Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/8490
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dc.contributor.authorallScollo, S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.contributor.authorallBoselli, A.; CNISM and IMAA-CNR, C.da S. Loja, 85050 Tito Scalo, Potenza, Italyen
dc.contributor.authorallColtelli, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.contributor.authorallLeto, G.; Osservatorio Astrofisico di Catania, INAF,en
dc.contributor.authorallPisani, G.; CNISM and Dipartimento di Scienze Fisicheen
dc.contributor.authorallSpinelli, N.; CNISM and Dipartimento di Scienze Fisicheen
dc.contributor.authorallWang, X.; CNISM and CNR-SPIN, Dipartimento di Scienze Fisicheen
dc.date.accessioned2013-01-23T13:12:22Zen
dc.date.available2013-01-23T13:12:22Zen
dc.date.issued2012-09-24en
dc.identifier.urihttp://hdl.handle.net/2122/8490en
dc.description.abstractIn this paper, we use data obtained from LiDAR measurements during an ash emission event on 15 November 2010 at Mt. Etna, in Italy, in order to evaluate the spatial distribution of volcanic ash in the atmosphere. A scanning LiDAR system, located at 7 km distance from the summit craters, was directed toward the volcanic vents and moved in azimuth and elevation to analyse different volcanic plume sections. During the measurements, ash emission from the North East Crater and high degassing from the Bocca Nuova Crater were clearly visible. Fromour analysis we were able to: (1) evaluate the region affected by the volcanic plume presence; (2) distinguish volcanic plumes containing spherical aerosols from those having non-spherical ones; and (3) estimate the frequency of volcanic ash emissions. Moreover, the spatial distribution of ash mass concentration was evaluated with an uncertainty of about 50 %.We found that, even during ash emission episodes characterised by low intensity like the 15 November 2010 event, the region in proximity of the summit craters should be avoided by air traffic operations, the ash concentration being greater than 4×10−3g/m3. The use of a scanning permanent LiDAR station may usefully monitor the volcanic activity and help to drastically reduce the risks to aviation operations during the frequent Etna eruptions.en
dc.language.isoEnglishen
dc.publisher.nameSpringer Berlin Heidelbergen
dc.relation.ispartofBulletin of volcanologyen
dc.relation.ispartofseries10/74 (2012)en
dc.subjectlidaren
dc.subjectvolcanic ashen
dc.titleMonitoring Etna volcanic plumes using a scanning LiDARen
dc.typearticleen
dc.description.statusPublisheden
dc.description.pagenumber2383-2395en
dc.subject.INGV01. Atmosphere::01.01. Atmosphere::01.01.08. Instruments and techniquesen
dc.identifier.doi10.1007/s00445-012-0669-yen
dc.description.obiettivoSpecifico3.6. Fisica del vulcanismoen
dc.description.journalTypeJCR Journalen
dc.description.fulltextrestricteden
dc.relation.issn0258-8900en
dc.relation.eissn1432-0819en
dc.contributor.authorScollo, S.en
dc.contributor.authorBoselli, A.en
dc.contributor.authorColtelli, M.en
dc.contributor.authorLeto, G.en
dc.contributor.authorPisani, G.en
dc.contributor.authorSpinelli, N.en
dc.contributor.authorWang, X.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italiaen
dc.contributor.departmentCNISM and IMAA-CNR, C.da S. Loja, 85050 Tito Scalo, Potenza, Italyen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italiaen
dc.contributor.departmentOsservatorio Astrofisico di Catania, INAF,en
dc.contributor.departmentCNISM and Dipartimento di Scienze Fisicheen
dc.contributor.departmentCNISM and Dipartimento di Scienze Fisicheen
dc.contributor.departmentCNISM and CNR-SPIN, Dipartimento di Scienze Fisicheen
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.deptCNISM and IMAA-CNR-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia-
crisitem.author.deptOsservatorio Astrofisico di Catania, INAF,-
crisitem.author.deptCNISM and Dipartimento di Fisica, Università di Napoli “Federico II”, Naples, Italy,-
crisitem.author.deptDipartimento di Fisica, Università di Napoli “Federico II”, Napoli-
crisitem.author.orcid0000-0001-8704-8629-
crisitem.author.orcid0000-0002-4996-7648-
crisitem.author.orcid0000-0001-7868-3946-
crisitem.author.orcid0000-0002-0040-5011-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent01. Atmosphere-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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