| Understanding fault rupture during major earthquakes, and the resulting ground motions, is limited by our observational capabilities. Observations of very large amplitude seismic waves, especially direct measurements of displacement, would make a significant improvement in constraining the size of dynamic strains that trigger remote seismicity and in revealing details of the source rupture process. For example, accelerometers capture the details of strong ground shaking near the source, but it is difficult to convert the acceleration measurements unambiguously to displacement which is required for determining the source time history. Broad-band seismometers are more sensitive, and have better resolution of ground motion, but frequently clip, saturate, or become non-linear even at great distances from a large earthquake. Interferometric Synthetic Aperture Radar (InSAR) observations can produce spatially rich images of some components of surface displacement surrounding a rupture, but InSAR fails in many regions and has no temporal resolution to resolve dynamic phenomena. Global Positioning System (GPS) geodetic measurements have been important for resolving static offsets, but are usually sampled at such a low rate that resolving details of the rupture process was not frequently attempted. |
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Our group has worked on GPS seismic signals for the Denali, Tokachi-Oki, Parkfield, and San Simeon Earthquakes. Our model for the Tokachi-Oki rupture can be seen here. Please click on the publications listed below for more information about the other earthquakes.
Our work is funded by NFS (EAR-0337206 and EAR-0538116) and the USGS NEHRP (Tokachi-Oki earthquake). Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of NSF.
Please send questions and comments to kristinem.larson at gmail.com
Archived Results at IRIS:
Publications:
Background Information on High-Rate GPS