T. Hara et Rj. Geller, ANOMALOUSLY LARGE NEAR-FIELD RAYLEIGH-WAVES EXCITED BY THE 1992 LANDERS, CALIFORNIA, EARTHQUAKE, Bulletin of the Seismological Society of America, 84(3), 1994, pp. 751-760
The epicenter of the Landers, California, earthquake (28 June 1992; M(
W) = 7.3) was located near the TERRAscope network of broadband seismic
stations. The direct Rayleigh wave arrivals, R1, were clipped, and th
e first two later arrivals, R2 and R3, were contaminated by the waves
from a large aftershock, but, as reported by Kanamori et al. (1992a),
the amplitudes of R4 and later great circle Rayleigh wave arrivals (fu
ndamental mode spheroidal free oscillations) are about 10 times larger
than predicted by synthetic seismograms for a spherically symmetric e
arth model. We show that, for the moment tensor of the Landers event (
predominantly vertical strike slip), the amplitudes of synthetics at t
he TERRAscope stations for a laterally heterogeneous, rotating, ellipt
ical model are about 10 times greater than those for a spherically sym
metric model. Because the anomaly ratio is sensitive to both the sourc
e model and the three-dimensional (3D) earth model, we do not attempt
to reproduce the exact anomaly ratios recorded by the various stations
. To explain the existence of near-field amplitude anomalies in genera
l, we use the first-order Born approximation to find the perturbation
to the synthetic seismogram resulting from lateral heterogeneity, elli
pticity, and the earth's rotation. In a coordinate system with the sou
rce on the z axis a point-source strike-slip earthquake on a vertical
fault plane in a spherically symmetric medium excites Rayleigh waves w
ith azimuthal order +/-2 only; these waves have a near-field vertical
displacement of zero at the source; the displacement increases with th
e square of epicentral distance for any given azimuth. Coupling as a r
esult of asphericity allows such a source to excite Rayleigh waves wit
h azimuthal order zero, whose near-field amplitude is independent of e
picentral distance, thereby generating large near-field amplitude anom
alies. We conduct numerical experiments to study the influence of vari
ous parameters on near-field amplitude anomalies.