Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/11671
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dc.date.accessioned2018-04-06T06:59:26Zen
dc.date.available2018-04-06T06:59:26Zen
dc.date.issued2017-05-27en
dc.identifier.urihttp://hdl.handle.net/2122/11671en
dc.description.abstractThere is a growing concern about the mercury (Hg) vented from submarine hydrothermal fluids to the marine surrounding and exchange of dissolved gaseous mercury (DGM) between the sea surface and the atmosphere. A geochemical survey of thermal waters collected from submarine vents at Panarea Island (Aeolian Islands, southern Italy) was carried out in 2015 (15–17th June and 17–18th November), in order to investigate the concentration of Hg species in hydrothermal fluids and the vertical distribution in the overlying water column close to the submarine exhalative area. Specific sampling methods were employed by Scuba divers at five submarine vents located along the main regional tectonic lines. The analysis of the hydrothermal fluids indicates a site-to-site variation, with filtered total mercury (FTHg) concentrations ranging from 1072 to 4711 pM, as a consequence of the gas bubbles partial dissolution. These results are three orders of magnitude higher than the FTHg concentrations found in the overlying seawater column (ranging from 5.3 to 6.3 pM in the mid waters), where the efficient currents and vertical mixing result in more dilution, and potentially rapid transfer of the dissolved gaseous Hg to the atmosphere. Dissolved gaseous mercury (DGM) and gaseous elemental mercury (GEM) were simultaneously measured and combined in a gas-exchange model to calculate the sea-air Hg0 evasional flux. Based on the data of DGM (range: 0.05–0.22 pM) and atmospheric GEM (range: 1.7 ± 0.35–6.4 ± 2.6 ng m−3), we argue that the surface seawater off Panarea is mostly supersaturated in dissolved elemental gaseous mercury compared to the atmosphere, with a sea-air Hg0 net flux ranging from 0.7 to 9.1 ng m−2 h−1 (average: ~4.5 ± 3.5 ng m−2 h−1). Since the empirical gas-exchange model does not include the contribution of Hg0 released as gas bubbles rising from the vents toward sea-surface, the calculated Hg0 evasional flux for this location is most likely larger.en
dc.language.isoEnglishen
dc.relation.ispartofMarine Chemistryen
dc.relation.ispartofseries/194 (2017)en
dc.subjectDissolved gaseous mercuryen
dc.subjectHydrothermal fluidsen
dc.titleHydrochemical mercury distribution and air-sea exchange over the submarine hydrothermal vents off-shore Panarea Island (Aeolian arc, Tyrrhenian Sea)en
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber63-78en
dc.subject.INGVmercury distribution and air-sea exchange over submarine hydrothermal ventsen
dc.identifier.doi10.1016/j.marchem.2017.04.003en
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dc.description.obiettivoSpecifico6A. Geochimica per l'ambienteen
dc.description.journalTypeJCR Journalen
dc.contributor.authorBagnato, E.en
dc.contributor.authorOliveri, E.en
dc.contributor.authorAcquavita, A.en
dc.contributor.authorCovelli, S.en
dc.contributor.authorPetranich, E.en
dc.contributor.authorBarra, M.en
dc.contributor.authorItaliano, Francescoen
dc.contributor.authorParello, F.en
dc.contributor.authorSprovieri, M.en
dc.contributor.departmentDipartimento di Fisica e Geologia, Università degli Studi di Perugiaen
dc.contributor.departmentIstituto per l'Ambiente Marino Costiero, Consiglio Nazionale delle Ricerche, Torretta Granitola (TP)en
dc.contributor.departmentAgenzia Regionale per la Protezione dell'Ambiente del Friuli Venezia Giuliaen
dc.contributor.departmentDipartimento di Matematica e Geoscienze (DMG), Università degli Studi di Trieste,en
dc.contributor.departmentDipartimento di Matematica e Geoscienze (DMG), Università degli Studi di Trieste,en
dc.contributor.departmentIstituto per l'Ambiente Marino Costiero, Consiglio Nazionale delle Ricerche, Napolien
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Palermo, Palermo, Italiaen
dc.contributor.departmentDipartimento di Scienze della Terra e del Mare (DiSTeM), Università degli Studi di Palermoen
dc.contributor.departmentIstituto per l'Ambiente Marino Costiero, Consiglio Nazionale delle Ricerche, Torretta Granitola (TP)en
item.languageiso639-1en-
item.cerifentitytypePublications-
item.openairetypearticle-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
item.grantfulltextrestricted-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.deptCNR - ISMAR-
crisitem.author.deptAgenzia Regionale per la Protezione dell'Ambiente del Friuli Venezia Giulia-
crisitem.author.deptDipartimento di Matematica e Geoscienze (DMG), Università degli Studi di Trieste,-
crisitem.author.deptDipartimento di Matematica e Geoscienze (DMG), Università degli Studi di Trieste,-
crisitem.author.deptCNR, Istituto per l'Ambiente Marino Costiero,(IAMC-CNR)-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Palermo, Palermo, Italia-
crisitem.author.deptUniversità di Palermo, DiSTeM, Italy-
crisitem.author.deptIstituto per l'Ambiente Marino Costiero, Consiglio Nazionale delle Ricerche, Torretta Granitola (TP)-
crisitem.author.orcid0000-0003-2285-0842-
crisitem.author.orcid0000-0002-9483-4481-
crisitem.author.orcid0000-0002-9465-6398-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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