Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/9643
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dc.contributor.authorallCioni, R.; Università di Pisaen
dc.contributor.authorallLongo, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Pisa, Pisa, Italiaen
dc.contributor.authorallMacedonio, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
dc.contributor.authorallSantacroce, R.; Università di Pisaen
dc.contributor.authorallSbrana, A.; Università di Pisaen
dc.contributor.authorallSulplizio, R.; Università di Pisaen
dc.contributor.authorallAndronico, D.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.date.accessioned2015-05-28T05:58:09Zen
dc.date.available2015-05-28T05:58:09Zen
dc.date.issued2003en
dc.identifier.urihttp://hdl.handle.net/2122/9643en
dc.description.abstractA general methodology of pyroclastic fall hazard assessment is proposed on the basis of integrated results of field studies and numerical simulations. These approaches result in two different methods of assessing hazard: (1) the ‘‘field frequency,’’ based on the thickness and distribution of past deposits and (2) the ‘‘simulated probability,’’ based on the numerical modeling of tephra transport and fallout. The proposed methodology mostly applies to volcanoes that, by showing a clear correlation between the repose time and the magnitude of the following eruptions, allows the definition of a reference ‘‘maximum expected event’’ (MEE). The application to Vesuvius is shown in detail. Using the field frequency method, stratigraphic data of 24 explosive events in the 3–6 volcanic explosivity index range in the last 18,000 years of activity are extrapolated to a regular grid in order to obtain the frequency of exceedance in the past of a certain threshold value of mass loading (100, 200, 300, and 400 kg/m2). Using the simulated probability method, the mass loading related to the MEE is calculated based on the expected erupted mass (5 1011 kg), the wind velocity profiles recorded during 14 years, and various column heights and grain-size populations. The role of these factors was parametrically studied performing 160,000 simulations, and the probability that mass loading exceeded the chosen threshold at each node was evaluated. As a general rule, the field frequency method results are more reliable in proximal regions, provided that an accurate database of field measurements is available. On the other hand, the simulated probability method better describes events in middle distal areas, provided that the MEE magnitude can be reliably assumed. In the Vesuvius case, the integration of the two methods results in a new fallout hazard map, here presented for a mass loading value of 200 kg/m2.en
dc.language.isoEnglishen
dc.relation.ispartofJournal of Geophysical Researchen
dc.relation.ispartofseries/108 (2003)en
dc.subjectpyroclastic flows, numerical simulationsen
dc.titleAssessing pyroclastic fall hazard through field data and numerical simulation: Example from Vesuviusen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber2063-2083en
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.03. Magmasen
dc.identifier.doi10.1029/2001JB000642en
dc.description.obiettivoSpecifico3V. Dinamiche e scenari eruttivien
dc.description.journalTypeJCR Journalen
dc.description.fulltextopenen
dc.contributor.authorCioni, R.en
dc.contributor.authorLongo, A.en
dc.contributor.authorMacedonio, G.en
dc.contributor.authorSantacroce, R.en
dc.contributor.authorSbrana, A.en
dc.contributor.authorSulplizio, R.en
dc.contributor.authorAndronico, D.en
dc.contributor.departmentUniversità di Pisaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Pisa, Pisa, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
dc.contributor.departmentUniversità di Pisaen
dc.contributor.departmentUniversità di Pisaen
dc.contributor.departmentUniversità di Pisaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italiaen
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 Pisa, Pisa, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OV, Napoli, Italia-
crisitem.author.deptDipartimento di Scienze della Terra, Pisa, Italy-
crisitem.author.deptDipartimento di Scienze della Terra, Via S. Maria 53, 56126 Pisa, Italy.-
crisitem.author.deptCIRISIVU, c/o Dipartimento Geomineralogico, Universita' di Bari-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia-
crisitem.author.orcid0000-0002-2526-9095-
crisitem.author.orcid0000-0001-6590-6346-
crisitem.author.orcid0000-0001-6604-1479-
crisitem.author.orcid0000-0001-7424-8429-
crisitem.author.orcid0000-0003-1373-0603-
crisitem.author.orcid0000-0002-3930-5421-
crisitem.author.orcid0000-0002-8333-1547-
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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