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Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/2620
DC FieldValueLanguage
dc.contributor.authorallRizi, V.; INGen
dc.contributor.authorallD'Altorio, A.; Dipartimento di Fisica, Università di L'Aquilaen
dc.contributor.authorallMasci, F.; INGen
dc.contributor.authorallPitari, G.; Dipartimento di Fisica, Università di L'Aquilaen
dc.contributor.authorallVisconti, G.; Dipartimento di Fisica, Università di L'Aquilaen
dc.date.accessioned2007-10-12T09:56:49Zen
dc.date.available2007-10-12T09:56:49Zen
dc.date.issued1993-01en
dc.identifier.urihttp://hdl.handle.net/2122/2620en
dc.description.abstractA simple method for calculating the surface area density of aerosol particles starting from lidar backscattering ratios is described in this work. Surface density is the key parameter to be included in model assessments of the ozone perturbation following the eruption of Mt. Pinatubo. As an example we have used a photochemical 2D model to calculate the sensitivity of O3 depletion to the surface density of volcanic aerosols. Monthly averaged profiles of ozone concentration measured with a DIAL system for ten months after the eruption are also shown.en
dc.description.sponsorshipINGen
dc.language.isoEnglishen
dc.publisher.nameSIFen
dc.relation.ispartofIl Nuovo Cimentoen
dc.relation.ispartofseries16 C, 1, 1993en
dc.subjectvolcanic aerosolen
dc.subjectozoneen
dc.titleGROUND-BASED MONITORING OF PINATUBO AEROSOLS AND OZONE AT L'AQUILA, ITALY: II. CALCULATION OF AEROSOL SURFACE DENSITY FOR PHOTOCHEMICAL MODELSen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber97-1001en
dc.subject.INGV01. Atmosphere::01.01. Atmosphere::01.01.99. General or miscellaneousen
dc.description.obiettivoSpecifico1.8. Osservazioni di geofisica ambientaleen
dc.description.journalTypeJCR Journalen
dc.description.fulltextopenen
dc.contributor.authorRizi, V.en
dc.contributor.authorD'Altorio, A.en
dc.contributor.authorMasci, F.en
dc.contributor.authorPitari, G.en
dc.contributor.authorVisconti, G.en
dc.contributor.departmentINGen
dc.contributor.departmentDipartimento di Fisica, Università di L'Aquilaen
dc.contributor.departmentINGen
dc.contributor.departmentDipartimento di Fisica, Università di L'Aquilaen
dc.contributor.departmentDipartimento di Fisica, Università di L'Aquilaen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptING-
crisitem.author.deptDipartimento di Fisica, Università di L'Aquila-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptDipartimento di Fisica, Università di L'Aquila-
crisitem.author.deptDipartimeto di Fisica, Università di L'Aquila, Italy-
crisitem.author.orcid0000-0003-2314-3023-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent01. Atmosphere-
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