A very broad-band stochastic source model used for near source strong motion prediction

The simulation of near‐source ground motion requires the calculation of ground motion in a very broad‐band frequency range (typically from 10 s to 0.1 s). However, the calculation of complete Green's function is too time consuming for high‐frequency simulations. We present a method to obtain ve...

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Bibliographic Details
Published in:Geophysical research letters Vol. 25; no. 7; pp. 1063 - 1066
Main Authors: Berge, Catherine, Gariel, Jean-Christophe, Bernard, Pascal
Format: Journal Article
Language:English
Published: Washington, DC Blackwell Publishing Ltd 01-04-1998
American Geophysical Union
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Summary:The simulation of near‐source ground motion requires the calculation of ground motion in a very broad‐band frequency range (typically from 10 s to 0.1 s). However, the calculation of complete Green's function is too time consuming for high‐frequency simulations. We present a method to obtain very broad‐band synthetic seismograms, combining the kinematic spectral source model of Bernard et al., [1996], and an algorithm, based on the wavenumber technique of Bouchon and Aki, [1977]. High‐frequency radiations are evaluated with ray theory and a broad‐band dislocation defined on a finely discretized fault plane. The low‐frequency radiations due to the near‐ and intermediate‐fields are calculated with the complete field algorithm on a low‐wavenumber filtered dislocation. This dislocation is defined on a coarse grid over the fault, hence significantly reducing the computing time. We apply this method to compute the ground motion at a station located near an extended fault, where the near‐, intermediate‐ and far‐field radiations are important.
Bibliography:ark:/67375/WNG-DSB1G24V-2
istex:DCC02EBC4710940FA25F209BAC7B74F3EFD01ABA
ArticleID:98GL00732
ISSN:0094-8276
1944-8007
DOI:10.1029/98GL00732