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