Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/7735
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dc.contributor.authorallArienzo, I.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
dc.contributor.authorallHeumann, A.; GZG, Abteilung Geochemie, Goldschmidtstr. 1, 37077 Göttingen, Germanyen
dc.contributor.authorallWörner, G.; GZG, Abteilung Geochemie, Goldschmidtstr. 1, 37077 Göttingen, Germanyen
dc.contributor.authorallCivetta, L.; Dipartimento di Scienze Fisiche, Università di Napoli “Federico II”, Monte S. Angelo, Napoli, Italyen
dc.contributor.authorallOrsi, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
dc.date.accessioned2012-02-16T16:10:26Zen
dc.date.available2012-02-16T16:10:26Zen
dc.date.issued2011-04-30en
dc.identifier.urihttp://hdl.handle.net/2122/7735en
dc.description.abstractThe Campi Flegrei caldera collapsed 39 ka in the Neapolitan area (southern Italy) after the Campanian Ignimbrite eruption. This eruption, recognized as the largest and the most cataclysmic volcanic event in the Mediterranean area over the past 200 ka, extruded not less than 300 km3 of trachytic magma. Controversy exists over the timescales required to assemble a such large volume of silicic melt and thus whether large magmatic reservoirs can actually persist below active volcanic systems over prolonged periods of time. Uranium-series analyses have been performed on Campanian Ignimbrite whole-rocks, glass matrixes and separated minerals, and the obtained results have been interpreted in combination with data on Sr, Nd, Pb isotopes from literature. The compositionally most evolved sample which is most radiogenic with respect to Sr isotopes records a reference age of 71 ka. By contrast, U-Th internal isochrones of the three compositionally least evolved samples give identical initial Th isotope ratios and yield consistent ages predating the eruption by up to 6.4 ka. The highest Pb and Nd isotopic ratios and 230Th/232Th activity ratios together with the oldest reference age of the most evolved samples suggest the existence of a resident magma body possibly related to a magmatic system that is known to have fed earlier magmatic activity in the Campi Flegrei area. Conversely, the younger age of the least evolved and least radiogenic magma dates the crystallization/differentiation event of a chemically and isotopically new magma batch entering the reservoir of the resident magma some few thousand years before the cataclysmic eruption. Therefore, the time preceding this large caldera-forming eruption during which the large volume of Campanian Ignimbrite magma assembled and mixed is 6.4 ± 2.1 ka.en
dc.description.sponsorshipThis study benefited from the financial support of the 5th Framework Programme of the European Union within the ERUPT project.en
dc.language.isoEnglishen
dc.publisher.nameElsevier Science Limiteden
dc.relation.ispartofEarth and planetary science lettersen
dc.relation.ispartofseries/306 (2011)en
dc.subjectU-Th isotopesen
dc.subjectCampanian Ignimbriteen
dc.titleProcesses and timescales of magma evolution prior to the Campanian Ignimbrite eruption (Campi Flegrei, Italy)en
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber217-228en
dc.subject.INGV05. General::05.02. Data dissemination::05.02.01. Geochemical dataen
dc.identifier.doi10.1016/j.epsl.2011.04.002en
dc.description.obiettivoSpecifico3.5. Geologia e storia dei vulcani ed evoluzione dei magmien
dc.description.journalTypeJCR Journalen
dc.description.fulltextrestricteden
dc.relation.issn0012-821Xen
dc.relation.eissn1385-013Xen
dc.contributor.authorArienzo, I.en
dc.contributor.authorHeumann, A.en
dc.contributor.authorWörner, G.en
dc.contributor.authorCivetta, L.en
dc.contributor.authorOrsi, G.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
dc.contributor.departmentGZG, Abteilung Geochemie, Goldschmidtstr. 1, 37077 Göttingen, Germanyen
dc.contributor.departmentGZG, Abteilung Geochemie, Goldschmidtstr. 1, 37077 Göttingen, Germanyen
dc.contributor.departmentDipartimento di Scienze Fisiche, Università di Napoli “Federico II”, Monte S. Angelo, Napoli, Italyen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
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 OV, Napoli, Italia-
crisitem.author.deptAbteilung Geochemie, GZG, Georg-August-Universität Göttingen, Goldschmidtstr. 1, 37077 Göttingen, Germany-
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.orcid0000-0002-6213-056X-
crisitem.author.orcid0000-0002-3809-2276-
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.parent05. General-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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