dc.contributor.authorHummon, Cheryl
dc.contributor.authorSchneider, Craig L.
dc.contributor.authorYeats, Robert S.
dc.contributor.authorDolan, James F.
dc.contributor.authorSieh, Kerry
dc.contributor.authorHuftile, Gary J.
dc.date.accessioned2013-03-11T08:22:48Z
dc.date.available2013-03-11T08:22:48Z
dc.date.copyright1994en_US
dc.date.issued1994
dc.identifier.citationHummon, C., Schneider, C. L., Yeats, R. S., Dolan, J. F., Sieh, K. E., & Huftile, G. J. (1994). Wilshire fault: Earthquakes in Hollywood?. Geology, 22(4), 291-294.en_US
dc.identifier.issn0091-7613en_US
dc.identifier.urihttp://hdl.handle.net/10220/9375
dc.description.abstractThe Wilshire fault is a potentially seismogenic, blind thrust fault inferred to underlie and cause the Wilshire arch, a Quaternary fold in the Hollywood area, just west of downtown Los Angeles, California. Two inverse models, based on the Wilshire arch, allow us to estimate the location and slip rate of the Wilshire fault, which may be illuminated by a zone of microearthquakes. A fault-bend fold model indicates a reverse-slip rate of 1.5-1.9 mm/yr, whereas a three-dimensional elastic-dislocation model indicates a right-reverse slip rate of 2.6-3.2 mm/yr. The Wilshire fault is a previously unrecognized seismic hazard directly beneath Hollywood and Beverly Hills, distinct from the faults under the nearby Santa Monica Mountains.en_US
dc.language.isoenen_US
dc.relation.ispartofseriesGeologyen_US
dc.rights© 1994 Geological Society of Americaen_US
dc.subjectDRNTU::Science::Geology::Volcanoes and earthquakes
dc.titleWilshire fault : earthquakes in Hollywood?en_US
dc.typeJournal Article
dc.identifier.doihttp://dx.doi.org/10.1130/0091-7613(1994)022<0291:WFEIH>2.3.CO;2


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