Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/4742
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dc.contributor.authorallZonno, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Milano-Pavia, Milano, Italiaen
dc.contributor.authorallMusacchio, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Milano-Pavia, Milano, Italiaen
dc.contributor.authorallBasili, R.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallImperatori, W.; Institute of Geophysics-ETH, Zurichen
dc.contributor.authorallMai, P. M.; Institute of Geophysics-ETH, Zurichen
dc.date.accessioned2008-12-15T10:00:19Zen
dc.date.available2008-12-15T10:00:19Zen
dc.date.issued2008-12en
dc.identifier.urihttp://hdl.handle.net/2122/4742en
dc.description.abstractIn the framework of an ongoing Italian national research project we are studying the Messina 1908 earthquake, the first to be recorded adequately by seismological and geodetic instrumentation that allowed subsequent quantitative investigations of its source properties. We use a high-frequency stochastic finite-fault modeling (Motazedian and Atkinson, 2005) to simulate the ground-shaking for a number of different source models (Basili et al. 2008), either constrained from past source studies of this event or simulated. Although inherently kinematic, our approach accounts for the physics of the source using a procedure to generate physically consistent earthquake-rupture models (Guatteri et al., 2004). Considering the width of the seismogenic zone and appropriate source-scaling relation, we generate heterogeneous slip models that obey to the source complexity of past earthquakes (Mai and Beroza, 2002). By also constraining the point of rupture initiation based on empirical findings and energy-balance arguments (Mai et al., 2005), we generate a suite of earthquake source models to compute far-field ground-shaking. The Housner parameter from the stochastic high-frequency simulations is than compared with the felt intensity (MCS scale). The developed procedure is a necessary tool to take into account the influence of directivity effects in simulating ground shaking scenarios using realistic slip distribution on the fault. Furthermore, we carry out full-wavefield ground-motion calculations (at frequencies f < 3 Hz) to compare those low-frequency simulations with (a) the stochastic simulations and (b) appropriate ground-motion prediction equations. The combined approach helps to examine the validation range of the two methods (distinguishing the influence of the near-field and far-field motions on the shaking level), and may serve as a basis to develop a hybrid technique which combines the two methods for generating fully broadband synthetic seismograms.en
dc.language.isoEnglishen
dc.relation.ispartofAGU 2008 Fall Meeting - Special Session S02 - The M7.1 Messina, Italy, Earthquake and Tsunami of 28 December 1908: 100 Years of Research on an Important Desructive Earthquakeen
dc.subjectStochastic ground-motion simulationen
dc.subjectFull-wavefield ground-motion simulationen
dc.subjectFinite-fault simulationen
dc.subjectHousner parameteren
dc.subjectSlip Distributionen
dc.subjectMessina 1908 earthquake (Southern Italy)en
dc.titleSTOCHASTIC AND FULL-WAVEFIELD FINITE-FAULT GROUND-MOTION SIMULATIONS OF THE M7.1, MESSINA 1908 EARTHQUAKE (Southern Italy)en
dc.typePoster sessionen
dc.description.statusUnpublisheden
dc.subject.INGV04. Solid Earth::04.06. Seismology::04.06.99. General or miscellaneousen
dc.description.ConferenceLocationSan Francisco, CA U.S.Aen
dc.description.obiettivoSpecifico4.1. Metodologie sismologiche per l'ingegneria sismicaen
dc.description.fulltextopenen
dc.contributor.authorZonno, G.en
dc.contributor.authorMusacchio, G.en
dc.contributor.authorBasili, R.en
dc.contributor.authorImperatori, W.en
dc.contributor.authorMai, P. M.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Milano, Milano, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Milano, Milano, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.departmentInstitute of Geophysics-ETH, Zurichen
dc.contributor.departmentInstitute of Geophysics-ETH, Zurichen
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 Milano, Milano, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Milano, Milano, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.deptInstitute of Geophysic, ETH Zurich, Switzerland-
crisitem.author.deptDivision of Physical Sciences & Engineering, King Abdullah University of Science & Technology (KAUST), Thuwal, Saudi Arabia-
crisitem.author.orcid0000-0003-0873-9187-
crisitem.author.orcid0000-0003-1509-2182-
crisitem.author.orcid0000-0002-1213-0828-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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