Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/9583
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dc.contributor.authorallBlythe, L. S.en
dc.contributor.authorallDeegan, F. M.; Department of Geological Sciences Stockolm University Swedenen
dc.contributor.authorallFreda, C.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallJolis, E. M.; CEMPEG, Uppsala University, Swedenen
dc.contributor.authorallMasotta, M.; Bahyerisches Geoinstitut Bahyretuh Germanyen
dc.contributor.authorallMisiti, V.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallTaddeucci, J.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallTroll, V. R.; CEMPEG, Uppsala University, Swedenen
dc.date.accessioned2015-04-29T09:52:34Zen
dc.date.available2015-04-29T09:52:34Zen
dc.date.issued2015-04-17en
dc.identifier.urihttp://hdl.handle.net/2122/9583en
dc.description.abstractWe conducted quantitative textural analysis of vesicles in high temperature and pressure carbonate assimilation experiments (1200 °C, 0.5 GPa) to investigate CO2 generation and subsequent bubble migration from carbonate into magma. We employed Mt. Merapi (Indonesia) and Mt. Vesuvius (Italy) compositions as magmatic starting materials and present three experimental series using (1) a dry basaltic-andesite, (2) a hydrous basaltic-andesite (2 wt% H2O), and (3) a hydrous shoshonite (2 wt% H2O). The duration of the experiments was varied from 0 to 300 s, and carbonate assimilation produced a CO2-rich fluid and CaO-enriched melts in all cases. The rate of carbonate assimilation, however, changed as a function of melt viscosity, which affected the 2D vesicle number, vesicle volume, and vesicle size distribution within each experiment. Relatively low-viscosity melts (i.e. Vesuvius experiments) facilitated efficient removal of bubbles from the reaction site. This allowed carbonate assimilation to continue unhindered and large volumes of CO2 to beliberated, a scenario thought to fuel sustained CO2-driven eruptions at the surface. Conversely, at higher viscosity (i.e. Merapi experiments), bubble migration became progressively inhibited and bubble concentration at the reaction site caused localised volatile over-pressure that can eventually trigger short-lived explosive outbursts. Melt viscosity therefore exerts a fundamental control on carbonate assimilation rates and, by consequence, the style of CO2-fuelled eruptions.en
dc.language.isoEnglishen
dc.publisher.nameSpringer Verlag Germanyen
dc.relation.ispartofContributions to Mineralogy and Petrologyen
dc.relation.ispartofseries/169 (2015)en
dc.subjectCO2en
dc.subjectcarbonate assimilationen
dc.subjectmelt viscosityen
dc.subjectbubble size distributionen
dc.subjecterutpion styleen
dc.titleCO2 bubble generation and migration during magma-carbonate interactionen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber42en
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.02. Experimental volcanismen
dc.identifier.doi10.1007/s00410-015-1137-4en
dc.description.obiettivoSpecifico3V. Dinamiche e scenari eruttivien
dc.description.journalTypeJCR Journalen
dc.description.fulltextopenen
dc.relation.issn0010-7999en
dc.relation.eissn1432-0967en
dc.contributor.authorBlythe, L. S.en
dc.contributor.authorDeegan, F. M.en
dc.contributor.authorFreda, C.en
dc.contributor.authorJolis, E. M.en
dc.contributor.authorMasotta, M.en
dc.contributor.authorMisiti, V.en
dc.contributor.authorTaddeucci, J.en
dc.contributor.authorTroll, V. R.en
dc.contributor.departmentDepartment of Geological Sciences Stockolm University Swedenen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.departmentCEMPEG, Uppsala University, Swedenen
dc.contributor.departmentBahyerisches Geoinstitut Bahyretuh Germanyen
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.departmentCEMPEG, Uppsala University, Swedenen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptDepartment of Earth Sciences, CEMPEG, Uppsala University,-
crisitem.author.deptDepartment of Geosciences, Swedish Museum of Natural History-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.deptDipartimento di Scienze della Terra, Sapienza—Universita` di Roma,-
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.deptUppsala University-
crisitem.author.orcid0000-0002-9065-9225-
crisitem.author.orcid0000-0002-2320-8096-
crisitem.author.orcid0000-0003-1804-0847-
crisitem.author.orcid0000-0002-6151-7789-
crisitem.author.orcid0000-0002-0516-3699-
crisitem.author.orcid0000-0003-1891-3396-
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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