Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/10713
DC FieldValueLanguage
dc.date.accessioned2018-02-16T07:50:32Zen
dc.date.available2018-02-16T07:50:32Zen
dc.date.issued2013-07en
dc.identifier.urihttp://hdl.handle.net/2122/10713en
dc.description.abstractWe model interevent times and Coulomb static stress transfer on the rupture segments along the Corinth Gulf extension zone, a region with a wealth of observations on strong-earthquake recurrence behavior. From the available information on past seismic activity, we have identified eight segments without significant overlapping that are aligned along the southern boundary of the Corinth rift. We aim to test if strong earthquakes on these segments are characterized by some kind of time-predictable behavior, rather than by complete randomness. The rationale for time-predictable behavior is based on the characteristic earthquake hypothesis, the necessary ingredients of which are a known faulting geometry and slip rate. The tectonic loading rate is characterized by slip of 6 mm/yr on the westernmost fault segment, diminishing to 4 mm/yr on the easternmost segment, based on the most reliable geodetic data. In this study, we employ statistical and physical modeling to account for stress transfer among these fault segments. The statistical modeling is based on the definition of a probability density distribution of the interevent times for each segment. Both the Brownian Passage-Time (BPT) and Weibull distributions are tested. The time-dependent hazard rate thus obtained is then modified by the inclusion of a permanent physical effect due to the Coulomb static stress change caused by failure of neighboring faults since the latest characteristic earthquake on the fault of interest. The validity of the renewal model is assessed retrospectively, using the data of the last 300 years, by comparison with a plain time-independent Poisson model, by means of statistical tools including the Relative Operating Characteristic diagram, the R-score, the probability gain and the log-likelihood ratio. We treat the uncertainties in the parameters of each examined fault source, such as linear dimensions, depth of the fault center, focal mechanism, recurrence time, coseismic slip, and aperiodicity of the statistical distribution, by a Monte Carlo technique. The Monte Carlo samples for all these parameters are drawn from a uniform distribution within their uncertainty limits. We find that the BPT and the Weibull renewal models yield comparable results, and both of them perform significantly better than the Poisson hypothesis. No clear performance enhancement is achieved by the introduction of the Coulomb static stress change into the renewal model.en
dc.language.isoEnglishen
dc.relation.ispartofJournal of Geophysical Research: Solid Earthen
dc.relation.ispartofseries7/118(2013)en
dc.titleRenewal models and coseismic stress transfer in the Corinth Gulf, Greece, fault systemen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber3655–3673en
dc.identifier.URLhttp://onlinelibrary.wiley.com/doi/10.1002/jgrb.50277/pdfen
dc.subject.INGV04.06. Seismologyen
dc.subject.INGV05.08. Risken
dc.identifier.doi10.1002/jgrb.50277en
dc.description.obiettivoSpecifico5T. Modelli di pericolosità sismica e da maremotoen
dc.description.obiettivoSpecifico6T. Variazioni delle caratteristiche crostali e precursorien
dc.description.journalTypeJCR Journalen
dc.contributor.authorConsole, Rodolfoen
dc.contributor.authorFalcone, Giuseppeen
dc.contributor.authorKarakostas, Vassilisen
dc.contributor.authorMurru, Mauraen
dc.contributor.authorPapadimitriou, Eleftheriaen
dc.contributor.authorRhoades, Daviden
dc.contributor.departmentCenter of Integrated Geomorphology for the Mediterranean Area, Potenza, Italyen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italiaen
dc.contributor.departmentGeophysics Department, Aristotle University of Thessaloniki, Thessaloniki, Greeceen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italiaen
dc.contributor.departmentGeophysics Department, Aristotle University of Thessaloniki, Thessaloniki, Greeceen
dc.contributor.departmentGNS Science, Lower Hutt, New Zealanden
item.openairetypearticle-
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.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.deptGeophysics Department, Aristotle University of Thessaloniki, Thessaloniki, Greece-
crisitem.author.deptGNS Science, Lower Hutt, New Zealand-
crisitem.author.orcid0000-0002-2554-4421-
crisitem.author.orcid0000-0002-9999-6770-
crisitem.author.orcid0000-0002-7385-394X-
crisitem.author.orcid0000-0003-3574-2787-
crisitem.author.orcid0000-0002-9512-9215-
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.classification.parent05. General-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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