Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/6510
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dc.contributor.authorallDe’ Michieli Vitturi, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Pisa, Pisa, Italiaen
dc.contributor.authorallClarke, A. B.; School of Earth and Space Exploration, Arizona State University, Tempe, Arizona, USA; INGV Sezione di Pisa, Pisa, Italyen
dc.contributor.authorallNeri, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Pisa, Pisa, Italiaen
dc.contributor.authorallVoight, B.; College of Earth and Mineral Sciences, Pennsylvania State University, University Park, Pennsylvania, USAen
dc.date.accessioned2011-01-10T15:00:53Zen
dc.date.available2011-01-10T15:00:53Zen
dc.date.issued2010-07-01en
dc.identifier.urihttp://hdl.handle.net/2122/6510en
dc.description.abstractThe transient dynamics of magma ascent during dome-forming eruptions were investigated and the effects of magma chamber pressure perturbations on eruption rate are illustrated. The numerical model DOMEFLOW, developed by the authors for this work, is applied to the problem. DOMEFLOW is a transient 1.5D isothermal two-phase flow model of magma ascent through an axisymmetric conduit of variable radius, which accounts for gas exsolution, bubble growth, crystallization induced by degassing, permeable gas loss through overlying magma and through conduit walls, as well as viscosity changes due to crystallization and degassing. For runs in which chamber pressure increases, the time required to reach the new steady state (transition time) is a complex function of the pressure perturbation, while for decreasing chamber pressure, transition time is a monotonic function of the magnitude of the pressure perturbation. The transition to the new steady state is mainly controlled by magma compressibility, travel time (time required for one parcel of magma to travel from chamber to surface), and the time over which the pressure perturbation occurs. Results of many runs (> 300) were analyzed using dimensional analysis to reveal a general relationship which predicts the temporal evolution of magma effusion rate for a given sudden increase in chamber pressure; the product of the change in steady-state extrusion rate and the time required to reach the new steady state is linearly proportional to the normalized change in chamber pressure, the volume of the conduit, and the ratio of top and bottom conduit radii, and inversely proportional to the cubic root of volatile fraction. This relationship is used to interpret observed variations in two ongoing dome-building eruptions, the Soufrière Hills volcano, Montserrat, and Merapi volcano, Indonesia.en
dc.language.isoEnglishen
dc.publisher.nameElsevieren
dc.relation.ispartofEarth and Planetary Science Lettersen
dc.relation.ispartofseries3-4/292(2010)en
dc.subjectconduit dynamicsen
dc.subjectconduit geometryen
dc.subjectmagma ascenten
dc.subjecteffusion rateen
dc.subjectcomputational modelen
dc.subjectdome-buildingen
dc.titleTransient effects of magma ascent dynamics along a geometrically variable dome-feeding conduiten
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber541-553en
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.03. Magmasen
dc.subject.INGV05. General::05.01. Computational geophysics::05.01.05. Algorithms and implementationen
dc.identifier.doi10.1016/j.epsl.2010.04.029en
dc.description.obiettivoSpecifico3.6. Fisica del vulcanismoen
dc.description.journalTypeJCR Journalen
dc.description.fulltextreserveden
dc.contributor.authorDe’ Michieli Vitturi, M.en
dc.contributor.authorClarke, A. B.en
dc.contributor.authorNeri, A.en
dc.contributor.authorVoight, B.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Pisa, Pisa, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Pisa, Pisa, Italiaen
dc.contributor.departmentCollege of Earth and Mineral Sciences, Pennsylvania State University, University Park, Pennsylvania, USAen
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 Pisa, Pisa, Italia-
crisitem.author.deptArizona State University, USA-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Pisa, Pisa, Italia-
crisitem.author.deptDepartment of Geosciences, Penn State University, University Park, Pennsylvania, USA-
crisitem.author.orcid0000-0002-6750-9245-
crisitem.author.orcid0000-0002-3536-3624-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent05. General-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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