Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/13577
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dc.date.accessioned2020-05-05T12:17:07Z-
dc.date.available2020-05-05T12:17:07Z-
dc.date.issued2003-
dc.identifier.urihttp://hdl.handle.net/2122/13577-
dc.description.abstractThe late Pleistocene trachytic Campanian Ignimbrite underlies much of the Campanian Plain near Naples, Italy, and occurs in valleys in the mountainous area surrounding the plain out to about 80 km from its source, the Campi Flegrei caldera. At sites within 15 km of the Campi Flegrei, anisotropy of magnetic susceptibility (AMS) principal directions indicate that, in the absence of significant topography, deposition came from a flow moving in a roughly radial direction. AMS studies of the more distal ignimbrite reveal downhill and/or downvalley flow directions prior to deposition, even where these directions are at high angles to a generally radial transport direction from the vent. On the flanks of Roccamonfina Volcano, flow was directly downhill, as if the source of the ignimbrite was the summit of the volcano. In most localities, the ignimbrite consists of a single massive deposit. In a few localities in the Apennine Mountains, however, the confluence of multiple drainage systems off mountains resulted in multiple local flow units that cannot be correlated between valleys. A detailed study of the ignimbrite in the flat Titerno River valley near Massa shows that the AMS fabrics are not due to late-stage creeping during deposition or compaction. Well-defined, but non-parallel AMS fabrics from vertical and lateral sections in the Massa area are best explained by the merging of gravity currents flowing down the valley and steep valley sides to form a single aggradational deposit. Clast compositions and AMS axes at Mondragone indicate that the pyroclastic flow encountered the Monte Massico massif and was partially blocked, so that flow during deposition was toward the Campi Flegrei. Similar AMS data from sites along the edge of the Campanian Plain indicate back-flow off the first ridge of the Apennine Mountains reached at least 5 km from their base. The Campanian Ignimbrite was deposited from a density-stratified pyroclastic flow. The depositional system consisted of the lower, denser portion of the current, and was controlled by topography. The grouping of the AMS axes is interpreted to indicate that deposition occurred under laminar flow conditions.en_US
dc.language.isoEnglishen_US
dc.relation.ispartofBulletin of Volcanologyen_US
dc.relation.ispartofseries/65 (2003)en_US
dc.titleAnisotropy of magnetic susceptibility studies of depositional processes in the Campanian Ignimbrite, Italyen_US
dc.typearticleen
dc.description.statusPublisheden_US
dc.type.QualityControlPeer-revieweden_US
dc.description.pagenumber55–72en_US
dc.identifier.doi10.1007/s00445-002-0241-2en_US
dc.description.obiettivoSpecifico5V. Processi eruttivi e post-eruttivien_US
dc.description.journalTypeJCR Journalen_US
dc.relation.issn0258-8900en_US
dc.contributor.authorOrt, Michael-
dc.contributor.authorOrsi, Giovanni-
dc.contributor.authorPappalardo, Lucia-
dc.contributor.authorFisher, Richard V-
dc.contributor.departmentCenter for Environmental Sciences and Education and Departmentof Geologyen_US
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OV, Napoli, Italiaen_US
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OV, Napoli, Italiaen_US
dc.contributor.departmentDepartment of Geological Sciences, University of California,Santa Barbaraen_US
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 EnÍironmental Sciences and Geology, Northern Arizona UniÍersity, Flagstaff, AZ, USA-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OV, Napoli, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OV, Napoli, Italia-
crisitem.author.deptDepartment of Geological Sciences, University of California, Santa Barbara, CA 93106, USA-
crisitem.author.orcid0000-0002-3548-3554-
crisitem.author.orcid0000-0002-9187-252X-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.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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