|
|
||||||||
INSTITUTE OF TECTONICS UNIVERSITY OF CALIFORNIA, SANTA CRUZ, SANTA CRUZ, CALIFORNIA 95064
SEISMOLOGICAL LABORATORY CALIFORNIA INSTITUTE OF TECHNOLOGY, PASADENA, CALIFORNIA 91125
Abstract
We studied strong-motion spectra observed for three Mw 7.8 to 8.0 earthquakes (the 1985 Michoacán, Mexico; 1985 Valparaíso, Chile; and 1983 Akita-Oki, Japan earthquakes). We determined the decay of spectral amplitude with distance from the station, considering different measures of distance from a finite fault. We compared strong-motion spectra (Fourier acceleration spectra) observed for these three earthquakes with those estimated from the source spectrum determined from teleseismic P waves. We scaled the teleseismic source spectra to produce reference strong-motion spectra at periods from 1 to 10 sec using a simple physical model of far-field S body waves from a point source recorded at the surface of a homogeneous half-space. For all three earthquakes the reference spectral amplitudes at periods of 1 to 5 sec are about half the observed ones at distances of about 50 km. The difference increases as the distance increases. At distances of 200 to 300 km, the reference spectrum is about 1/10 of the observed one. The difference between the reference and the observed spectrum is attributed to the contribution of phases other than direct S waves and to site response. We applied corrections for the finiteness (spatial extent) of the source using a simple model of rupture propagation on a dipping two-dimensional fault. Including the source finiteness did not improve the estimate substantially at periods from 1 to 20 sec, but it modeled significant changes in the signal duration as a function of azimuth for the 1985 Michoacán earthquake. Our results can be used to establish empirical relations between the observed spectra and the half-space responses, depending on the distance and the site condition. If such empirical relations can be established, source spectra determined from teleseismic records may be used to estimate strong motions.
This article has been cited by other articles:
![]() |
Radiated Energy from the 16 October 1999 Hector Mine Earthquake: Regional and Teleseismic Estimates Bulletin of the Seismological Society of America, May 1, 2002; 92(4): 1256 - 1265. |
||||
![]() |
C. Mendoza, S. Hartzell, and T. Monfret Wide-band analysis of the 3 March 1985 central Chile earthquake: Overall source process and rupture history Bulletin of the Seismological Society of America, April 1, 1994; 84(2): 269 - 283. [Abstract] [PDF] |
||||
![]() |
S. H. HARTZELL Estimation of near-source ground motions from a teleseismically derived rupture model of the 1989 Loma Prieta, California, earthquake Bulletin of the Seismological Society of America, October 1, 1992; 82(5): 1991 - 2013. [Abstract] [PDF] |
||||
![]() |
D. A. WALKER, C. S. MCCREERY, and Y. HIYOSHI T-phase spectra, seismic moments, and tsunamigenesis Bulletin of the Seismological Society of America, June 1, 1992; 82(3): 1275 - 1305. [Abstract] [PDF] |
||||
![]() |
S. K. SINGH, M. ORDAZ, and R. R. CASTRO Mismatch between teleseismic and strong-motion source spectra Bulletin of the Seismological Society of America, June 1, 1992; 82(3): 1497 - 1502. [PDF] |
||||
![]() |
S. H. HARTZELL, G. S. STEWART, and C. MENDOZA Comparison of L1 and L2 norms in a teleseismic waveform inversion for the slip history of the Loma Prieta, California, earthquake Bulletin of the Seismological Society of America, October 1, 1991; 81(5): 1518 - 1539. [Abstract] [PDF] |
||||
| HOME | HELP | FEEDBACK | SUBSCRIPTIONS | ARCHIVE | SEARCH | TABLE OF CONTENTS |