Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/10136
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dc.contributor.authorallPischiutta, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallFondriest, M.; Earth Sciences Department Padua Universityen
dc.contributor.authorallDemurtas, M.; Earth Sciences Department Padua Universityen
dc.contributor.authorallDi Toro, G.; School of Earth, Atmospheric and Environmental Sciences, The University of Manchesteren
dc.contributor.authorallRovelli, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.date.accessioned2015-08-17T07:35:54Zen
dc.date.available2015-08-17T07:35:54Zen
dc.date.issued2014-12-15en
dc.identifier.urihttp://hdl.handle.net/2122/10136en
dc.description.abstractTo infer the occurrence of directional amplification effects, we performed ambient noise measurements along a 200m transect crossing the Campo Imperatore fault zone (Central Italy), an exhumed analogue of the faults responsible of the L'Aquila 2009 earthquake sequence, We have recently found in several fault zones that ambient noise is not randomly polarized, but it is amplified on the horizontal plane along a specific site-dependent direction. The analysis repeated using earthquake signals revealed that S-coda waves and surface waves show the same polarization direction, independently of the earthquake backazimuth and focal mechanism. We have explained the observed directional amplifications in terms of fractured rocks in the fault damage zone, polarization being oriented orthogonally to fractures produced by the kinematic stress component. Therefore ground motion directional amplification could be related to the higher compliance of fractured rocks. In the other studies the fracture pattern was derived from numerical-analytical modeling based on the fault geometry and kinematics, or compared with the fast direction of shear wave obtained by seismic anisotropy analysis. The aim of this study is to compare observations with fracture measurements (strike, dip, dip-azimuth, spacing, later continuity, etc.) performed in the selected fault zone. We thus acquired ambient noise using 25 stations installed along a transect where detailed structural geological measurements were carried out. Ambient noise was recorded for around 1 hour, and was processed to compute the horizontal-to-vertical noise spectral ratio as a function of frequency and direction of motion. Wavefield polarization was investigated in the time–frequency domain as well. We found that, in spite of the complexity of the seismic data, the observed polarization pattern is generally oriented orthogonal to the measured dominant fracture system, confirming the existence of a high angle relation between ground motion polarization and fracture systems.en
dc.language.isoEnglishen
dc.relation.ispartofAGU fall meeting 2014en
dc.subjectDirectional Amplificationen
dc.subjectFault damage zoneen
dc.titleDirectional resonance and wavefield polarization in the damage zone of the Campo Imperatore fault, central Italy.en
dc.typeConference paperen
dc.description.statusUnpublisheden
dc.subject.INGV04. Solid Earth::04.06. Seismology::04.06.04. Ground motionen
dc.description.ConferenceLocationSan Franciscoen
dc.description.obiettivoSpecifico3T. Pericolosità sismica e contributo alla definizione del rischioen
dc.description.fulltextopenen
dc.contributor.authorPischiutta, M.en
dc.contributor.authorFondriest, M.en
dc.contributor.authorDemurtas, M.en
dc.contributor.authorDi Toro, G.en
dc.contributor.authorRovelli, A.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.departmentEarth Sciences Department Padua Universityen
dc.contributor.departmentEarth Sciences Department Padua Universityen
dc.contributor.departmentSchool of Earth, Atmospheric and Environmental Sciences, The University of Manchesteren
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
item.openairetypeConference paper-
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 Roma2, Roma, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.orcid0000-0001-9991-5048-
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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