Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/8488
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dc.contributor.authorallScollo, S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.contributor.authorallKahn, R. A.; Atmospheres Laboratory, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA.en
dc.contributor.authorallNelson, D. L.; Raytheon Company, Pasadena, California, USA.en
dc.contributor.authorallColtelli, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.contributor.authorallDiner, D. J.; Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA.en
dc.contributor.authorallGaray, M. J.; Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA.en
dc.contributor.authorallRealmuto, V. J.; Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA.en
dc.date.accessioned2013-01-23T13:05:47Zen
dc.date.available2013-01-23T13:05:47Zen
dc.date.issued2012en
dc.identifier.urihttp://hdl.handle.net/2122/8488en
dc.description.abstractIn the last twelve years, Mt. Etna, located in eastern Sicily, has produced a great number of explosive eruptions. Volcanic plumes have risen to several km above sea level and created problems for aviation and the communities living near the volcano. A reduction of hazards may be accomplished using remote sensing techniques to evaluate important features of volcanic plumes. Since 2000, the Multiangle Imaging SpectroRadiometer (MISR) on board NASA’s Terra spacecraft has been extensively used to study aerosol dispersal and to extract the three-dimensional structure of plumes coming from anthropogenic or natural sources, including volcanoes. In the present work, MISR data from several explosive events occurring at Etna are analyzed using a program named MINX (MISR INteractive eXplorer). MINX uses stereo matching techniques to evaluate the height of the volcanic aerosol with a precision of a few hundred meters, and extracts aerosol properties from the MISR Standard products. We analyzed twenty volcanic plumes produced during the 2000, 2001, 2002–03, 2006 and 2008 Etna eruptions, finding that volcanic aerosol dispersal and column height obtained by this analysis is in good agreement with ground-based observations. MISR aerosol type retrievals: (1) clearly distinguish volcanic plumes that are sulphate and/or water vapor dominated from ash-dominated ones; (2) detect even low concentrations of volcanic ash in the atmosphere; (3) demonstrate that sulphate and/or water vapor dominated plumes consist of smaller-sized particles compared to ash plumes. This work highlights the potential of MISR to detect important volcanic plume characteristics that can be used to constrain the eruption source parameters in volcanic ash dispersion models. Further, the possibility of discriminating sulphate and/or water vapor dominated plumes from ash-dominated ones is important to better understand the atmospheric impact of these plumesen
dc.language.isoEnglishen
dc.relation.ispartofJOURNAL OF GEOPHYSICAL RESEARCHen
dc.relation.ispartofseries/117 (2012)en
dc.subjectvolcanic ash plumeen
dc.subjectMISRen
dc.titleMISR observations of Etna volcanic plumesen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumberD06210en
dc.subject.INGV01. Atmosphere::01.01. Atmosphere::01.01.99. General or miscellaneousen
dc.identifier.doi10.1029/2011JD016625,en
dc.description.obiettivoSpecifico1.5. TTC - Sorveglianza dell'attività eruttiva dei vulcanien
dc.description.journalTypeJCR Journalen
dc.description.fulltextrestricteden
dc.contributor.authorScollo, S.en
dc.contributor.authorKahn, R. A.en
dc.contributor.authorNelson, D. L.en
dc.contributor.authorColtelli, M.en
dc.contributor.authorDiner, D. J.en
dc.contributor.authorGaray, M. J.en
dc.contributor.authorRealmuto, V. J.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italiaen
dc.contributor.departmentAtmospheres Laboratory, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA.en
dc.contributor.departmentRaytheon Company, Pasadena, California, USA.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italiaen
dc.contributor.departmentJet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA.en
dc.contributor.departmentJet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA.en
dc.contributor.departmentJet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA.en
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.deptAtmospheres Laboratory, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA.-
crisitem.author.deptRaytheon Company, Pasadena, California, USA.-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia-
crisitem.author.deptJet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA.-
crisitem.author.deptJet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA.-
crisitem.author.deptJet Propulsion Laboratory, California Institute of Technology.-
crisitem.author.orcid0000-0001-8704-8629-
crisitem.author.orcid0000-0001-7868-3946-
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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