Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/6508
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dc.contributor.authorallColò, L.; Università degli Sudi di Firenze, Dipartimento di Scienze della Terra, Firenze, Italyen
dc.contributor.authorallRipepe, M.; Università degli Sudi di Firenze, Dipartimento di Scienze della Terra, Firenze, Italyen
dc.contributor.authorallBaker, D. R.; Earth and Planetary Sciences, McGill University, Montreal, QC, Canadaen
dc.contributor.authorallPolacci, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Pisa, Pisa, Italiaen
dc.date.accessioned2011-01-10T14:56:39Zen
dc.date.available2011-01-10T14:56:39Zen
dc.date.issued2010-04-01en
dc.identifier.urihttp://hdl.handle.net/2122/6508en
dc.description.abstractExplosive activity at Stromboli is explained in terms of dynamics of large gas bubbles that ascend in the magma conduit and burst at the free surface generating acoustic pressure that propagates as infrasonic signals in the atmosphere. The rate and the amplitude of the infrasonic activity is directly linked to the rate and the overpressure of the bursting gas bubbles and thus reflects the rate at which magma column degasses under non-equilibrium pressure conditions. We investigate the link between explosive degassing and magma vesiculation by comparing the rate of infrasonic activity with the bubble size distributions (BSDs) of scoria clasts collected during several days of explosive activity at Stromboli. BSDs of scoria show a characteristic power law distribution, which reflect a gas bubble concentration mainly controlled by a combined process of bubble nucleation and coalescence. The cumulative distribution of the infrasonic pressure follows two power laws, indicating a clear separation between the frequent, but weak, bursting of small gas bubbles (puffing) and the more energetic explosions of large gas slugs. The exponents of power laws derived for puffing and explosive infrasonic activity show strongly correlated (0.96) changes with time indicating that when the puffing rate is high, the number of energetic explosions is also elevated. This correlation suggests that both puffing and explosive activity are driven by the same magma degassing dynamics. In addition, changes of both infrasonic power law exponents are very well correlated (0.92 with puffing and 0.87 with explosions) with variations of the BSD exponents of the scoria clasts, providing evidence of the strong interplay between scoria vesiculation and magma explosivity. Our analysis indicates that variable magma vesiculation regimes recorded in the scoria correlate with the event number and energy of the explosive activity. We propose that monitoring infrasound on active volcanoes may be an alternative way to look at the vesiculation process in open conduit systems.en
dc.language.isoEnglishen
dc.publisher.nameElsevieren
dc.relation.ispartofEarth and Planetary Science Lettersen
dc.relation.ispartofseries3-4/292(2010)en
dc.subjectStrombolian activityen
dc.subjectmagma vesiculationen
dc.subjectinfrasounden
dc.subjectconduit dynamicsen
dc.subjectexplosive volcanismen
dc.subjectbubble size distributionen
dc.titleMagma vesiculation and infrasonic activity at Stromboli open conduit volcanoen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber274-280en
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.03. Magmasen
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.05. Volcanic rocksen
dc.identifier.doi10.1016/j.epsl.2010.01.018en
dc.description.obiettivoSpecifico1.5. TTC - Sorveglianza dell'attività eruttiva dei vulcanien
dc.description.journalTypeJCR Journalen
dc.description.fulltextreserveden
dc.contributor.authorColò, L.en
dc.contributor.authorRipepe, M.en
dc.contributor.authorBaker, D. R.en
dc.contributor.authorPolacci, M.en
dc.contributor.departmentUniversità degli Sudi di Firenze, Dipartimento di Scienze della Terra, Firenze, Italyen
dc.contributor.departmentUniversità degli Sudi di Firenze, Dipartimento di Scienze della Terra, Firenze, Italyen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, 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.deptDipartimento di Scienze della Terra, Università degli Studi di Firenze, 50121 Florence, Italy-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Pisa, Pisa, Italia-
crisitem.author.orcid0000-0002-6543-3283-
crisitem.author.orcid0000-0003-3318-8700-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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