Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/6478
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dc.contributor.authorallDel Gaudio, P.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallMollo, S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallVentura, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallIezzi, G.; Università G.D'Annunzio, Chieti/Pescara, Italyen
dc.contributor.authorallTaddeucci, J.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallCavallo, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.date.accessioned2010-12-30T09:24:13Zen
dc.date.available2010-12-30T09:24:13Zen
dc.date.issued2010en
dc.identifier.urihttp://hdl.handle.net/2122/6478en
dc.description.abstractTwo sets of cooling experiments were run at 500 MPa conditions for one anhydrous and one hydrous (H2O=1.3 wt.%) starting basaltic melts: a) five cooling rates (15, 9.4, 3, 2.1, and 0.5 °C/min) between 1250 and 1000 °C, and b) a 0.5 °C/min cooling rate from 1250 to 1191, 1167, 1100, 1090, 1075, 1050, 1025 and 1000 °C final temperatures. Cooling rate plays a major role in the differentiation of run products. At the lower cooling rate, glasses of tephri-phonolitic and trachy-andesitic composition have been detected. At comparable cooling rate, the dry glasses show a larger compositional variability and degree of differentiation than the hydrous products. The amount of crystallizing solid phases is always larger in the dry products. It is strongly controlled by both cooling rate and water content and massive crystallization occurs only at lower cooling rates. At a constant cooling rate, massive crystallization is observed at lower temperatures. Clinopyroxene, plagioclase and oxide occur in the anhydrous products, whereas plagioclase crystallization is suppressed in the hydrous ones. The lack of plagioclase results from the faster crystallization kinetics for Feand Mg-bearing phases than for tectosilicates. Textural coarsening occurs at high cooling rate and, for a constant cooling rate, at higher temperatures. The textural and compositional variability observed at the margin of dikes may not mirror flow differentiation processes but could be due to cooling rate variations. Early homogeneous magma batches subjected to cooling rate-induced differentiation may also produce heterogeneous rocks similar to that originated by magma mingling. Cooling rate-related differentiation influences the physical properties (viscosity and density) of magmas. Dry or H2O-poor magmas resulting from low cooling rate differentiation are not allowed to rise within dikes. Viscosity variations induced by cooling rate may be responsible for flow localization within conduits. The effects of cooling rate should be incorporated in fluid-mechanical models of magma ascent.en
dc.language.isoEnglishen
dc.relation.ispartofChemical Geologyen
dc.relation.ispartofseries/270 (2010)en
dc.subjectcooling rateen
dc.subjectbasalten
dc.subjectdikeen
dc.subjectdifferentiationen
dc.subjectstorageen
dc.subjecttransporten
dc.titleCooling rate-induced differentiation in anhydrous and hydrous basalts at 500 MPa: Implications for the storage and transport of magmas in dikesen
dc.typearticleen
dc.description.statusPublisheden
dc.description.pagenumber164-178en
dc.subject.INGV04. Solid Earth::04.04. Geology::04.04.05. Mineralogy and petrologyen
dc.identifier.doi10.1016/j.chemgeo.2009.11.014en
dc.description.obiettivoSpecifico2.3. TTC - Laboratori di chimica e fisica delle rocceen
dc.description.journalTypeJCR Journalen
dc.description.fulltextreserveden
dc.contributor.authorDel Gaudio, P.en
dc.contributor.authorMollo, S.en
dc.contributor.authorVentura, G.en
dc.contributor.authorIezzi, G.en
dc.contributor.authorTaddeucci, J.en
dc.contributor.authorCavallo, A.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 G.D'Annunzio, Chieti/Pescara, Italyen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, 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 ONT, Roma, Italia-
crisitem.author.deptUniversità di Roma "La Sapienza"-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.deptUniversità degli studi G. D'annunzio, Chieti Pescara, Italy-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.orcid0000-0002-0977-1237-
crisitem.author.orcid0000-0001-9388-9985-
crisitem.author.orcid0000-0002-0516-3699-
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-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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