Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/7389
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dc.contributor.authorallConsole, R.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallDi Luccio, F.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallMurru, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallImoto, M.; National Institute for Earth Science and Disaster Prevention, Tennodai 3-1, Tsukuba-shi, Ibaraki-ken, 305 Japanen
dc.contributor.authorallStavrakakis, G.; National Observatory of Athens, Geodynamic Institute, PO Box 20048, GR-11810, Athens, Greeceen
dc.date.accessioned2012-01-19T07:28:58Zen
dc.date.available2012-01-19T07:28:58Zen
dc.date.issued1999en
dc.identifier.urihttp://hdl.handle.net/2122/7389en
dc.description.abstractThe aim of this work is to quantitatively set up a simple hypothesis for occurrence of earthquakes conditioned by prior events, on the basis of a previously existing model and the use of recent instrumental observations. A simple procedure is presented in order to determine the conditional probability of pairs of events (foreshock-mainshock, mainshock-aftershock) with short time and space separation. The first event of a pair should not be an aftershock, i.e., itmust not be related to a stronger previous event. The Italian earthquake catalog of the Istituto Nazionale di Geofisica (ING) (1975–1995, M > 3:4), the earthquake catalog of the Japan Meteorological Agency (JMA) (1983– 1994, M > 3:0) and that of the National Observatory of Athens (NOA) (1982–1994, M > 3:8) were analyzed. The number of observed pairs depends on several parameters: the size of the space-time quiescence volume defining nonaftershocks, the inter event time, the minimum magnitude of the two events, and the spatial dimension of the alarm volume after the first event. The Akaike information criterion has been adopted to assess the optimum set of space-time parameters used in the definition of the pairs, assuming that the occurrence rate of subsequent events may be modeled by two Poisson processes with different rates: the higher rate refers to the space-time volume defined by the alarms and the lower one simulates earthquakes that occur in the nonalarm space-time volume. On the basis of the tests carried out on the seismic catalog of Italy, the occurrence rate of M > 3:8 earthquakes followed by a M > 3:8 mainshock within 10 km and 10 days (validity) is 0.459. We have observed, for all three catalogs, that the occurrence rate density for the second event of a couple (mainshock or aftershock) of magnitude M2 subsequent to a non aftershock of magnitude M1 in the time range T can be modeled by the following relationship: .T , M2/ D 10a 0Cb.M1􀀀M2/ with b varying from 0.74 (Japan) to 1.09 (Greece). The decrease of the occurrence rate in time for a mainshock after a foreshock or for large aftershocks after a mainshock, for all three databases, obeys the Omori’s law with p changing from 0.94 (Italy) to 2.0 (Greece).en
dc.language.isoEnglishen
dc.publisher.nameKluwer Academic Publishersen
dc.relation.ispartofNatural Hazardsen
dc.relation.ispartofseries/19 (1999)en
dc.subjectforeshock, aftershock, validity, probability gain, Akaike information criterionen
dc.titleShort Term and Short Range Seismicity Patterns in Different Seismic Areas of the Worlden
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber107-121en
dc.subject.INGV04. Solid Earth::04.06. Seismology::04.06.02. Earthquake interactions and probabilityen
dc.description.journalTypeJCR Journalen
dc.description.fulltextreserveden
dc.contributor.authorConsole, R.en
dc.contributor.authorDi Luccio, F.en
dc.contributor.authorMurru, M.en
dc.contributor.authorImoto, M.en
dc.contributor.authorStavrakakis, G.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.departmentNational Institute for Earth Science and Disaster Prevention, Tennodai 3-1, Tsukuba-shi, Ibaraki-ken, 305 Japanen
dc.contributor.departmentNational Observatory of Athens, Geodynamic Institute, PO Box 20048, GR-11810, Athens, Greeceen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
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.deptNational Research Institute for Earth Science and Disaster Prevention, Japan-
crisitem.author.deptNational Observatory of Athens, Institute of Geodynamics, Athens, Greece-
crisitem.author.orcid0000-0002-9924-3736-
crisitem.author.orcid0000-0002-7385-394X-
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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