Welcome to the new version of CaltechAUTHORS. Login is currently restricted to library staff. If you notice any issues, please email coda@library.caltech.edu
Published February 1993 | Published
Journal Article Open

Locating earthquakes with amplitude: Application to real-time seismology

Abstract

Earthquakes are traditionally located using travel times. However, since the ground-motion amplitude generally decays with the distance from the source, it should also be possible to locate earthquakes using amplitude data. Amplitudes are affected by many factors other than the distance, so that we do not expect to be able to locate the epicenter, the location of the initial rupture, very accurately with amplitude data. However, locating earthquakes with amplitudes has its own merits: (1) For postearthquake emergency services, it is often more important to know the spatial distribution of strong-motion parameters such as peak acceleration and peak velocity than the rupture initiation point itself (National Research Council, 1991). This is especially true for thrust earthquakes (e.g., 1971 San Fernando earthquake; 1987 Whittier Narrows earthquake) or events with large rupture zones. (2) The amplitudes are usually much easier to determine than the arrival times, especially for events with complex rupture patterns or with immediate foreshocks in which event association can be difficult. For application to real-time earthquake information systems such as CUBE (Caltech/USGS Broadcast of Earthquakes; Kanamori et al., 1991), the amplitude method could provide a quick and robust way to send useful information for emergency operations. Here, we report a few examples and propose a method for future implementation in a CUBE-type system.

Additional Information

© 1993 Seismological Society of America. Discussions during the Seismological Laboratory coffee break with Don Anderson, Jim Mori, David Wald, and Tom Heaton motivated this study. This research was conducted under the CUBE project and the TERRAscope project, which is supported by the L. K. Whittier and Arco Foundations. Contribution No. 5199, Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California.

Attached Files

Published - 264.full.pdf

Files

264.full.pdf
Files (306.7 kB)
Name Size Download all
md5:98b469490160a27bdba20831766e98d7
306.7 kB Preview Download

Additional details

Created:
August 22, 2023
Modified:
October 26, 2023