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1 Department of Earth and Planetary
Science
University of California
Berkeley, California
94720-4767
(K.M.J., R.B.)
2 Department of Geological
Sciences
Indiana University
2002 E. 10th Street
Bloomington, Indiana
47405
(K.M.J.)
3 Department of Aerospace Engineering
Sciences
University of Colorado
Boulder, Colorado
80309-0429
(K.L.)
The abundance of geodetic and seismic data recording postseismic deformation following the 2004 Parkfield earthquake provides an unprecedented opportunity to resolve frictional properties on the Parkfield section of the San Andreas fault. The Parkfield segment is a transition between the locked section to the southeast that last ruptured in the 1857 Fort Tejon earthquake and the creeping section to the northwest. We develop three-dimensional rate- and state-dependent friction models of afterslip following the 2004 earthquake to investigate the frictional behavior of the fault. It is assumed that the coseismic rupture occurred on an area of the fault surrounded by aseismic creep that accelerated after the earthquake. We estimate the distribution of coseismic slip, afterslip, and ratestate frictional parameters by inverting a two-step slip model. In the model we (1) estimate the coseismic slip distribution from 1-Hz Global Positioning System (GPS) data and (2) use the corresponding coseismic shear stress change on the fault as input into a numerical afterslip model governed by ratestate friction. We find the ratestate frictional parameter A B, an indicator of frictional stability, is in the range 104103 at 50 MPa normal stress, which is near the transition from potentially unstable (negative AB) to nominally stable (positive AB) friction. The estimate of AB values falls within a wide range of experimental values reported for serpentinite, which crops out along the San Andreas fault zone. The critical slip distance, dc, which characterizes the distance over which strength breaks down during a slip event, is in the range 0.010.1 m, consistent with seismic estimates and a fault gouge thickness of 110 m. The afterslip model reproduces most features observed in the GPS time-series data including high surface velocities in the first few months after the earthquake and lower rates at later times, as well as the cumulative postseismic displacement. The model tends to underpredict the displacement data at later times, suggesting that perhaps the modeled afterslip period ends too quickly or an unmodeled deformation process dominates the signal at later times.
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