The 1999 Hector Mine Earthquake,
Southern California: Vector Near-Field Displacements from ERS InSAR
David
T. Sandwell, Lydie Sichoix, and Bridget Smith
Institute of Geophysics and Planetary Physics,
Scripps Institution of Oceanography, La Jolla, CA
submitted to: BSSA, Special Section on the Hector Mine Earthquake, October
16, 2000
in press: August 2001
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Abstract
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 N-S oriented fault and optimal for an E-W 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 1-2 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
sub-pixel cross-correlation of features in the before and after amplitude
images. In addition to strike- 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.