Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/11530
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dc.date.accessioned2018-03-26T14:08:59Zen
dc.date.available2018-03-26T14:08:59Zen
dc.date.issued2017en
dc.identifier.urihttp://hdl.handle.net/2122/11530en
dc.description.abstractGeological evidences of volcanicconduitwidening arecommonin mostpyroclastic deposits (e.g. presence oflith- ic fragments from different depths), suggesting a continuous modi fi cation of the conduit geometry during volca- nic eruptions. However, the controlling factors of the mechanisms driving conduit enlargement (e.g. erosion, local collapse) are still partially unclear, as well as the in fl uence of conduit geometry on the eruptive dynamics. Although numerical models have been systematically employed to study volcanic conduits, their mechanical sta- bility and the eruptive dynamics related to non-cylindrical conduits have been poorly addressed. We present here a 1D steady-state model which includes the main processes experimented by ascending magmas (i.e. crystallization, rheological changes, fragmentation, drag forces, outgassing and degassing), and the application of two mechanical stability criteria (Mohr – Coulomb and Mogi – Coulomb), in order to study the collapse conditions of volcanic conduits during a representative explosive rhyolitic eruption. It emerges that me- chanical stability of volcanic conduits is mainly controlled by its radial dimension, and a minimum radius for reaching stable conditions can be computed, as a function of water content and inlet overpressure. Additionally, for a set of input parameters thought typical of explosive rhyolitic volcanism, we estimated a minimum magma fl ux for developing a mechanically stable conduit (~7 ∙ 10 7 − 3 ∙ 10 8 kg/s). Results are consistent with the unsteady character usually observed in sub-Plinian eruptions, opposite to mainly stationary Plinian eruptions, commonly characterized by higher magma discharge rates. We suggest that cylindrical conduits represent a mechanically stable con fi guration only for large radii. Because the instability conditions are not uniform along the conduit, the widening processes probably lead to conduit geometries with depth-varying width. Consequently, as our model is able to consider volcanic conduits with depth-dependent radius, two plausible and previously untested geometries have been studied, evidencing major and complex modi fi cations in some eruptive parameters (par- ticularly, exit pressure and mass discharge rate), and suggesting that the geometry acquired by the conduit as it is widened influences the eruptive dynamicsen
dc.language.isoEnglishen
dc.relation.ispartofJournal of Volcanology and Geothermal Researchen
dc.relation.ispartofseries/339 (2017)en
dc.titleStability of volcanic conduits during explosive eruptionsen
dc.typearticleen
dc.description.statusPublisheden
dc.description.pagenumber52-62en
dc.identifier.doi10.1016/j.jvolgeores.2017.05.003en
dc.description.obiettivoSpecifico2V. Struttura e sistema di alimentazione dei vulcanien
dc.description.obiettivoSpecifico5V. Dinamica dei processi eruttivi e post-eruttivien
dc.description.journalTypeJCR Journalen
dc.contributor.authorAravena, Álvaroen
dc.contributor.authorde' Michieli Vitturi, Mattiaen
dc.contributor.authorCioni, Raffaelloen
dc.contributor.authorNeri, Augustoen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Pisa, Pisa, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Pisa, Pisa, 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 Pisa, Pisa, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Pisa, Pisa, Italia-
crisitem.author.orcid0000-0003-3494-191X-
crisitem.author.orcid0000-0002-6750-9245-
crisitem.author.orcid0000-0002-2526-9095-
crisitem.author.orcid0000-0002-3536-3624-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.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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