Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/10545
DC FieldValueLanguage
dc.contributor.authorallDominguez, L.en
dc.contributor.authorallPioli, L.en
dc.contributor.authorallBonadonna, C.en
dc.contributor.authorallConnor, C. B.en
dc.contributor.authorallAndronico, D.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.contributor.authorallHarris, A. J. L.en
dc.contributor.authorallRipepe, M.en
dc.date.accessioned2017-03-24T09:30:10Zen
dc.date.available2017-03-24T09:30:10Zen
dc.date.issued2016en
dc.identifier.urihttp://hdl.handle.net/2122/10545en
dc.description.abstractPulsatory eruptions are marked by a sequence of explosions which can be separated by time intervals ranging from a few seconds to several hours. The quantification of the periodicities associated with these eruptions is essential not only for the comprehension of the mechanisms controlling explosivity, but also for classification purposes. We focus on the dynamics of pulsatory activity and quantify unsteadiness based on the distribution of the repose time intervals between single explosive events in relation to magma properties and eruptive styles. A broad range of pulsatory eruption styles are considered, including Strombolian, violent Strombolian and Vulcanian explosions. We find a general relationship between the median of the observed repose times in eruptive sequences and the viscosity of magma given by eta approximate to 100.t(median). This relationship applies to the complete range of magma viscosities considered in our study (10(2) to 10(9) Pas) regardless of the eruption length, eruptive style and associated plume heights, suggesting that viscosity is the main magma property controlling eruption periodicity. Furthermore, the analysis of the explosive sequences in terms of failure time through statistical survival analysis provides further information: dynamics of pulsatory activity can be successfully described in terms of frequency and regularity of the explosions, quantified based on the log-logistic distribution. A linear relationship is identified between the log-logistic parameters, mu and s. This relationship is useful for quantifying differences among eruptive styles from very frequent and regular mafic events (Strombolian activity) to more sporadic and irregular Vulcanian explosions in silicic systems. The time scale controlled by the parameter mu, as a function of the median of the distribution, can be therefore correlated with the viscosity of magmas; while the complexity of the erupting system, including magma rise rate, degassing and fragmentation efficiency, can be also described based on the log-logistic parameter s, which is found to increase from regular mafic systems to highly variable silicic systems. These results suggest that the periodicity of explosions, quantified in terms of the distribution of repose times, can give fundamental information about the system dynamics and change regularly across eruptive styles (i.e., Strombolian to Vulcanian), allowing for direct comparison and quantification of different types of pulsatory activity during these eruptions. (C) 2016 Elsevier B.V. All rights reserved.en
dc.language.isoEnglishen
dc.publisher.nameElsevier Science Limiteden
dc.relation.ispartofEarth and planetary science lettersen
dc.relation.ispartofseries/444(2016)en
dc.subjectexplosions pulsatory activity magma viscosity repose interval source dynamics eruptive styleen
dc.titleQuantifying unsteadiness and dynamics of pulsatory volcanic activityen
dc.typearticleen
dc.description.statusPublisheden
dc.description.pagenumber160-168en
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.07. Instruments and techniquesen
dc.identifier.doi10.1016/j.epsl.2016.03.048en
dc.description.obiettivoSpecifico3V. Dinamiche e scenari eruttivien
dc.description.journalTypeJCR Journalen
dc.description.fulltextrestricteden
dc.relation.issn0012-821Xen
dc.relation.eissn1385-013Xen
dc.contributor.authorDominguez, L.en
dc.contributor.authorPioli, L.en
dc.contributor.authorBonadonna, C.en
dc.contributor.authorConnor, C. B.en
dc.contributor.authorAndronico, D.en
dc.contributor.authorHarris, A. J. L.en
dc.contributor.authorRipepe, M.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, 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 OE, Catania, Italia-
crisitem.author.orcid0000-0002-7093-6555-
crisitem.author.orcid0000-0003-1006-7703-
crisitem.author.orcid0000-0002-2368-2193-
crisitem.author.orcid0000-0002-8333-1547-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
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