Abstract
Seismic exploration of both Palaeozoic and active strike-slip zones
shows strike-slip faults that penetrate all or most of the crust.
Offsets on the Moho are evident, particularly at young and active
zones with a component of compression, such as the Alpine Fault of
New Zealand where a change in crustal thickness of about 20 km is
observed. Moho offsets for the old Palaeozoic strike-slip zones are
usually much less prominent. Careful migration of crustal seismic
reflection data from some of these zones shows that instead of sharp
offsets, the Moho structure consists of a localized keel-type crustal
thickening of a few kilometres in amplitude and occurs over a zone
approximately 10 km wide. The large Moho offsets of young strike-slip
zones may in some cases partially decay with time. Active strike-slip
zones are becoming an important focus of study, but seismic exploration
is hampered by complex near-surface geology, 3D structure and the
difficulty of imaging steeply dipping structure in the subsurface.
In order to meet this challenge, a wide range of seismic techniques
is now being deployed. These include wide-angle seismic reflection,
refraction, P-wave delays and the study of guided S-waves. Results
from California give geophysical images of vertical strike-slip faults
that penetrate to the Moho. In contrast, the Alpine Fault of New
Zealand appears to be a surface manifestation of an inclined (\~40
deg) ramp, extending down to the lower crust and along which uplift
and exhumation of the continental crust, and possibly strike-slip
motion, is taking place.
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