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50thKaikoura05 -1- Kaikoura 2005 CHARACTERISATION OF NEW ...

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oundaries and with immature source areas for their<br />

sediments.<br />

ORAL<br />

GEOPHYSICAL EXPLORATION <strong>OF</strong> THE<br />

ALPINE FAULT ZONE AND EVIDENCE FOR<br />

HIGH FLUID PRESSURE<br />

Tim Stern 1 , David Okaya 2 & Stuart Henrys 3<br />

School of Earth Sciences, Victoria University<br />

Dept. of Geol. Sci., Uni. of Southern California,<br />

Los Angeles, USA<br />

IGNS, Lower Hutt.<br />

(tim.stern*vuw.ac.nz)<br />

A fresh look at the problem of sustaining fluid<br />

pressures in active fault zones can be obtained by<br />

studying a major continental transform other than<br />

the San Andreas Fault. The Alpine Fault (AF) of<br />

central South Island is one such example. From a<br />

global perspective the AF is unusual as it is a<br />

continental transform where both strike-slip (~ 35<br />

mm/y) and dip slip (~10 mm/y) movement take<br />

place on the same fault plane. Moreover,<br />

geophysical evidence shows this fault plane dips at<br />

40 to 60 o from the Earth’s surface down to a depth<br />

of at least 30 km where it soles out into what we<br />

interpret to be a decollement surface. Detailed<br />

analysis of seismic travel time anomalies and<br />

seismic reflection amplitudes show that above the<br />

dipping fault-plane is a banana-shaped region<br />

where seismic P-wave velocities are reduced by 6-<br />

10%. This low-velocity region has dimensions of<br />

roughly 20 x 40 km with the shallowest and deepest<br />

points being at ~ 8 and 35 km, respectively. A<br />

magnetotelluric study shows a low electrical<br />

resistivity zone in the crust that correlates closely<br />

with the region of low seismic velocities.<br />

Interconnected water at, or close to, lithostatic<br />

pressure is the physical condition that would give<br />

rise to both the low resistivity and low P-wave<br />

velocities. Corroborative geological evidence for<br />

high fluid pressures can be seen in the form of<br />

young, undeformed, quartz veins that are within<br />

freshly exhumed crust east of the surface exposure<br />

of the Alpine fault. The question then arises: how<br />

are high fluid pressures contained in the fault zone?<br />

A simple answer is that fluid is supplied to the root<br />

of the fault zone at a rate that is higher than it can<br />

be removed via porous flow through the crust.<br />

Greywacke-schist rocks that are transported into the<br />

fault zone are thickened as they travel down a<br />

decollement surface; this surface has been partially<br />

imaged with seismic reflection methods. As the<br />

crustal rocks are thickened water will be released<br />

(zeolite � amphibolite prograde metamorphism) at<br />

an estimated rate of 0.15 % wt per km of burial. On<br />

the basis of our seismic crustal structure models,<br />

and assuming a regular continental permeability of<br />

10 -17 m 2 , we calculate that water is supplied to the<br />

root of the Alpine fault zone at a rate that is about<br />

40 times greater than it can bleed off through crust<br />

of regular permeability.<br />

For the majority of plate motion to be carried on a<br />

single inclined fault plane the fault itself is likely to<br />

be weak or of low friction. Most continental<br />

transforms with a component of convergence<br />

partition motion into a vertical strike slip fault and<br />

distributed thrust faults. Southern California is an<br />

example. We therefore argue that it is high fluid<br />

pressure, due largely to fluid-release from prograde<br />

metamorphism that reduces effective normal<br />

stresses in the Alpine fault zone. And it is possibly<br />

this reduction in normal stresses that allows plate<br />

motion to focus on a single inclined plane. In light<br />

of recently published findings of periodic slip and<br />

“slow” seismic tremor associated with fluidsaturated<br />

parts of other plate boundaries, it seems<br />

important to undertake long-term seismic and GPS<br />

monitoring of the central section of the Alpine<br />

Fault.<br />

ORAL<br />

SEISMIC HAZARD ANALYSIS IN <strong>NEW</strong><br />

ZEALAND DURING THE LIFETIME <strong>OF</strong> THE<br />

GEOLOGICAL SOCIETY<br />

M.W. Stirling, G.H. McVerry, K.R. Berryman,<br />

&W.D.Smith<br />

Institute of Geological & Nuclear Sciences, PO<br />

Box 30368, Lower Hutt<br />

(m.stirling*gns.cri.nz)<br />

New Zealand sits astride the boundary of the<br />

Australian and Pacific Plates, where relative plate<br />

motion is expressed by frequent, and often<br />

damaging earthquakes. The Geological Society of<br />

New Zealand has been in existence throughout the<br />

evolution of earthquake hazard analysis in New<br />

Zealand, and many Society members have<br />

contributed to the associated advances in the<br />

science. The 1960s saw major contributions to<br />

understanding the patterns of seismicity in New<br />

Zealand, and the relationships between active faults<br />

and earthquakes. Prominent scientists such as the<br />

late Frank Evison and late Gerald Lensen were<br />

leaders in these efforts, along with Robin Adams,<br />

who showed the importance of parameters like<br />

tectonic setting, fault slip type and soil properties in<br />

the assessment of earthquake hazard. The USAbased<br />

formulation of probabilistic seismic hazard<br />

(PSH) methodology by Allin Cornell in the late<br />

1960s led to the development of PSH models for<br />

New Zealand in the 1970s and 80s. These PSH<br />

models were often the combined products of<br />

engineering seismologists, seismologists and<br />

geologists, but largely limited to the historical<br />

record of seismicity. The well-known “Smith and<br />

50 th <strong>Kaikoura</strong>05 -83- <strong>Kaikoura</strong> <strong>2005</strong>

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