Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/348
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dc.contributor.authorallMartelli, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italiaen
dc.contributor.authorallNuccio, P. M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italiaen
dc.contributor.authorallStuart, F. M.; Isotope Geosciences Unit, Scottish Universities Environmental Research Centre, East Kilbride G75 0QF, UKen
dc.contributor.authorallBurgess, R.; Department of Earth Sciences, Manchester University, Manchester M13 9PL, UKen
dc.contributor.authorallEllam, R. M.; Isotope Geosciences Unit, Scottish Universities Environmental Research Centre, East Kilbride G75 0QF, UKen
dc.contributor.authorallItaliano, F.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italiaen
dc.date.accessioned2005-08-05T07:55:51Zen
dc.date.available2005-08-05T07:55:51Zen
dc.date.issued2004en
dc.identifier.urihttp://hdl.handle.net/2122/348en
dc.description.abstractA study of the He isotopic ratios of fluid inclusions in olivine and pyroxene from the Roman Comagmatic Province (RCP),Italy, is presented together with 87Sr/86Sr isotope compositions of the whole rock or pyroxene phenocrysts. A clear covariation in He and Sr isotopes is apparent, with a strong northward increase in radiogenic He and Sr being evident. He and Sr isotopes ratios range from 3He/4He = 5.2 Ra and 87Sr/86Sr = 0.7056 in south Campania, to 3He/4He = 0.44 Ra and 87Sr/86Sr = 0.715905 in the northernmost Latium. Helium isotope ratios are significantly lower than MORB values and are among the lowest yet measured in subduction zone volcanism. The 3He/4He of olivine and pyroxene phenocryst-hosted volatiles appear to be little influenced by posteruptive processes and magma–crust interaction. The 3He/4He–87Sr/86Sr covariation is consistent with binary mixing between an asthenospheric mantle similar to HIMU ocean island basalts, and an enriched (radiogenic) mantle end member generated from subduction of the Ionian/Adriatic plate. The contribution of radiogenic He from metasomatic fluids and postmetasomatism radiogenic ingrowth in the wedge is strongly dependent on the initial He concentration of the mantle. Only when asthenosphere He concentrations are substantially lower than the MORB source mantle, and metasomatism occurred at the beginning of the subduction (f30 Ma), can ingrowth in the mantle wedge account for the 3He/4He of the most radiogenic basalts.en
dc.description.sponsorship- European Social Fund - Scottish Universities - Carnegie Trust for the Universities of Scotland.en
dc.format.extent516427 bytesen
dc.format.extent539 bytesen
dc.format.mimetypeapplication/pdfen
dc.format.mimetypetext/htmlen
dc.language.isoEnglishen
dc.publisher.nameElsevieren
dc.relation.ispartofEarth and Planetary Science Lettersen
dc.relation.ispartofseries224 (2004)en
dc.subjectRoman Comagmatic Provinceen
dc.subjectfluid inclusionsen
dc.subjectheliumen
dc.subjectstrontiumen
dc.titleHelium–strontium isotope constraints on mantle evolution beneath the Roman Comagmatic Province, Italyen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber295–308en
dc.identifier.URLhttp://www.sciencedirect.com/en
dc.subject.INGV04. Solid Earth::04.01. Earth Interior::04.01.03. Mantle and Core dynamicsen
dc.subject.INGV04. Solid Earth::04.07. Tectonophysics::04.07.02. Geodynamicsen
dc.subject.INGV04. Solid Earth::04.07. Tectonophysics::04.07.06. Subduction related processesen
dc.subject.INGV04. Solid Earth::04.07. Tectonophysics::04.07.08. Volcanic arcsen
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.01. Gasesen
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.05. Volcanic rocksen
dc.identifier.doidoi:10.1016/j.epsl.2004.05.025en
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dc.description.fulltextpartially_openen
dc.contributor.authorMartelli, M.en
dc.contributor.authorNuccio, P. M.en
dc.contributor.authorStuart, F. M.en
dc.contributor.authorBurgess, R.en
dc.contributor.authorEllam, R. M.en
dc.contributor.authorItaliano, F.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italiaen
dc.contributor.departmentIsotope Geosciences Unit, Scottish Universities Environmental Research Centre, East Kilbride G75 0QF, UKen
dc.contributor.departmentDepartment of Earth Sciences, Manchester University, Manchester M13 9PL, UKen
dc.contributor.departmentIsotope Geosciences Unit, Scottish Universities Environmental Research Centre, East Kilbride G75 0QF, UKen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italiaen
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crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Palermo, Palermo, Italia-
crisitem.author.deptUniversità di Palermo-
crisitem.author.deptIsotope Geosciences Unit, Scottish Universities Environmental Research Centre, East Kilbride G75 0QF, UK-
crisitem.author.deptSchool of Earth and Environmental Sciences, University of Manchester, Manchester, UK-
crisitem.author.deptSUERC, UK-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Palermo, Palermo, Italia-
crisitem.author.orcid0000-0001-8525-1754-
crisitem.author.orcid0000-0001-7674-8718-
crisitem.author.orcid0000-0002-9465-6398-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
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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