Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/8933
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dc.contributor.authorallMather, T.; Univ Oxforden
dc.contributor.authorallWitt, M.; Univ Oxforden
dc.contributor.authorallPyle, D.; Univ Oxforden
dc.contributor.authorallQuayle, B.; Univ Oxforden
dc.contributor.authorallAiuppa, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italiaen
dc.contributor.authorallBagnato, E.; Univ Palermoen
dc.contributor.authorallMartin, R.; Univ Cambridgeen
dc.contributor.authorallSims, K.; University of Wyomingen
dc.contributor.authorallEdmonds, M.; Univ Cambridgeen
dc.contributor.authorallSutton, J.; U.S. Geological Survey,en
dc.contributor.authorallIlyinskaya, E.en
dc.date.accessioned2014-02-17T13:24:10Zen
dc.date.available2014-02-17T13:24:10Zen
dc.date.issued2012-04-15en
dc.identifier.urihttp://hdl.handle.net/2122/8933en
dc.description.abstractVolcanic plume samples taken in 2008 and 2009 from the Halemàumàu eruption at Kīlauea provide new insights into Kīlauea's degassing behaviour. The Cl, F and S gas systematics are consistent with syn-eruptive East Rift Zone measurements suggesting that the new Halemàumàu activity is fed by a convecting magma reservoir shallower than the main summit storage area. Comparison with degassing models suggests that plume halogen and S composition is controlled by very shallow (<3m depth) decompression degassing and progressive loss of volatiles at the surface. Compared to most other global volcanoes, Kīlauea's gases are depleted in Cl with respect to S. Similarly, our Br/S and I/S ratio measurements in Halemàumàu's plume are lower than those measured at arc volcanoes, consistent with contributions from the subducting slab accounting for a significant proportion of the heavier halogens in arc emissions. Analyses of Hg in Halemàumàu's plume were inconclusive but suggest a flux of at least 0.6kgday -1 from this new vent, predominantly (>77%) as gaseous elemental mercury at the point of emission. Sulphate is an important aerosol component (modal particle diameter ∼0.44μm). Aerosol halide ion concentrations are low compared to other systems, consistent with the lower proportion of gaseous hydrogen halides. Plume concentrations of many metallic elements (Rb, Cs, Be, B, Cr, Ni, Cu, Mo, Cd, W, Re, Ge, As, In, Sn, Sb, Te, Tl, Pb, Mg, Sr, Sc, Ti, V, Mn, Fe, Co, Y, Zr, Hf, Ta, Al, P, Ga, Th, U, La, Ce, Pr, Nd, Sm, Eu, Gd, Tb, Dy, Er, Tm) are elevated above background air. There is considerable variability in metal to SO 2 ratios but our ratios (generally at the lower end of the range previously measured at Kīlauea) support assertions that Kīlauea's emissions are metal-poor compared to other volcanic settings. Our aerosol Re and Cd measurements are complementary to degassing trends observed in Hawaiian rock suites although measured aerosol metal/S ratios are about an order of magnitude lower than those calculated from degassing trends determined from glass chemistry. Plume enrichment factors with respect to Hawaiian lavas are in broad agreement with those from previous studies allowing similar element classification schemes to be followed (i.e., lithophile elements having lower volatility and chalcophile elements having higher volatility). The proportion of metal associated with the largest particle size mode collected (>2.5μm) and that bound to silicate is significantly higher for lithophiles than chalcophiles. Many metals show higher solubility in pH 7 buffer solution than deionised water suggesting that acidity is not the sole driver in terms of solubility. Nonetheless, many metals are largely water soluble when compared with the other sequential leachates suggesting that they are delivered to the environment in a bioavailable form. Preliminary analyses of environmental samples show that concentrations of metals are elevated in rainwater affected by the volcanic plume and even more so in fog. However, metal levels in grass samples showed no clear enrichment downwind of the active vents. © 2011 Elsevier Ltd.en
dc.language.isoEnglishen
dc.publisher.nameElsevier Science Limiteden
dc.relation.ispartofGeochimica et cosmochimica actaen
dc.relation.ispartofseries/83 (2012)en
dc.subjectacidity; aerosol; degassing; emission; halogen; isotopic ratio; lava; magma chamber; mercury (element); particle size; plume; solubility; trace metal; volcanic eruption; volcanoen
dc.titleHalogens and trace metal emissions from the ongoing 2008 summit eruption of Kīlauea volcano, Hawaìien
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber292-323en
dc.subject.INGV01. Atmosphere::01.01. Atmosphere::01.01.07. Volcanic effectsen
dc.identifier.doi10.1016/j.gca.2011.11.029en
dc.description.obiettivoSpecifico4V. Vulcani e ambienteen
dc.description.journalTypeJCR Journalen
dc.description.fulltextrestricteden
dc.relation.issn0016-7037en
dc.relation.eissn1872-9533en
dc.contributor.authorMather, T.en
dc.contributor.authorWitt, M.en
dc.contributor.authorPyle, D.en
dc.contributor.authorQuayle, B.en
dc.contributor.authorAiuppa, A.en
dc.contributor.authorBagnato, E.en
dc.contributor.authorMartin, R.en
dc.contributor.authorSims, K.en
dc.contributor.authorEdmonds, M.en
dc.contributor.authorSutton, J.en
dc.contributor.authorIlyinskaya, E.en
dc.contributor.departmentUniv Oxforden
dc.contributor.departmentUniv Oxforden
dc.contributor.departmentUniv Oxforden
dc.contributor.departmentUniv Oxforden
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italiaen
dc.contributor.departmentUniv Palermoen
dc.contributor.departmentUniv Cambridgeen
dc.contributor.departmentUniversity of Wyomingen
dc.contributor.departmentUniv Cambridgeen
dc.contributor.departmentU.S. Geological Survey,en
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptDepartment of Earth Sciences, University of Oxford-
crisitem.author.deptDepartment of Earth Sciences, University of Oxford-
crisitem.author.deptEarth Science Department, University of Oxford, UK-
crisitem.author.deptUniv Oxford-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Palermo, Palermo, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OV, Napoli, Italia-
crisitem.author.deptDepartment of Earth Sciences, University of Cambridge, UK.-
crisitem.author.deptUniversity of Wyoming-
crisitem.author.deptMontserrat Volcano Observatory, Montserrat, West Indies-
crisitem.author.deptU.S. Geological Survey,-
crisitem.author.orcid0000-0003-4259-7303-
crisitem.author.orcid0000-0002-0254-6539-
crisitem.author.orcid0000-0003-2285-0842-
crisitem.author.orcid0000-0003-1243-137X-
crisitem.author.orcid0000-0002-3663-9506-
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-
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