Clustering of velocities in a GPS network spanning the Sierra Nevada Block, the Northern Walker Lane Belt, and the Central Nevada Seismic Belt, California-Nevada
The deformation across the Sierra Nevada Block, the Walker Lane Belt, and the Central Nevada Seismic Belt (CNSB) between 38.5°N and 40.5°N has been analyzed by clustering GPS velocities to identify coherent blocks. Cluster analysis determines the number of clusters required and assigns the GPS stati...
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Veröffentlicht in: | Journal of geophysical research. Solid earth 2013-09, Vol.118 (9), p.4937-4947 |
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Format: | Artikel |
Sprache: | eng |
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Zusammenfassung: | The deformation across the Sierra Nevada Block, the Walker Lane Belt, and the Central Nevada Seismic Belt (CNSB) between 38.5°N and 40.5°N has been analyzed by clustering GPS velocities to identify coherent blocks. Cluster analysis determines the number of clusters required and assigns the GPS stations to the proper clusters. The clusters are shown on a fault map by symbols located at the positions of the GPS stations, each symbol representing the cluster to which the velocity of that GPS station belongs. Fault systems that separate the clusters are readily identified on such a map. Four significant clusters are identified. Those clusters are strips separated by (from west to east) the Mohawk Valley‐Genoa fault system, the Pyramid Lake‐Wassuk fault system, and the Central Nevada Seismic Belt. The strain rates within the westernmost three clusters approximate simple right‐lateral shear (~13 nstrain/a) across vertical planes roughly parallel to the cluster boundaries. Clustering does not recognize the longitudinal segmentation of the Walker Lane Belt into domains dominated by either northwesterly trending, right‐lateral faults or northeasterly trending, left‐lateral faults.
Key Points
Clustering of GPS velocities suggests 4 clusters separated by 3 boundaries
Central cluster boundary corresponds to the Pyramid Lake‐Wassuk fault system
Other boundaries correspond to the Mohawk Valley fault system and the CNSB |
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ISSN: | 2169-9313 2169-9356 |
DOI: | 10.1002/jgrb.50340 |