Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/399
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dc.contributor.authorallAiuppa, A.; Dipartimento Chimica e Fisica della Terra ed applicazioni, Università di Palermo, Palermo, Italyen
dc.contributor.authorallInguaggiato, S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italiaen
dc.contributor.authorallMcGonigle, A. J. S.; Department of Geography, University of Cambridge, Cambridge, UKen
dc.contributor.authorallO'Dwyer, M.; Department of Physics and Astronomy, University of Glasgow, Glasgow, UKen
dc.contributor.authorallOppenheimer, C.; Department of Geography, University of Cambridge, Cambridge, UKen
dc.contributor.authorallPadgett, M. J.; Department of Physics and Astronomy, University of Glasgow, Glasgow, UKen
dc.contributor.authorallRouwet, D.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italiaen
dc.contributor.authorallValenza, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italiaen
dc.date.accessioned2005-09-12T14:03:01Zen
dc.date.available2005-09-12T14:03:01Zen
dc.date.issued2005en
dc.identifier.urihttp://hdl.handle.net/2122/399en
dc.description.abstractWe present here new measurements of sulfur dioxide and hydrogen sulfide emissions from Vulcano, Etna, and Stromboli (Italy), made by direct sampling at vents and by filter pack and ultraviolet spectroscopy in downwind plumes. Measurements at the F0 and FA fumaroles on Vulcano yielded SO2/H2S molar ratios of 0.38 and 1.4, respectively, from which we estimate an H2S flux of 6 to 9 for the summit crater. For Mt. Etna and Stromboli, we found SO2/H2S molar ratios of 20 and 15, respectively, which combined with SO2 flux measurements, suggest H2S emission rates of 50 to 113 and 4 to 8, respectively. We observe that source and plume SO2/H2S ratios at Vulcano are similar, suggesting that hydrogen sulfide is essentially inert on timescales of seconds to minutes. This finding has important implications for estimates of volcanic total sulfur budget at volcanoes since most existing measurements do not account for H2S emission.en
dc.format.extent539 bytesen
dc.format.extent665710 bytesen
dc.format.mimetypetext/htmlen
dc.format.mimetypeapplication/pdfen
dc.language.isoEnglishen
dc.publisher.nameElsevieren
dc.relation.ispartofGeochimica et Cosmochimica Actaen
dc.relation.ispartofseries7/69(2005)en
dc.subjectH2S atmospheric budgeten
dc.subjectvolcanic degassingen
dc.titleH2S fluxes from Mt. Etna, Stromboli, and Vulcano (Italy) and implications for the sulfur budget at volcanoesen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber1861–1871en
dc.identifier.URLhttp://www.sciencedirect.com/en
dc.subject.INGV01. Atmosphere::01.01. Atmosphere::01.01.07. Volcanic effectsen
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.01. Gasesen
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.06. Volcano monitoringen
dc.subject.INGV05. General::05.02. Data dissemination::05.02.01. Geochemical dataen
dc.identifier.doi10.1016/j.gca.2004.09.018en
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dc.description.fulltextpartially_openen
dc.contributor.authorAiuppa, A.en
dc.contributor.authorInguaggiato, S.en
dc.contributor.authorMcGonigle, A. J. S.en
dc.contributor.authorO'Dwyer, M.en
dc.contributor.authorOppenheimer, C.en
dc.contributor.authorPadgett, M. J.en
dc.contributor.authorRouwet, D.en
dc.contributor.authorValenza, M.en
dc.contributor.departmentDipartimento Chimica e Fisica della Terra ed applicazioni, Università di Palermo, Palermo, Italyen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italiaen
dc.contributor.departmentDepartment of Geography, University of Cambridge, Cambridge, UKen
dc.contributor.departmentDepartment of Physics and Astronomy, University of Glasgow, Glasgow, UKen
dc.contributor.departmentDepartment of Physics and Astronomy, University of Glasgow, Glasgow, UKen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italiaen
item.openairetypearticle-
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item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Palermo, Palermo, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Palermo, Palermo, Italia-
crisitem.author.deptDepartment of Geography, University of Cambridge, Downing Place, CB2 3EN Cambridge, UK-
crisitem.author.deptDepartment of Physics and Astronomy, University of Glasgow, Glasgow, UK-
crisitem.author.deptDepartment of Physics and Astronomy, University of Glasgow, Glasgow, UK-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Bologna, Bologna, Italia-
crisitem.author.deptDiSTeM, Universit a degli Studi di Palermo, Palermo, Italy-
crisitem.author.orcid0000-0002-0254-6539-
crisitem.author.orcid0000-0003-3726-9946-
crisitem.author.orcid0000-0003-4506-7260-
crisitem.author.orcid0000-0003-3366-3882-
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.parent01. Atmosphere-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent05. General-
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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