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Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/9830
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dc.contributor.authorallAiuppa, A.; DiSTeM, Università di Palermoen
dc.contributor.authorallTamburello, G.; DiSTeM, Università di Palermoen
dc.contributor.authorallDi Napoli, R.; DiSTeM, Università di Palermoen
dc.contributor.authorallCardellini, C.; Dipartimento di Scienze della Terra, Università di Perugiaen
dc.contributor.authorallChiodini, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
dc.contributor.authorallGiudice, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italiaen
dc.contributor.authorallGrassa, F.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italiaen
dc.contributor.authorallPedone, M.; DiSTeM, Università di Palermoen
dc.date.accessioned2015-06-09T10:40:13Zen
dc.date.available2015-06-09T10:40:13Zen
dc.date.issued2013-10-02en
dc.identifier.urihttp://hdl.handle.net/2122/9830en
dc.description.abstractThe fumarolic gas output has not been quantified for any of the currently deforming calderas worldwide, due to the lack of suitable gas flux sensing techniques. In view of resumption of ground uplift (since 2005) and the associated variations in gas chemistry, Campi Flegrei, in southern Italy, is one of the restless calderas where gas flux observations are especially necessary. Here we report the first ever obtained estimate of the Campi Flegrei fumarolic gas output, based on a set of MultiGAS surveys (performed in 2012 and 2013) with an ad-hoc-designed measurement setup. We estimate that the current Campi Flegrei fumarolic sulphur (S) flux is low, on the order of 1.5–2.2 tons/day, suggesting substantial scrubbing of magmatic S by the hydrothermal system. However, the fumarolic carbon dioxide (CO2) output is ∼460±160 tons/day (mean±SD), which is surprisingly high for a dormant volcano in the hydrothermal stage of activity, and results in a combined (fumaroles + soil) CO2 output of ∼1560 tons/day. Assuming magma to be the predominant source, we propose that the current CO2 output can be supplied by either (i) a large (0.6–4.6 km3), deeply stored (>7 km) magmatic source with low CO2 contents (0.05–0.1 wt%) or (ii) by a small to medium-sized (∼0.01–0.1 km3) but CO2-rich (2 wt%) magma, possibly stored at pressures of ∼100 to 120 MPa. Independent geophysical evidence (e.g., inferred from geodetic and gravity data) is needed to distinguish between these two possibilities.en
dc.language.isoEnglishen
dc.publisher.nameAmerican Geophysical Unionen
dc.relation.ispartofGeochemistry, Geophysics, Geosystemsen
dc.relation.ispartofseries/14(2013)en
dc.subjectCampi Flegreien
dc.subjectcalderasen
dc.subjectgas outputen
dc.titleFirst observations of the fumarolic gas output from a restless caldera: implications for the current period of unrest (2005-2013) at Campi Flegreien
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber4153–4169en
dc.identifier.URLhttp://onlinelibrary.wiley.com/doi/10.1002/ggge.20261/abstracten
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.01. Gasesen
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.03. Magmasen
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.06. Volcano monitoringen
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.07. Instruments and techniquesen
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.08. Volcanic risken
dc.identifier.doi10.1002/ggge.20261en
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dc.description.obiettivoSpecifico2V. Dinamiche di unrest e scenari pre-eruttivien
dc.description.journalTypeJCR Journalen
dc.description.fulltextrestricteden
dc.relation.eissn1525-2027en
dc.contributor.authorAiuppa, A.en
dc.contributor.authorTamburello, G.en
dc.contributor.authorDi Napoli, R.en
dc.contributor.authorCardellini, C.en
dc.contributor.authorChiodini, G.en
dc.contributor.authorGiudice, G.en
dc.contributor.authorGrassa, F.en
dc.contributor.authorPedone, M.en
dc.contributor.departmentDiSTeM, Università di Palermoen
dc.contributor.departmentDiSTeM, Università di Palermoen
dc.contributor.departmentDiSTeM, Università di Palermoen
dc.contributor.departmentDipartimento di Scienze della Terra, Università di Perugiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italiaen
dc.contributor.departmentDiSTeM, Università di Palermoen
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crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Palermo, Palermo, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Bologna, Bologna, Italia-
crisitem.author.deptUniversità di Palermo, DiSTeM, Italy-
crisitem.author.deptDipartimento di fisica e Geologia di Perugia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Bologna, Bologna, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia-
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.orcid0000-0002-0254-6539-
crisitem.author.orcid0000-0001-7770-5226-
crisitem.author.orcid0000-0002-6175-3124-
crisitem.author.orcid0000-0002-0628-8055-
crisitem.author.orcid0000-0002-9410-4139-
crisitem.author.orcid0000-0001-5043-792X-
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.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.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
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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