Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/8468
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dc.contributor.authorallAvallone, Antonio; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italiaen
dc.contributor.authorallRovelli, Antonio; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallBen-Zion, Yehuda; University of Southern Californiaen
dc.date.accessioned2012-12-19T08:04:18Zen
dc.date.available2012-12-19T08:04:18Zen
dc.date.issued2010en
dc.identifier.urihttp://hdl.handle.net/2122/8468en
dc.description.abstractThe ground motion of the April 6th 2009 Mw 6.3 L'Aquila (Central Italy) earthquake, occurred on a SW-dipping normal fault, was successfully recorded by one of the GPS stations installed near L'Aquila before the seismic event and acquiring with a high sampling rate (10 Hz). These data provide valuable ground displacement time histories in the near source. GPS and strong motion data provided reliable reconstruction of the main features around the source. However, a low frequency (about 1 Hz) nearly-harmonic large oscillation (about 40 cm peak-to-peak) detected at this GPS station 5 s after the beginning of the coseismic dynamic deformation, and spanning about 6.5 s, was not possible to be fit by reliable source modeling. 1 Hz nearly-harmonic oscillations are also observed by a co-located seismological station installed one year after the mainshock. Both the GPS and the seismic stations are located on the eastern slope of the Mt. Ocre ridge, along which runs the the Monticchio-Fossa fault, a shallow and steep NE-dipping antithetic fault bordering the Aterno Valley graben. We have checked that the late large-amplitude coseismic displacement can be generated by energy trapped in this fault. We have obtained satisfactory results by using a line dislocation in a structure consisting in two quarter-spaces separated by vertical fault layers. Our best fit corresponds to a model characterized by a vertical 200 m-wide fault zone with impedance contrasts with respect to the adjacent left and right quarter-spaces of about 17% and 40%, respectively.en
dc.language.isoEnglishen
dc.relation.ispartofAGU 2010 Fall Meetingen
dc.subjectHRGPSen
dc.subjecttrapped wavesen
dc.titleTrapped seismic fault zone energy recorded by a high-rate GPS stationen
dc.typePoster sessionen
dc.description.statusPublisheden
dc.subject.INGV04. Solid Earth::04.07. Tectonophysics::04.07.99. General or miscellaneousen
dc.description.ConferenceLocationSan Francisco, California (USA)en
dc.description.obiettivoSpecifico3.1. Fisica dei terremotien
dc.description.fulltextopenen
dc.contributor.authorAvallone, Antonioen
dc.contributor.authorRovelli, Antonioen
dc.contributor.authorBen-Zion, Yehudaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione ONT, Roma, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.departmentUniversity of Southern Californiaen
item.openairetypePoster session-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione ONT, Roma, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.deptUniversity of Southern California-
crisitem.author.orcid0000-0002-0264-2897-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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