Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/10406
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dc.contributor.authorallPulvirenti, F.; Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, Chinaen
dc.contributor.authorallAloisi, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.contributor.authorallJin, S.; Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, Chinaen
dc.date.accessioned2016-11-28T07:47:57Zen
dc.date.available2016-11-28T07:47:57Zen
dc.date.issued2017-09en
dc.identifier.urihttp://hdl.handle.net/2122/10406en
dc.description.abstractIn this paper, the relationship between the dike-forming magmatic intrusions and the faulting process at Mount Etna is investigated in terms of Coulomb stress changes. As case study, a complete time-dependent 3-D finite element model for the 2002-2003 eruption at Mount Etna is presented. In the model, which takes into account the topography, medium heterogeneities and principal fault systems in a viscoelastic/plastic rheology, we sequentially activated three dike-forming processes and looked at the induced temporal evolution of the Coulomb stress changes, during the co-intrusive and post-intrusive periods, on Pernicana and Santa Venerina faults. We investigated where and when fault slips were encouraged or not, and consequently how earthquakes may have been triggered. Results show positive Coulomb stress changes for the Pernicana Fault in accordance to the time, location and depth of the 27th October 2002 Pernicana earthquake (Md = 3.5). The amount of Coulomb stress changes in the area of Santa Venerina Fault, as induced by dike-forming intrusions only, is instead almost negligible and, probably, not sufficient to trigger the 29th October Santa Venerina earthquake (Md = 4.4), occurred two days after the start of the eruption. The necessary Coulomb stress change value to trigger this earthquake is instead reached if we consider it as induced by the 27th October Pernicana biggest earthquake, combined with the dike-induced stresses.en
dc.description.sponsorshipMED-SUV FP7 Project (Grant number 308665)en
dc.language.isoEnglishen
dc.publisher.nameElsevier Science Limiteden
dc.relation.ispartofJournal of volcanology and geothermal researchen
dc.relation.ispartofseries/334 (2017)en
dc.subjectCoulomb stress changesen
dc.subjectFinite Element Modelen
dc.subjectViscoelasticityen
dc.subjectEarthquakesen
dc.subjectMount Etnaen
dc.titleTime-dependent Coulomb stress changes induced by the 2002-2003 Etna magmatic intrusions and implications on following seismic activitiesen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber185-196en
dc.subject.INGV04. Solid Earth::04.03. Geodesy::04.03.01. Crustal deformationsen
dc.subject.INGV04. Solid Earth::04.03. Geodesy::04.03.06. Measurements and monitoringen
dc.subject.INGV04. Solid Earth::04.03. Geodesy::04.03.07. Satellite geodesyen
dc.subject.INGV04. Solid Earth::04.03. Geodesy::04.03.08. Theory and Modelsen
dc.subject.INGV04. Solid Earth::04.06. Seismology::04.06.02. Earthquake interactions and probabilityen
dc.subject.INGV04. Solid Earth::04.06. Seismology::04.06.08. Volcano seismologyen
dc.subject.INGV04. Solid Earth::04.07. Tectonophysics::04.07.05. Stressen
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.03. Magmasen
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.06. Volcano monitoringen
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.08. Volcanic risken
dc.subject.INGV05. General::05.01. Computational geophysics::05.01.03. Inverse methodsen
dc.identifier.doi10.1016/j.jvolgeores.2016.11.001en
dc.description.obiettivoSpecifico4V. Dinamica dei processi pre-eruttivien
dc.description.journalTypeJCR Journalen
dc.description.fulltextrestricteden
dc.relation.issn0377-0273en
dc.relation.eissn1872-6097en
dc.contributor.authorPulvirenti, F.en
dc.contributor.authorAloisi, M.en
dc.contributor.authorJin, S.en
dc.contributor.departmentShanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, Chinaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italiaen
dc.contributor.departmentShanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, Chinaen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptComsol Multiphysics GmbH, 37073 Gottingen, Germany-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia-
crisitem.author.deptShanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China-
crisitem.author.orcid0000-0002-9945-4138-
crisitem.author.orcid0000-0002-5108-4828-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent05. General-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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