong> project is to include a flash steamcycle ?• How are resources and reserves to becategorised when estimates are based onnumerical simulation models ?• How is energy already extracted to be dealtwith in <strong>the</strong> case <strong>of</strong> project with an existingproduction history ?• How is energy remaining after <strong>the</strong> assumedproject life to be categorised ? Although<strong>the</strong>se projects have been based onmagmatic-related resources which do notoccur in Australia, some <strong>of</strong> <strong>the</strong> insightsgained in <strong>the</strong> process will have application as<strong>Australian</strong> projects move towardscommercialisation, and as <strong>Australian</strong> listedcompanies develop this type <strong>of</strong> systemelsewhere in <strong>the</strong> world.*SKM PO Box 9806 Newmarket, Auckland, NZJLawless@skm.co.nz305


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Small <strong>Australian</strong> seismic events and <strong>the</strong>ir effectsDavid N. Love 1* , Gary Gibson 2 , Russell Cuthbertson 3 and Wayne Peck 21 PIRSA, GPO Box 1671, Adelaide SA 50012 ES&S, 8 River St Richmond Vic 31213 ES&S, 81 Bishop St Kelvin Grove Qld 4059* Corresponding author: david.love@sa.gov.auWe review four small earthquakes in Australia andhighlight various seismological aspects that arerelevant when considering induced seismicity.The four events are in <strong>the</strong> magnitude range 2.5 to4.1, a range that is likely to be <strong>of</strong> interest for thoseinvestigating geo<strong>the</strong>rmally induced events.Keywords: Australia, earthquake, induced event,intensityMt Barker (South Australia) event16 April <strong>2010</strong> Magnitude 3.8This earthquake occurred at 11:27pm on Fridaynight, about 25 km from <strong>the</strong> Adelaide CBD. Itwas widely felt, with a massive response to policeand radio stations. There was no indication that<strong>the</strong> phone system failed, or that power outagesoccurred. The Primary Industries and ResourcesSA (PIRSA) earthquake network operatedsmoothly through <strong>the</strong> event, giving a very goodlocation and magnitude estimate in less than 3minutes. It took about 15 minutes to quicklyreview <strong>the</strong> event, and report it to <strong>the</strong> emergencyservices. The location was not entered on <strong>the</strong>PIRSA website until after <strong>the</strong> weekend. The firstepicentre entry on <strong>the</strong> US Geological Surveywebsite was about 100 km in error, but with alisted error estimate <strong>of</strong> 152 km. The firstGeoscience Australia (GA) magnitude estimatewas 3.2. While <strong>the</strong> internet remained operating,<strong>the</strong> GA and PIRSA websites were overloaded fora time. The PIRSA website received about13,000 hits, a record. Hundreds <strong>of</strong> <strong>the</strong>seemanated from overseas.ABC radio Adelaide is normally run from Sydneylate at night, but <strong>the</strong> Adelaide station wasreopened in response to overwhelming publicinterest. Twitter and Facebook registered a hugeamount <strong>of</strong> traffic. AdelaideNow website hadabout 1400 comments in short time; USGS DidYou Feel It (DYFI) website plotted over 300replies in less than one hour, and ES&S and GAhad many replies to <strong>the</strong>ir website questionnaire.Management, particularly those associated wi<strong>the</strong>mergency response, expressed frustration at notknowing where to go for <strong>the</strong> best information at<strong>the</strong> eraly stages. In <strong>the</strong> following few weeks, alarge number <strong>of</strong> insurance claims were lodged,with an estimate <strong>of</strong> 1,000 by one loss adjuster.PIRSA circulated a questionnaire, but responseshave not yet been analysed. Of <strong>the</strong> responses,only <strong>the</strong> USGS Did You Feel It system wasavailable within a short time frame. As <strong>the</strong>earthquake was not in <strong>the</strong> US, <strong>the</strong> locationinformation was limited to 6 ‘city’ locations,instead <strong>of</strong> postcode areas, rendering it <strong>of</strong> limitedvalue.There is a clear need for a DYFI system to beoperated within Australia which can moreeffectively utilise location and intensityinformation, and disseminate it rapidly.The depth <strong>of</strong> this earthquake was 25 km, with anuncertainty <strong>of</strong> about 2 km. This is quite deep forAustralia. Normally depths <strong>of</strong> hypocentres arenot available due to poor network coverage,however <strong>the</strong> new Adelaide network is producingaccurate depths for a moderate number <strong>of</strong> events.The magnitudes for stations <strong>of</strong> <strong>the</strong> Adelaidenetwork ranged from 3.2 to 4.1, for stations <strong>of</strong> <strong>the</strong>GA network 3.5 to 4.2, and for stations <strong>of</strong> <strong>the</strong>ES&S network 3.4 to 4.0. These magnitudeswere from peak amplitude measurements <strong>of</strong>seismographs, not moment magnitudes. Verylittle has been published on magnitudes inAustralia in <strong>the</strong> last decade. Very few studieshave been done to investigate corrections forindividual sites on <strong>the</strong> basis <strong>of</strong> local geology, or tosee how well magnitudes compare betweennetworks.The Eugowra (New South Wales) event21 August 1994 Magnitude 4.1This was <strong>the</strong> largest <strong>of</strong> a swarm <strong>of</strong> hundreds <strong>of</strong>events that occurred near <strong>the</strong> town <strong>of</strong> Eugowra,east <strong>of</strong> Orange, in country NSW. The swarmwas very shallow, mostly less than 1 km deep.(Gibson et al, 1994)The number <strong>of</strong> events, initially increasing in sizeresulted in public meetings being called. Therewas some concern, but generally not great. Themain shock did stop <strong>the</strong> serious drinkers in <strong>the</strong>hotel for 5 minutes, but damage was limited tominor cracking and contents.Portable instrumentation was installed close to <strong>the</strong>activity at an early stage in <strong>the</strong> swarm. From abeginning <strong>of</strong> one instrument, <strong>the</strong>re was anincrease eventually to 8 instruments, atmoderately high sample rates <strong>of</strong> 200 to 400 sps.This resulted in probably <strong>the</strong> most accurately306


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>recorded sequence <strong>of</strong> events in <strong>Australian</strong>seismological history. It was possible todemonstrate <strong>the</strong> fault plane that accounted formost <strong>of</strong> <strong>the</strong> events in <strong>the</strong> sequence (figure 1).This, in conjunction with <strong>the</strong> local topography,gave a convincing geological story. It was alsopossible to roughly estimate <strong>the</strong> size <strong>of</strong> <strong>the</strong> mainshock at about 1 km square from <strong>the</strong> accuratelocation <strong>of</strong> <strong>the</strong> shocks in <strong>the</strong> following 9 days(figure 2). Aftershocks in <strong>the</strong> following 9 monthswere spread out still fur<strong>the</strong>r. No o<strong>the</strong>r earthquakeunder magnitude 5.5 has been monitored wellenough to show <strong>the</strong> size, dip and strike <strong>of</strong> <strong>the</strong>faulted area. No fault mechanism was producedfor any <strong>of</strong> <strong>the</strong> events, but <strong>the</strong> geologicalconclusion is that it was mainly thrust.Figure 2: Hypocentres <strong>of</strong> <strong>the</strong> Eugowra earthquake swarm.The 22-30 August hypocentres outline an area <strong>of</strong>approximately 1 square km, which was probably <strong>the</strong> rupturesurface <strong>of</strong> <strong>the</strong> largest event, magnitude 4.1.Figure 1: Hypocentres <strong>of</strong> <strong>the</strong> Eugowra earthquake swarmshowing a shallow fault rupture clearly dipping to <strong>the</strong> northwest.One accelerograph recorded a peak value <strong>of</strong>0.97g. This is <strong>the</strong> largest acceleration recordedto date from an earthquake in Australia. Thefrequency <strong>of</strong> this peak was above 50 Hz.Unfortunately <strong>the</strong> sampling rate on <strong>the</strong> instrumentwas insufficient to calculate a velocity. Thedamage was very minor, demonstrating thatacceleration is definitely not a good parameter touse when considering a management plan forinduced events. Velocity is a much betterpredictor <strong>of</strong> damage, although it does not solve allproblems. Detailed intensity information was notprocessed for this event, as a large effort was putinto monitoring.Acacia Ridge (Queensland) event18 July 1996 Magnitude 2.7This earthquake shows that even small events,which <strong>of</strong>ten may not be felt in o<strong>the</strong>r countries, arestill noticed in Australia. This earthquakeoccurred at 3:40pm in <strong>the</strong> suburbs <strong>of</strong> Brisbane,only 13km from <strong>the</strong> central business district. Itinitially produced only a small number <strong>of</strong> reports,however press reports and a phone surveycollected over 150 intensity reports (Lynam andCu<strong>the</strong>rbertson 1997). The general radius <strong>of</strong>perceptibility <strong>of</strong> <strong>the</strong> main felt area was about 14km with ano<strong>the</strong>r felt area to <strong>the</strong> south-west and anisolated report as far as 70km away. Intensitiesassigned were low, with no reports reachingintensity 5 (figure 3).The higher intensities were concentrated around<strong>the</strong> epicentre, and in a separate area to <strong>the</strong> southwest.The intervening area had lower intensitiesand even not felt replies. Variations in <strong>the</strong>intensities showed some correlation with surficialgeology; lower intensities were associated withareas <strong>of</strong> Mesozoic sandstones and coal measuresand Cainozoic sandstones and basalts, whilehigher intensities occurred on <strong>the</strong> Palaeozoicbasement rocks. This observation, somewhatcontrary to what is usually observed, is thought tobe due to <strong>the</strong> high frequency nature <strong>of</strong> thisrelatively small magnitude event. Attenuation <strong>of</strong><strong>the</strong> high frequency energy in <strong>the</strong> Mesozoic andCainozoic rocks may have been more significant307


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>than <strong>the</strong> amplifying effects normally associatedwith surface sediments and lower frequencies <strong>of</strong>larger events. Many smaller events are noticedmore by <strong>the</strong> noise, emanating from very highfrequencies, than <strong>the</strong> vibration.While <strong>the</strong>re were nine seismographs within 90km, <strong>the</strong> distribution <strong>of</strong> <strong>the</strong>se meant that <strong>the</strong>re is anuncertainty <strong>of</strong> several kilometres in <strong>the</strong> epicentre(particularly in a NE-SW direction) and <strong>the</strong> depthis unknown. This is common for most events inAustralia. This lack <strong>of</strong> hypocentral depths meansthat <strong>the</strong>re are limited data available to compareintensities with hypocentral distances at <strong>the</strong> closedistances that are <strong>of</strong> interest to <strong>the</strong> geo<strong>the</strong>rmalindustry.The good seismograph distribution meant that <strong>the</strong>epicentre and depth were known to within about 2km. This is fairly unusual for Australia. It has<strong>the</strong> benefit that any measured velocities andestimated intensities can be included in morespecific attenuation analyses for smallearthquakes at close range. Peak amplitudes for<strong>the</strong> four closest seismographs were in <strong>the</strong> 10 to25 Hz range. Individual station magnitudesvaried from 2.0 to 3.4.Figure 3: Isoseismal map <strong>of</strong> <strong>the</strong> Acacia Ridge earthquake.Source: Geoscience AustraliaCaulfield (Melbourne) event22 October 2006 Magnitude 2.5An even smaller event was widely felt inMelbourne at 10:36pm while most people werequietly at home.Information for this isoseismal map (figure 4) wascollected by <strong>the</strong> intensity form on <strong>the</strong> ES&Swebsite. As a result, in contrast to <strong>the</strong> AcaciaRidge earthquake, it has only one not felt reply.There are only two MM5 intensity reports listed,again showing <strong>the</strong> expected low intensities.Despite <strong>the</strong> very low magnitude <strong>of</strong> <strong>the</strong> event, and<strong>the</strong> low intensities reported to <strong>the</strong> ES&S website,<strong>the</strong>re were many insurance claims made,primarily for cracked plaster, cracked and liftedtiles and o<strong>the</strong>r cosmetic damage.Figure 4: Isoseismal map <strong>of</strong> <strong>the</strong> Caulfield earthquakeConclusionsQuite small events are felt, heard and newsworthyin Australia, even though <strong>the</strong> real damageconsequences are minor or non-existent. While<strong>the</strong>re is a considerable amount <strong>of</strong> information <strong>of</strong>interest and value available to <strong>the</strong> geo<strong>the</strong>rmalindustry, some extra effort could improve <strong>the</strong> datacollection and interpretation to more suitablyaddress <strong>the</strong> needs <strong>of</strong> <strong>the</strong> industry.Information that is accurate, and quickly availablesaves <strong>the</strong> difficulty and complaints that comelater, from <strong>the</strong> inability <strong>of</strong> management and <strong>the</strong>public to find <strong>the</strong> information when desired.308


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Given <strong>the</strong> large public response, even for smallevents, <strong>the</strong>re is clearly a need for a goodcommunity consultation program which addressesperceived risk as well as <strong>the</strong> risk <strong>of</strong> damage.A ‘Did You Feel It’ intensity collection system, runin Australia would significantly improve <strong>the</strong>collection <strong>of</strong> intensity data, particularly over <strong>the</strong>important populated areas, and make it rapidlyavailable in easily understood form. This will leadto improved attenuation formulae. The projectshould be easy and inexpensive. Improvedintensity data will give a much clearer indication <strong>of</strong><strong>the</strong> level <strong>of</strong> induced seismicity that may betolerated, and <strong>the</strong> level <strong>of</strong> public response tovibrations.There are currently New Generation Attenuation(NGA) formulae in use in earthquake hazardassessment. (Power et al, 2008) Thedevelopment <strong>of</strong> modified NGA formulae to cover<strong>the</strong> magnitude range 3 to 5 would also providevaluable tools for use in induced seismicity riskassessments. The current NGA formulae aredesigned for higher magnitudes and lowerfrequencies, and not suitable to be extrapolatedbeyond <strong>the</strong>se ranges. There is a vast amount <strong>of</strong>recorded information for smaller earthquakes.Unfortunately <strong>the</strong>se are nearly all from overseasevents. Events from stable continental areas,especially Australia would be needed, particularlyfor better handling <strong>of</strong> high frequencies.More detailed monitoring, particularly active andpopulated areas would lead to improved sourceinformation, and more local data for modified NGAformulae. Unfortunately this is a more expensiveexercise, and most populated areas are notmonitored to this extent. More portabledeployments <strong>of</strong> larger scale to measure swarmsor aftershocks at close range, and with highersample rates, would provide valuable informationon velocities, accelerations, rupture sizes andfocal mechanisms <strong>of</strong> use to <strong>the</strong> industry. This isnot done as <strong>of</strong>ten now as it was in <strong>the</strong> past.The collection <strong>of</strong> intensity data in <strong>the</strong> samelocalities as velocity data will fur<strong>the</strong>r improve <strong>the</strong>estimation <strong>of</strong> effects and damage in populatedareas.There is a need to compare magnitude dataacross Australia, review magnitude formulaecurrently in use, begin usage <strong>of</strong> momentmagnitudes, and investigate seismograph sitemagnitude corrections. This is not difficult, buthas not been happening over <strong>the</strong> last decade,with limited interaction between seismologicalobservatories.ReferencesGibson, G., Wesson, V. and Jones, T., 1994, TheEugowra NSW Earthquake Swarm <strong>of</strong> 1994,Seminar <strong>Proceedings</strong>, <strong>Australian</strong> EarthquakeEngineering Society pp71 - 80Lynam, C. and Cuthberton, R., 1997, The AcaciaRidge (Brisbane) earthquake <strong>of</strong> 18 July 1996,Queensland University Advanced Centre forEarthquake Studies, Report no 2, pp71 - 81.Power, M., Chiou, B., Abrahamson, N.,Bozorgnia, Y., Shantz, T. and Roblee, C., 2008,An overview <strong>of</strong> <strong>the</strong> NGA Project 3, EarthquakeSpectra v1 n4, pp 3 - 22309


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Community Consultation Best Practice ManualSteve Kennedy 2 , Chris Mat<strong>the</strong>ws 1 *, Damia Ettakadoumi 2 , Cynthia Crowe 21 <strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong> Association. PO Box 1048 Flagstaff Hill SA 51592 Department <strong>of</strong> Primary Industries GPO Box 4440 Melbourne VIC 3001The <strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong> GroupTechnical Interest Group 1 (AGEG TIG 1) and <strong>the</strong><strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong> Association(AGEA) have collaborated on a project to producea best practice manual (BPM) on communityconsultation for <strong>the</strong> development <strong>of</strong> geo<strong>the</strong>rmalprojects in Australia.There is a growing expectation from <strong>the</strong>community, government regulators and leadingindustry players that stakeholders and <strong>the</strong> widercommunity will be fully informed and encouragedto provide input to decision making about <strong>the</strong>industry activities that have <strong>the</strong> potential to affect<strong>the</strong>ir communities.AGEG and AGEA undertook <strong>the</strong> project to create<strong>the</strong> BPM with <strong>the</strong> following objectives: Companies meet government regulationsand expectations Companies meet community expectationsand maintain <strong>the</strong> ‘social licence to operate’ All parties follow <strong>the</strong> <strong>Australian</strong> MinisterialCouncil for Minerals and PetroleumResources (MCMPR) Principles forengagement with communities andstakeholders Give clear advice to developers on <strong>the</strong>intricacies (such as timing) <strong>of</strong> reporting toboth <strong>the</strong> community and corporate regulatorssuch as <strong>the</strong> ASX.When scoping this project, AGEG and AGEArecognised that <strong>the</strong>re is a significant body <strong>of</strong> workthat already exists on best practice communityengagement, both in <strong>the</strong> <strong>Australian</strong> resourcesindustry and in <strong>the</strong> international community.It is for this reason that AGEG and AGEA decidedto create tailored “best practice notes” that drawon <strong>the</strong> existing body <strong>of</strong> knowledge and provideguidance in <strong>the</strong> context <strong>of</strong> <strong>the</strong> emerginggeo<strong>the</strong>rmal energy sector in Australia.The “notes” format (ra<strong>the</strong>r than a single manual)means that each <strong>the</strong>me <strong>of</strong> communityengagement is a stand-alone document.Companies can pick and choose <strong>the</strong> topics thatare useful or relevant to <strong>the</strong>m at <strong>the</strong> time. As <strong>the</strong>geo<strong>the</strong>rmal industry matures and communityengagement principles change over time, <strong>the</strong>notes can be individually modified without havingto update an entire manual.The best practice notes series is a precursor to amore complete BPM on community engagement,to be completed by AGEG and AGEA in <strong>the</strong> nearfuture.Keywords: Community and Stakeholderengagement, best practice manual, keymessages, communicating risks, mediamanagement, outrage management, geo<strong>the</strong>rmalenergy, Australia, South <strong>Australian</strong> ResourcesIndustry Code <strong>of</strong> Practice for Stakeholder andCommunity Engagement, <strong>Australian</strong> Geo<strong>the</strong>rmal<strong>Energy</strong> Group, <strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong>Association.Context: The need for communityconsultationThe emerging geo<strong>the</strong>rmal industry as a whole(including government regulators, developers andstakeholders) understands <strong>the</strong> need to establishcommunity understanding and support,sometimes known as <strong>the</strong> “social licence tooperate” (SLO). Variation in Australia’spopulation density and land use across <strong>the</strong>country means that <strong>the</strong> SLO will be more difficultto obtain in densely populated areas such asVictoria and New South Wales, compared withsparsely populated areas such as far nor<strong>the</strong>rnSouth Australia. Failure to achieve <strong>the</strong> SLO maylead to delays in approving <strong>the</strong> project, result inexpensive or onerous conditions or, in somecases, may even lead to <strong>the</strong> rejection <strong>of</strong> aproposal by regulators.The regulatory process is likely to proceed moresmoothly and expeditiously if effective stakeholderand community engagement has, as far aspractical, addressed stakeholder concerns prior toapplying for <strong>the</strong> required approvals (SACOME2009).The best practice manual processSeveral organisations have worked over <strong>the</strong> lastfew years to establish a standard <strong>of</strong> practice thatmeets <strong>the</strong> requirements <strong>of</strong> best practicecommunity consultation in resource development.A number <strong>of</strong> benchmarking documents alreadyexist that outline standards for stakeholder andcommunity engagement that communities canexpect from geo<strong>the</strong>rmal developers. Theseinclude documents published by <strong>the</strong> MineralsCouncil <strong>of</strong> Australia (e.g. MCA 2005), <strong>the</strong> MCMPR(MCMPR 2005) and <strong>the</strong> International Associationfor Public Participation (e.g. IAP2 2007).400


A number <strong>of</strong> state government departments alsohave manuals on community engagement. Theseinclude <strong>the</strong> Department <strong>of</strong> Primary IndustriesVictoria (DPI Victoria <strong>2010</strong>) and <strong>the</strong> Western<strong>Australian</strong> Government (WA Department <strong>of</strong>Indigenous Affairs 2005).Drawing on and complying with <strong>the</strong>se and o<strong>the</strong>rdocuments, <strong>the</strong> South <strong>Australian</strong> Chamber <strong>of</strong>Minerals and <strong>Energy</strong> (SACOME), in collaborationwith Community Engagement Group Australia(cega) and Primary Industry and Resources SA(PIRSA) produced a Code <strong>of</strong> Practice forStakeholder and Community Engagement in <strong>the</strong>SA resources industry (SACOME 2009). ASupporting Document, also published in 2009,supplemented <strong>the</strong> Code, which includedguidelines and a community engagement toolkitdesigned by cega.Best practice notesWith <strong>the</strong> knowledge that several benchmarkdocuments already exist that adequately meetnationally and internationally recognisedstandards, AGEG and AGEA decided to createtailored “best practice notes” that draw on <strong>the</strong>existing body <strong>of</strong> knowledge and provide guidancein <strong>the</strong> context <strong>of</strong> <strong>the</strong> emerging geo<strong>the</strong>rmal energysector in Australia.<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>ReferencesDepartment <strong>of</strong> Primary Industries, <strong>2010</strong>,Geo<strong>the</strong>rmal <strong>Energy</strong> in Victoria LandholderInformation.International Association For Public Participation(IAP2), 2007, Core Values.Minerals Council <strong>of</strong> Australia, 2005, EnduringValue, <strong>the</strong> <strong>Australian</strong> Minerals IndustryFramework for Sustainable Development,Guidance for Implementation.Ministerial Council for Mineral and PetroleumResources, 2005, Principles for Engagement withCommunities and Stakeholders.SACOME, 2009, South <strong>Australian</strong> ResourceIndustry Code <strong>of</strong> Practice for Stakeholder andCommunity Engagement. Code and SupportingDocument.Western <strong>Australian</strong> Government Department <strong>of</strong>Indigenous Affairs, 2005, Engaging withAboriginal Western <strong>Australian</strong>s.Each note covers one <strong>of</strong> <strong>the</strong> following topics:Existing resources and tools for communityengagementIdentifying and engaging stakeholdersKey messages about geo<strong>the</strong>rmal energyHow to communicate messages about risksSkills required for community engagementMedia managementOutrage managementThe best practice notes series is a precursor to amore complete BPM on community engagement,to be completed by AGEG and AGEA in <strong>the</strong> nearfuture.AGEA Membership commitment tobest practiceThe final objective <strong>of</strong> <strong>the</strong> BPM process is thatmembers <strong>of</strong> AGEA, <strong>the</strong> peak geo<strong>the</strong>rmal industrybody, will sign up and agree to abide by bestpractice community engagement as a prerequisitefor being members.The undertaking <strong>of</strong> this commitment will give allstakeholders, whe<strong>the</strong>r <strong>the</strong>y be governmentfunding bodies, communities, regulators or anyo<strong>the</strong>r stakeholder groups, comfort that world’sbest practice is being applied when <strong>Australian</strong>geo<strong>the</strong>rmal projects are being undertaken.401


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Optimising ORC use in <strong>Australian</strong> Geo<strong>the</strong>rmal ApplicationsCraig Morgan 1 , David Paul 21Pacific Heat and Power, Level 14, 500 Collins Street, Melbourne VIC 30002 Pratt & Whitney Power Systems, 400 Main Street, East Hartford, Connecticut, USA* Corresponding Author: craig.morgan@pacificheatandpower.com, +61 3 9013 4425IntroductionSince Pratt & Whitney Power Systems acquired amajority stake in Turboden in 2009, many hotsedimentary aquifer geo<strong>the</strong>rmal powerapplications across <strong>the</strong> world have beenassessed. A variety <strong>of</strong> power configurations havesubsequently been developed and costed thathave relevance for <strong>the</strong> future <strong>of</strong> <strong>the</strong> <strong>Australian</strong>geo<strong>the</strong>rmal industry.This paper summarises <strong>the</strong> key considerationsmade in designing systems, as well as factors thataffect overall performance.Keywords: PureCycle®, Pratt & Whitney PowerSystems, Turboden, Organic Rankine Cycle,Pacific Heat and PowerInput conditionsInput conditions for ORC use in geo<strong>the</strong>rmalapplications across <strong>the</strong> world vary substantially: Geo<strong>the</strong>rmal brine input conditions varysuch as 74C in shallow and small scaleAlaskan wells, 98C in Birdsville, 130Cfrom a hot sedimentary aquifer in <strong>the</strong>USA, 150C at <strong>the</strong> outlet <strong>of</strong> a hightemperature separator in New Zealand, oras high as 240C+ in enhancedgeo<strong>the</strong>rmal applications. Thesetemperature conditions, including flowrate may also change over time. Air temperatures vary from -5 C to 50C+during <strong>the</strong> day in desert regions <strong>of</strong>Australia. Water for cooling is sometimes available,but many times it is not. <strong>Energy</strong> prices vary between AUD 5c/kWhto 20 c/kWh, and is sometimes a marketrate or government-regulated. Incentives include Renewable <strong>Energy</strong>Certificates equivalent to 2-4 c/kWh, ortax-incentive regimes. Well and steam field developments varyfrom free-flowing wells to 5km-deep wells. Noise restrictions vary from site to sitedepending on <strong>the</strong> location <strong>of</strong> <strong>the</strong> plant. Flammability and toxicity <strong>of</strong> ORC workingfluids is subject to a variety <strong>of</strong> planningregulations. Atmospheric conditions can include H2Swhich aggressively corrodes copper inplant and equipment. Some project developers wish to contractfor supply and commission <strong>of</strong> <strong>the</strong> ORConly, whilst o<strong>the</strong>rs wish for a fullypackaged Engineer-Procure-Construct(EPC) solution.Amongst this, <strong>the</strong> ORC supplier must optimiseeach individual application according to a specificclient’s requirement, generally for highesteconomic return on <strong>the</strong>ir project and notnecessarily lowest specific cost <strong>of</strong> <strong>the</strong> power plant($/kW).ORC design considerationsApart from <strong>the</strong> input conditions, keyconsiderations in <strong>the</strong> ORC system design include: Corrosion → special and costly materialsfor <strong>the</strong> heat exchangers influence <strong>the</strong> unitcost significantly increase lead time. Scaling → <strong>the</strong>re may be limits to <strong>the</strong>minimum temperature <strong>of</strong> <strong>the</strong> geo<strong>the</strong>rmalbrine due to deposition <strong>of</strong> silica or o<strong>the</strong>rproducts. Fouling → removable covers and straightcleanable tubes assist in cleaning and ongoingefficiency. Cascade use and cogeneration (using <strong>the</strong>condensing heat for o<strong>the</strong>r purposes) canimprove feasibility. Working fluid flammability can be an issuefor urban areas / insurance cost. Vapour plume from cooling towers areunsightly and <strong>the</strong>re is a need for makeupwater in evaporative devices. There is a larger footprint required, andadditional noise emissions from <strong>the</strong> fansin an air condenser or fin/fan cooler.Water use is becoming a significant issue.Evaporative cooling towers feature: Smaller footprint. Lower noise emissions. Fresh water consumption. Chemical water treatment requiringoperation cost and environmentalimpacts.402


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Air condensers feature: Larger footprint. Higher noise emissions. No water needed. Virtually no environmental impact and lowoperating costs.O<strong>the</strong>r options include hybrid cooling systems thatoperate dry in winter and cooler ambientconditions, whilst using water in hotter conditions.Critical issues we observe are: Investment costs need to take intoconsideration initial capital requirements,ongoing costs, and future wateravailability. The generated yearly power output istightly linked to cooling conditions andparasitic loads, and is particularlysignificant for cooler resources.The best solution is dependent on <strong>the</strong> application,but in <strong>the</strong> main we see <strong>Australian</strong> clientspreferring dry or hybrid cooling systems <strong>of</strong> somesort.ORC performance & practical systemsAvailability <strong>of</strong> PWPS and Turboden ORCtechnologies in real world applications is at >98%. Maintenance costs are very low relative too<strong>the</strong>r power generation technologies such asengines, gas turbines or steam turbines.The selection <strong>of</strong> working fluid is influenced by:• Cost.• Environmental impact.• Pressure levels selected.• Heat input curve.• Enthalpy drop & flow rate.• Flammability.• Cooling system.The optimal fluid, pressure levels, and turbine sizevaries from case to case.In hot sedimentary aquifer applications <strong>the</strong>geo<strong>the</strong>rmal fluid normally stays in liquid phase.Currently <strong>the</strong> most proven and reliable ORCtechnology uses single-phase working fluids in‘normal’ pressure cycles. These systems can becascaded using multiple pressure levels toapproach <strong>the</strong> ideal Lorentz cycle, minimisingdisadvantages whilst maximising <strong>the</strong> benefits <strong>of</strong>reliable systems.Technical innovationsThe product development team continue to makesystem improvements that increase efficiency,broaden <strong>the</strong> variety <strong>of</strong> suitable applications, andprovide <strong>the</strong> ability to operate in with zero water forcooling. Features available are:• Air condenser for use in areas with limitedaccess to water. The refrigerant iscondensed directly in <strong>the</strong> air-condenser tomaximise heat transfer.• Coatings and equipment modificationssuch as those necessary for a high H2Senvironment in some internationalgeo<strong>the</strong>rmal fields.• High pressure evaporators may also beselected on a case by case basis forsome applications.Price vs PerformanceA manufacturer is able to design for maximumefficiency, or minimum specific cost. It is criticalthat <strong>the</strong> client and equipment supplier worktoge<strong>the</strong>r to optimise <strong>the</strong> unit design for eachspecific application. The chart below illustratesthis.403


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>The table shows price/power ratios for differentpossible configurations <strong>of</strong> an air-cooled ORC unit(installed, BoP excluded) for <strong>the</strong> same Project.Generally speaking <strong>the</strong> price/power ratio isinfluenced by <strong>the</strong> boundary conditions as follows: a colder(hotter) geo<strong>the</strong>rmal water willraise(decrease) <strong>the</strong> price/power ratio. a more aggressive and impuregeo<strong>the</strong>rmal water will raise <strong>the</strong>price/power ratio. a higher(lower) average annual airtemperature will raise(decrease) <strong>the</strong>price/power ratio.But in <strong>the</strong> design phase <strong>the</strong> choice between abigger or a smaller heat exchanger will influenceperformance and price, that means also <strong>the</strong>price/power ratioThe future and corporate updatePWPS and Turboden have recently beensuccessful in winning orders for a 5 MWgeo<strong>the</strong>rmal power plant in Germany (based on<strong>the</strong> Turboden technology), and a 500kWgeo<strong>the</strong>rmal power plant in Taiwan (based onPureCycle®).ConclusionThere is a wide variety <strong>of</strong> input conditions anddesign considerations that influence <strong>the</strong> final cost<strong>of</strong> an ORC power plant, and as such each project,whilst based on modular technology, will mostlikely be configured in a project-specific manner. Itis <strong>the</strong>refore critical that you work closely with yourequipment supplier to optimise <strong>the</strong> configurationto balance: Technical performance Efficiency Economic performance, Reliability and Operability404


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Mineral scaling in geo<strong>the</strong>rmal fields: A reviewYung Ngothai 1 *, Norio Yanagisawa 3 , Allan Pring 2 , Peter Rose 4 , Brian O'Neill 1 , Joël Brugger 21School <strong>of</strong> Chemical Engineering, The University <strong>of</strong> Adelaide, SA 50052 South <strong>Australian</strong> Museum, North Terrace, Adelaide, SA, 50003 Institute for Geo-Resources and Environment, AIST, Tsukuba, 305-8567, JAPAN4 <strong>Energy</strong> and Geoscience Institute, The University <strong>of</strong> Utah, Utah 84109, USA.*Corresponding author: yung.ngothai@adelaide.edu.auAbstractGeo<strong>the</strong>rmal power is an established energysource in several countries, for example NewZealand and Iceland. However <strong>the</strong> proposedgeo<strong>the</strong>rmal operations in South Australia occursat a much greater depth (5 km) and <strong>the</strong> heatsource is radioactive decay ra<strong>the</strong>r than volcanism.A number <strong>of</strong> issues relating to <strong>the</strong> geochemistry <strong>of</strong>geo<strong>the</strong>rmal fluids are required to be consideredand explored to ensure safe, economic energyproduction from geo<strong>the</strong>rmal fields. Low pH andsaline waters, at temperatures much greater than200 o C, are highly corrosive, and it is vital toprevent <strong>the</strong> generation <strong>of</strong> scales as <strong>the</strong> brines aretransported to <strong>the</strong> surface. This paper provides areview on silica, calcite and metal sulphide scalingat various geo<strong>the</strong>rmal fields. The solubility <strong>of</strong> silicaand calcite as a function <strong>of</strong> temperature and/orpressure were discussed and how it affectsscaling at various locations in <strong>the</strong> geo<strong>the</strong>rmalplant.Keywords: silica scaling, calcite scaling, metalsulphide scaling, EGS, HDR.IntroductionIn many developed geo<strong>the</strong>rmal fields in USA,New Zealand, Indonesia, Japan etc., mineralscales tend to precipitate with change <strong>of</strong> fluidtemperature and/or pressure, leading to fluid flowproblems. To overcome <strong>the</strong> operational problemsassociated with this scaling, several methodshave been developed to eliminate and/or reduce<strong>the</strong> amount <strong>of</strong> mineral deposition. It is howeverimportant that we fur<strong>the</strong>r investigate <strong>the</strong>mechanisms involved and <strong>the</strong> relation betweenmineral scaling and <strong>the</strong> physical and geochemicalcharacteristics <strong>of</strong> <strong>the</strong> rocks and fluids in <strong>the</strong>geo<strong>the</strong>rmal system under exploitation.For future geo<strong>the</strong>rmal systems, research anddevelopment <strong>of</strong> Enhanced Geo<strong>the</strong>rmal System(EGS) is required at a rapid pace, especially inAustralia.The outline <strong>of</strong> EGS (or Hot dry rock – HDR)system is described as follow; injected water isheated in artificial reservoir constructed usinghydr<strong>of</strong>racturing technology by flowing through ahigh temperature granite. The heated fluidproduced in reservoir, is used for powergeneration.The first EGS project was carried out at FentonHill, New Mexico (USA), which ran from 1970.After that o<strong>the</strong>r EGS projects were established ina number <strong>of</strong> countries e.g., Japan (at Hijiori),Soultz, France, etc. Metal corrosion and mineralscaling were observed at <strong>the</strong>se EGS systems. Forexample, in Soultz, metal corrosion occurred dueto high Cl concentrations (Baticci et al, <strong>2010</strong>)while in Hijiori, anhydrite and calcite scalingoccurred in <strong>the</strong> lower production wells andpipelines at ground level due to dissolution <strong>of</strong>anhydrite in <strong>the</strong> reservoir by <strong>the</strong> injected lowtemperature water (Yanagisawa et al., 2008).These problems are common to <strong>the</strong> welldevelopedconventional geo<strong>the</strong>rmal power plantsand likely to feature in EGS systems.This paper presents a brief review <strong>of</strong> mineralscaling in geo<strong>the</strong>rmal fields and discussion forfuture EGS development.Mineral scalingThe fluid in a natural geo<strong>the</strong>rmal system has along residence time (thousands <strong>of</strong> years) at arelatively high temperature (> 150 o C – 300 o C)which <strong>the</strong>refore indicates a significant rock-waterinteraction. Since <strong>the</strong> system has had a longresidence time, it is <strong>of</strong>ten assumed to be in a state<strong>of</strong> chemical equilibrium (Grigsby et al., 1989).Therefore, when fresh water is introduced into <strong>the</strong>system to extract heat, <strong>the</strong> system is no longer inequilibrium, which leads to precipitation anddissolution <strong>of</strong> different parts <strong>of</strong> <strong>the</strong> mineralassemblage. Precipitation, or scaling, is one <strong>of</strong><strong>the</strong> major problems in geo<strong>the</strong>rmal energyextractions. Minerals may precipitate dependingon <strong>the</strong> compositions <strong>of</strong> <strong>the</strong> granite and <strong>the</strong>injected brine.In geo<strong>the</strong>rmal fields, it has been reported thatsilica, calcium carbonate, anhydrite, metalsulphides and iron minerals scales precipitatedaround production and injection wells and in <strong>the</strong>piping.Silica scalingSilica scaling is a well known problem inconventional geo<strong>the</strong>rmal systems, which occursdue to <strong>the</strong> presence <strong>of</strong> amorphous silica, duringheat extraction or partial flashing (Robinson,1982). Amorphous silica can contain severalmetals such as iron, magnesium, and calcium, etc.405


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Silica scale precipitated in many geo<strong>the</strong>rmal fieldsdue to its high solubility at high temperature in <strong>the</strong>reservoir through water-rock interactions and <strong>the</strong>solubility rapidly decreases with decreasingtemperature. The solubility <strong>of</strong> silica is alsostrongly dependant on pH. For example, ironbearedamorphous silica tends to precipitated atfluid mixing points. At this point, temperature,pressure and pH <strong>of</strong> fluid change rapidly andleading to significant changes in solubility andchemical equilibrium leading to silica precipitation.Fur<strong>the</strong>rmore, silica has several structural phases,for example, quartz and amorphous silica whilesilica exists in solution both as a polymer and amonomer form. This variety leads to a complexarray <strong>of</strong> mechanisms for silica precipitation,especially in lower temperature environment suchas at <strong>the</strong> injection well.The dissolution <strong>of</strong> solid silica phases (SiO 2 ) inwater has been extensively studied (Mackenzieand Gees, 1971; Owen, 1975; Robinson, 1982).The solubility data for various silica phases(Rimstidt, 1980 cited from Robinson, 1982) areshown in Figure 1 where <strong>the</strong> solubility <strong>of</strong> differentsilica phases is plotted versus temperature.Quartz is <strong>the</strong>rmodynamically <strong>the</strong> most stablephase <strong>of</strong> silica thus its solubility at any giventemperature is lower relative to o<strong>the</strong>r silicaphases.dissolved silica in <strong>the</strong> brine may <strong>the</strong>n becomesupersaturated. Depending on <strong>the</strong> degree <strong>of</strong>supersaturation <strong>the</strong> dissolved monomeric silicamay nucleate and deposit as amorphous silicascale on equipment, such as heat exchangersurfaces (Chan, 1989). The factors which affect<strong>the</strong> solubility <strong>of</strong> amorphous silica in solutioninclude temperature, pH, pressure and saltcontent (Chan, 1989). Gunnarsson & Arnórsson(2005) state that <strong>the</strong>re are two processesinvolving aqueous silica that occur in anamorphous silica super-saturated solution. Thefirst process is <strong>the</strong> direct precipitation <strong>of</strong>amorphous silica directly onto <strong>the</strong> surface <strong>of</strong>equipment. The second is <strong>the</strong> tendency for silicato polymerise and form colloids that remain insuspension for long periods <strong>of</strong> time. Polymericsilica has less tendency to precipitate fromsolution than monomeric silica.Kinetics <strong>of</strong> silica dissolution needs to beestablished in order to evaluate <strong>the</strong> likelihood <strong>of</strong>silica scaling. Factors that control <strong>the</strong> rate <strong>of</strong>polymerization <strong>of</strong> dissolved silica are pH, salinity,degree <strong>of</strong> supersaturation, presence <strong>of</strong> solidsubstances, and temperature (Angcoy, <strong>2010</strong>).Bethke (1996) compiled <strong>the</strong> rate constants forquartz and amorphous silica dissolution whichwere originally determined by Rimstidt andBarnes (1980), are shown in Table 1.Table 1: Rate constants <strong>of</strong> quartz and amorphous silicadissolutionFigure 1: Equilibrium solubilities <strong>of</strong> silica phasesSilica concentrations in geo<strong>the</strong>rmal reservoirwaters at 200-350˚C are approximately 300-700mg/kg SiO 2 (Gunnarsson & Arnórsson, 2005).Fournier and Rowe (1966) state that <strong>the</strong> silicacontent in geo<strong>the</strong>rmal waters is controlled by <strong>the</strong>solubility <strong>of</strong> quartz at depth and not <strong>the</strong> solubility<strong>of</strong> amorphous silica at and near <strong>the</strong> surface <strong>of</strong> <strong>the</strong>ground. When hot brine is brought to <strong>the</strong> surface itis ei<strong>the</strong>r flashed or cooled while passing through apower plant system to release its available<strong>the</strong>rmal energy. Chan (1989) states that <strong>the</strong>Calcite scalingCalcite or aragonite (CaCO 3 ) scaling is also a wellknown problem in conventional geo<strong>the</strong>rmalsystems, Calcite scale occurs near <strong>the</strong> flashingpoint in <strong>the</strong> production wells due to decrease incalcite solubility.Calcium solubility varies with <strong>the</strong> pressure <strong>of</strong> CO 2(P CO2 ) and temperature <strong>of</strong> <strong>the</strong> fluid. Figure 2shows <strong>the</strong> calcium solubility curve as a function <strong>of</strong>P CO2 and temperature by Fournier (1985). It isnoted from this curve that under <strong>the</strong> sametemperature condition, calcite solubility is higherwith respected to increase <strong>of</strong> P CO2 . This explainswhy it is common to observe scaling at <strong>the</strong>flashing point. During flashing, where vapourrelease occurs causes <strong>the</strong> P CO2 to decreases,406


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>calcite solubility <strong>the</strong>refore drops and calcite scaleprecipitates <strong>the</strong>re. Fur<strong>the</strong>rmore, as calcitesolubility is lower at high temperature conditions,calcite precipitation tends to occur at deep pointsin production wells and could be a seriousproblem. Many geo<strong>the</strong>rmal fields with highcalcium or hydro-carbonate concentrationexperience calcite scale problems. In Japan,especially at <strong>the</strong> Mori and Oku-Aizu geo<strong>the</strong>rmalfield calcite scaling is a serious problem.Figure 2: Solubilities <strong>of</strong> calcite as a function <strong>of</strong> temperatureand pressure <strong>of</strong> CO2To prevent calcite scaling in wells, variouschemical inhibitors have been used in manygeo<strong>the</strong>rmal fields. For example, sodiumpolyacrylate, C 2 H 3 COONa, has been used forseveral Japanese geo<strong>the</strong>rmal fields and hot spas.Similar chemicals have been used around <strong>the</strong>world. At high fluid temperature, sodiumpolyacrylate reacts with calcium ion to makecomplex. Calcium complex cannot react with <strong>the</strong>bicarbonate ion (HCO 3) to precipitate calciumcarbonate. Thus, this sodium polyacrylate inhibitoris effective to prevent calcite scaling. For aproduction well, a capillary tube is inserted intowell until it reaches <strong>the</strong> depth <strong>of</strong> <strong>the</strong> flashing pointand <strong>the</strong> chemical inhibitor is <strong>the</strong>n injected directlyat this point and prevents scaling.In Japan, metal sulphide scaling is found in Oku-Aizu (Nitta et al., 1991) and Yamagawa (Akaku,1988). At Oku-Aizu geo<strong>the</strong>rmal field, <strong>the</strong> sulphurremoval system near power plant has been builtto prevent sulphide scaling.The sulphide mineral scaling indicate <strong>the</strong>conditions in <strong>the</strong> deep-seated reservoir,especially in granitic rocks. For example, at <strong>the</strong>Kakkonda geo<strong>the</strong>rmal area, in north-easternJapan, <strong>the</strong>re is a 80 MW geo<strong>the</strong>rmal power plantusing high temperature fluid from <strong>the</strong> reservoir at<strong>the</strong> boundary between <strong>the</strong> Quaternary Kakkondagranite and <strong>the</strong> Pre-Tertiary formations at about3km depth. Metal sulphide minerals deposit in <strong>the</strong>production wellhead and pipelines (Yanagisawa etal., 2000).The metal sulphide scales are classified into twotypes, based on sulphide mineralogy. These arePb-Zn rich type and Cu rich type. Pb-Zn rich scaleis found in Well-19 located at <strong>the</strong> marginal part <strong>of</strong><strong>the</strong> Kakkonda granite as shown in Figure 3. It ismainly composed <strong>of</strong> amorphous silica, galena(PbS), sphalerite (ZnS) and pyrite (FeS 2 ). Thebrine <strong>of</strong> WD-1a at 3.7km depth, in <strong>the</strong> QuaternaryKakkonda granite rock, underlied Well-19, is richin Pb and Zn and <strong>the</strong> scale in Well-19 is <strong>of</strong> similarcomposition.. Cu-rich scale is found in Well-13,located at <strong>the</strong> central part <strong>of</strong> <strong>the</strong> Kakkonda granite.It is mainly composed <strong>of</strong> amorphous silica,chalcocite (Cu 2 S), bornite (Cu 5 FeS4), loellingite(FeAs 2 ) and native antimony (Sb). It is also rich inAu, Ag, As, Cr, Ni and Mo compared to Pb-richscale.Similarly <strong>the</strong> solubility <strong>of</strong> anhydrite (CaSO 4 ) islower at higher temperature and tends toprecipitate deep in <strong>the</strong> production wells and at <strong>the</strong>peak temperature point. In this case, with <strong>the</strong>temperature <strong>of</strong> fluid from deeper parts increasesanhydrite precipitate due to its decreasingsolubility. It has been reported that in Japan, Moriand Sumikawa geo<strong>the</strong>rmal fields experienceanhydrite scaling.Metal sulphide scalingMetal sulphide scaling is <strong>of</strong>ten occurred involcanic or high Cl environment. For example, atSalton Sea geo<strong>the</strong>rmal field, <strong>the</strong> salinity (35%NaCl) and metal concentrations (around 20%copper) in <strong>the</strong> fluid are very high (Skinner et al.,1967), many sulphide minerals form scales, suchas bonite (Cu 5 FeS 4 ), chalcocite (Cu 2 S) have beenfound.Figure 3: Schematic geo<strong>the</strong>rmal cross-section <strong>of</strong> <strong>the</strong>Kakkonda geo<strong>the</strong>rmal system including well name and metalin precipitated sulphide and brine in graniteScaling in EGS systemIn EGS system, several different types <strong>of</strong> scalemineral precipitated in <strong>the</strong> Hijiori system, located407


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>in Yamagata Prefecture <strong>of</strong> Japan (Yanagisawa etal., 2008). At <strong>the</strong> Hijiori field tests wereundertaken using a series <strong>of</strong> hydraulic stimulationexperiments. A heating reservoir was created at2000m depth, after which river water was injectedinto <strong>the</strong> fractured reservoir, heated in reservoirand returned to installations on <strong>the</strong> ground level..Scaling at surface installations and in deep wells(HDR-2 and HDR-3) are shown in Figure 4.Anhydrite deposited in <strong>the</strong> deeper parts <strong>of</strong> <strong>the</strong>production wells, while silica and calciumcarbonate precipitated at <strong>the</strong> surface downstream<strong>of</strong> <strong>the</strong> wellhead. Amounts <strong>of</strong> precipitationdepended on <strong>the</strong> temperature and chemicalcomposition <strong>of</strong> <strong>the</strong> produced fluid. In HDR-2,which is closer to <strong>the</strong> injection well, most <strong>of</strong> <strong>the</strong>scale was calcium carbonate; in HDR-3, which isfur<strong>the</strong>r away from <strong>the</strong> injection well, <strong>the</strong>re wasslight precipitation <strong>of</strong> amorphous silica. As fluidcirculation progressed and temperaturedecreased, scaling in <strong>the</strong> flow line <strong>of</strong> well HDR-2changed from amorphous silica to calciumcarbonate.Figure 5 shows <strong>the</strong> depth temperature pr<strong>of</strong>ile. Aswater was injected anhydrite dissolved around <strong>the</strong>injection well, <strong>the</strong> water heated as it flowedthrough <strong>the</strong> reservoir, and anhydrite precipitateddue to lower solubility at higher temperatures.Injection60ton/hourWaterScales at pipeline <strong>of</strong> HDR-2 and 3Anhydrite dissolvedCaSO 4→ Ca 2+ + SO2-4Hot water lineSeparatorHDR2:Calcite/Aragonite HDR3:SilicaFlow in reservoirHeatingHDR2 : 130C, 24ton/hHDR3 : 170C, 8ton/hWellheadAnhydriteIncluding CalciteFigure 4: Scale sampling site and photo at Hijiori siteFigure 5: Temperature pr<strong>of</strong>iles in <strong>the</strong> Hijiori wells measuredin July 2002Reference:Akaku, K., 1988, Geochemistry <strong>of</strong> mineraldeposition from geo<strong>the</strong>rmal waters: DepositionProcesses <strong>of</strong> common minerals found in variousgeo<strong>the</strong>rmal fields and case study in <strong>the</strong> Fushimegeo<strong>the</strong>rmal field, Chinetsu, 25, p.154-171 (inJapanese).Angcoy, E.C. and Arnórsson, S., <strong>2010</strong>, AnExperiment on Monomeric and Polymeric SilicaPrecipitation Rates from Supersaturated Solutions,<strong>Proceedings</strong> <strong>of</strong> World Geo<strong>the</strong>rmal Congress,2710, p.1-6.Azaroual, M. and Fouillac, C., (1997).Experimental Study and Modelling <strong>of</strong> Granite-Distilled Water Interactions at 180 o C and 14 bars.Applied Geochemistry, 12, pp. 55-73Baticci, F., Genter, A., Huttenloch, P. and Zorn, R.,<strong>2010</strong>, Corrosion and Scaling Detection in <strong>the</strong>Soultz EGS Power Plant, Upper Rhine Graben,France, <strong>Proceedings</strong> <strong>of</strong> World Geo<strong>the</strong>rmalCongress, 2721, p.1-11.Bethke, C. M., 1996, Geochemical ReactionModelling. Concepts and Applications, OxfordUniversity Press, New York.Chan, S., 1989, A Review on Solubility andPolymerisation <strong>of</strong> Silica’, Geo<strong>the</strong>rmics, vol. 18, pp.49-56.Fournier, R. O., 1985, Carbonate transport anddeposition in <strong>the</strong> epi<strong>the</strong>rmal environment; inBerger, B. R., and Bethke, P. M. (eds.), Geologyand geochemistry <strong>of</strong> epi<strong>the</strong>rmal systems: Reviewsin Economic Geology, v. 2, pp. 63–72.Gunnarsson, I. and Arnórsson, S., 2005, Impact<strong>of</strong> Silica Scaling on <strong>the</strong> Efficiency <strong>of</strong> HeatExtraction from High-Temperature Geo<strong>the</strong>rmalFluids, Geo<strong>the</strong>rmics, vol. 34, pp. 320-329.Mackenzie, F. T. and Gees, R., 1971, Quartz:Syn<strong>the</strong>sis at Earth-Surface Conditions, Science,New Series, 173, pp. 533-535.408


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Nitta, T., Adachi, M., Takahashi, M., Inoue, K. andAbe, Y., 1991, Heavy metal precipitation fromgeo<strong>the</strong>rmal fluid <strong>of</strong> 87N-15T production well in <strong>the</strong>Okuaizu geo<strong>the</strong>rmal field, Tohoku distinct, Japan.Resource Geology, 41, p.231-242 (in Japanese).Owen, L. B., 1975, Precipitation <strong>of</strong> AmorphousSilica from High-Temperature HypersalineGeo<strong>the</strong>rmal Brine, California University,Livermore (USA), Lawrence Livermore Lab.,Technical ReportRimstidt J. D. and Barnes, H. L., 1980, TheKinetics <strong>of</strong> Silica-Water Reactions, Geochimica etCosmochimica Acta, 44, pp. 1683-1700.Skinner, B. J., White, D.E., Rose, H. J., Jr. andMays R.E., 1967, Sulfides associated with <strong>the</strong>Salton Sea geo<strong>the</strong>rmal brine., Economic Geology,62, p.316-330.Yanagisawa, N., Fujimoto, K. and Hishi, Y.,2000,Sulfide scaling <strong>of</strong> deep-geo<strong>the</strong>rmal well atKakkonda geo<strong>the</strong>rmal field in Japan, <strong>Proceedings</strong><strong>of</strong> World Geo<strong>the</strong>rmal Congress, p.1969-1974.Yanagisawa, N., Matsunaga, I., Sugita, H., Sato,M. and Okabe, T., 2008, Temperature dependentscale precipitation in <strong>the</strong> Hijiori Hot Dry Rocksystem., Geo<strong>the</strong>rmics, 37, p.1-18.Robinson, B. A., 1982, Quartz Dissolution andSilica Deposition in Hot Dry Rock Geo<strong>the</strong>rmalsystems, Thesis.409


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Direct GeoExchange Cooling for <strong>the</strong> <strong>Australian</strong> Square KilometerArray Pathfinder – Field TrialDonald J. B. Payne 1,2* , and Dezso Kiraly 31 School <strong>of</strong> Physics, University <strong>of</strong> Melbourne, Parkville, VIC, 3010.2Direct <strong>Energy</strong> Pty. Ltd., 6 Alma Rd, St Kilda, VIC, 3182.3 CSIRO Astronomy and Space Sciences, Corner Vimiera & Pembroke Rd, Marsfield, 2122.* Corresponding author: djbpayne@unimelb.edu.au; 0414 990 310Direct Geoexhange Heat Pumps (DGHPs)provide chilling via refrigerant-carrying copperloops buried in <strong>the</strong> ground which act as acondenser and achieve higher efficiency thanequivalent air source heat pumps because <strong>of</strong> <strong>the</strong>ground’s constant heat capacity. DGHPs areparticularly suited to desert environments withmore extreme ambient temperatures. The<strong>Australian</strong> Square Kilometer Array Pathfinder(ASKAP) radio telescope will be an array <strong>of</strong> 36 x12-m diameter parabolic dish antennae situated inBoolardy, WA each requiring 5 – 9 kW th coolingfor computer equipment and pedestal. Followingsuccessful tests <strong>of</strong> a prototype installation atMarsfield, NSW (ground temperature 17 C) aDGHP is installed at antenna site #29 (<strong>the</strong> firsterected). The DGHP provides chilling to a variabletest load (3.6, 4.8, 8.4, 9.6, 13.2 kW) via a 200 Lwater buffer. 6 x 30m bores containing copperloops deliver up to 14 kW <strong>of</strong> chilling to maintain 13- 15 C water temperature in <strong>the</strong> buffer. 5 databores monitor ground temperature variation in <strong>the</strong>centre <strong>of</strong> <strong>the</strong> 6 active bores and at 0.3, 0.6, 3.0,6.0 m (outside <strong>the</strong> bore field). System pressures &power are also monitored. A higher-than-expectedbaseline ground temperature <strong>of</strong> 27 C is measuredand verified by three methods. The nominal 14kW DGHP can maintain 15 C water temperatureat all loads including 13.2 kW. Note that 0.5 kWpump heating means <strong>the</strong> effective load is 13.7kW. We describe <strong>the</strong> results from this fieldinstallation in detail and present an abridged set<strong>of</strong> data.Keywords:Direct Geoexchange, Direct Use, Geo<strong>the</strong>rmalHeat PumpDirect GeoexchangeThe emerging geo<strong>the</strong>rmal industry in Australia isfocused on producing electricity (“indirect use”)and should begin delivering substantial resultsover <strong>the</strong> next decade. Direct Use geo<strong>the</strong>rmalenergy is more efficiently available as it entailsonly one energy conversion (absorption orradiation <strong>of</strong> heat), ra<strong>the</strong>r than <strong>the</strong> several thatoccur in electricity generation and usage, wi<strong>the</strong>ach step losing a percentage on conversion.Geo<strong>the</strong>rmal Heat Pumps (GHPs) are a direct use<strong>of</strong> geo<strong>the</strong>rmal energy which involve circulating afluid (water, brine or refrigerant) through earthloops (poly pipe or copper) a few tens <strong>of</strong> metresdeep (Fig. 1, Payne et al. 2008).Direct Geoexchange Heat Pumps (DGHPs) whichcirculate refrigerant through copper loops havegreater efficiency than water-loop GHPs because:(i) copper is more <strong>the</strong>rmally conductive thaninsulating plastic;(ii) latent heat transfers directly with <strong>the</strong> groundon evaporation or condensation; and(iii) an intermediate water-to-refrigerant heatexchanger between <strong>the</strong> ground loops andcompressor is not required.DGHPs transfer heat via 30-metre deep, 75-mmdiameter bore holes compared with 100-metredeep, 150-mm diameter bores used for water-loopGHPs. A continuous, closed loop <strong>of</strong> copperpiping is inserted and sealed with a <strong>the</strong>rmallyconductive grout (cement). Below 5 metres <strong>the</strong>Earth remains at a stable temperature all-yearround(27 o C at Boolardy, WA). The smallertemperature difference between <strong>the</strong> heatsource/sink and <strong>the</strong> building or water to beheated/cooled results in lower head pressure andenergy requirement <strong>of</strong> <strong>the</strong> compressor comparedto conventional heating and cooling systems. A“desuperheater” may be employed in chillingapplications to fur<strong>the</strong>r optimise <strong>the</strong> performanceand produce hot water or air which can be usedusefully elsewhere.ASKAPThe <strong>Australian</strong> Square Kilometer Array Pathfinder(ASKAP) radio telescope is an array <strong>of</strong> 36 x 12-mdiameter parabolic dish antennae situated inBoolardy WA (Fig. 2) whose constructioncommenced in early <strong>2010</strong> and is a precursor to<strong>the</strong> Square Kilometer Array (SKA) <strong>of</strong> severalthousand 12-m dishes. A prototype <strong>of</strong> <strong>the</strong>Electronics Systems (ES) and Phased Array Feed(PAF) package to be cooled has been installed at<strong>the</strong> CSIRO <strong>Australian</strong> Telescope National Facility(ATNF) headquarters in Marsfield, NSW. Thesetwo components should not exceed 20 - 30 o Cunder all operating and wea<strong>the</strong>r conditions andrequire an estimated heat dissipation <strong>of</strong> 5 – 7kW th . Various cooling methods have beenconsidered and <strong>the</strong> extreme desert temperaturesand high price <strong>of</strong> diesel generated power stronglyfavour a DGHP solution. The results <strong>of</strong> testing <strong>of</strong>a DGHP at Boolardy are summarised in thispaper.410


System DesignCooling is provided by a 14 kW th DGHP whichcirculates refrigerant (R407C) through 6 x 30-mcopper earth loops to a refrigerant-to-water, coilin-tankheat exchanger. Water in <strong>the</strong> 200 L buffertank is chilled to 7 – 15 o C. Water is circulatedfrom this buffer tank to <strong>the</strong> PAF & ES to deliver<strong>the</strong> required cooling to <strong>the</strong> heating load (<strong>the</strong>“secondary” circuit). The design <strong>of</strong> <strong>the</strong> secondarycircuit is beyond <strong>the</strong> scope <strong>of</strong> this paper – here<strong>the</strong> performance as a function <strong>of</strong> <strong>the</strong>rmal load isexplored by a test load. The test load is a 50 Lwater tank with three elements (3.6, 4.8, 4.8 kW)that can be switched on to produce 3.6, 4.8, 8.4,9.6, 13.2 kW. A circulation pump continuallycirculates water through this test load andcontributes circa 0.5 kW <strong>of</strong> heating. A controllerachieves <strong>the</strong> specified water temperature.Earth Loop InstallationThe 14 kW th system requires 6 x 30-m copperearth loops (½-inch vapour and ¼-inch liquid) withPVC insulation on <strong>the</strong> upper 15-m <strong>of</strong> <strong>the</strong> liquid lineto minimise heat transfer between <strong>the</strong> two andstop flashing <strong>of</strong> <strong>the</strong> liquid refrigerant. 70-mmdiameter holes are drilled vertically 30-m deep ina hexagonal configuration around a point 10mfrom <strong>the</strong> pedestal foundation edge with 3-mspacing between <strong>the</strong>m to allow sufficient <strong>the</strong>rmaldiffusion through <strong>the</strong> ground. After insertion <strong>of</strong> <strong>the</strong>loops <strong>the</strong> holes are filled with a <strong>the</strong>rmallyconductive (geo<strong>the</strong>rmal) grout (e.g. 111-mix,Therm-Ex, IDP-357, Baro<strong>the</strong>rm) ensuring that<strong>the</strong>re are no air pockets. The liquid & vapourlines from <strong>the</strong> earth loops are brazed to <strong>the</strong>irrespective manifolds (½-inch liquid & 7/8-inchvapour) using a 15% silver brazing alloy. Theliquid line is insulated with ½-inch non-corrosiveinsulation material (e.g. Armaflex, Insul-Lock) andrun towards <strong>the</strong> heat pump (compressor) with amaximum length <strong>of</strong> 40-m. 5 data bores were alsodrilled. The location <strong>of</strong> all bores was logged bytriangulation to GPS pegs on <strong>the</strong> foundation (asshown below).<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Buffer Tank, Heat Exchanger & Test LoadChilling is delivered through a submerged copperevaporator coil inside a 200 L buffer tank – this isin contrast to <strong>the</strong> brazed-plate heat exchangerused in <strong>the</strong> Marsfield installation. Water flows over<strong>the</strong> coils via a central perforated copper pipe toensure effective heat transfer. A minimum flowrate <strong>of</strong> 0.6 L/s (36 L/min) is required to achievethis. A 50 L test tank equipped with threeswitchable heating coils (4.8, 4.8 & 3.6 kW)simulates <strong>the</strong> load. The test tank is connected to<strong>the</strong> buffer tank via 32mm polyethylene pipe.Figure 4: Evaporator coil & load tankHeat Pump Design & RefrigerationThe DGHP installed at Boolardy differs from thatinstalled Marsfield in <strong>the</strong> following ways:- The desuperheater coil is built into <strong>the</strong>unit- The unit is cooling only having noreversing valve- It has a nominal capacity <strong>of</strong> 14 kWth (cf.10.5 kWth) to cater for pedestal coolingFigure 1: Loops, liquid & vapour manifold andtrenches.The components are described in turn.Compressor: A 3-phase Scroll compressor drives<strong>the</strong> heat pump with compression ratio <strong>of</strong> 4. Itsefficiency is a function <strong>of</strong> <strong>the</strong> evaporating andcondensing temperatures (pressures).411


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Active Charge Control (ACC): This:• prevents liquid refrigerant from reaching <strong>the</strong>compressor by acting as a reservoir;• evaporates refrigerant to keep <strong>the</strong> systemproperly charged and to eliminate superheat;• improves volumetric efficiency, reduces powerdraw, and lets compressor run cooler;• enables passage <strong>of</strong> oil entrained in refrigerant;• indicates refrigerant level via 3 sight glasses.Liquid Flow Control (LFC): This is an efficientThermal Expansion Valve (TXV) which:• Sets proper refrigerant flow rate based oncondenser (upstream) operating conditions;• Ensures zero sub-cooling so condenser is fullyactive;• Reduces compressor discharge pressure andlowers power requirement;• Prevents vapor from “blowing through”.Oil Separator: Oil lubricates <strong>the</strong> compressor and<strong>the</strong> oil separator acts with <strong>the</strong> ACC to prevent oilfrom migrating down <strong>the</strong> earth loops.Dryer: This filters and dries <strong>the</strong> refrigerant beforeit enters <strong>the</strong> LFC.Refrigerant: R407C [HFC azeotrope: R32 (23%)+ R125 (25%) + R134a (52%)]. Future work willexplore o<strong>the</strong>r HFC and hydrocarbon refrigerants.Expected PerformanceThe Air-Conditioning, Heating and RefrigerationInstitute (AHRI) has a well-established standardfor DGHPs: ANSI/ARI Standard 870, 2001. Also,DGHPs are <strong>Energy</strong>Star rated, endorsed by <strong>the</strong>Environmental Protection Authority (EPA) andElectrical Testing Laboratories (ETL) tested. TheDGHP manufacturer, EarthLinked, providesperformance tables which are derived from both<strong>the</strong> Scroll compressor’s performance and fieldtrials. For an earth temperature <strong>of</strong> 27 o C andchilling water to 15 o C, <strong>the</strong> expected Coefficient <strong>of</strong>Performance (COP = <strong>the</strong>rmal energy removed/electrical energy input) is 4.5 – 5.0 depending onload. The <strong>the</strong>oretical maximum (Carnot cycle)performance for cooling is given by T evap /(T cond –T evap ) where T cond is <strong>the</strong> condensing temperatureand T evap <strong>the</strong> evaporating temperature (Kelvin)and is 7.7 for T cond = 42 o C and T evap = 6 o C whichcorrespond to <strong>the</strong> above conditions. Select7s<strong>of</strong>tware from Emerson Climate Technologies(manufacturer <strong>of</strong> Copeland Scroll compressors)suggests 14 kW.MethodologyFigure 5: Final setupTo find <strong>the</strong> most efficient means <strong>of</strong> cooling, <strong>the</strong>COP is measured as a function <strong>of</strong> <strong>the</strong> controllableaspects <strong>of</strong> <strong>the</strong> system. The key controllablevariables are:Buffer Set Point (T b-set ): <strong>the</strong> temperature to which<strong>the</strong> buffer tank is controlled to be chilled – it ismeasured inside <strong>the</strong> buffer tank.Buffer Maximum (T b-max ): <strong>the</strong> buffer tanktemperature at which <strong>the</strong> controller switches on<strong>the</strong> chilling DGHP.Cabinet Set Point (T cabinet ): <strong>the</strong> temperature towhich <strong>the</strong> cabinet is cooled.Secondary Load (P load ): <strong>the</strong> <strong>the</strong>rmal power whichis simulated with a set <strong>of</strong> heaters.Tank Load (P tank ): <strong>the</strong>re are no elements in <strong>the</strong>tank.O<strong>the</strong>r input variables include:Ambient Temperature: this includes both <strong>the</strong> wet(T wet ) and dry (T dry ) bulb temperatures.Environmental Gain (P envt ): <strong>the</strong> tank & pipes areinsulated but <strong>the</strong>re is still environmental gain.Tank Volume (V tank ): <strong>the</strong> buffer tank volume.Water Volume (V water ): volume <strong>of</strong> water in <strong>the</strong>system: tank, primary & secondary pipes.Output variables include:Compressor Electrical Power (P comp ): <strong>the</strong>electrical power used by <strong>the</strong> compressor.Cycle Time (t cycle ): <strong>the</strong> time between compressorstart-ups.Compressor Time (t comp ): <strong>the</strong> time <strong>the</strong>compressor is on during a cycle.Duty Cycle (D): <strong>the</strong> percentage <strong>of</strong> time <strong>the</strong>compressor is on (t comp /t cycle ).Earth Loop Temperatures (T 5–30m ): Thetemperatures measured at 5, 10, 15, 20, 25 &30m.Refrigerant liquid & vapour temperature (T liq ,T vap ): <strong>the</strong> temperatures to and from <strong>the</strong> earthloopsSuction, Head & Return Pressures (P head , P suc,P ret ): The pressures in & out <strong>of</strong> <strong>the</strong> compressorand returning from <strong>the</strong> earth loops.412


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>ResultsCOP CalculationThe default input values are: T b-set = 13 o C, T b-max= 15 o C, T cabinet = 23 o C, P load = 8.4 kW th , P tank = 0,V tank = 200 L, V water = 273 L. The ambienttemperature varies between 10 and 35 o C during<strong>the</strong> test periods and future results will becalibrated against this. An estimate <strong>of</strong> <strong>the</strong>environmental gain was determined by cooling <strong>the</strong>buffer to 15 o C, leaving <strong>the</strong> system <strong>of</strong>f andmeasuring <strong>the</strong> time taken (t envt ) for <strong>the</strong>temperature to increase a known amount (∆T test ).P envt = C pw .V water .ρ w . ∆T test /t envt where C pw = 4.2kJ/(kg.K) is <strong>the</strong> specific heat <strong>of</strong> water, ρ w = 1 kg/Lis <strong>the</strong> density <strong>of</strong> water. It was found that for ∆T test= 2 K, t envt = 135 min giving P envt = 208 W.Figure 5 shows <strong>the</strong> temperature and pressureoutputs for <strong>the</strong> above input conditions. From<strong>the</strong>se results, <strong>the</strong> COP can be derived. We findt cycle = 1160 sec, t comp = 780 sec, giving D =67.24%. There is a temperature overshoot <strong>of</strong>typically 0.3 – 0.5 K below T b-set and above T b-maxgiving ∆T = 2.8 K. The power required to reduce<strong>the</strong> system water temperature is P water =C pw .V water .ρ w . ∆T/t comp = 4.12 kW th .The electric power consumed by <strong>the</strong> compressor+ pump + monitoring equipment is measuredcontinuously along with <strong>the</strong> electric powerrequired for <strong>the</strong> pump alone. This allows <strong>the</strong> totalelectrical energy consumed over a known number<strong>of</strong> cycles to be computed. For this run, E = 3.081MJ is consumed over n cycle = 3 cycles (19.33 min)and <strong>the</strong> average power (directly monitored) P comp= E/(t comp .n cycle ) = 3.95 kW elec .COP = [P water + (P load + P envt )/D]/P comp = 4.46. Notethat D accounts for <strong>the</strong> fact that <strong>the</strong> load andenvironment are constantly delivering heat to <strong>the</strong>system which must be dissipated by <strong>the</strong> heatpump whilst on.Using this method (see appendix), <strong>the</strong> COP iscalculated as a function <strong>of</strong> load and DGHPconfiguration and plotted below. It is clear that <strong>the</strong>system should not be designed to run with a100% duty cycle. An initial configuration <strong>of</strong> <strong>the</strong>system had <strong>the</strong> heat pump unit 30 m away from<strong>the</strong> earth loops. After moving <strong>the</strong> DGHP to within4 m <strong>of</strong> <strong>the</strong> earth loops, <strong>the</strong> pressure drop across<strong>the</strong> earth loops was 5 – 15 PSI lower. Also, <strong>the</strong>manifold pit was initially exposed for testing andthus about 15 m <strong>of</strong> <strong>the</strong> copper earth loops wasexposed to air and thus not efficiently dissipatingheat. Backfilling <strong>the</strong> manifold pit boosted <strong>the</strong>performance.Mean Earth TemperatureThe undisturbed mean ground temperature wasmeasured every 5m to 30m down six bore holes(two active and four data) via temperaturesensors. One <strong>of</strong> <strong>the</strong> bore holes (B5) has sensorsat 1, 2 and 3m also. Initial temperature readingswere measured on 4 th May <strong>2010</strong> and <strong>the</strong>y werecorroborated with data loggers (LASCAR EL-USB-2) on 2 nd June <strong>2010</strong> (late Spring in Australia,equivalent to November in <strong>the</strong> Nor<strong>the</strong>rnHemisphere). The temperature is plotted as afunction <strong>of</strong> depth below and corroborates withwhat is expected. Independent verification <strong>of</strong>temperature data has been important as <strong>the</strong>expected mean earth temperature was 23 C. A120m test hole for water geoexchange was drilledat <strong>the</strong> Murchison Radio Observatory central siteapproximately 2 km away from <strong>the</strong> DGHPinstallation at antenna #29. Bore water inhabitedthis hole at a depth <strong>of</strong> 31.3m. The data loggerswere hung down <strong>the</strong> hole to a depth <strong>of</strong> 30m on arope at depths 0.5,5,15,30 m and left for 20 hrwith resultant mean earth temperatures <strong>of</strong> 21,29.5, 27.5, 27 respectively (see figure). A sample<strong>of</strong> <strong>the</strong> bore water (jar down rope) was taken andits temperature upon extraction was just under 27C measured with a probe <strong>the</strong>rmometer. Thisprovides a third means <strong>of</strong> verifying <strong>the</strong> boretemperature and corroborates.413


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>DC19.00 DC1918Physical AI4-10 WT TANK 1 - OUTPUT4-11 AMBIENT - OUTPUT.AI.01.05.09 - OUTPUT.AI.01.05.10 - OUTPUT17161514131206/03 00:30 01:00 01:30 02:00 02:30 03:0000:31 Thu 06/03DC47.79 DC4846Physical AI3-1 LB1 TMP 5 - OUTPUT3-2 LB1 TMP 10 - OUTPUT3-3 LB1 TMP 15 - OUTPUT3-4 LB1 TMP 20 - OUTPUT3-5 LB1 TMP 25 - OUTPUT3-6 LB1 TMP 30 - OUTPUT444240383606/03 00:30 01:00 01:30 02:00 02:30 03:0002:42 Thu 06/03PSI393.93 PSI400350Physical AI.AI.01.02.01 - OUTPUT1-01 COMP LP - OUTPUT1-02 COMP HP - OUTPUT1-03 COMP L/L - OUTPUT300250200150100Ground pH & Bore water salinity5006/03 00:30 01:00 01:30 02:00 02:30 03:0001:46 Thu 06/03The pH and salinity <strong>of</strong> bore water used for <strong>the</strong><strong>the</strong>rmal grout was measured with testing strips.pH = 7.8 - 8.2 - acidity is thus not an issue forcorrosion <strong>of</strong> <strong>the</strong> copper loops. The chloride levelsare circa 850 mg/L. This is a borderline reading <strong>of</strong><strong>the</strong> bore water. The aquifer was not penetrated by<strong>the</strong> site #29 bores and <strong>the</strong> ground is probablybenign. Taking a conservative approach, aCathodic Protection System will be installed forthis system – a solar solution for its power isbeing exploring.Abridged ResultsFor <strong>the</strong> presentation <strong>of</strong> data, a period from 12:00– 3:00am on 3 rd June <strong>2010</strong> was chosen. Belowappear <strong>the</strong> water (buffer tank) temperatures,temperatures down LB1, pressures, 15m boretemperature for all active bores, refrigeranttemperatures throughout <strong>the</strong> system, and electricpower. Also initially available temperatures from<strong>the</strong> data bores are plotted: B5 0.3m data bore,15m bore temperature for all data bores, B4 6mdata bore.DC40393837363539.98 DCPhysical AI3406/03 00:30 01:00 01:30 02:00 02:30 03:00DC908070605040302085.77 DC00:16 Thu 06/031006/03 00:30 01:00 01:30 02:00 02:30 03:00KW544.97 KWPhysical AI01:41 Thu 06/03Physical AI3-13 LB3 TP 15 - OUTPUT3-3 LB1 TMP 15 - OUTPUT3-9 LB2 TMP 15 - OUTPUT5-8 B5 TMP 13M - OUTPUT3-14 LB4 TP 15 - OUTPUT3-15 LB5 TP 15 - OUTPUT3-16 LB6 TP 15 - OUTPUT4-2 HP TEMP - OUTPUT4-3 LIQUID TMP - OUTPUT4-6 WT IN 1A - OUTPUT4-8 WT OUT 1A - OUTPUT5-2 M/VAPOUR - OUTPUT5-3 M/ LIQUID - OUTPUTCOMP SUCT TEMP - OUTPUT4-13 KWH 1 - OUTPUT4-14 KWH 2 - OUTPUT321006/03 00:30 01:00 01:30 02:00 02:30 03:0001:22 Thu 06/03414


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>DC31.030.530.029.529.028.528.027.527.0BENCH TOP26.505/29 05/30 05/31 06/01 06/02 06/03DC29.229.028.828.628.428.228.027.827.627.49 DCBENCH TOP27.405/29 05/30 05/31 06/01 06/02 06/03DC30.029.529.028.528.027.36 DC03:17 Thu 06/03Physical AI5-8 B5 TMP 13M - OUTPUT5-4 B5 TMP 1M - OUTPUT5-5 B5 TMP 2M - OUTPUT5-6 B5 TEMP 3M - OUTPUT5-7 B5 TEMP 8M - OUTPUT5-4 B5 TMP 1M - OUTPUT5-5 B5 TMP 2M - OUTPUT5-6 B5 TEMP 3M - OUTPUT5-7 B5 TEMP 8M - OUTPUT5-8 B5 TMP 13M - OUTPUT5-8 B5 TMP 13M - OUTPUT5-8 B5 TMP 13M - OUTPUT2-12 B4 TMP 15 - OUTPUT2-06 B3 TMP 15 - OUTPUT1-6 B1 TMP 15M - OUTPUT1-12 B2 TMP 15 - OUTPUT2-12 B4 TMP 15 - OUTPUT2-06 B3 TMP 15 - OUTPUT1-6 B1 TMP 15M - OUTPUT1-12 B2 TMP 15 - OUTPUT2-15 B4 TMP 30 - OUTPUT2-14 B4 TMP 25 - OUTPUT2-13 B4 TMP 20 - OUTPUT2-12 B4 TMP 15 - OUTPUT2-11 B4 TMP 10 - OUTPUT2-10 B4 TMP 05 - OUTPUTThis corroborates with data obtained fromMarsfield – it was expected that <strong>the</strong> higher groundtemperature would slightly reduce output &performance. As in Marsfield, it has beendemonstrated that COP decreases as a function<strong>of</strong> load in <strong>the</strong> secondary circuit (which determines<strong>the</strong> duty cycle) simulated by a test tank. Fur<strong>the</strong>rresults are being obtained for this configurationand additional experiments include <strong>the</strong> use <strong>of</strong>alternative refrigerants. The <strong>the</strong>rmal conductivity& o<strong>the</strong>r properties <strong>of</strong> <strong>the</strong> ground will be calculatedby comparison with analytic and numericalmodels.AcknowledgementsThis scientific work uses data obtained from <strong>the</strong>Murchison Radio-astronomy Observatory. Weacknowledge <strong>the</strong> Wajarri Yamatji people as <strong>the</strong>traditional owners <strong>of</strong> <strong>the</strong> Observatory site. Weacknowledge <strong>the</strong> CSIRO, CASS team includingGrant Hampson, Evan Davis, Antony Schinckel,Graham Allen, Steve Broadhurst along withRobert Rechtman & Mike Francis <strong>of</strong> Direct<strong>Energy</strong>, David & Peter Manoni from Geo<strong>the</strong>rmalWA, Hugh Campbell & Nigel Foster <strong>of</strong> DongaraDrilling and Shannon Lovett, Nick Holt & MarkAlden <strong>of</strong> Emerson Climate Technologies.27.5References27.006/03 00:30 01:00 01:30 02:00 02:30 03:00DC5654525048464442403836343254.59 DC02:51 Thu 06/03Physical AI3006/02 12:00 16:00 20:00 06/0313:54 Wed 06/025-2 M/VAPOUR - OUTPUT5-3 M/ LIQUID - OUTPUT3-3 LB1 TMP 15 - OUTPUT3-2 LB1 TMP 10 - OUTPUT3-1 LB1 TMP 5 - OUTPUT3-4 LB1 TMP 20 - OUTPUT3-5 LB1 TMP 25 - OUTPUT3-6 LB1 TMP 30 - OUTPUTAnalytic derivation <strong>of</strong> <strong>the</strong> expected groundtemperatures will be presented in a future paper.As seen above, after <strong>the</strong> compressor starts, <strong>the</strong>ground temperatures rise asymptotically towardssaturation at which <strong>the</strong>rmal output matches<strong>the</strong>rmal dissipation in <strong>the</strong> ground. Maximum load(13.2 kW th ) was applied from 10:38am to 17:17and <strong>the</strong> water temperature was held down to 15C. After switching <strong>of</strong>f <strong>the</strong> load, <strong>the</strong> groundrecovers. At 18:11 a 3.6 kW load is applied, at18:45, 4.8 kW and at 19:26:30, 8.4 kW.Conclusions & Fur<strong>the</strong>r WorkDGHPs are an efficient solution for heating andcooling and are particularly suitable for cooling ina desert environment with no power infrastructure.It has been shown that a DGHP is able to deliver13-15 C chilled water despite high groundtemperatures <strong>of</strong> 27.5 C. It does with a COPbetween 4 and 5 for <strong>the</strong> expected load range.Payne, D. J. B., Hampson, G., Kiraly, D. andDavis, E. Direct GeoExchange Cooling for <strong>the</strong><strong>Australian</strong> Square Kilometer Array Pathfinder,<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> 2009Payne, D. J. B., Ward, M. And King, R. L.,Position Paper: Direct Use Geo<strong>the</strong>rmalApplications, <strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong>Association (AGEA), Feb 2008.Yu MZ, Peng XF, Li XD, Fang ZH, A simplifiedmodel for measuring <strong>the</strong>rmal properties <strong>of</strong> deepground soil, Experimental Heat Transfer, 17(2):119-130, 2004.Cui, Ping, H. Yang and Z. Fang, Heat transferanalysis <strong>of</strong> ground heat exchangers with inclinedboreholes, Applied Thermal Engineering, Vol.26,1169-1175Marcotte, Denis and Philippe Pasquier, The effect<strong>of</strong> borehole inclination <strong>of</strong> fluid and groundtemperature for GLHE systems, Geo<strong>the</strong>rmics,Volume 38, Issue 4, pp 392-398Bristow, K. L., R. D. White, and G. J. Kluitenberg,Comparison <strong>of</strong> single and dual probes formeasuring soil <strong>the</strong>rmal properties with transien<strong>the</strong>ating, Aust. J. Soil Res. 32, pp. 447–464415


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>A Research Well for <strong>the</strong> Pawsey Geo<strong>the</strong>rmal Supercomputer CoolingProjectKlaus Regenauer-Lieb* 1,2 and <strong>the</strong> WAGCoE team 1,2,3 , Peter Malin 4 and <strong>the</strong> IESE team, Steve Harvey 2and <strong>the</strong> CSIRO CESRE team, Edson Nakagawa 2 and CSIRO’S Geo<strong>the</strong>rmal & Petroleum Portfolio, HalGurgency 5 and <strong>the</strong> QGECE team1,2, 3 Western <strong>Australian</strong> Geo<strong>the</strong>rmal Centre <strong>of</strong> Excellence,1 The University <strong>of</strong> Western Australia, M004, 35 StirlingAv. 6009,Crawley2 CSIRO Earth Science & Resources Engineering, ARRC, 26 Dick Perry Avenue, Kensington, Western Australia 61513 Curtin University, Kent Street, Bentley, Perth Western Australia, 61024 Institute for Earth Science Engineering, University <strong>of</strong> Auckland, Auckland, NZ5 Queensland Geo<strong>the</strong>rmal Centre <strong>of</strong> Excellence, The University <strong>of</strong> QueenslandBrisbane, Queensland, 4072 AustraliaAbstract:The <strong>Australian</strong> Government has funded <strong>the</strong>Pawsey supercomputer in Perth, providingcomputational infrastructure intended to support<strong>the</strong> future operations <strong>of</strong> <strong>the</strong> <strong>Australian</strong> SquareKilometre Array (SKA) and to boost nextgenerationcomputational geosciences inAustralia. Supplementary Federal EIF funds havebeen directed to <strong>the</strong> development <strong>of</strong> a geo<strong>the</strong>rmalexploration well to research <strong>the</strong> potential for direc<strong>the</strong>at use applications at <strong>the</strong> Pawsey Centre site.Cooling <strong>the</strong> Pawsey supercomputer may beachieved by geo<strong>the</strong>rmal heat exchange ra<strong>the</strong>rthan by conventional electrical power cooling,thus reducing <strong>the</strong> carbon footprint <strong>of</strong> <strong>the</strong> PawseyCentre and demonstrating an innovative greentechnology that is widely applicable in industryand urban centres across <strong>the</strong> world. Theexploration well is scheduled to be completed in2013, with drilling due to commence in <strong>the</strong> thirdquarter <strong>of</strong> 2011. One year is allocated to finalizing<strong>the</strong> design <strong>of</strong> <strong>the</strong> exploration, monitoring andresearch well, and first concepts will be presentedat AGEC for discussion and participation.Success in <strong>the</strong> geo<strong>the</strong>rmal exploration andresearch program will result in an industrial-scalegeo<strong>the</strong>rmal cooling facility at <strong>the</strong> Pawsey Centre,and will provide a world-class student trainingenvironment in geo<strong>the</strong>rmal energy systems.Keywords: Direct Heat, Absorption Chiller, HotSedimentary Aquifer, SKA, High PerformanceComputingIntroductionJune 9th, <strong>2010</strong> marks <strong>the</strong> first step to one <strong>of</strong> <strong>the</strong>largest direct heat demonstrators in Australia. Adirect heat geo<strong>the</strong>rmal demonstration project,using hot sedimentary aquifers to provide coolingand ventilation to <strong>the</strong> Pawsey High-PerformanceComputing Centre and <strong>the</strong> co-located CSIROfacility <strong>the</strong> <strong>Australian</strong> Resources Research Centresecured funding through <strong>the</strong> Sustainability Round<strong>of</strong> <strong>the</strong> Education Investment Fund (EIF). ThePawsey Centre demonstrator is part <strong>of</strong> <strong>the</strong>infrastructure <strong>of</strong> Australia and New Zealand’s bidto host <strong>the</strong> SKA (square kilometre array) radiotelescope. The Pawsey Centre (see Figure 1)supports <strong>the</strong> enormous data requirements fordeep space research and is also planned to be aprime enabling platform for Australia’scomputational geoscience and nanosciencecommunities. The supercomputer-cooling projectwill be <strong>the</strong> first <strong>of</strong> its kind and will demonstrate <strong>the</strong>feasibility for widespread use <strong>of</strong> <strong>the</strong> clean andsustainable geo<strong>the</strong>rmal energy source to power,for example, hospitals, shopping centres ando<strong>the</strong>r industrial scale applications.The Pawsey Centre is to be situated on <strong>the</strong> deepsediments <strong>of</strong> <strong>the</strong> Perth Basin, where a verticalsequence <strong>of</strong> hot sedimentary aquifers suitable fordirect heat geo<strong>the</strong>rmal applications is now beingstudied.Construction on <strong>the</strong> exploration well project isscheduled to commence in November <strong>2010</strong>,drilling <strong>of</strong> <strong>the</strong> exploration hole is scheduled forNovember 2011 and <strong>the</strong> project is to becompleted in August 2013 (see table 1), <strong>the</strong>provisional timetable is coordinated with <strong>the</strong>international SKA decision-making process.Australia and New Zealand, toge<strong>the</strong>r, are incompetition with an African SKA bid, involvingSouth Africa, Namibia, Botswana, Mozambique,Madagascar, Mauritius, Kenya and Ghana. Adecision is expected to be made in 2012. ThePawsey Centre geo<strong>the</strong>rmal demonstrator is part<strong>of</strong> a portfolio <strong>of</strong> solar and geo<strong>the</strong>rmaltechnologies, notably an additional ground sourceheat pump design for radio antenna cooling. Theoverall goal is to supply a reliable and clean,sustainable energy solution for <strong>the</strong> <strong>Australian</strong>/NZSKA bid.This contribution gives a brief overview <strong>of</strong> <strong>the</strong>entire concept, its location, timing, and <strong>the</strong> aboveand below ground technology concepts plannedto support <strong>the</strong> design <strong>of</strong> a production geo<strong>the</strong>rmallypowered cooling system. Collaborations between<strong>Australian</strong> and NZ researchers on potentialdesigns for <strong>the</strong> exploration well are discussed.416


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>The Pawsey Supercomputer Coolingproject, a brief overviewOne <strong>of</strong> <strong>the</strong> strategic goals <strong>of</strong> <strong>the</strong> successful EIFSustainability Round proposal is to form throughdemonstration projects a joint research focus forscientists and students from all over Australia andNZ in renewable energy, as well as in astronomy,computer science, engineering, geology andenvironmental management.Figure 1. The Pawsey High-Performance ComputingCentre cooling project will be located on <strong>the</strong> CSIROTechnology Park site near <strong>the</strong> Perth CBD close toWestern <strong>Australian</strong> universities.The Pawsey Supercomputer Cooling (PSC)project is located centrally in Perth (Figure 1) andits collaborations with <strong>Australian</strong> and NZ partnerssets a sound basis for achieving this goal. Theadditional placement <strong>of</strong> a research well <strong>of</strong>fers <strong>the</strong>necessary infrastructure investment for researchcollaboration in <strong>the</strong> wider <strong>Australian</strong> and NZgeoscience community for testing, monitoring andexploitation <strong>of</strong> hot sedimentary aquifers.The PSC direct heat geo<strong>the</strong>rmal demonstratorutilises a hot sedimentary aquifer under Perth withan estimated temperature <strong>of</strong> 100 C at 3 kmdepth.Based on <strong>the</strong> available information andextrapolation from a 3 km deep petroleumexploration well (Cockburn 1, see Figure 3)located 21 km away from <strong>the</strong> Pawsey site onepossible scenario could be a 3 km deep extractionand injection well into <strong>the</strong> Cadda formation with ameasured permeability <strong>of</strong> 632-732 mDarcy and ameasured layer thickness <strong>of</strong> 350 m. Ano<strong>the</strong>roptional target layer is <strong>the</strong> Yarragadee aquiferdirectly above <strong>the</strong> Cadda formation featuringpermeabilities <strong>of</strong> up 1200 mDarcy according to<strong>the</strong> Cockburn 1 records. The advantage <strong>of</strong> thistarget is its expected lower salinity than <strong>the</strong>Cadda Formation. Shallower portions <strong>of</strong> <strong>the</strong>Yarragadee aquifer have been successfully usedin ten different fully commercial low-temperatureprojects in Perth, mainly for swimming poolheating. The injection wells in such systems aremuch shallower than <strong>the</strong> extraction bores whichimplies minimal risk <strong>of</strong> <strong>the</strong>rmal breakthrough. Theselection <strong>of</strong> injection depth is governed by localpermeability, net formation water balance andwater quality. Choice <strong>of</strong> <strong>the</strong> lower Yarragadeeover <strong>the</strong> Cadda will depend on <strong>the</strong> trade <strong>of</strong>fbetween flow rates and temperaturesencountered in <strong>the</strong> exploration well.The first design <strong>of</strong> <strong>the</strong> above ground infrastructurecomprises two absorption chillers (Figure 4) at aFigure 2. Str atigraphy along a se ction through Cockburn 1 deep petroleum exploration well, passing ~20 km to<strong>the</strong> south-west <strong>of</strong> <strong>the</strong> Pawsey Centre. Section from Crostella and Backhouse (2000).417


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>maximum capacity 5 MW th each, one unit isimplemented as a backup unit. The dimension foreach chiller is around 9.38m(L) x 2.2m (W) x 3.6m(H). The absorption chillers require heat rejectionwith an approximate maximum capacity <strong>of</strong> 25MW th . The preliminary design will be adjustedonce <strong>the</strong> actual cooling requirement <strong>of</strong> <strong>the</strong> PSC isknown.which could be abstracted for testing small scaleabove ground demonstrators. Key aspects <strong>of</strong> <strong>the</strong>sampling include water quality analyses thatprovide important indicators for heat exchangeplant and reinjection sustainability. Given, <strong>the</strong> longlead-up time for commencement <strong>of</strong> drilling (Table1) <strong>the</strong> design <strong>of</strong> <strong>the</strong> exploration well and <strong>the</strong>above and below ground research componentsare fully open for discussion. In <strong>the</strong> spirit <strong>of</strong> <strong>the</strong>EIF funding we call here for active researchcollaborations that can complement <strong>the</strong> fundedinfrastructure with <strong>the</strong> best available expertise andinterpretation.Figure 3. The Pawsey High Performance Computercooling demonstrator design scheme consists <strong>of</strong>absorption chiller technology driven by heat from <strong>the</strong>hot sedimentary aquifer.Table1 Preliminary Timetable*Planned ProjectMilestonePlanned CompletionDateProject start October <strong>2010</strong>Perth geo<strong>the</strong>rmal drillingprogram commencesPerth geo<strong>the</strong>rmal drillingcompletedAugust 2011November 2011Project completion December 2013* timings are tentative only and subject to revisionThe Dual Purpose <strong>of</strong> <strong>the</strong>Exploration/Research WellThe exploration/research well is designed for adual purpose: (1) it breaks <strong>the</strong> ground and obtains<strong>the</strong> first direct samples <strong>of</strong> <strong>the</strong> chosen site prior toinstallation <strong>of</strong> <strong>the</strong> geo<strong>the</strong>rmal production wells;and (2) it <strong>of</strong>fers <strong>the</strong> unique opportunity forimplementing purpose-designed downholesensors,long term monitoring and active testing.An additional attraction for research may be asmall flux <strong>of</strong> geo<strong>the</strong>rmal waters from <strong>the</strong> aquifer,Preliminary design scenarios <strong>of</strong> <strong>the</strong>Exploration wellThere is no hard data indicating watertemperature (and chemistry) at depths <strong>of</strong> ~3 km in<strong>the</strong> Perth Basin – <strong>the</strong> proposed depth <strong>of</strong> <strong>the</strong>geo<strong>the</strong>rmal production wells. Data acquired from<strong>the</strong> drilling program associated with <strong>the</strong> UWAgeo<strong>the</strong>rmal demonstration site will provide abetter indication <strong>of</strong> water temperature at depth in<strong>the</strong> Perth Basin, but will not obviate <strong>the</strong> need for<strong>the</strong> ARRC geo<strong>the</strong>rmal exploration/research well.This depth <strong>of</strong> drilling is based on data sourcedfrom a ~800m Water Corporation bore adjacent to<strong>the</strong> ARRC site. Data recently acquired from reloggingthis bore by <strong>the</strong> WA Geo<strong>the</strong>rmal Centre <strong>of</strong>Excellence suggests water temperatures <strong>of</strong>~100 C at a depth <strong>of</strong> 3 km. Temperature, (fluidand sediment) chemistry and permeability datawill be acquired through <strong>the</strong> proposed geo<strong>the</strong>rmalexploration/research well. Data on <strong>the</strong> advectiveregimes operating at depth in <strong>the</strong> stratigraphicsequence will also be sought in order to facilitate<strong>the</strong> construction <strong>of</strong> a geo<strong>the</strong>rmal reservoir modelfor <strong>the</strong> Pawsey Centre.The reservoir model will include hydro<strong>the</strong>rmal flowprocesses necessary to describe circulationphenomena in moderate-permeability HSAgeo<strong>the</strong>rmal plays. The reservoir model will inform<strong>the</strong> design specifications <strong>of</strong> <strong>the</strong> subsequentproduction and injection well infrastructure.In preparation to <strong>the</strong> EIF bid IPS Australasia hasbeen tasked to prepare potential design scenariosfor <strong>the</strong> exploration well which are here laid openfor discussion. A number <strong>of</strong> scenarios have beenconsidered for <strong>the</strong> drilling, evaluation, testing andcompletion <strong>of</strong> <strong>the</strong> exploration well with proposedschematics shown in Figure 4.Scenario 1 (Base Case)Scenario 1 (Base Case) is designed with a three-final hole sectionstring casing program withcased with 178mm (7”) casing to 3000 m TrueVertical Depth from Rotary Table (TVD RT)(Figure 5). This design places <strong>the</strong> 244 mm (9-418


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>5/8”) surface casing at 1000 m TVD RT in <strong>the</strong>Yarragadee Formation and contains <strong>the</strong> aboveLeederville and South Perth Shale behind casing(Figure 2). This design <strong>of</strong>fers a 216 mm (8-1/2”)open hole to conduct straddle testing <strong>of</strong> <strong>the</strong>proposed target intervals to 3000 m TVD RT.testing <strong>of</strong> <strong>the</strong> proposed target intervals to 3000 mTVD RT. The 152 mm (6”) hole section drilled to3500 m TVD RT will allow formation evaluation <strong>of</strong>deeper target intervals with <strong>the</strong> option <strong>of</strong> testingand casing with a 5” liner.Figure 4. Wellbore schematics <strong>of</strong> <strong>the</strong> exploration wellaccording to a Desk Study <strong>of</strong> IPS AustralasiaFigure 5. Wellbore schematics <strong>of</strong> Scenario 1exploration well suggested by IPS Australasia (2009).The casing configuration is summarized asfollows:The 340 mm (13-3/8”) conductor shoe isset at a depth between 50 and 100 mTVD RT.The 244 mm (9-5/8”) casing shoe is set ata depth <strong>of</strong> approximately 1000 m TVDRT.At well TD <strong>of</strong> 3000 m TVD RT followingopen hole testing <strong>of</strong> target intervals, a178 mm (7”) casing string will be set.Scenario 2Scenario 2 is <strong>of</strong> a similar design to Scenario 1with a three-string casing program to 3000 m TVDRT with <strong>the</strong> addition <strong>of</strong> a 152 mm (6”) hole sectiondrilled to 3500 m TVD RT. This design places <strong>the</strong>244 mm (9-5/8”) surface casing at 1000 m TVDRT in <strong>the</strong> Yarragadee Formation and contains <strong>the</strong>above Leederville Formation and South PerthShale behind casing. This design <strong>of</strong>fers a216 mm (8-1/2”) open hole to conduct straddleThe casing configuration is summarized asfollows:The 340 mm (13-3/8”) conductor shoe isset at a depth between 50 and 100 mTVD RT.The 244 mm (9-5/8”) casing shoe is set ata depth <strong>of</strong> approximately 1000 m TVDRT.Following open hole testing <strong>of</strong> targetintervals to 3000 m TVD RT, a 178 mm(7”) casing string will be set.Preliminary Design <strong>of</strong> <strong>the</strong> ResearchEquipmentThe preliminary list <strong>of</strong> research equipment fordeployment in <strong>the</strong> exploration well includes:Along-Casing Sensors: Optical fibretemperature monitoring system (Raman scatteringbased), Optical fibre pressure, temperature,acoustic, EM (Bragg grating/cladding based),Surface optical system, electromagnetic/magnetotelluric-receiver-station.419


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Figure 6. Wellbore schematics <strong>of</strong> Scenario 2exploration well suggested by IPS Australasia (2009)Inside Hole: Water pressure tube, mechanicalpackers, banding stand<strong>of</strong>fs (cable protectorsbetween pipes), pressure transducer,geochemical / environmental monitoring samplingsystemDownhole Sonde: Deep sonde (seismometer)<strong>the</strong>rmistor, fluxmeters (desorption method whichneed to be deployed in packed zones to isolatefrom in-well gradients.Redeployable Wireline Exploration System:Wire / data cable and winch system flow meterdownhole formation imager, spectral gamma tool,electrical conductivity, caliper log.This equipment will allow us to monitor <strong>the</strong>pressure, temperature and acoustics <strong>of</strong> <strong>the</strong>aquifer along time and depth, collect fluid samplesat a range <strong>of</strong> depths for geochemistry analyses,seismic, flow rate and temperature data to monitor<strong>the</strong> impact <strong>of</strong> <strong>the</strong> production plant.Above Ground Engineering ResearchWhile this project is demonstrating <strong>the</strong> direct use<strong>of</strong> <strong>the</strong> geo<strong>the</strong>rmal heat in space cooling, ano<strong>the</strong>robjective for <strong>the</strong> <strong>Australian</strong> geo<strong>the</strong>rmal energysector is <strong>the</strong> generation <strong>of</strong> electricity usinggeo<strong>the</strong>rmal heat. Additional targets are pro<strong>of</strong> <strong>of</strong>technology for geo<strong>the</strong>rmal desalination <strong>of</strong>seawater, saline aquifer water and industrialprocess water. Both <strong>Australian</strong> based inventionsare currently being built with support from differentCentres <strong>of</strong> Excellence in Australia.The Queensland Geo<strong>the</strong>rmal <strong>Energy</strong> Centre <strong>of</strong>Excellence (QGECE) is developing newsupercritical cycle technologies to increaseelectricity production from a given geo<strong>the</strong>rmalresource by up to 25% for low temperaturegeo<strong>the</strong>rmal resources and by up to 50% for hightemperature geo<strong>the</strong>rmal resources. One <strong>of</strong> <strong>the</strong>current research projects at <strong>the</strong> QGECE is aimingto develop a 100-kWe portable power plant todemonstrate a supercritical power generationcapability for a sub-150C geo<strong>the</strong>rmal resource.Using this plant as a test bed, optimum designand operating conditions can be ascertained forelectricity generation using <strong>the</strong> geo<strong>the</strong>rmal fluidproduced by a Perth Basin hot sedimentaryaquifer in local ambient conditions.The Western <strong>Australian</strong> Geo<strong>the</strong>rmal Centre <strong>of</strong>Excellence (WAGCoE) in collaboration with <strong>the</strong>National Centre <strong>of</strong> Excellence for Desalinationintends to use <strong>the</strong> extracted geo<strong>the</strong>rmal waterboth as a heat source and feedstock to develop aWAGCoE’s protected distillation baseddesalination technology by constructing acontainerized 4 m 3 /day desalination plant, asschematically suggested in Figure 7. Thistechnology is expected to boost <strong>the</strong> freshwateryield <strong>of</strong> conventional technology by 30%.Hot groundwaterMulti-effect distillation plantFigure 7. A geo<strong>the</strong>rmal distillation desalinationplantReferencesSalineground waterConcentrateDistilled waterCrostella and Backhouse (2000) Goelogy andPetroleum Exploration <strong>of</strong> <strong>the</strong> Central andSou<strong>the</strong>rn Perth Basin, Western Australia,Geological Survey <strong>of</strong> Western Australia, DMPReport 57IPS Australasia (2009) A Desk Study: ProposedGeo<strong>the</strong>rmal Project at <strong>the</strong> <strong>Australian</strong> ResourcesResearch Centre.420


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong> <strong>Conference</strong> <strong>2010</strong>Fracture Stimulation – legal risks and liabilitiesKyra Reznikov, Senior Associate, FinlaysonsAbstractFracture stimulation (also known as hydraulicstimulation) involves pumping water at highpressure into a well, which causes fracturing <strong>of</strong><strong>the</strong> rock. This additional fracturing enhances <strong>the</strong>permeability <strong>of</strong> <strong>the</strong> hot dry rock in order to createan efficient hydraulic loop for <strong>the</strong> purposes <strong>of</strong>harnessing geo<strong>the</strong>rmal energy.seek to mitigate <strong>the</strong>ir potential liabilities wherefracture stimulation is proposed.The process <strong>of</strong> fracturing <strong>the</strong> rock can also giverise to seismicity events – that is, it can inducesmall earthquakes which have <strong>the</strong> potential todamage property and infrastructure not onlywithin <strong>the</strong> exploration licence area but also onadjacent land and fur<strong>the</strong>r afield.The paper will examine <strong>the</strong> legal risks andpotential consequences <strong>of</strong> fracture stimulation,including:• damage caused by seismicity eventscould result in <strong>the</strong> commission <strong>of</strong> an<strong>of</strong>fence under environment protectionlegislation (which prohibits <strong>the</strong> causing<strong>of</strong> harm to <strong>the</strong> environment, propertyand <strong>the</strong> health, safety and amenity <strong>of</strong>people) or under resources legislation(which for instance prohibitsinterference with mining operations);• landowners or operators <strong>of</strong>infrastructure that suffer damage to<strong>the</strong>ir property may also seekcompensation for losses caused by <strong>the</strong>seismicity events;• if concerned about <strong>the</strong> potential impactson <strong>the</strong> environment and property,regulators could issue orderspreventing fracture stimulation, orallowing it only after precautionarymeasures are put in place.The paper will discuss <strong>the</strong> legal riskmanagement measures that geo<strong>the</strong>rmaloperators should include in project planning to421


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>QGECE Mobile Geo<strong>the</strong>rmal Test Plant & ORC Cycle ChallengesAndrew S. Rowlands and Jason CzaplaThe Queensland Geo<strong>the</strong>rmal <strong>Energy</strong> Centre <strong>of</strong> Excellence (QGECE),The University <strong>of</strong> Queensland, St Lucia, Brisbane, Qld 4072*Corresponding author: a.rowlands@uq.edu.auGeo<strong>the</strong>rmal energy reserves in Australia have <strong>the</strong>potential to provide electrical energy for hundreds<strong>of</strong> years. However, due to <strong>the</strong> variety <strong>of</strong>temperatures in geo<strong>the</strong>rmal resources a one-sizefits-allapproach to surface power infrastructure isnot appropriate. Fur<strong>the</strong>rmore, <strong>the</strong> use <strong>of</strong>traditional steam as a working fluid is rarely afeasible option because resource temperatures liein <strong>the</strong> range <strong>of</strong> 100-200°C. To overcome this,organic fluids with lower boiling points than steammay be utilised as working fluids in organicrankine cycles (ORC) in binary power plants. Dueto differences in <strong>the</strong>rmodynamic properties,certain fluids are able to extract more heat from agiven resource than o<strong>the</strong>rs over certaintemperature and pressure ranges. Thisphenomenon enables <strong>the</strong> tailoring <strong>of</strong> power cycleinfrastructure to best match <strong>the</strong> geo<strong>the</strong>rmalresource through careful selection <strong>of</strong> <strong>the</strong> workingfluid and turbine design optimisation to yield <strong>the</strong>optimum overall cycle performance. Here we lookat a selection <strong>of</strong> promising ORC cycles using arange <strong>of</strong> high-density working fluids operating atsub-, or trans-critical conditions that are beingstudied by QGECE as potential binary cyclesystems; discuss <strong>the</strong> challenges facing design <strong>of</strong>ORC cycles and how some <strong>of</strong> <strong>the</strong>se challengesare being addressed in <strong>the</strong> QGECE MobileGeo<strong>the</strong>rmal Test Plant.Keywords: Geo<strong>the</strong>rmal energy, Organic RankineCycle, Working fluids.Modelling Binary Power CyclesIn this investigation, <strong>the</strong> <strong>the</strong>rmodynamic cycle <strong>of</strong>an ORC was simulated for conditionsrepresentative <strong>of</strong> a geo<strong>the</strong>rmal power station.The ORC was modelled as (1) pump work in, (2)heat addition in (i.e. pre-heater, evaporator,superheater), (3) turbine work out, (4) heatrejection out (i.e. pre-cooler, condenser) and (6)regeneration (when <strong>the</strong> temperatures allow).Figure 1 illustrates <strong>the</strong> basic layout <strong>of</strong> an ORCand denotes <strong>the</strong> state points for calculating<strong>the</strong>rmodynamic properties.The fluids database employed was <strong>the</strong> NIST’sREFPROP (NIST 2007). REFPROP <strong>of</strong>fersequations <strong>of</strong> state for 84 pure fluids as well asuser defined mixtures. However, only pure fluidswere used in this analysis (Mixtures may be <strong>the</strong>focus <strong>of</strong> future work).To allow for ranking results <strong>of</strong> <strong>the</strong> various cycles,<strong>the</strong> critical metric used for comparing fluids andcycles is Brine Consumption (β) (Franco, 2009)defined as follows:β = W net / mf geo (kJ/kg)Figure 1: General ORC LayoutWhere W net (kW) is <strong>the</strong> net work produced by <strong>the</strong>cycle and <strong>the</strong> mf geo (kg/s) is <strong>the</strong> mass flow rate <strong>of</strong><strong>the</strong> geo<strong>the</strong>rmal brine. Greater β values indicate agreater yield <strong>of</strong> energy production per unit mass<strong>of</strong> brine. This can be a good metric forgeo<strong>the</strong>rmal energy because it focuses onoptimising <strong>the</strong> energy produced for <strong>the</strong>geo<strong>the</strong>rmal brine produced.The cycle analysis performed indicates that <strong>the</strong>pinch point in an evaporator has a significantimpact on β. This is in agreement with whato<strong>the</strong>rs have stated previously in o<strong>the</strong>r publications(i.e. Saleh 2007). The pinch point is a product <strong>of</strong><strong>the</strong> working fluid’s latent heat <strong>of</strong> evaporation(which is pressure dependent). Minimising pinchpoint effects will allow <strong>the</strong> cycle to make moreefficient use <strong>of</strong> <strong>the</strong> brine flow rate in <strong>the</strong>evaporator.In an ideal scenario <strong>the</strong> brine would cool to <strong>the</strong>inlet temperature <strong>of</strong> <strong>the</strong> working fluid and <strong>the</strong>working fluid would heat up to <strong>the</strong> inlettemperature <strong>of</strong> <strong>the</strong> brine, transferring all <strong>the</strong> heatfrom <strong>the</strong> brine to <strong>the</strong> working fluid. However,<strong>the</strong>re will always be a temperature differentialbetween <strong>the</strong> brine and working fluid becausesome temperature difference is required to drive422


heat through <strong>the</strong> walls <strong>of</strong> <strong>the</strong> heat exchanger.The aim <strong>the</strong>n, is to minimise <strong>the</strong> temperaturedifferential and extract as much heat as possiblefrom <strong>the</strong> brine flow.Figure 2 shows an example <strong>of</strong> a T-s diagram andassociated pinch point plot. The cycle representsa subcritical cycle with superheating.T, o C1<strong>2010</strong>0806040200-20T-S Cycle Diagram (R152a)21ThdThc3 4Thb756T, o C150140130120110Brine Temp.Working Fluid Temp.Tca50 1001009080701000 1500 2000600Tcb TccEntropy, J/kg-KEvaporator Length ProportionFigure 2: T-s diagram and pinch point plot for R152a (Tgeo150°C and Tamb 40°C).Figure 3 shows an example <strong>of</strong> a T-s diagram andassociated pinch point plot. The cycle representsa supercritical cycle. It can be seen that atsupercritical conditions <strong>the</strong> effect <strong>of</strong> pinch point isgone.T, o C1801601401<strong>2010</strong>0806040Thb ThaT-S Cycle Diagram (C5F12)Thd21Tca200 200 400Entropy, J/kg-K7TcbThc34 56TccT, o C2001801601401<strong>2010</strong>080Evaporator Pinch PointBrine Temp.Working Fluid Temp.600 50 100Evaporator Length ProportionFigure 3: T-s diagram and pinch point plot for C5F12 (Tgeo –200°C and Tamb 40°C).Supercritical cycles have <strong>the</strong> potential to yieldefficient cycles because <strong>the</strong>y minimise pinch pointeffects in <strong>the</strong> evaporator and <strong>the</strong>re tends to be alarge enthalpy differential available across <strong>the</strong>turbine in <strong>the</strong> cycle analysis. However, athorough turbine analysis must be undertaken inconjunction with <strong>the</strong> cycle analysis to validate <strong>the</strong>calculated turbine work out from <strong>the</strong> cycleanalysis.Fluid PerformanceThree general categories <strong>of</strong> geo<strong>the</strong>rmaltemperature ranges were focused on to see howdifferent fluids performed at different operatingconditions. The ranges were labelled as low, midand high at temperatures <strong>of</strong> 100, 150 and 200°C,respectively. The ambient temperature was set at40 o C to represent high temperatures that can beseen in central Queensland where our research is<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>focused. For each temperature range <strong>the</strong> fluidswere ranked in ascending order <strong>of</strong> <strong>the</strong>ir calculatedβ. An abbreviated summary <strong>of</strong> <strong>the</strong> results isshown below in Tables 1-3.An obvious trend in <strong>the</strong> results tabulated above isthat haloalkanes perform well at temperatureconditions associated with geo<strong>the</strong>rmal resources.Table 1: Top 5 Fluids (Tgeo = 100°C)Fluid β (kJ/kg) Evap. CaseC4F10 2.07 SubcriticalC5F12 2.06 SubcriticalRC318 2.04 SubcriticalR227ea 2.04 SubcriticalR236FA 2.03 SubcriticalTable 2: Top 5 Fluids (Tgeo = 150°C)Fluid β (kJ/kg) Evap. CaseR152a 18.55 SuperheatedR134A 18.40 SuperheatedRC318 18.28 SuperheatedCOS 18.14 SuperheatedR236FA 17.78 SuperheatedTable 3: Top 5 Fluids (Tgeo = 200°C)Fluid β (kJ/kg) Evap. CaseC5F12 57.91 SupercriticalR236EA 55.67 SupercriticalISOBUTAN 54.61 SupercriticalR152a 52.06 SupercriticalDME 51.35 SupercriticalPerformance maps were also generated for eachfluid for a range <strong>of</strong> temperature conditions (T geoand T amb ). This allows for visualisation <strong>of</strong> howcycle performance can vary with changing inletbrine temperatures (i.e. a geo<strong>the</strong>rmal source maycool over its operating life) and ambient airtemperature (i.e. for air cooled systems thisrepresents shifts in temperature throughout <strong>the</strong>day/night and seasonal change). This can beuseful in ensuring that <strong>the</strong> fluid and cycle selectedwill operate effectively at all anticipated operatingconditions. Figure 5 shows an exampleperformance plot for R245fa. The top plot in <strong>the</strong>figure shows T geo and T amb on <strong>the</strong> x and y-axeswhile β is on <strong>the</strong> z-axis. It is intuitive that whenT amb is at a minimum and T geo is at a maximum βwould be at its peak value. It is perhaps not sointuitive to see that evaporator pressureassociated with <strong>the</strong> optimum β for a given set <strong>of</strong>T geo and T amb varies as it does. This can be an423


important factor in plants performance. Iftemperatures vary, <strong>the</strong>n so should <strong>the</strong> pressure(along with o<strong>the</strong>r parameters that can beoptimised similarly) to achieve <strong>the</strong> bestperformance.Brine Consumption, kj/kgOptimum Evaporator Pressure, kpa10080604020320 0600050004000300020001000320 0310310300Tamb, K300Tamb, KOptimum Brine Consumption Performance Plot <strong>of</strong> R245fa290290280280360360380380400400420Tgeo, KOptimum Evaporator Pressure Performance Plot <strong>of</strong> R245fa420Tgeo, KFigure 4: Performance plots for R245fa, optimum brineconsumption (top) and associated evaporator pressure(bottom)Haloalkanes as Working FluidsMany haloalkanes, especially <strong>the</strong>hydr<strong>of</strong>luorocarbons, such as ,1,1,3,3-,Pentafluoropropane (HFC-245fa) and 1,1,1,2-Tetrafluoroethane (HFC-134a), which is inwidespread use as a refrigerant, are inflammable,non-toxic and relatively inert. These propertiesmake <strong>the</strong>m highly attractive to use as workingfluids in binary power cycles.One <strong>of</strong> <strong>the</strong> drawbacks <strong>of</strong> <strong>the</strong>se fluids is <strong>the</strong>rmalstability, which, in most cases, is less than <strong>the</strong>non-halogenated hydrocarbon equivalent andmay limit <strong>the</strong> maximum temperature for which<strong>the</strong>y can be used in power cycles. This is an area<strong>of</strong> significant uncertainty for ORC technologybased on current generation fluids.Some <strong>of</strong> <strong>the</strong> decomposition products can not onlycause system performance to degrade but arealso toxic and/or strong acids that may negativelyimpact plant. While some degradation <strong>of</strong> <strong>the</strong>cycle fluid to a static level may be tolerable incertain situations, gross scale degradation overtime <strong>of</strong> <strong>the</strong> working fluid is not acceptable.While <strong>the</strong>re have been a number <strong>of</strong> studies(Angelino, 2003; Calderazzi, 1997) looking at <strong>the</strong>stability <strong>of</strong> <strong>the</strong>se fluids, existing data does notnecessarily agree on exact degradationtemperatures and have, in general, looked only at<strong>the</strong> stability when in contact with stainless steel,440440460460480480<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>which has negligible catalytic interaction.However, in real-world applications <strong>the</strong> workingfluid may come into contact with a number <strong>of</strong>different materials, all <strong>of</strong> which may interactdifferently with <strong>the</strong> working fluid and may fur<strong>the</strong>rreduce <strong>the</strong> reported degradation temperature.Fur<strong>the</strong>r effects, including atmosphericcontamination (e.g. <strong>the</strong> presence <strong>of</strong> smallamounts <strong>of</strong> water, which may acceleratedecomposition) have not been thoroughlyinvestigated to <strong>the</strong> best <strong>of</strong> our knowledge.This is <strong>of</strong> concern when designing a plant as <strong>the</strong>presence <strong>of</strong> materials that may act as catalysts fordegradation must be avoided in all parts <strong>of</strong> <strong>the</strong>system that come into contact with <strong>the</strong> workingfluid. Even common materials used in heatexchangers may be cause for concern.Optimising <strong>the</strong> Operating PressureNot only do certain fluids perform better thano<strong>the</strong>rs at certain temperatures, but <strong>the</strong>re exists anoptimum pressure for cycle performance.Net Power (kW)5004003002001000Power vs Pressure(150°C Resource)0 2000 4000 6000Pressure (kPa)HFC-134aHFC-245faFigure 5: Optimum cycle pressures at 150°Cfor HFC-134a and HFC-245fa.The general assumption that higher pressuredirectly translates to higher work output does notnecessarily hold true at pressures both below andabove <strong>the</strong> critical pressure, depending on <strong>the</strong> fluidin question. Figure 5 shows <strong>the</strong> calculated poweroutput over a range <strong>of</strong> pressures for HFC-134aand HFC-245fa at operating temperatures <strong>of</strong>150°C. As can be seen, at this temperature <strong>the</strong>optimum system pressure for <strong>the</strong>se two fluids isdifferent and produces significantly different netpower outputs.Optimising <strong>the</strong> TurbineWorking fluid properties, resource temperature,flow rate and condensing pressure are allvariables that dictate turbine design. In mostinstances, <strong>the</strong> goal is to generate <strong>the</strong> highestoutput power possible. Therefore designoptimisation centres around generating <strong>the</strong>highest efficiency turbine. Generally, this resultsin turbine designs that need to operate at highrotational speeds that are not suitable for direct424


coupling to grid synchronous generators. QGECEis focussing on optimising turbines that haveoperational speeds <strong>of</strong> 24,000 RPM (400 Hz). Thisresults in high operating efficiencies and iscompatible with existing power electronics, suchas that found in aircraft. To date, current QGECEpreliminary turbine design has not indicateddramatic differences in turbine efficiencies forvarious ORC cycles operating with pressure ratios<strong>of</strong> between 2 and 6.Optimising <strong>the</strong> CycleSo far we have touched on a number <strong>of</strong>considerations <strong>of</strong> various key cycle componentsincluding <strong>the</strong> working fluid, system operatingpressure and turbine design. When combined, adifferent picture may begin to emerge as to <strong>the</strong>composition <strong>of</strong> elements that yields optimumpower output for a given resource temperature.For instance, depending on <strong>the</strong> design conditionsassumed in <strong>the</strong> <strong>the</strong>rmodynamic cycle analysis,<strong>the</strong> pressure ratio calculated that gives anoptimum <strong>the</strong>oretical cycle performance may resultin a suboptimal turbine efficiency, which mayaffect <strong>the</strong> initial ranking <strong>of</strong> working fluid selection.Net Power (kW)5004003002001000Net Power vs Pump Efficiency0 0.2 0.4 0.6 0. 8Pump EfficiencyHFC-134aHFC-245faη pump = 0.65P = 1200 kPaFigure 6: Effect <strong>of</strong> ηpump on net power.Fur<strong>the</strong>rmore, variations in efficiencies <strong>of</strong> o<strong>the</strong>rcomponents in <strong>the</strong> system are <strong>of</strong>ten neglected in<strong>the</strong>oretical studies for ease <strong>of</strong> comparison, butcan have a large impact on overall systemperformance. For instance, <strong>the</strong> benefits <strong>of</strong> transandsupercritical cycles can be harnessed only ifhigh performance pumps or compressors exist for<strong>the</strong> required conditions, o<strong>the</strong>rwise a subcriticalcycle may become increasingly attractive due tolower pump work and reduced operatingpressures. Figure 6 shows <strong>the</strong> impact on netpower for a supercritical HFC-134a cycleoperating at 5 MPa compared to an optimisedsubcritical HFC-245fa cycle operating at 1.2 MPaat <strong>the</strong> same temperature.QGECE Mobile Test Plant (Terragen)The Terragen Project is a QGECE initiative todevelop a modular portable transcritical powerplant able to generate approx. 75 kW <strong>of</strong> powerfrom geo<strong>the</strong>rmal or waste heat sources. One <strong>of</strong><strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong><strong>the</strong> primary goals is to demonstrate that usefulamounts <strong>of</strong> energy can be produced even fromlow-grade resources using transcritical fluids.Terragen consists <strong>of</strong> three containerised modules:a control module, power-plant module and an aircondenser module. The system is beingdesigned around two working fluids HFC-134aand HFC-245fa using oil-free technologies.Terragen will be a real-world demonstration andvalidation <strong>of</strong> cycles and technologies beingdeveloped at QGECE and will primarily be anexperimental rig based at The University <strong>of</strong>Queensland’s rural Pinjarra campus. Theportable nature <strong>of</strong> Terragen means that it will alsobe available for companies to carry out welltestingand help prove <strong>the</strong> electricity-generationcapability <strong>of</strong> resources to assist with attractingpublic and private sector funding.Terragen is currently under development incollaboration with our project partner, Verdicorp,and is expected to be completed mid-late 2011.ConclusionsThe general assumption that higher pressuredirectly translates to higher work output does notnecessarily hold true at pressures both below andabove <strong>the</strong> critical pressure, depending on <strong>the</strong> fluidin question. Figure 5 above shows <strong>the</strong> calculatedpower output over a range <strong>of</strong> pressures for HFC-134a and HFC-245fa at operating temperatures <strong>of</strong>150°C.In developing an ORC that generates optimumcycle power output from a given resource <strong>the</strong>reare a number <strong>of</strong> critical considerations including,but not limited to, selection <strong>of</strong> best-suited fluid foroperating temperature; selecting optimisedoperating pressures for chosen fluid; optimisedturbine design and selection <strong>of</strong> auxiliary cyclecomponents that complement <strong>the</strong>se major cycleelements.Future work will work towards verifying <strong>the</strong>predicted performances experimentally both in <strong>the</strong>lab at small power scales and at larger scaleusing <strong>the</strong> QGECE Mobile Plant. Fur<strong>the</strong>rmore,future work will address <strong>the</strong> life cycle analysis <strong>of</strong>implementing various sub- and transcritical cyclesto verify that <strong>the</strong> cycles that give <strong>the</strong> bestperformance <strong>the</strong>oretically still out-perform <strong>the</strong>o<strong>the</strong>r cycles on an economic and feasibility basis.ReferencesAngelino G, Invernizzi C, 2003, Int J. Refrig. 26(1)Calderazzi L, di Paliano PC, 1997, Int J. Refrig. 20(1).Villani M. Franco, A., 2009, “Optimal design <strong>of</strong> binary cyclepower plants for water-dominated, medium-temperaturegeo<strong>the</strong>rmal fields”. Geo<strong>the</strong>rmics, 38(4): 379 – 391Lemmon, E.W., H. M. M. M. NIST Standard ReferenceDatabase 23: Reference FluidThermodynamic and TransportProperties-REFPROP 2007425


Saleh, B., Koglbauer, G., Wendland, M., Fischer, J., “WorkingFluids For Low Temperature Organic Rankine Cycle” <strong>Energy</strong>,2007, 32, 1210–1221<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>426


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong><strong>Australian</strong> geo<strong>the</strong>rmal Industry working with Investors - Defining <strong>the</strong>key parameters contributing to <strong>the</strong> long run marginal cost <strong>of</strong>geo<strong>the</strong>rmal and providing a comparison benchmark on <strong>the</strong> keyunknownsJonathan Teubner*,* Business Development Manager, Petra<strong>the</strong>rm Ltd, 1/129 Greenhill Road Unley SA 5061,AbstractThe development <strong>of</strong> <strong>the</strong> <strong>Australian</strong> geo<strong>the</strong>rmalindustry is unique as, especially in <strong>the</strong> earlyexploratory phases, <strong>the</strong> industry is driven bycapital investment raised via equity markets. Thisequity is supported in some instances by grantsprovided by <strong>the</strong> Commonwealth Governmentthrough its Geo<strong>the</strong>rmal Drilling Program (GDP)and, in <strong>the</strong> case <strong>of</strong> <strong>the</strong> commercial demonstration<strong>of</strong> <strong>the</strong> technology, via <strong>the</strong> Renewable <strong>Energy</strong>Development program (REDP).The costs involved in <strong>the</strong> deep exploration phaseare significant, as are those involved in <strong>the</strong>commercial demonstration <strong>of</strong> <strong>the</strong> technology. It isunderstood by <strong>the</strong> industry that until it has beenable to prove <strong>the</strong> commercial reality <strong>of</strong> its projects,all funding is required to come from equitymarkets or government grants.<strong>Australian</strong> geo<strong>the</strong>rmal companies are <strong>the</strong>refore, inessence, competing for a limited pool <strong>of</strong> riskcapital from <strong>the</strong> equity markets and grant moniesfrom <strong>the</strong> Commonwealth government. This moneywill be provided to those projects and companieswhich are expected to deliver a commercialproject and this provide <strong>the</strong> best returns.A number <strong>of</strong> reviews by Equity brokerage firmshave been provided recently (Morgan Stanley,RBS Morgans and Goldman Sachs JB Were)reviewing <strong>the</strong> prospects <strong>of</strong> <strong>the</strong> industry andcommenting on each <strong>of</strong> <strong>the</strong> companies within <strong>the</strong>sector. It is not <strong>the</strong> purpose <strong>of</strong> this paper to reviewindividual companies’ prospects, however <strong>the</strong>sepapers have provided a summary <strong>of</strong> <strong>the</strong> keyparameters for company attractiveness: Experience <strong>of</strong> <strong>the</strong> board andmanagement; Presence <strong>of</strong> project partners, and <strong>the</strong>experience and size <strong>of</strong> such; Development options <strong>of</strong> <strong>the</strong> company(effectively <strong>the</strong> breadth <strong>of</strong> <strong>the</strong> projectjteubner@petra<strong>the</strong>rm.com.au4(x,t) x l* *u * portfolio to diversify risk);l Funding capability through access togovernment grants and large partners atei<strong>the</strong>r <strong>the</strong> project or equity level; Project quality assessed in respect <strong>of</strong>location, quality and riskThe ability to attract <strong>the</strong> capital (human as well asfinancial) to develop a project is ultimately afunction <strong>of</strong> <strong>the</strong> project quality. The project qualityin turn is a function <strong>of</strong> a number <strong>of</strong> competingfactors which will be discussed in more detailbelow, but is ultimately determined by <strong>the</strong>expected cost <strong>of</strong> production <strong>of</strong> geo<strong>the</strong>rmal energyarising from <strong>the</strong> project.<strong>Australian</strong> geo<strong>the</strong>rmal companies <strong>the</strong>refore arecompeting for limited capital allocations on <strong>the</strong>basis <strong>of</strong> <strong>the</strong>ir project’s forecast cost <strong>of</strong> production.This cost <strong>of</strong> production is typically evidenced by acalculated Levelized Cost <strong>of</strong> Electricity (LCoE) orLong Run Marginal Cost (LRMC).Recognizing <strong>the</strong> importance <strong>of</strong> this figure in <strong>the</strong>allocation <strong>of</strong> capital within <strong>the</strong> industry, <strong>the</strong><strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Energy</strong> Association(AGEA) formed an Economics Committee todevelop a framework for <strong>the</strong> reporting <strong>of</strong>Economic parameters to <strong>the</strong> public to ensureconsistency across releases.This paper represents that framework whichdefines <strong>the</strong> key parameters in <strong>the</strong> economicassessment <strong>of</strong> <strong>the</strong> project, and thus whichassumptions need to be released to support anyeconomic releases. Fur<strong>the</strong>r, it also provides datasets where available <strong>of</strong> what has been achievablein respect <strong>of</strong> <strong>the</strong>se assumptions elsewhere in <strong>the</strong>world to give interested parties an independentbenchmark <strong>of</strong> what has been previously achievedand prompting explanations from companies as towhere <strong>the</strong>ir assumptions sit on this frequencydistribution curve and why.The paper highlights <strong>the</strong> close cooperation thatexists between <strong>the</strong> investment community and <strong>the</strong>geo<strong>the</strong>rmal industry and is an example <strong>of</strong> how <strong>the</strong>informational needs <strong>of</strong> investors can be met by acooperative industry approach. It is an excellentguide to how companies can work with investorsin o<strong>the</strong>r emerging technology markets.u u uu 0426


COMMUNITY TRUSTEngagement & Communication<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>O. Boushel, *T.Hazou, C. Scott & Roger WindersSINCLAIR KNIGHT MERZ 590 Orrong Road, Armadale, 3143, VIC*Corresponding author: thazou@skm.com.auEffective community engagement from <strong>the</strong> start <strong>of</strong>any project is critical to gaining public support.The geo<strong>the</strong>rmal industry in Australia facesparticular challenges in consulting with <strong>the</strong>community because its technology is relativelyunknown. The challenge includes:1. a process <strong>of</strong> public education;2. a process <strong>of</strong> managing public perceptions<strong>of</strong> risk.Add to <strong>the</strong>se <strong>the</strong> range <strong>of</strong> views about climatechange and confusion around <strong>the</strong> role <strong>of</strong>renewable energy in general and <strong>the</strong> communityengagement task can seem daunting.Local community concern about geo<strong>the</strong>rmalprojects in <strong>the</strong>ir vicinity should <strong>the</strong>refore come asno surprise.Planning for community concern and taking anapproach that prioritises long-term relationshipbuilding with <strong>the</strong> community is critical tosuccessful project management. Thispresentation will provide a practical introduction tocommunity relations and consultationmanagement drawing on lessons both from <strong>the</strong>geo<strong>the</strong>rmal and <strong>the</strong> broader renewables sector.The presentation will provide a brief outline <strong>of</strong> <strong>the</strong>context <strong>of</strong> community consultation, a consultationframework, as well as some practical Do’s andDon’ts.Keywords:Stakeholder relations, community relations,consultation and engagement; outrage mitigation;action research; public relations, Strategiccommunications; risk; consultation tools andmethods; program evaluation.IntroductionStakeholder and community relations (SCR) is acomplex and demanding aspect <strong>of</strong> corporatemanagement and design and construct projectdelivery. SCR is now very much part <strong>of</strong> <strong>the</strong>industry and business landscape and is seen asan integral aspect to Corporate SocialResponsibility (CSR) and Public Relations (PR).In <strong>the</strong> coming pages, an introduction to PR, CSRand SCR and <strong>the</strong>ir differences will be provided,followed by an overview <strong>of</strong> communityconsultation practice. This will include anillustration <strong>of</strong> <strong>the</strong> distinct aspects <strong>of</strong> SCR and whatdifferentiates it from PR and reputationmanagement. This will be followed by anexplanation <strong>of</strong> community consultation principles,frameworks, and tools. Finally, an illustration <strong>of</strong>how SCR is used in a practical context will beprovided with an explanation <strong>of</strong> some ‘rules <strong>of</strong>engagement’ or practice Do’s and Don’ts. This willprovide an ability to identify <strong>the</strong> practices andskills required to perform in <strong>the</strong> field <strong>of</strong>stakeholder and community relations.Stakeholders and communitiesStakeholder and community relations (SCR) is afield <strong>of</strong> practice that demands expertise, andpr<strong>of</strong>essionalism. It has emerged from a range <strong>of</strong>industries and pr<strong>of</strong>essions and covers a widevariety <strong>of</strong> work practices and organisationalfunctions. Understanding this diversity andintersections will assist in grasping <strong>the</strong> competingexpectations <strong>of</strong> <strong>the</strong> field.Public relations (PR) can be defined as “<strong>the</strong>ethical and strategic management <strong>of</strong>communication and relationships in order to buildand develop coalitions and policy, identify andmanage issues and create and direct messagesto achieve sound outcomes within a sociallyresponsible framework” (Johnston & Zawawi,2004). Through this definition <strong>the</strong> PR pr<strong>of</strong>ession is<strong>of</strong>ten seen as ‘<strong>the</strong> custodian <strong>of</strong> reputationmanagement.’ As such PR <strong>of</strong>ten overlaps manyaspects <strong>of</strong> organisational management such asmarketing, media and crisis management,investor and community relations, internalcommunications, ethical conduct and strategicplanning.If PR generally (in all its forms) is aboutcommunicating a message and “staying onmessage” <strong>the</strong>n SCR is <strong>the</strong> ability to adapt andchange <strong>the</strong> message in order to prioritiserelationships. SCR is about ‘winning trust’ andunderstanding <strong>the</strong> community in a manner thatimpacts on actions and words for <strong>the</strong> long-term.SCR pr<strong>of</strong>essionals are ideally <strong>the</strong> first to identifyissues and challenges and must <strong>the</strong>n manage <strong>the</strong>discussion on behalf <strong>of</strong> <strong>the</strong> organisation (Moore,1996).Corporate Social Responsibility (CSR) has alsoemerged as an important corporate function inrecent years. CSR is recognition by corporationsand organisations that <strong>the</strong>y exist in a socialenvironment. It is a reflection <strong>of</strong> <strong>the</strong> ‘triple bottomline’ and <strong>the</strong> need for organisations to addresspublic concerns <strong>of</strong> ‘accountability andresponsibility’ (Regester, 2001). In fact, CSR has427


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>developed to <strong>the</strong> point where it is no longer “Dono harm” and it is “Do good beyond <strong>the</strong> narrowlimits <strong>of</strong> making pr<strong>of</strong>it” (Argenti and Forman,2002). With this has come a sophisticatedunderstanding <strong>of</strong> public communications on CSRmatters. Aside from issues <strong>of</strong> ethical conductcommunities have grown to understand that PR is<strong>the</strong> outward sign <strong>of</strong> an organisations inwardcharacter (Moore, 1996), resulting in a growingparadigm shift towards social responsibility.CSR has growing recognition by management <strong>of</strong>its importance and influence in creating positiveoutcomes for organisations and achieving longtermgoals. As a result <strong>of</strong> CSR expectationsgovernments, organisations, and companies arenow investing time and energy into SCR. TypicallySCR exists on two levels (Tymson and Lazar,2002). 1. The local level: to help an organisationcommunicate with local leaders, residents andorganisations to facilitate positive relations andgood outcomes. 2. The corporate level: toacknowledge an organisation as a citizen within awider social framework.As a result, SCR has developed as a distinct areafor four important reasons. First, it is concernedwith outcomes and impacts ra<strong>the</strong>r than image andmessage. That is it is concerned less with howsomething will look in <strong>the</strong> media and more withwhat will happen as a result (Fletcher, 1999).Second, SCR emphasises ‘outside-in’ thinkingand <strong>the</strong> ability to see an organisation from <strong>the</strong>outside point <strong>of</strong> view inwards (Regester, 2001).Third, SCR is crucially distinguished by “two-waycommunication”. Communication is an interactiveprocess between parties ra<strong>the</strong>r than a process <strong>of</strong>‘delivering on message’; it requires a dynamicability to listen, reflect and respond to concernsand desires (Forrest and Mayes, 1997). Finally,SCR is about developing and maintaining positivelong-term relationships (Forrest and Mayes,1997).Changing socio-political environmentCommunities are increasingly active andinformed. We live in a media environment whereinformation is more accessible than it has everbeen, and an increasing number <strong>of</strong> technologiesassist communities to network and (if necessary)mobilise against projects. Both new technologyand changes in legislation are creating moreopportunities for communities to engage in andinfluence individual project proposals.Globalisation described as a process by whichregional economies, societies, and cultures havebecome integrated and shrinking through a globalnetwork <strong>of</strong> communication, transportation, andtrade (Appadurai, 1996) has had an acute impacton community, government and corporateexpectations.Social media, mobile phones and <strong>the</strong> internetenables social networks to activate with a speedthat was unthinkable until recently. The expense<strong>of</strong> media access no longer impedes communityparticipation in <strong>the</strong> public sphere as new media iswidely accessible for minimal cost, and reachesbroad audiences. Evolution <strong>of</strong> Web 2.0 throughapplications that facilitate interactive sharing,inter-operability, user-centred design, andcollaboration on <strong>the</strong> World Wide Web is also key(Tim O'Reilly 2005. retrieved 2006-08-06).Traditional modes <strong>of</strong> PR communication usingstatic and mass communication channels arebecoming less relevant and proving less effectiveas people rely on alternative sources <strong>of</strong>information (represented below). One-waychannels <strong>of</strong> connecting with <strong>the</strong> target are “atypical monologue model with little if any openexchange <strong>of</strong> ideas, thoughts, or information. Theone-way arrows represent one way informationflows, as opposed to dialogue.” (Mark Parker.retrieved <strong>2010</strong>-09-04).Figure 1: http://smartselling.wordpress.com/tag/web-20/In this context, and <strong>the</strong> growth <strong>of</strong> <strong>the</strong> ‘informationage’ <strong>the</strong>re is a higher demand on corporations “tomanage <strong>the</strong> establishment and maintenance <strong>of</strong>credibility and trust” (Tymson and Lazar, 2002).Johnston and Zawawi (2004) also point out that areflexive and socially conscious management <strong>of</strong>communications within a socially aware andinformed environment is critical. People todaywant to and do know more about organisationsgenerally. “More people want to know more about<strong>the</strong> organisation <strong>the</strong>y are working for, <strong>the</strong>organisation <strong>the</strong>y are buying from, and <strong>the</strong>organisations <strong>the</strong>y are investing in” (Tymson andLazar, 2002).In recent years, community engagement hasbecome part <strong>of</strong> business as usual for capitalintensive projects and <strong>the</strong>ir proponents. Whilestakeholder engagement has always beenrequired to some extent, <strong>the</strong> geo<strong>the</strong>rmal industry(along with o<strong>the</strong>rs) is now being asked t<strong>of</strong>ormalise and improve its approach.428


Community expectationsThe increase in community activism andawareness has been facilitated by changes inlegislation that reflect <strong>the</strong> public’s desire to beinvolved in helping guide how <strong>the</strong>ir communitiesgrow and adapt to projects. Often projects nowhave federal, state and council triggers inplanning processes that require publicconsultation to be included in any planningprocess. Importantly <strong>the</strong>se triggers mean that <strong>the</strong>support <strong>of</strong> key stakeholders such as governmentfor a project, hinges on what benefit <strong>the</strong> projecthas for <strong>the</strong> wider public.At <strong>the</strong> most basic level <strong>the</strong>se new technologiesmay be restricted to email, blogs or basicwebsites. However, improvements incommunications technologies have allowed even<strong>the</strong> smallest groups to advocate for or express<strong>the</strong>ir concerns about projects in very polished,convincing campaigns using technologies such asinteractive websites such as, Facebook, YouTubeor Twitter.These technologies are not only being utilised by<strong>the</strong> public, but increasingly by developers andproject proponents to effectively engage a widerrange <strong>of</strong> people, improve <strong>the</strong> effectiveness <strong>of</strong>communication strategies and ga<strong>the</strong>r criticalinformation from <strong>the</strong> public that may affect <strong>the</strong>community. For example, VicRoads isundertaking a consultation process for its HoddleStreet Study by using an online tool called “Bang<strong>the</strong> Table” to ga<strong>the</strong>r feedback from <strong>the</strong> widercommunity about key considerations in <strong>the</strong>irplanning study such as existing operations, <strong>the</strong>role <strong>of</strong> public transport and bicycle access.The wider public is also becoming bettereducated, improving <strong>the</strong>ir ability and desire toengage in policy and planning processes inincreasingly sophisticated ways. Fur<strong>the</strong>r, <strong>the</strong>reare increasing expectations for companies tomeasure up to community expectations <strong>of</strong> socialresponsibility and to earn <strong>the</strong>ir ‘social license tooperate’. These expectations are <strong>of</strong>ten shared by<strong>the</strong> bodies responsible for approving projects.This can translate into unexpected and unforseendemands on companies to deliver in areas thatwere previously viewed as outside <strong>the</strong>ir area <strong>of</strong>responsibility. Relevant recent examples <strong>of</strong> thisinclude <strong>the</strong> $5 million Regional Benefits Programundertaken as part <strong>of</strong> <strong>the</strong> Sugarloaf PipelineProject (Melbourne Water. retrieved <strong>2010</strong>-09-02)or <strong>the</strong> AGL Hallett Wind Farm Community Fundwith total annual total grants $22,000 available forcommunities and communities in <strong>the</strong> Nor<strong>the</strong>rnAreas Council (NAC. retrieved <strong>2010</strong>-09-02).Government expectationsGovernments also expect an in-depth level <strong>of</strong>community consultation as part <strong>of</strong> corporate andindustry performance.<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Directions to proponents for <strong>the</strong> preparation <strong>of</strong>development approvals <strong>of</strong>ten include specificelements relating ei<strong>the</strong>r to community consultationand/or social impact assessment.Local government in particular is establishingconsultation requirements as part <strong>of</strong> approvalsprocesses above and beyond regular publicexhibitions and notices.Funding and tender requirements now emphasisecommunity consultation obligations forcingindustry to respond to contractual and approvalsrequirements.Industry expectationsThere is a growing awareness by industry thateffective community engagement ra<strong>the</strong>r thanbeing a regulatory burden, provides opportunitiesto improve project delivery through <strong>the</strong> earlyidentification <strong>of</strong> issues, contribute to socialwellbeing, and to deliver on CSR andsustainability agendas.Corporations (venture partners, banks andfinanciers) now have high expectations thatcompanies will manage community relations in aproactive and responsible manner.For <strong>the</strong>se reasons, community expectations <strong>of</strong>companies to deliver open and accountableconsultation processes are now, as great as <strong>the</strong>yhave ever been. Community engagementstrategies for geo<strong>the</strong>rmal projects mustacknowledge and navigate through thisenvironment.Effective engagementGeo<strong>the</strong>rmal energy, like many renewable energysources, is a relatively new industry in someregions. In <strong>the</strong>se cases communities are unlikelyto have an understanding <strong>of</strong> what potentialdevelopment projects involve. As a result, anycommunity engagement will also need to play aneducative role with <strong>the</strong> public, shaping communityperceptions <strong>of</strong> <strong>the</strong> industry.Consultation methodologyA number <strong>of</strong> effective consultation methodologiesare available to guide public engagement. Thetwo major approaches utilised in Australia are <strong>the</strong>Organisation for Economic Co-operation andDevelopment (OECD) model and InternationalAssociation <strong>of</strong> Public Participation (IAP2)spectrum <strong>of</strong> engagement.The OECD model provides three differentapproaches to consultation depending on <strong>the</strong>context in which it occurs:• Notification• Consultation• Participation429


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Notification in itself is not consultation as it is aone way process in which <strong>the</strong> organisationinforms <strong>the</strong> public. This is <strong>of</strong>ten <strong>the</strong> first step inconsultation where people are notified about <strong>the</strong>project;Consultation involves <strong>the</strong> two-way flow <strong>of</strong>information between <strong>the</strong> project and <strong>the</strong> widercommunity. This process may be used to allowgroups to voice <strong>the</strong>ir concerns about <strong>the</strong> project,ask questions or provide feedback.Participation involves <strong>the</strong> public in <strong>the</strong> decisionmaking process.The IAP2 spectrum, which shares a lot incommon with <strong>the</strong> OECD model, is fast becomingaccepted as a baseline by a range <strong>of</strong>stakeholders in Australia and internationally.The IAP2 spectrum has five engagementapproaches:1. Inform2. Consult3. Involve4. Collaborate5. EmpowerEach type <strong>of</strong> engagement is tailored to desiredengagement goals as shown in <strong>the</strong> table below.ApproachInformConsultInvolveCollaborateEmpowerGoalProvide <strong>the</strong> public with informationabout a project, plan or actionObtain feedback from <strong>the</strong> publicabout a project, plan or actionContinually obtain feedback andconsideration from <strong>the</strong> public atseveral stages throughout <strong>the</strong>projectWork with <strong>the</strong> public on <strong>the</strong> project,involving <strong>the</strong>m in <strong>the</strong> planning anddecision makingProviding <strong>the</strong> public with decisionmaking power on a project.accommodate differences in <strong>the</strong> public and <strong>the</strong>socio-political environment.Importantly, where a community engagementprogram has worked well for a project, it is criticalto review and reassess before reapplying it.Different communities, environments andtechnologies will require a different approach.Planned and structured approaches to communityconsultation not only produce <strong>the</strong> best results butalso leave a lasting impression and communityconfidence in corporate processes.Action researchA good practical approach to evaluating SCRmethods and tools is to adopt an Action ResearchMethodology (ARM). Action research is simply aform <strong>of</strong> self-reflective enquiry undertaken byparticipants in social situations in order to improve<strong>the</strong> rationality and basis <strong>of</strong> <strong>the</strong>ir own practices,<strong>the</strong>ir understanding <strong>of</strong> <strong>the</strong>se practices and <strong>the</strong>situations in which <strong>the</strong> practices are carried out.(Carr & Kemmis, 1986).Action Research does not set out to answer ahypo<strong>the</strong>sis or find a single ‘objective truth’. Itfocuses on a development process that engagesindividuals and enables change and improvedperformance.Action research can be done through a range <strong>of</strong>‘typical’ survey and interview research methods. Acrucial aspect is that each method should inform acircular model <strong>of</strong> inquiry. This allows for <strong>the</strong>building <strong>of</strong> improvements into practice. To do thisit involves participants in a collaborative approachto investigation in order to resolve specificproblems or create systematic (change) actions(Stringer, 1999).The action research cycle, involves four keysteps; planning, action, observation, reflection:Figure 2: IAP2 Approaches and Engagement GoalsThese approaches are not mutually exclusive.Often, several different approaches are used withdiffering aspects <strong>of</strong> a project. For example, aproponent may inform <strong>the</strong> public about a project,consult landholders about land access, involvelocal government in traffic management plansduring construction, and empower landholders in<strong>the</strong> reinstatement process.In <strong>the</strong> context <strong>of</strong> a single project, <strong>the</strong> project teamneeds to continually assess <strong>the</strong> tools andapproaches used for <strong>the</strong>ir efficacy with <strong>the</strong> public.Where appropriate, tools should be adapted toFigure 3: http://cadres.pepperdine.edu/ccar/define.htmlAction research is particularly well suited to SCRas its intent is not only to ‘get <strong>the</strong> job done’ but t<strong>of</strong>acilitate improvements. It does this by taking an‘organisational change’ approach based onparticipation and involvement.430


Consultation toolsThere are a number <strong>of</strong> tools available for use toengage <strong>the</strong> community. As shown in <strong>the</strong> IAP2spectrum below, <strong>the</strong>se can be grouped accordingto <strong>the</strong> engagement approach used. Typicalexamples include:• Information sheets / community bulletins• Web sites, blogs and email• Community Information sessions• Focus groups, surveys• Public meetings and public comment• Workshops and advisory committees• Community reference groups• Citizen juries and community ballots<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>decided to not undertaken any engagement or touse an inform approach to let any adjoininglandholders know. As such, a letter to localhouseholds about <strong>the</strong> project may be all that isrequired.However, a greenfield development that will occurin close proximity to adjoining properties mayrequire a different approach. The possibility <strong>of</strong>community concerns about issues such asproperty acquisition, noise, vibration and amenityissues may mean that failure to consult <strong>the</strong> publicmay result in community outrage, confusion andmisinformation. To avoid this, a consultingapproach may be deemed most appropriate withadjoining landholders. This may involve in personmeetings, a public information session or o<strong>the</strong>rtools that are appropriate in this context.Advantages/DisadvantagesDifferent engagement approaches create differentlevels <strong>of</strong> expectations within <strong>the</strong> public. Theseengagement approaches carry implicitundertakings. These are described as follows:Figure 4: http://iap2.org.auThese tools need to be selected on <strong>the</strong> basis <strong>of</strong><strong>the</strong> engagement goals <strong>of</strong> <strong>the</strong> project. Engagementgoals should be determined by a number <strong>of</strong>factors, most importantly <strong>the</strong> possible risks to <strong>the</strong>project, <strong>the</strong> organisation and its reputation.While risks are best determined in terms <strong>of</strong>specific issues relative to a project, <strong>the</strong>y are <strong>of</strong>tena product <strong>of</strong> a number <strong>of</strong> factors, as follows:• The number and type <strong>of</strong> stakeholders• The characteristics <strong>of</strong> <strong>the</strong> community• Potential issues associated with <strong>the</strong> project(perceived or real)• The potential benefits <strong>of</strong> <strong>the</strong> project for <strong>the</strong>community (perceived or real)• Stage <strong>of</strong> <strong>the</strong> projectFor example, undertaking a number <strong>of</strong> upgradesto an existing plant that may have short termconstruction noise impacts in a sparselypopulated during <strong>the</strong> day may be determined tobe a low risk activity from a communityconsultation perspective. Therefore it may beGoalInformConsultInvolveCollaborateEmpowerFigure 5: Source: http://iap2.org.auUndertakingWe will keep you informed.We will keep you informed,listen to and acknowledgeconcerns and provide feedbackon how public input influenced<strong>the</strong> decision.We will work with you to ensurethat your concerns andaspirations are directly reflectedin <strong>the</strong> alternatives developedand provide feedback on howpublic input influenced <strong>the</strong>decision.We will look to you for directadvice and innovation informulating solutions andincorporate your advice andrecommendations into <strong>the</strong>decisions to <strong>the</strong> maximumextent possible.We will implement what youdecide.The tools used <strong>of</strong>ten vary according to <strong>the</strong>engagement goals. Using <strong>the</strong> right tools allows fortargeted community engagement that is costeffective, timely and addresses risks posed bypotential public outrage.Each approach has a number <strong>of</strong> advantages anddisadvantages when <strong>the</strong>y are used with differentcommunities or in a particular context.Consideration <strong>of</strong> <strong>the</strong>se aspects when determiningwhich tools to use is a worthwhile exercise. This431


should not deter taking a certain approach, butra<strong>the</strong>r allow strategic consideration and planningfor some <strong>of</strong> <strong>the</strong> challenges that may face aparticular project.The following table contrasts <strong>the</strong> advantages anddisadvantages <strong>of</strong> each public participation goaland will help in evaluating program planning anddecisions.Goal Advantage Disadvantage• Inexpensive• Limited• Allows control <strong>of</strong> information caninformationbe meaningfully• Widecommunicateddissemination <strong>of</strong> • Communityinformationconcerns can beignored• Allows for• Can be difficult tocommunitymanage publicfeedbackexpectations• Inexpensive• Superficial issues• can reach large can be raisednumbers <strong>of</strong>• Potential forpeoplesmall vocal• Improvedgroups todecision making dominate publicconsultationInformConsultInvolveCollaborateEmpower• Provides greaterinsight into publicissues andperspectives andhow <strong>the</strong>se wereformed• Createscommunityownership <strong>of</strong> <strong>the</strong>project• Createscommunityownership <strong>of</strong> <strong>the</strong>project• Increase publictrust in <strong>the</strong>organisation• Can fosterinnovative localsolutions• Well suited tosmaller issues• Createsownership in <strong>the</strong>community over<strong>the</strong> project• Can increasecommunitysupport <strong>of</strong> aproject• can increasepublic trust in <strong>the</strong>organisation• Can createinnovative localsolutions• Well suited tosmall localisedissues• Can be resourceintensive• Smaller crosssection <strong>of</strong> <strong>the</strong>public engaged• Can lead to directconflict with <strong>the</strong>community aboutproject goals• Can be resourceintensive• Smaller crosssection <strong>of</strong> <strong>the</strong>public engaged• Public decisionsnot alwaysfeasible, leadingto conflictbetweenproponents and<strong>the</strong> community• Can be resourceintensive• Smaller crosssection <strong>of</strong> <strong>the</strong>public engaged• Public decisionsnot alwaysfeasible, leadingto conflictbetweenproponents and<strong>the</strong> community• Not suited totechnicalsolutionsFigure 6: Advantages and Disadvantage <strong>of</strong> IAP2 Goals<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Do’s and Don’tsWhile each consultation program must be tailormadeto particular project circumstances, it ispossible to draw out a number <strong>of</strong> ‘consultationdo’s and don’ts’ from past experiences; including:Trust and transparency• Following through on what is promised. If youcan’t commit to a date, action or event, <strong>the</strong>ndon’t promise you will.• It’s never enough to say ‘trust me’ to <strong>the</strong>public, be prepared with evidence to supportany claims made.• Inform <strong>the</strong> community where and to whatextent <strong>the</strong>y can influence a decision andwhere <strong>the</strong>y cannot.Timeliness and planning• Provide <strong>the</strong> opportunity for <strong>the</strong> public toparticipate as fully as possible within <strong>the</strong>timeframe established• Ensure that Community engagement is anintegral part <strong>of</strong> <strong>the</strong> project planning processNew technology• Don’t be afraid to use new technologies,particularly where <strong>the</strong>y can help you engage• Don’t assume that everyone has access to oris comfortable with <strong>the</strong> internetIntegrated design processes• Community engagement needs to beintegrated into <strong>the</strong> design process. Involvingit at this stage allows for <strong>the</strong> identification <strong>of</strong>likely issues early in <strong>the</strong> process where <strong>the</strong>ycan be addressed in a cost effective manner.Failure to do this can result in costly revisionsand risks <strong>of</strong> project delays during <strong>the</strong>construction stage.Evaluating Choices• Don’t be afraid to ask for help from within <strong>the</strong>industry or outside <strong>of</strong> it. If you’re not sure youare better <strong>of</strong>f getting some specialist advice.• Do take a systematic approach toconsidering tools, methods and consultationapproaches.Respect and Recognition• Do acknowledge that local communities havean interest in your project and will want a sayand input.• Don’t treat communities as ‘stupid’ or unableto grasp technology; if you do <strong>the</strong>y may goelsewhere and get <strong>the</strong> ‘wrong’ information.• Do try to simplify things and use common‘spoken’ language to explain difficultconcepts or technology.• Do involve <strong>the</strong> community early and establisha ‘bank <strong>of</strong> goodwill’ that you can draw on ifsomething goes wrong or a future presentsitself.432


SummaryAs a fledgling industry in Australia, geo<strong>the</strong>rmalenergy developers have an opportunity to ‘standon <strong>the</strong> shoulders <strong>of</strong> o<strong>the</strong>rs’, drawing on lessonslearnt by o<strong>the</strong>r industries and sharing experiencesfrom within <strong>the</strong> geo<strong>the</strong>rmal sector. Thispresentation aims to pool that knowledge and linkit to <strong>the</strong> engagement challenges faced by <strong>the</strong>industry today.Stakeholder and community relations is clearlyabout communicating ‘early and <strong>of</strong>ten’establishing associations, mutual worth andinvestment in publics (Forrest and Mayes, 1997).Investing in a long-term relationship to understandcommunity views, predict issues, reflect concerns,communicate on target, and maintain credibilitycan only be done with pro-active andcomprehensive relations (Ledingham andBruning, 2000). If SCR is about establishingcredibility and trust <strong>the</strong>n maintaining positiveenduring relationships becomes <strong>the</strong> cornerstone<strong>of</strong> SCR practice.This puts <strong>the</strong> industry in a unique position.Geo<strong>the</strong>rmal power doesn’t have a legacy <strong>of</strong>negative community perceptions based on noise,amenity or o<strong>the</strong>r factors and has <strong>the</strong> opportunityto create an enduring positive image madepossible by clear communication and a ‘mature’,and sensible approach to communityengagement.ReferencesAppadurai, A. (1996) Modernity at Large: culturaldimensions <strong>of</strong> globalization. Minneapolis:University <strong>of</strong> Minnesota Press.Argenti, P and J Forman (2002) The Power <strong>of</strong>Corporate Communication, crafting <strong>the</strong> voiceand image <strong>of</strong> your business, Boston:McGraw-Hill Pty. Ltd.Brackertz, N., Zwart, Meredyth, D. and LissRalston (2005) Community Consultation andhard to reach concepts and practice inVictoria local government. Hawthorn: Institutefor Social Research, Swinburne University <strong>of</strong>Technology.Riel, M. (<strong>2010</strong>) Center for Collaborative ActionResearchhttp://cadres.pepperdine.edu/ccar/define.html(CFCAR. retrieved <strong>2010</strong>-08-04).Fletcher, M (1999) Managing Communication inLocal Government, London: Kogan Page Ltd.Forrest, C and R Mayes, (1997) The PracticalGuide to Environmental CommunityRelations, New York, John Wiley and SonsInc.<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Globalization. (<strong>2010</strong>)http://en.wikipedia.org/wiki/Globalisation(Wikipedia. retrieved <strong>2010</strong>-09-17).Johnston, J and C Zawawi (2004) PublicRelations: Theory and Practice, 2nd Edition,NSW: Allen and Unwin.Ledingham and Bruning, (2000) Public Relationsas Relationship Management, Mahwah, NJ:Lawrence Erlbaum Associates Inc.Melbourne Water Sugarloaf Pipeline Alliance(2008)http://www.sugarloafpipeline.com.au/content/about_<strong>the</strong>_project/regional_benefits.asp(Melbourne Water. retrieved <strong>2010</strong>-09-02)Moore, S (1996) An Invitation to Public Relations,London: Cassell Pty. Ltd.Nor<strong>the</strong>rn Areas Council and AGL (<strong>2010</strong>)http://www.nacouncil.sa.gov.au/webdata/resources/files/AGL_HWF_Community_Fund_Application_NAC_10.pdf (NAC. retrieved <strong>2010</strong>-09-02).Parker, M. (<strong>2010</strong>)http://smartselling.wordpress.com/tag/web-20/(Mark Parker. Retrieved <strong>2010</strong>-09-04).Regester, M. Managing Corporate ReputationThrough Crisis in Jolly, A (Ed), (2001)Managing Corporate Reputations, London:Kogan Page Ltd.Sandman, P. (1993) Responding to communityoutrage: strategies for effective risk. AmericanIndustrial Hygiene Association, Fairfax.Stringer, T. (1999) Action Research 2nd Ed.Thousand Oaks: SAGE Publications Inc.Tymson, C, Lazar, P and R Lazar (2002) TheNew <strong>Australian</strong> and New Zealand PublicRelations Manual, Chatswood: TymsonCommunications.O'Reilly, T. (2005) "What Is Web 2.0". O'ReillyNetwork.http://www.oreillynet.com/pub/a/oreilly/tim/news/2005/09/30/what-is-web-20.html.Retrieved 2006-09-17433


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Geo<strong>the</strong>rmal energy legislation developments in QueenslandMelissa Zillmann* and Myria Makras<strong>Energy</strong> Industry Policy Division, Department <strong>of</strong> Employment, Economic Development and Innovation, 61 Mary Street,Brisbane Qld 4000Corresponding author: melissa.zillmann@deedi.qld.gov.auThe Geo<strong>the</strong>rmal <strong>Energy</strong> Act <strong>2010</strong> (<strong>the</strong> Act) waspassed by <strong>the</strong> Queensland Parliament in August<strong>2010</strong>. The Act has been primarily established toprovide a regulatory framework for <strong>the</strong> production<strong>of</strong> geo<strong>the</strong>rmal energy.On commencement, <strong>the</strong> Act will repeal <strong>the</strong> currentGeo<strong>the</strong>rmal Exploration Act 2004 (<strong>the</strong> ExplorationAct) which solely regulates geo<strong>the</strong>rmalexploration. The new Act largely duplicates <strong>the</strong>current exploration legislation, howeverexperience and feedback gained from operation<strong>of</strong> <strong>the</strong> Exploration Act has led to some beneficialchanges to <strong>the</strong> exploration regime.Importantly <strong>the</strong> Act introduces a regulatory regimefor geo<strong>the</strong>rmal production which will enablegeo<strong>the</strong>rmal exploration permit holders to progressto a production tenure when a suitable geo<strong>the</strong>rmalresource has been identified.This paper outlines <strong>the</strong> key changes to <strong>the</strong>exploration regime and <strong>the</strong> framework forgeo<strong>the</strong>rmal production included in <strong>the</strong> Act.Keywords: Queensland, geo<strong>the</strong>rmal energylegislation, geo<strong>the</strong>rmal production, productionthreshold, geo<strong>the</strong>rmal exploration, Geo<strong>the</strong>rmal<strong>Energy</strong> Act <strong>2010</strong>, Geo<strong>the</strong>rmal Exploration Act2004.Geo<strong>the</strong>rmal <strong>Energy</strong> Act <strong>2010</strong>The Queensland Government recognises <strong>the</strong>importance <strong>of</strong> geo<strong>the</strong>rmal energy as a valuableenergy resource that has <strong>the</strong> potential tocontribute significantly towards reducing <strong>the</strong>State’s carbon footprint. The QueenslandRenewable <strong>Energy</strong> Plan launched in June 2009outlined a roadmap for <strong>the</strong> expansion <strong>of</strong> <strong>the</strong>renewable energy sector in Queensland. The Planforecasts 250 megawatts <strong>of</strong> generation capacitybased on geo<strong>the</strong>rmal energy in Queensland’sgeneration capacity mix by 2020. Development <strong>of</strong>this Act is a key milestone that will supportdevelopment <strong>of</strong> <strong>the</strong> geo<strong>the</strong>rmal industry inQueensland and enable this forecast to be met.The objectives <strong>of</strong> <strong>the</strong> Act are to encourage andfacilitate <strong>the</strong> safe exploration for, and production<strong>of</strong>, geo<strong>the</strong>rmal energy. This will be achieved byproviding for <strong>the</strong> grant <strong>of</strong> geo<strong>the</strong>rmal explorationpermits to explore for sources <strong>of</strong> geo<strong>the</strong>rmalenergy across <strong>the</strong> State and for <strong>the</strong> grant <strong>of</strong>geo<strong>the</strong>rmal production leases for large-scalegeo<strong>the</strong>rmal production.Where possible, <strong>the</strong> Act aims to ensure maximumconsistency with Queensland’s existing resourcebasedlegislation and geo<strong>the</strong>rmal legislation <strong>of</strong>o<strong>the</strong>r jurisdictions.Changes to geo<strong>the</strong>rmal energyexploration in QueenslandLand available for geo<strong>the</strong>rmal explorationUnder <strong>the</strong> current Exploration Act, an explorationpermit can only be obtained when <strong>the</strong> State hasfacilitated a land release for competitive tender.This means <strong>the</strong> timing <strong>of</strong> exploration, and <strong>the</strong> landmade available, is at <strong>the</strong> discretion <strong>of</strong> <strong>the</strong> State.Under <strong>the</strong> new Act, applications for explorationpermits will be available via two processes.Firstly, <strong>the</strong> tender process provided in <strong>the</strong>Exploration Act has been modified and is referredto as a ‘released area’ process. This will providean ‘application period’ where applications may bemade. Any applications within this period will beconsidered competitively after <strong>the</strong> period ends.Secondly, a new process which enables eligiblepersons to apply for exploration permits over land<strong>of</strong> <strong>the</strong>ir choice and at a time appropriate to <strong>the</strong>m isintroduced by <strong>the</strong> Act. This process is referred toas an ‘over <strong>the</strong> counter application’. Theintroduction <strong>of</strong> this new application process willprovide greater flexibility in gaining access to landfor geo<strong>the</strong>rmal exploration activities and supportincreased geo<strong>the</strong>rmal exploration in Queensland.In addition to making more land available forexploration, <strong>the</strong> exploration regime under <strong>the</strong> newAct increases <strong>the</strong> maximum area that can beapplied for under an exploration permit. The areawill be increased from 200 sub blocks (600 km 2 )to 50 blocks (3,750 km 2 ) which brings <strong>the</strong>exploration permit area into line with o<strong>the</strong>r Statesand increases <strong>the</strong> chances <strong>of</strong> identifying acommercially viable geo<strong>the</strong>rmal energy resource.The term <strong>of</strong> an exploration tenure has also beenincreased under <strong>the</strong> Act from 12 to 15 years.Exploration ExemptionTo encourage use <strong>of</strong> geo<strong>the</strong>rmal energy for <strong>the</strong>purposes <strong>of</strong> geo<strong>the</strong>rmal heat pumps for heatingand cooling buildings, <strong>the</strong> Act does not regulateexploration for <strong>the</strong>se purposes. Exploration <strong>of</strong> thisnature will generally depend on shalloweroperations within <strong>the</strong> relevant property boundary,which will not have <strong>the</strong> same impact on <strong>the</strong>environment and landholders as o<strong>the</strong>r explorationactivities.434


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Retention StatusIt is recognised that <strong>the</strong>re may be delays between<strong>the</strong> discovery <strong>of</strong> a geo<strong>the</strong>rmal resource and itscommercialisation. These delays could be relatedto factors such as investment attraction,development <strong>of</strong> infrastructure or securing supplycontracts.To address <strong>the</strong>se issues, <strong>the</strong> Act introduces aretention status by way <strong>of</strong> a ‘Potential Geo<strong>the</strong>rmalCommercial Area’. This is similar to <strong>the</strong> retentionstatus provided for under <strong>the</strong> Petroleum and Gas(Production and Safety) Act 2004. The ‘PotentialGeo<strong>the</strong>rmal Commercial Area’ can be granted forup to 5 years but it can not extend beyond <strong>the</strong>maximum term allowed for in <strong>the</strong> underlyingexploration permit.The grant <strong>of</strong> a ‘Potential Geo<strong>the</strong>rmal CommercialArea’ may provide an exemption fromrelinquishment provisions and may enablesuspension <strong>of</strong> <strong>the</strong> exploration permit’s workprogram where appropriate. However, anevaluation program will be required to ensure that<strong>the</strong> exploration permit continues to be activelydeveloped and brought to production.Production TestingThe Act provides clarity that restricted productiontesting can be carried out under an explorationpermit to determine whe<strong>the</strong>r a geo<strong>the</strong>rmalresource is suitable for commercial development.The commercial grade <strong>of</strong> <strong>the</strong> geo<strong>the</strong>rmal energyresource will need to be quantified before anapplication for a production lease can be made.Before testing can commence, a test plan must beprovided and any relevant authorities will need tobe obtained.Transitional provisions for ExplorationAct permit holdersThe Act provides existing exploration permitholders a period <strong>of</strong> 12 months to transition to <strong>the</strong>new geo<strong>the</strong>rmal energy framework after <strong>the</strong>commencement <strong>of</strong> <strong>the</strong> Act. Whilst <strong>the</strong> Actcontains extensive provisions that automaticallytransfer tenures, decisions and processes to <strong>the</strong>Act, current exploration permit holders will need tocomply with <strong>the</strong> requirement to obtain anenvironmental authority. A period <strong>of</strong> 12 monthsfrom commencement <strong>of</strong> <strong>the</strong> Act has been deemeda sufficient timeframe to comply with thisrequirement.Geo<strong>the</strong>rmal production regimeThe primary purpose <strong>of</strong> <strong>the</strong> Act is to introduce aframework for geo<strong>the</strong>rmal production. Theprincipal means for allocating geo<strong>the</strong>rmalresources for production are via a productionlease.Under <strong>the</strong> Act, a production lease can only beapplied for on <strong>the</strong> basis <strong>of</strong> an existing explorationpermit. A person who is not an exploration permitholder can only apply for a production lease if it isdone jointly with an exploration permit holder orwith <strong>the</strong> consent <strong>of</strong> <strong>the</strong> exploration permit holder.These provisions give priority production rights toexploration permit holders provided <strong>the</strong>y complywith <strong>the</strong> requirements <strong>of</strong> <strong>the</strong> Act.Scope <strong>of</strong> <strong>the</strong> Act (for production)The proposed geo<strong>the</strong>rmal energy regime providesfor a sliding scale <strong>of</strong> regulation <strong>of</strong> geo<strong>the</strong>rmalenergy production under several QueenslandActs, according to <strong>the</strong> scale <strong>of</strong> production.Activities that are small or medium scaleproduction will not be regulated by <strong>the</strong> Act.Fur<strong>the</strong>rmore, <strong>the</strong> Act is not intended to regulateany associated use <strong>of</strong> <strong>the</strong> geo<strong>the</strong>rmal energyproduced, such as in power stations or industrialactivities. To minimise regulatory duplication, <strong>the</strong>use <strong>of</strong> geo<strong>the</strong>rmal energy will be regulated whenit triggers existing legislation such as <strong>the</strong>Electricity Act 1994 and <strong>the</strong> Sustainable PlanningAct 2009. For example, a production lease holdermay be granted rights to extract geo<strong>the</strong>rmalenergy which may be used to produce electricity,but approvals to supply electricity must beobtained under <strong>the</strong> Electricity Act 1994 and <strong>the</strong>building <strong>of</strong> any necessary infrastructure must beauthorised under <strong>the</strong> Sustainable Planning Act2009.Small to medium scale production thresholdThe use <strong>of</strong> heat pumps (considered as smallscale production) will be encouraged under thisframework since <strong>the</strong>ir use is not regulated by <strong>the</strong>Act and its requirements to obtain a productionlease and provide development plans.Under <strong>the</strong> Plumbing and Drainage Act 2002,installation <strong>of</strong> pipes for <strong>the</strong> purpose <strong>of</strong> conveyingwater within premises may only be undertaken bya licensed plumber. It is proposed to amend <strong>the</strong>Plumbing and Drainage Regulation 2003 to allow<strong>the</strong> Queensland Plumbing and Wastewater Codeto provide a framework for <strong>the</strong> regulation <strong>of</strong> <strong>the</strong>installation <strong>of</strong> geo<strong>the</strong>rmal heat pumpsGeo<strong>the</strong>rmal energy production below <strong>the</strong> largescale production threshold that is not via heatpump technology is considered to be mediumscale production and it will not be regulated by <strong>the</strong>Act. Instead it will be regulated if <strong>the</strong> geo<strong>the</strong>rmalenergy use triggers requirements under existinglegislation such as <strong>the</strong>:ooSustainable Planning Act 2009 (materialchange <strong>of</strong> use provisions)Water Act 2000 (taking or interfering withwater provisions)o Environmental Protection Act 1994(environmentally relevant activitiesprovisions)435


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>Large scale production thresholdThe Act only regulates <strong>the</strong> large-scale production<strong>of</strong> geo<strong>the</strong>rmal energy. The Act provides that <strong>the</strong>threshold for large scale production will beprescribed in <strong>the</strong> supporting geo<strong>the</strong>rmalregulation.Currently a power threshold which is nottechnology-specific and is flexible enough to applyto a variety <strong>of</strong> geo<strong>the</strong>rmal production applicationsis being considered to define <strong>the</strong> large-scaleproduction threshold. A power threshold providesa direct measure <strong>of</strong> <strong>the</strong> rate <strong>of</strong> production <strong>of</strong> <strong>the</strong>geo<strong>the</strong>rmal resource that does not depend onhow <strong>the</strong> resource is being utilised, thus avoiding<strong>the</strong> need to consider conversion efficiency.A primary policy consideration for setting <strong>the</strong>threshold is that it should be set at a level lowenough to enable commercial geo<strong>the</strong>rmalproduction activities <strong>of</strong> potential importance to bemonitored by <strong>the</strong> Government. However, thisneeds to be balanced so that <strong>the</strong> threshold is sethigh enough to ensure that <strong>the</strong> uptake <strong>of</strong>smaller-scale geo<strong>the</strong>rmal activities which may<strong>of</strong>fset carbon emissions are not unnecessarilycaptured or stifled by a requirement to have aproduction lease. Fur<strong>the</strong>r consultation will beundertaken during preparation <strong>of</strong> <strong>the</strong> supportingregulation about how <strong>the</strong> large-scale productionthreshold will be defined.Geo<strong>the</strong>rmal production leasesA geo<strong>the</strong>rmal production lease must be appliedfor if <strong>the</strong> proposed activities will trigger <strong>the</strong>threshold for large sale production. Geo<strong>the</strong>rmalenergy production is defined in <strong>the</strong> Act as <strong>the</strong>recovery <strong>of</strong> geo<strong>the</strong>rmal energy from beneath oron <strong>the</strong> surface <strong>of</strong> <strong>the</strong> land in which it is contained.The area required for geo<strong>the</strong>rmal production isnot as large as <strong>the</strong> area required for geo<strong>the</strong>rmalexploration. Hence <strong>the</strong> Act allows for a maximumproduction lease area <strong>of</strong> 25 blocks (1, 875km 2 ).A production lease applicant must prepare adevelopment plan setting out how <strong>the</strong> geo<strong>the</strong>rmalenergy resource will be developed, and <strong>the</strong>proposed rate <strong>of</strong> energy production. The grant <strong>of</strong>a production lease requires <strong>the</strong> holder tocommence commercial production within 2 years<strong>of</strong> its grant. To allow <strong>the</strong> ongoing monitoring <strong>of</strong>resource development, <strong>the</strong> holder will be requiredto submit fur<strong>the</strong>r development plans during <strong>the</strong>term <strong>of</strong> <strong>the</strong> lease.A geo<strong>the</strong>rmal production lease has an initialmaximum term <strong>of</strong> 30 years. Subsequent renewals<strong>of</strong> <strong>the</strong> lease are limited to a maximum <strong>of</strong> 20 years,with no limit on <strong>the</strong> number <strong>of</strong> renewals that canbe made.Sub-lease <strong>of</strong> geo<strong>the</strong>rmal production leaseA holder <strong>of</strong> a geo<strong>the</strong>rmal production lease maysublease an area <strong>of</strong> <strong>the</strong> lease to a third party. Thesublease is subject to approval by <strong>the</strong> Minister.Where a sublease has been approved andregistered, <strong>the</strong> holder <strong>of</strong> <strong>the</strong> geo<strong>the</strong>rmalproduction lease must continue to comply withany terms and conditions <strong>of</strong> <strong>the</strong> lease including<strong>the</strong> area <strong>of</strong> <strong>the</strong> sublease.RoyaltyThe Act provides that a royalty is payable on <strong>the</strong>use <strong>of</strong> geo<strong>the</strong>rmal energy. The royalty rate will bespecified in <strong>the</strong> supporting regulation.The Queensland Government recognises that <strong>the</strong>geo<strong>the</strong>rmal industry is in its infancy and facestechnological and financial barriers todevelopment. Key features <strong>of</strong> <strong>the</strong> royaltyprovisions include a royalty holiday and royaltyfree threshold that are aimed at reducing costs togeo<strong>the</strong>rmal production during <strong>the</strong> early start-upstages.A royalty holiday that provides a full exemptionfrom <strong>the</strong> payment <strong>of</strong> any royalties will be provideduntil 2020. Whilst <strong>the</strong> first half <strong>of</strong> <strong>the</strong> next decadeis expected to be characterised by increasedexploration activity, <strong>the</strong> later part <strong>of</strong> <strong>the</strong> decadeshould see geo<strong>the</strong>rmal projects coming intoproduction and benefiting from this initiative.After 2020, a royalty-free threshold will ensurethat in <strong>the</strong> early years <strong>of</strong> production when financialmargins may be low, a royalty is not payable if <strong>the</strong>wellhead value is below <strong>the</strong> royalty-free threshold.General authority provisionsA number <strong>of</strong> key provisions apply to bo<strong>the</strong>xploration permits and production leases. Theseprovisions are outlined below.Environmental managementPersons proposing to carry out geo<strong>the</strong>rmalactivities are required to obtain <strong>the</strong> relevantenvironmental authority under <strong>the</strong> EnvironmentalProtection Act 1994 before an exploration permitor a production lease can be granted.Exploration activities conducted under anexploration permit will be classified as level 2environmentally relevant activities under <strong>the</strong>Environmental Protection Regulation 2008(environmental regulation), unless <strong>the</strong>se activitiesoperate in an environmentally sensitive area orare associated with an environmentally relevantactivity stated in schedule 2 <strong>of</strong> <strong>the</strong> environmentalregulation.Production activities conducted under aproduction lease will be classified as level 1 orlevel 2 environmentally relevant activities,depending upon <strong>the</strong> scale <strong>of</strong> production andassociated environmental harm. This approach436


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>largely ensures consistency with existingQueensland resource-based legislation in relationto environmental management requirements.Where <strong>the</strong> geo<strong>the</strong>rmal energy produced is usedfor ano<strong>the</strong>r activity that is an environmentallyrelevant activity under <strong>the</strong> environmentalregulation e.g. aquaculture, that activity willrequire <strong>the</strong> relevant authority under <strong>the</strong>Environmental Protection Act 2009 and <strong>the</strong>environmental regulation.Water ManagementThe Act does not create any rights to water. Anyrelevant authorisations under <strong>the</strong> Water Act 2000must be obtained before an exploration permit ora production lease can be granted. The waterauthority will ensure that <strong>the</strong> taking <strong>of</strong> water forgeo<strong>the</strong>rmal energy exploration or production ismanaged within a whole-<strong>of</strong>-catchment plan thatensures environmental flows are maintained.The grant <strong>of</strong> a geo<strong>the</strong>rmal tenure will not createany preference or priority for <strong>the</strong> grant <strong>of</strong> a waterentitlement. Geo<strong>the</strong>rmal tenure holders will betreated <strong>the</strong> same way as any o<strong>the</strong>r potential waterusers and may need to pay <strong>the</strong> market price for awater entitlement in order to consume water in <strong>the</strong>process <strong>of</strong> exploring for or producing geo<strong>the</strong>rmalenergy.The Act also mandates that an exploration permitor production lease applicant must assess anypotential structural or o<strong>the</strong>r impacts on aquifers <strong>of</strong><strong>the</strong> carrying out <strong>of</strong> <strong>the</strong> proposed activities. TheMinister must consider this issue when decidingwhe<strong>the</strong>r to grant <strong>the</strong> exploration permit orproduction lease.SafetyGeo<strong>the</strong>rmal drilling and related activities aresimilar to those for petroleum and gas activities.Therefore, <strong>the</strong> safety and health aspects <strong>of</strong>geo<strong>the</strong>rmal energy exploration and production willprimarily be regulated under Queensland’sPetroleum and Gas (Production and Safety) Act2004 (P&G Act).Currently, <strong>the</strong> definitions <strong>of</strong> operating plant undersection 670 <strong>of</strong> <strong>the</strong> P&G Act only apply to certainauthorised activities carried out in a geo<strong>the</strong>rmaltenure area.In practice this would mean that o<strong>the</strong>r authorisedactivities on <strong>the</strong> tenure are regulated under <strong>the</strong>Workplace Health and Safety Act 1995 (WH&SAct). The P&G Act and <strong>the</strong> WH&S Act have beenamended to clarify <strong>the</strong> different responsibilities <strong>of</strong><strong>the</strong> Department <strong>of</strong> Employment, EconomicDevelopment and Innovation and WorkplaceHealth and Safety Queensland in relation tosafety management on a geo<strong>the</strong>rmal tenure.The construction <strong>of</strong> new operating plant willcontinue to be covered by <strong>the</strong> WH&S Act.Geo<strong>the</strong>rmal exploration activities that involve, forexample, seismic testing and drilling, will continueto be regulated under <strong>the</strong> P&G Act. O<strong>the</strong>ractivities associated with geo<strong>the</strong>rmal exploration(for example, construction activities) will continueto be regulated under <strong>the</strong> WH&S Act.Petroleum type drilling does not occur in <strong>the</strong>production <strong>of</strong> Hot Sedimentary Aquifer (HSA)sources <strong>of</strong> geo<strong>the</strong>rmal energy. As such, <strong>the</strong> Actwill not apply <strong>the</strong> safety provisions contained in<strong>the</strong> P&G Act to HSA geo<strong>the</strong>rmal production,regardless <strong>of</strong> <strong>the</strong> scale <strong>of</strong> <strong>the</strong> operation. Theseoperations will continue to be covered by <strong>the</strong>WH&S Act.Overlapping authoritiesThe Act includes provisions about overlappingauthorities under different Acts. For example, aproponent may apply for a geo<strong>the</strong>rmal productionlease over an area where ano<strong>the</strong>r resource tenureexists under <strong>the</strong> P&G Act, <strong>the</strong> Greenhouse GasStorage Act 2009 or <strong>the</strong> Mineral Resources Act1989.The purpose <strong>of</strong> allowing overlapping authorities isto ensure <strong>the</strong> optimum use and appropriatemanagement <strong>of</strong> <strong>the</strong> area’s resources and isenshrined in all Queensland resource-basedlegislation.The decision as to which resource authority getspriority rests with <strong>the</strong> Minister, who must considerspecific criteria, including submissions made byeach authority holder who would be affected by<strong>the</strong> grant <strong>of</strong> a geo<strong>the</strong>rmal tenure over <strong>the</strong> sharedarea, as well as <strong>the</strong> public interest.The Act does not allow for an overlappingauthority to be provided for two geo<strong>the</strong>rmalenergy tenures. However, <strong>the</strong> Act allows ageo<strong>the</strong>rmal production lease holder to sub-lease apart <strong>of</strong> <strong>the</strong> land within <strong>the</strong> lease to any party thatis an eligible person, as defined by <strong>the</strong> Act.Land AccessThe Act contains landmark changes to <strong>the</strong> way anumber <strong>of</strong> Queensland resource tenure andauthority holders may access private land andhow compensation arrangements are arrived at.Under <strong>the</strong> changes, geo<strong>the</strong>rmal tenure applicantsand holders will have new responsibilities inrelation to land access.The Act introduces a requirement for allgeo<strong>the</strong>rmal authority holders to comply with aLand Access Code as a condition <strong>of</strong> <strong>the</strong> authority.The Land Access Code is structured in two parts:Part 1 which outlines non-statutory best practiceguidance for communication between authorityholders; and Part 2 which describes mandatoryconduct conditions that must be complied with byauthority holders.The Act introduces activity thresholds thatincrease <strong>the</strong> level <strong>of</strong> regulation as <strong>the</strong> intensity or437


<strong>Australian</strong> Geo<strong>the</strong>rmal <strong>Conference</strong> <strong>2010</strong>impact <strong>of</strong> <strong>the</strong> proposed activity increases. This isa sensible measure that balances <strong>the</strong> level <strong>of</strong>regulation with <strong>the</strong> level <strong>of</strong> impact.Early exploration activities may have minimalimpact on private or public landholders. The Actdefines <strong>the</strong>se as ‘preliminary activities’ whichmight include taking rock, water or soil samplesand walking <strong>the</strong> land.For preliminary activities, a geo<strong>the</strong>rmal tenureholder will be required to give each owner oroccupier <strong>of</strong> land within <strong>the</strong> tenure area an entrynotice and copy <strong>of</strong> <strong>the</strong> Land Access Code at least10 days prior to entry. Access for <strong>the</strong>se activitiesdoes not require a Conduct and CompensationAgreement.When <strong>the</strong> impacts <strong>of</strong> proposed activities on <strong>the</strong>private landholder or occupier are moresignificant, a higher level <strong>of</strong> accord is required.These activities are referred to as “advancedactivities”.To access land to conduct advanced activities,geo<strong>the</strong>rmal tenure holders must ei<strong>the</strong>r be party toa conduct and compensation agreement or adeferral agreement with each ‘eligible claimant’ for<strong>the</strong> land or have made an application to <strong>the</strong> LandCourt to determine compensation. As defined in<strong>the</strong> Act, an ‘eligible claimant’ is each owner oroccupier <strong>of</strong> private land or public land that is in <strong>the</strong>area <strong>of</strong>, or is access land for, <strong>the</strong> tenure. Whereagreement is not reached, <strong>the</strong> frameworkprovides for conferences or independentalternative dispute resolution (ADR) to be held.To assist in <strong>the</strong> negotiation process, standardconduct and compensation and deferralagreements have been developed in consultationwith resource and agriculture industry peakbodies, along with a negotiation tip sheet forlandholders.<strong>Conference</strong>s or ADR will become a legislativerequirement if agreement negotiations breakdown. Matters cannot be referred to <strong>the</strong> LandCourt for determination until a conference or ADRprocess has occurred. This requirement is aimedat resolving disputes early at <strong>the</strong> local level,without <strong>the</strong> expense <strong>of</strong> legal resolution.A detailed compliance and enforcement strategyis currently being developed to ensure that <strong>the</strong>senew land access provisions achieve <strong>the</strong>ir fulleffect on <strong>the</strong> ground, particularly with respect to<strong>the</strong> Land Access Code.Development <strong>of</strong> geo<strong>the</strong>rmal energysubordinate legislationThe Act will commence by proclamation. It isanticipated that <strong>the</strong> Act will commence in <strong>the</strong> laterpart <strong>of</strong> 2011. During <strong>the</strong> intervening period,supporting subordinate legislation, guidelines andtraining will be developed and systems upgradeswill be carried out in preparation for <strong>the</strong> Actcoming into force. There will be opportunities forindustry involvement in <strong>the</strong> development <strong>of</strong> <strong>the</strong>subordinate legislation in late <strong>2010</strong>/early 2011.438

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