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Scripps Institution of Oceanography
La Jolla, California
92093-0225
dsandwell{at}ucsd.edu
Two components of fault slip are uniquely determined from two line-of-sight
(LOS) radar interferograms by assuming that the fault-normal component of
displacement is zero. We use this approach with ascending and descending
interferograms from the ERS satellites to estimate surface slip along the
Hector Mine earthquake rupture. The LOS displacement is determined by visually
counting fringes to within 1 km of the outboard ruptures. These LOS estimates
and uncertainties are then transformed into strike- and dip-slip estimates and
uncertainties; the transformation is singular for a NS oriented fault
and optimal for an EW oriented fault. In contrast to our previous
strike-slip estimates, which were based only on a descending interferogram, we
now find good agreement with the geological measurements, except at the ends
of the rupture. The ascending interferogram reveals significant west-side-down
dip-slip (
1.0 m) which reduces the strike-slip estimates by 1 to 2 m,
especially along the northern half of the rupture. A spike in the strike-slip
displacement of 6 m is observed in central part of the rupture. This large
offset is confirmed by subpixel cross correlation of features in the before
and after amplitude images. In addition to strike slip and dip slip, we
identify uplift and subsidence along the fault, related to the restraining and
releasing bends in the fault trace, respectively. Our main conclusion is that
at least two look directions are required for accurate estimates of surface
slip even along a pure strike-slip fault. Models and results based only on a
single look direction could have major errors. Our new estimates of strike
slip and dip slip along the rupture provide a boundary condition for
dislocation modeling. A simple model, which has uniform slip to a depth of 12
km, shows good agreement with the observed ascending and descending
interferograms.
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