Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/8160
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dc.contributor.authorallMollo, S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallMisiti, V.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallScarlato, P.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallSoligo, M.; Università Roma Treen
dc.date.accessioned2012-10-11T14:03:30Zen
dc.date.available2012-10-11T14:03:30Zen
dc.date.issued2012en
dc.identifier.urihttp://hdl.handle.net/2122/8160en
dc.description.abstractBoth large (i.e. from hundreds to thousands of metres thick) and small (i.e. from centimetres to a few metres thick) magmatic intrusions are characterized by mineral compositional variations proceeding from the outermost to the innermost part of the intrusive body. However, in the case of large intrusions, mineral compositions become progressively more primitive (e.g. An-rich plagioclases and En-rich pyroxenes) from the chilled margin towards the interior; whereas, the opposite occurs for small intrusive bodies. Since it is unclear to what extent variable cooling rate conditions may alter the phase compositions, we have performed isothermal and dynamic experiments within a temperature interval of 1250–1100 °C using four different cooling rates of 150, 50, 10 and 2.5 °C/h. Numerical simulations of thermal regimes in and around small and large magmatic intrusions have also been performed and compared with phase compositional variations observed in our laboratory experiments. Results indicate that, over rapid cooling rate conditions, the crystal compositions faithfully reproduce those of high-temperature formations, i.e. An-rich plagioclases, En-rich pyroxenes and Usp-poor spinels. However, such a process is limited to a maximum distance of 2–3 m from the margin of the intrusion. Moreover, in active volcanic systems, heat fluxes are released from the main regions of magma storage into host rocks; therefore, only magmas solidifying at the contact of cold wall rocks may develop chilled margins with features related to rapid cooling rate conditions. In the presence of hot host rocks, thermal gradients are significantly reduced and the role played by cooling dynamics on textural and compositional variations of minerals is practically negligible.en
dc.language.isoEnglishen
dc.publisher.nameElsevier Science Limiteden
dc.relation.ispartofChemical geologyen
dc.relation.ispartofseries/322-323(2012)en
dc.subjectMagmatic intrusion Cooling rate Partition coefficient Thermometeren
dc.titleThe role of cooling rate in the origin of high temperature phases at the chilled margin of magmatic intrusionsen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber28-46en
dc.subject.INGV04. Solid Earth::04.04. Geology::04.04.05. Mineralogy and petrologyen
dc.identifier.doi10.1016/j.chemgeo.2012.05.029en
dc.description.obiettivoSpecifico2.3. TTC - Laboratori di chimica e fisica delle rocceen
dc.description.journalTypeJCR Journalen
dc.description.fulltextrestricteden
dc.relation.issn0009-2541en
dc.relation.eissn1872-6836en
dc.contributor.authorMollo, S.en
dc.contributor.authorMisiti, V.en
dc.contributor.authorScarlato, P.en
dc.contributor.authorSoligo, M.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.departmentUniversità Roma Treen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptUniversità di Roma "La Sapienza"-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.deptUniversità “Roma Tre"-
crisitem.author.orcid0000-0002-6151-7789-
crisitem.author.orcid0000-0003-1933-0192-
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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