Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/5858
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dc.contributor.authorallCimarelli, C.; Uniroma 3en
dc.contributor.authorallDi Traglia, F.; Unipisaen
dc.contributor.authorallTaddeucci, J.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.date.accessioned2010-01-25T11:20:06Zen
dc.date.available2010-01-25T11:20:06Zen
dc.date.issued2010-
dc.identifier.urihttp://hdl.handle.net/2122/5858en
dc.description.abstractPyroclast textures document volcanic conduit processes and may be key to hazard forecasting. Here we show that the relative abundance of mingled, variably crystallized domains in pyroclasts from scoria cone eruptions provide a record of magma ascent velocity and can be used to predict the onset of violent Strombolian activity. Scoria clasts from the Croscat Complex Scoria Cone (Spain) ubiquitously show m- to cm-sized, microlite-rich domains (MRD) intermingled with volumetrically-dominant, microlite-poor ones (MPD). Glass and bulk composition show that MRDs formed by microlite crystallization of MPDs, the former residing longer in a relatively cooler, degassed zone lining the conduit walls, the latter traveling faster in the central, hotter streamline. MPD and MRD magmas intermingled along the interface between the two velocity zones. The proportion of MPD and MRD in different tephra layers reflects the extent of the fast- and slow-flowing zones, thus reflecting the ascent velocity profile of magma during the different phases. At Croscat, the MPD/MRD volume ratio increased rapidly during the early Strombolian activity, peaked around the Strombolian to violent Strombolian shift, and then decreased smoothly irrespective of shifts in eruptive style. We suggest that magma ascent velocity escalated during the Strombolian phase due to the buoyant push of the underlying, volatile-rich magma that was about to drive the following violent Strombolian activity. Monitoring the MPD/MRD ratio of tephra during ongoing scoria cone eruptions may reveal changes in magma flow conditions and could forecast the onset of hazardous violent Strombolian activity.en
dc.language.isoEnglishen_US
dc.publisher.nameGeological Society of Americaen_US
dc.relation.ispartofGeologyen_US
dc.relation.ispartofseries5/38 (2010)en_US
dc.subjectbasalticen
dc.subjectviolent strombolianen
dc.titleBasaltic scoria textures from a zoned conduit as precursors to violent Strombolian activityen_US
dc.typearticleen
dc.description.statusPublisheden_US
dc.type.QualityControlPeer-revieweden_US
dc.description.pagenumber439–442en_US
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.06. Volcano monitoringen
dc.identifier.doi10.1130/G30720.1en_US
dc.description.obiettivoSpecifico2V. Struttura e sistema di alimentazione dei vulcanien_US
dc.description.journalTypeJCR Journalen_US
dc.description.fulltextopenen
dc.contributor.authorCimarelli, C.-
dc.contributor.authorDi Traglia, F.-
dc.contributor.authorTaddeucci, J.-
dc.contributor.departmentUniroma 3en_US
dc.contributor.departmentUnipisaen_US
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen_US
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OV, Napoli, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.orcid0000-0002-5707-5930-
crisitem.author.orcid0000-0001-5869-0743-
crisitem.author.orcid0000-0002-0516-3699-
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-
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