Bulletin of the Seismological Society of America; February 2005; v. 95; no. 1;
p. 75-108; DOI: 10.1785/0120030093
© 2005 Seismological Society of America
Asperity Model of an Earthquake: Dynamic Problem
Lane R. Johnson1 and
Robert M. Nadeau2
1 Center for Computational
Seismology
Earth Sciences Division, 90-116
Lawrence Berkeley National
Laboratory
One Cyclotron Road
Berkeley, California
94720
(L.R.J.)
2 Berkeley Seismological
Laboratory
University of California
Berkeley, California
94720
(R.M.N.)
A previous study that presented the static solution for an asperity model of
an earthquake is extended to solve the dynamic problem that develops when
failure occurs on the boundary of an asperity patch and then spreads over the
surrounding displacement shadow region. The boundary integral equation method is
coupled with basic constitutive equations for failure and friction to solve the
dynamic problem, with different parameters used for the strong asperity patch
and weak shadow region. No friction, displacement-weakening friction, and
velocity-strengthening friction are all investigated. Depending on the type and
amount of friction that is present, the dynamic solutions for slip on the fault
exhibit a range of different features, including overshoot of the static
solution and oscillation, rupture front velocities that may be greater than or
less than the S velocity and change with position, and either total or
partial release of the static moment. Common characteristics of the solutions
are that failure on the asperity patch is almost independent of failure on the
shadow region and that the displacement deficit on the shadow region is released
by propagating slip pulses. The stress concentrations of the asperity model are
sufficient to produce nonlinear elastic effects in a region extending outward
from the fault to distances comparable with the dimensions of the shadow region.
Beginning with the solutions for slip on the fault, waveforms are simulated for
an earthquake of magnitude Mw 1.44 and compared with data
recorded at a distance of 8.65 km. Simulations that contain both source and
propagation effects are capable of explaining most of the basic features of the
observational data, including general agreement with the shape of the waveforms
in the time domain, the levels and slopes of the spectra at low frequencies
(less than 10 Hz) and at high frequencies (greater than 100 Hz), and some of the
interference effects present in both the time and frequency domains.
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