Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/9351
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dc.contributor.authorallLe Corvec, N.; Lunar and Planetary Institute, USRA, Houston, Texas, USAen
dc.contributor.authorallWalter, T.; GFZ German Research Centre for Geosciences, Potsdamen
dc.contributor.authorallRuch, J.; King Abdullah University of Science and Technology, Thuwal, Saudi Arabiaen
dc.contributor.authorallBonforte, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.contributor.authorallPuglisi, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.date.accessioned2015-02-24T13:45:57Zen
dc.date.available2015-02-24T13:45:57Zen
dc.date.issued2014-07-10en
dc.identifier.urihttp://hdl.handle.net/2122/9351en
dc.description.abstractMount Etna volcano is subject to transient magmatic intrusions and flank movement. The east flank of the edifice, in particular, is moving eastward and is dissected by the Timpe Fault System. The relationship of this eastward motion with intrusions and tectonic fault motion, however, remains poorly constrained. Here we explore this relationship by using analogue experiments that are designed to simulate magmatic rift intrusion, flank movement, and fault activity before, during, and after a magmatic intrusion episode. Using particle image velocimetry allows for a precise temporal and spatial analysis of the development and activity of fault systems. The results show that the occurrence of rift intrusion episodes has a direct effect on fault activity. In such a situation, fault activitymay occur or may be hindered, depending on the interplay of fault displacement and flank acceleration in response to dike intrusion. Our results demonstrate that a complex interplaymay exist between an active tectonic fault system and magmatically induced flank instability. Episodes of magmatic intrusion change the intensity pattern of horizontal flank displacements andmay hinder or activate associated faults. We further compare our results with the GPS data of the Mount Etna 2001 eruption and intrusion. We find that syneruptive displacement rates at the Timpe Fault System have differed from the preeruptive or posteruptive periods, which shows a good agreement of both the experimental and the GPS data. Therefore, understanding the flank instability and flank stability at Mount Etna requires consideration of both tectonic and magmatic forcing.en
dc.language.isoEnglishen
dc.publisher.nameAmerican Geophysical Unionen
dc.relation.ispartofJournal of geophysical research - solid earthen
dc.relation.ispartofseries/119 (2014)en
dc.subjectanalogue modelsen
dc.subjectstrainen
dc.subjectstressen
dc.subjecteruptionen
dc.subjectflank dynamicsen
dc.subjectGPSen
dc.subjectfaultsen
dc.subjectEtnaen
dc.titleExperimental study of the interplay between magmatic rift intrusion and flank instability with application to the 2001 Mount Etna eruptionen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber5356-5368en
dc.subject.INGV04. Solid Earth::04.03. Geodesy::04.03.08. Theory and Modelsen
dc.identifier.doi10.1002/2014JB011224en
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dc.description.obiettivoSpecifico1V. Storia e struttura dei sistemi vulcanicien
dc.description.journalTypeJCR Journalen
dc.description.fulltextrestricteden
dc.relation.issn0148-0227en
dc.contributor.authorLe Corvec, N.en
dc.contributor.authorWalter, T.en
dc.contributor.authorRuch, J.en
dc.contributor.authorBonforte, A.en
dc.contributor.authorPuglisi, G.en
dc.contributor.departmentLunar and Planetary Institute, USRA, Houston, Texas, USAen
dc.contributor.departmentGFZ German Research Centre for Geosciences, Potsdamen
dc.contributor.departmentKing Abdullah University of Science and Technology, Thuwal, Saudi Arabiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italiaen
item.languageiso639-1en-
item.grantfulltextrestricted-
item.fulltextWith Fulltext-
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.openairetypearticle-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
crisitem.author.deptLunar and Planetary Institute, Universities Space Research Association, 3600 Bay Area Boulevard, Houston, Texas 77058, USA-
crisitem.author.deptDept. Physics of the Earth, Helmholtz-Zentrum Potsdam, Deutsches, GeoForschungsZentrum (GFZ), Telegrafenberg, 14473 Potsdam, Germany-
crisitem.author.deptDipartimento Scienze Geologiche, Università Roma Tre, Roma, Italy-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia-
crisitem.author.orcid0000-0001-5414-987X-
crisitem.author.orcid0000-0003-0435-7763-
crisitem.author.orcid0000-0003-4503-5808-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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