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Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/3012
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dc.contributor.authorallJovane, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallFlorindo, F.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallDinarès-Turell, J.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallSprovieri, M.; Istituto Ambiente Marino Costiero (CNR)en
dc.contributor.authorallActon, G.; University of California, Davisen
dc.contributor.authorallCoccioni, R.; Universita` degli Studi di Urbinoen
dc.contributor.authorallDall’Antonia, B.; Universita` di Pisaen
dc.date.accessioned2007-12-07T07:42:33Zen
dc.date.available2007-12-07T07:42:33Zen
dc.date.issued2007-11-10en
dc.identifier.urihttp://hdl.handle.net/2122/3012en
dc.description.abstractWe have conducted high-resolution paleomagnetic and rock magnetic studies, in addition to stable isotope analyses of the Massignano sedimentary section, which is the Global Stratotype Section and Point (GSSP) for the Eocene-Oligocene boundary. Our research builds upon the many past studies of the Massignano section in seeking to understand the timing and nature of the paleoenvironmental variations that occurred during the transition for the Earth’s climate system from greenhouse to icehouse. The new paleomagnetic results provide a refined magnetostratigraphy of the section and new age for the Eocene-Oligocene boundary at 33.7 Ma. Abrupt and large alternations in magnetic, concentration, composition, and grain sizes that occur in the high-resolution rock magnetic record are interpreted to be the result of rapid bimodal shifts in deep-sea circulation that affect sediment sources or transport. We speculate that currents flowing through the gateway between the Atlantic and Indo-pacific Oceans may have turned on and off as the gateway was progressively closing, resulting in the deposition of two different assemblages of magnetic minerals at Massignano. Finally, stable isotope (δ18O and δ13C) data collected on ostracod valves also suggest significant changes in sea bottom circulation in the Neo-Tethys Ocean at and about 2 m.y. before the Eocene-Oligocene boundary.en
dc.language.isoEnglishen
dc.publisher.nameAmerican Geophysical Union.en
dc.relation.ispartofJournal of geophysical researchen
dc.relation.ispartofseries/112 (2007)en
dc.subjectpaleomagnetismen
dc.subjectmassignanoen
dc.titleEocene-Oligocene paleoceanographic changes in the stratotype section, Massignano, Italy: Clues from rock magnetism and stable isotopesen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumberB11101en
dc.subject.INGV04. Solid Earth::04.05. Geomagnetism::04.05.06. Paleomagnetismen
dc.identifier.doi10.1029/2007JB004963en
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dc.description.obiettivoSpecifico2.2. Laboratorio di paleomagnetismoen
dc.description.journalTypeJCR Journalen
dc.description.fulltextreserveden
dc.contributor.authorJovane, L.en
dc.contributor.authorFlorindo, F.en
dc.contributor.authorDinarès-Turell, J.en
dc.contributor.authorSprovieri, M.en
dc.contributor.authorActon, G.en
dc.contributor.authorCoccioni, R.en
dc.contributor.authorDall’Antonia, B.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentIstituto Ambiente Marino Costiero (CNR)en
dc.contributor.departmentUniversity of California, Davisen
dc.contributor.departmentUniversita` degli Studi di Urbinoen
dc.contributor.departmentUniversita` di Pisaen
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 Roma2, Roma, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione AC, Roma, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptCNR-IAMC, Napoli-
crisitem.author.deptUniversity of California, Davis-
crisitem.author.deptUniversita` degli Studi di Urbino-
crisitem.author.deptUniversita` di Pisa-
crisitem.author.orcid0000-0002-6058-9748-
crisitem.author.orcid0000-0002-5546-2291-
crisitem.author.orcid0000-0002-3285-4022-
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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