Published December 14, 1993 | Version Published
Journal Article Open

An analysis of nearfield normal mode amplitude anomalies of the Landers Earthquake

  • 1. ROR icon California Institute of Technology

Abstract

The 1992 Landers earthquake (M_w=7.3) occurred in the middle of the TERRAscope network. Long-period Rayleigh waves recorded at the TERRAscope stations (Δ≤3°) after traveling around the Earth show large amplitude anomalies, one order of magnitude larger than spherical Earth predictions up to a period of about 600 s. The ground motions over the epicentral region at and after the arrival of R4–5 are in phase at all stations. These observations are inconsistent with the nearly vertical strike slip mechanism of the Landers earthquake. Synthetic seismograms for a rotating, elliptic and laterally heterogeneous Earth model calculated by the variational method agree well with the observed waveforms. Calculations for various 3D Earth models demonstrate that the amplitudes are very sensitive to the large scale aspherical structure in the crust and the mantle. The anomalies for modes shorter than 300 s period can be explained by lateral heterogeneity shallower than the upper mantle. Rotation of the Earth and lower mantle heterogeneity are required to explain mode amplitudes at longer periods. Current whole mantle seismic tomographic models can fully explain the observed amplitudes longer than 300 s. To assess the effect of the high order lateral heterogeneity in the mantle more precise estimate of the crustal correction is required.

Additional Information

© 1993 by the American Geophysical Union. Received July 7, 1993; revised October 12, 1993; accepted October 13, 1993. We thank T. Tanimoto and S. Tsuboi for useful discussions. We also thank W.-j. Su and R. L. Woodward for providing us with their whole mantle seismic models, A. Dziewonski for bringing the importance of the crustal correction to our attention, and an anonymous reviewer for valuable comments. A part of computations was supported by the JPL/Caltech supercomputing project. This research was partially supported by the U. S. Geological Survey Grant 1434-93-G-2287. This research was conducted under the TERRAscope project supported by the L. K. Whittier and Arco Foundations. Contribution No. S29S, Division of Geological and Planetary Sciences, California Institute of Technology.

Attached Files

Published - DLAgrl93.pdf

Files

DLAgrl93.pdf

Files (307.7 kB)

Name Size
md5:7544e5b01646222dedcbf9607cbccfb9
307.7 kB Preview Download

Additional details

Identifiers

Eprint ID
45661
Resolver ID
CaltechAUTHORS:20140512-084432682

Funding

USGS
1434-93-G-2287
L. K. Whittier Foundation
Arco Foundation

Dates

Created
2014-05-12
Created from EPrint's datestamp field
Updated
2021-11-10
Created from EPrint's last_modified field

Caltech Custom Metadata

Caltech groups
Division of Geological and Planetary Sciences (GPS)
Other Numbering System Name
Caltech Division of Geological and Planetary Sciences
Other Numbering System Identifier
5295