Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/3761
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dc.contributor.authorallColtelli, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.contributor.authorallMiraglia, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.contributor.authorallScollo, S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.date.accessioned2008-04-14T09:20:25Zen
dc.date.available2008-04-14T09:20:25Zen
dc.date.issued2008-03-27en
dc.identifier.urihttp://hdl.handle.net/2122/3761en
dc.description.abstractAbstract In this paper, we present a complete morphological characterization of the ash particles erupted on 18 December 2002 from Etna volcano, Italy. The work is based on the acquisition and processing of bidimensional digital images carried out by scanning electron microscopy (SEM) to obtain shape parameters by image analysis. We measure aspect ratio (AR), form factor (FF), compactness (CC), and rectangularity (RT) of 2065 ash particles with size between 0.026 and 1.122 mm. We evaluate the variation of these parameters as a function of the grainsize. Ash particles with a diameter of <0.125 mm vary from mostly equant to very equant, ash particles between 0.125 and 0.250 mm have an intermediate shape, and particles with diameters >0.250 mm are subelongate. We find that, on average, particles with a diameter of <0.250 mm are subrounded, particles between 0.250 and 0.50 mm are subangular, and particles >0.50 mm are angular. Using this morphological analysis and an empirical relation between the drag coefficient (CD) and Reynolds number (Re) of Wilson and Huang (Earth Planet Sci Lett 44:311–324, 1979), we calculate the terminal settling velocities (VWH). The comparisons between these velocities and those calculated with the formula of Kunii and Levenspiel (Fluidization engineering. Wiley, New York, pp 97, 1969) (VKL), which considers ash particles as spheres, show that VKL are in average 1.28 greater than VWH. Hence, we quantify the systematic error on the spatial distribution of the mass computed around the volcano carried out by tephra dispersal models when the particles are assumed to be spherical.en
dc.description.sponsorshipThis research was supported by an INGV-GNV fellowship and then by the FIRB Italian project “Sviluppo Nuove Tecnologie per la Protezione e Difesa del Territorio dai Rischi Naturali” funded by Italian Minister of University and Research (S. Scollo)en
dc.language.isoEnglishen
dc.publisher.namespringeren
dc.relation.ispartofBullettin of Volcanologyen
dc.relation.ispartofseries9/70 (2008)en
dc.subjectshape parametersen
dc.subjectterminal settling velocityen
dc.titleCharacterization of shape and terminal velocity of tephra particles erupted during the 2002 eruption of Etna volcano, Italyen
dc.typearticleen
dc.description.statusPublisheden
dc.description.pagenumber1103-1112en
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.99. General or miscellaneousen
dc.identifier.doi10.1007/s00445-007-0192-8en
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In:Shimozuru D, Yokoyama I (eds) Arc volcanism, physics and tectonics. Terra Scientific Publishing Company (TERRAPUB), Tokyo, pp 95–113 Swamee PK, Ojha CSP (1991) Drag coefficient and fall velocity of non-spherical particles. J Hydraul Eng 117:660–667 Taddeucci J, Pompilio M, Scarlato P (2002) Monitoring the explosive activity of the July–August 2001 eruption of M. Etna (Italy) by ash characterization. Geophys Res Lett 29, Art. No. 1230. DOI 10.1029/2001GL014372 Turton R, Clark NN (1987) An explicit relationship to predict spherical particle terminal velocity. Powder Technol 53:127– 129 Walker GPL (1971) Grain-size characteristics of pyroclastic deposits. J Geol 79:696–714 Wilson L, Huang TC (1979) The influence of shape on the atmospheric settling velocity of volcanic ash particles. Earth Planet Sci Lett 44:311–324en
dc.description.obiettivoSpecifico3.6. Fisica del vulcanismoen
dc.description.journalTypeJCR Journalen
dc.description.fulltextreserveden
dc.contributor.authorColtelli, M.en
dc.contributor.authorMiraglia, L.en
dc.contributor.authorScollo, S.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, 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.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia-
crisitem.author.orcid0000-0001-7868-3946-
crisitem.author.orcid0000-0001-9383-7683-
crisitem.author.orcid0000-0001-8704-8629-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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