Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/8548
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dc.contributor.authorallLippiello, E.; Seconda Università di Napolien
dc.contributor.authorallMarzocchi, W.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallde Arcangelis, L.; Seconda Università di Napolien
dc.contributor.authorallCataldo, G.; Seconda Università di Napolien
dc.date.accessioned2013-03-21T08:08:36Zen
dc.date.available2013-03-21T08:08:36Zen
dc.date.issued2012en
dc.identifier.urihttp://hdl.handle.net/2122/8548en
dc.description.abstractAn increase in the number of smaller magnitude events, retrospectively named foreshocks, is often observed before large earthquakes. We show that the linear density probability of earthquakes occurring before and after small or intermediate mainshocks displays a symmetrical behavior, indicating that the size of the area fractured during the mainshock is encoded in the foreshock spatial organization. This observation can be used to discriminate spatial clustering due to foreshocks from the one induced by aftershocks and is implemented in an alarm-based model to forecast m . 6 earthquakes. A retrospective study of the last 19 years Southern California catalog shows that the daily occurrence probability presents isolated peaks closely located in time and space to the epicenters of five of the six m . 6 earthquakes. We find daily probabilities as high as 25% (in cells of size 0.04 3 0.04deg2), with significant probability gains with respect to standard models.en
dc.language.isoEnglishen
dc.relation.ispartofScientific Reportsen
dc.relation.ispartofseries/2(2012)en
dc.subjectforeshocksen
dc.subjectearthquake forecasten
dc.titleSpatial organization of foreshocks as a tool to forecast large earthquakesen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber846en
dc.subject.INGV04. Solid Earth::04.06. Seismology::04.06.02. Earthquake interactions and probabilityen
dc.identifier.doi10.1038/srep00846en
dc.description.obiettivoSpecifico3.1. Fisica dei terremotien
dc.description.journalTypeN/A or not JCRen
dc.description.fulltextrestricteden
dc.contributor.authorLippiello, E.en
dc.contributor.authorMarzocchi, W.en
dc.contributor.authorde Arcangelis, L.en
dc.contributor.authorCataldo, G.en
dc.contributor.departmentSeconda Università di Napolien
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.departmentSeconda Università di Napolien
dc.contributor.departmentSeconda Università di Napolien
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptDepartment of Mathematics and Physics and CNISM, Second University of Naples-
crisitem.author.deptDepartment of Industrial and Information Engineering and CNISM Second University of Naples-
crisitem.author.deptSeconda Università di Napoli-
crisitem.author.orcid0000-0002-9114-1516-
crisitem.classification.parent04. Solid Earth-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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