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2011 - Cooperative Institute for Research in Environmental Sciences ...

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workflows that make use of SPIDR’s Simple Object Access<br />

Protocol (SOAP) web services and workflows that comb<strong>in</strong>e<br />

data from different datasets with<strong>in</strong> SPIDR and manipulate<br />

them, such as filter<strong>in</strong>g. In addition to this front-end,<br />

user-centric system, the beg<strong>in</strong>n<strong>in</strong>gs of a back-end workflow<br />

system were completed as well. http://spidr.ngdc.noaa.<br />

gov/worfklow<br />

A RESTful (REpresentational State Transfer) web service<br />

<strong>in</strong>terface was added to SPIDR allow<strong>in</strong>g easier access to the<br />

web service middle ware <strong>for</strong> those less versed <strong>in</strong> web service<br />

development, <strong>in</strong>clud<strong>in</strong>g sample clients <strong>in</strong> Perl, Python,<br />

IDL and Matlab/Octave, br<strong>in</strong>g<strong>in</strong>g SPIDR’s web services<br />

to a much larger community of science data customers.<br />

As a result of these new services, the SPIDR team received<br />

an NGDC customer service award and a NASA software<br />

award.<br />

• http://spidr.ngdc.noaa.gov/spidr/servletGetData?describe<br />

• http://spidr.ngdc.noaa.gov/spidr/tools.do<br />

The data dashboard was completed <strong>for</strong> three widely used<br />

datasets, ionospheric, geomagnetic and cosmic ray data,<br />

and allows a data customer or scientist to see latency of<br />

receipt of SPIDR’s hold<strong>in</strong>gs with<strong>in</strong> those doma<strong>in</strong>s. This <strong>in</strong><strong>for</strong>mation<br />

better supports the use of these data so it is clear<br />

when they were received and from where.<br />

• http://spidr.ngdc.noaa.gov/spidr/data_dashboard.do<br />

Product: Poster presentation, ‘Auroral Resources Toolkit<br />

(ART),’ at the Space Weather Workshop, April 27, <strong>2011</strong>.<br />

Milestone 2. Develop an operational version of the D-<br />

Region Absorption Prediction (D-RAP) Model<strong>in</strong>g System<br />

on the NGDC website, which will generate model outputs<br />

that are available from, and archived at, NGDC.<br />

This task is complete, and the data, model outputs and<br />

visualization are all available on the NGDC’s Solar and<br />

Terrestrial Physics Division (STPD) website. There is an<br />

opportunity <strong>for</strong> cont<strong>in</strong>ued development as well, to make<br />

or collaborate with another group to create an on-demand<br />

model run capability. This would be similar to what the<br />

NASA Goddard Space Flight Center Community Coord<strong>in</strong>ated<br />

Model<strong>in</strong>g Center (CCMC) does, and as such, they<br />

would make a good partner <strong>for</strong> do<strong>in</strong>g so. Discussions on<br />

this topic have been held, and the desire <strong>for</strong> a broader<br />

NGDC on-demand model run capability exists and was<br />

brought to light by said discussions.<br />

This dynamic/on-demand aspect of D-RAP would<br />

be a subset of the wider NGDC ef<strong>for</strong>t, so it will not be<br />

pursued as part of this milestone, but will be considered<br />

<strong>for</strong> the wider NGDC on-demand capability as a follow-up<br />

ef<strong>for</strong>t, whether that is an <strong>in</strong>-house project or collaboration<br />

with an outside organization. D-RAP Model<strong>in</strong>g System<br />

outputs are available from the NGDC/STP website, and<br />

are be<strong>in</strong>g archived at NGDC as well.<br />

• http://ngdc.noaa.gov/stp/iono/drap/<strong>in</strong>dex.html.<br />

Milestone 3. Develop a ‘Geomag Track<strong>in</strong>g Database’ to<br />

track geomagnetic data hold<strong>in</strong>gs at NGDC <strong>in</strong> order to<br />

modernize the geomagnetic data stewardship program<br />

and provide a tool that will help correct past difficulties <strong>in</strong><br />

data stewardship and dissem<strong>in</strong>ation.<br />

The Geomag Track<strong>in</strong>g Database was developed and<br />

operates accord<strong>in</strong>g to specification. This database <strong>in</strong>gests<br />

<strong>in</strong>ventory data <strong>in</strong> XML <strong>for</strong>mat and handles a dynamic<br />

100 CIRES Annual Report <strong>2011</strong><br />

range of metadata fields. The database allows sort<strong>in</strong>g of<br />

geomatic data and metadata <strong>in</strong> ways that were not be<strong>for</strong>e<br />

possible, provid<strong>in</strong>g a powerful new tool to the community<br />

and NGDC data managers.<br />

Product: Database was presented at the meet<strong>in</strong>g ‘Artifical<br />

Intelligence <strong>in</strong> the Earth’s Magnetic Field Study,’ <strong>in</strong><br />

Uglich, Russia, January <strong>2011</strong>.<br />

Milestone 4. Develop a ‘MIRror of onl<strong>in</strong>e MAGnetic data<br />

(MIRRMAG)’ data <strong>in</strong>gest system that will <strong>in</strong>gest available,<br />

onl<strong>in</strong>e geomagnetic data <strong>in</strong>to NGDC databases. Once<br />

<strong>in</strong>gested, the system will per<strong>for</strong>m any needed <strong>for</strong>mat process<strong>in</strong>g,<br />

load the data <strong>in</strong>to the SPIDR database, port the<br />

data to the NGDC FTP site, and port the data to the tape<br />

library <strong>in</strong>gest stag<strong>in</strong>g area.<br />

MIRRMAG <strong>in</strong>gest system is fully functional. The system<br />

<strong>in</strong>gests, processes and dissem<strong>in</strong>ates data as designed.<br />

This system streaml<strong>in</strong>es <strong>in</strong>gest and dissem<strong>in</strong>ation of<br />

geomagnetic observatory data, allow<strong>in</strong>g <strong>for</strong> more efficient<br />

use of data manager time and limit<strong>in</strong>g the potential<br />

problems that arise from more hands-on data management<br />

techniques. As an un<strong>for</strong>eseen benefit, this system<br />

has allowed <strong>for</strong> the geomagnetic data manager to take on<br />

an <strong>in</strong>creased workload <strong>in</strong> a time when resources are limited.<br />

As a result, our customer service and data-handl<strong>in</strong>g<br />

practices are per<strong>for</strong>m<strong>in</strong>g better <strong>in</strong> a more challeng<strong>in</strong>g<br />

environment.<br />

SWPC-01SolarDisturbances<strong>in</strong>the<br />

GeospaceEnvironment<br />

FEDERAL LEAD: VIC PIZZO<br />

CIRES LEAD: ALYSHA REINARD<br />

NOAA Goal 3: Weather and Water<br />

Project Goal: Improve the prediction of travel<strong>in</strong>g solar disturbances<br />

that impact the geospace environment. Such disturbances,<br />

which are associated with both coronal holes and coronal<br />

mass ejections from the sun, can cause substantial geomagnetic<br />

effects lead<strong>in</strong>g to the crippl<strong>in</strong>g of satellites, disruption of radio<br />

communications and damage to electric power grids.<br />

Milestone 1. In collaboration, SWPC will modify and test the<br />

empirical relationship l<strong>in</strong>k<strong>in</strong>g helicity and future flar<strong>in</strong>g potential<br />

of a given active region, and will evaluate its potential<br />

as a <strong>for</strong>ecast<strong>in</strong>g tool <strong>for</strong> solar flares.<br />

This project is just beg<strong>in</strong>n<strong>in</strong>g. We have hired a postdoc,<br />

who began work <strong>in</strong> April. She has just started this ef<strong>for</strong>t,<br />

and we expect to have results to report on next year.<br />

SWPC-02Model<strong>in</strong>gtheUpperAtmosphere<br />

FEDERAL LEAD: MICHAEL CRUMLY<br />

CIRES LEAD: TIMOTHY FULLER-ROWELL<br />

NOAA Goal 3: Weather and Water<br />

Project Goal: Quantify the impact of sudden stratospheric<br />

warm<strong>in</strong>gs (SSW) on the upper atmosphere. Recent observations<br />

suggest that SSW impact the dynamics and electrodynamics<br />

of the lower thermosphere, and change the diurnal<br />

variation of total electron, which is an important component<br />

of space weather. The recently developed Whole Atmosphere<br />

Model (WAM) simulates SSW naturally so will be used to quantify<br />

their impact on the thermosphere and ionosphere.

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