Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/10462
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dc.contributor.authorallPaonita, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italiaen
dc.contributor.authorallCadoux, A.; ISTOen
dc.contributor.authorallIacono Marziano, G.; ISTOen
dc.contributor.authorallDeloule, E.; CRPGen
dc.contributor.authorallAiuppa, A.; Unipaen
dc.contributor.authorallEby, N.; Massachusset universityen
dc.contributor.authorallCosta, M.; Unipaen
dc.contributor.authorallBrusca, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italiaen
dc.contributor.authorallBerlo, K.; McGill Universityen
dc.contributor.authorallGeraki, K.; Harwall Campusen
dc.contributor.authorallMather, T.; University of Oxforden
dc.contributor.authorallPyle, D.; University of Oxforden
dc.contributor.authorallDi Carlo, I.; ISTOen
dc.date.accessioned2017-02-23T10:13:41Zen
dc.date.available2017-02-23T10:13:41Zen
dc.date.issued2017en
dc.identifier.urihttp://hdl.handle.net/2122/10462en
dc.description.abstractMeasuring the low bromine abundances in Earth's materials remains an important challenge in order to constrain the geodynamical cycle of this element. Suitable standard materials are therefore required to establish reliable analytical methods to quantify Br abundances. In this study we characterise 21 Br-doped glasses synthesized from natural volcanic rocks of mafic to silicic compositions, in order to produce a new set of standards for Br analyses using various techniques. The nominal Br contents (amounts of Br loaded in the experimental samples) of 15 of 21 glasses were confirmed within 20% by instrumental neutron activation analysis (INAA). Using this newset of standards, we compare three micro-analytical approaches to measure Br contents in silicate glasses: synchrotron X-ray fluorescence (SR-XRF), laser ablation-inductively coupled plasma mass spectrometry (LA-ICP-MS), and secondary ion mass spectrometry (SIMS). With SR-XRF, the Br contents of the standard glasses were determined with the highest accuracy (b10% for Br ≥ 10 ppm; N25% for Br ≤ 5 ppm), and high precision (b10% for Br contents N10 ppm; 20–30% for Br ≤ 10 ppm). The detection limit was estimated to be b1 ppm Br. All those factors combined with a high spatial resolution (5 × 5 μm for the presented measurements), means that SR-XRF iswell suited to determine the lowBr abundance in natural volcanic glasses (crystal-hosted melt inclusions or matrix glasses of crystallized samples). At its current stage of development, the LA-ICP-MS method allows the measurement of hundreds to thousands ppm Br in silicate glasses with a precision and accuracy generally within 20%. The Br detection limit of this method has not been estimated but its low spatial resolution (90 μm) currently prevents its use to characterise natural volcanic glasses, however it is fully appropriate to analyse super liquidus or sparsely phyric, Br-rich experimental charges. Our study shows that SIMS appears to be a promising technique to measure the lowBr contents of natural volcanic glasses. Its spatial resolution is relatively good (~15 μm) and, similarly to SR-XRF, the detection limit is estimated to be ≤ 1 ppm. Using our new set of standards, the Br contents of two MPI-DING reference glasses containing ≤ 1.2 ppm of Br were reproduced with precision b5% and accuracy b20%. Moreover, SIMS presents the advantage of being a more accessible instrument than SR-XRF and data processing is more straightforward.en
dc.language.isoEnglishen
dc.publisher.nameElsevier Science Limiteden
dc.relation.ispartofChemical geologyen
dc.relation.ispartofseries/452(2017)en
dc.subjectbromineen
dc.subjectrock standardsen
dc.titleA new set of standards for in–situ measurement of bromine abundances in natural silicate glasses: Application to SR-XRF, LA-ICP-MS and SIMS techniquesen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber60-70en
dc.subject.INGV04. Solid Earth::04.08. Volcanology::04.08.05. Volcanic rocksen
dc.identifier.doi10.1016/j.chemgeo.2017.01.012en
dc.description.obiettivoSpecifico2V. Dinamiche di unrest e scenari pre-eruttivien
dc.description.journalTypeJCR Journalen
dc.description.fulltextrestricteden
dc.relation.issn0009-2541en
dc.relation.eissn1872-6836en
dc.contributor.authorPaonita, A.en
dc.contributor.authorCadoux, A.en
dc.contributor.authorIacono Marziano, G.en
dc.contributor.authorDeloule, E.en
dc.contributor.authorAiuppa, A.en
dc.contributor.authorEby, N.en
dc.contributor.authorCosta, M.en
dc.contributor.authorBrusca, L.en
dc.contributor.authorBerlo, K.en
dc.contributor.authorGeraki, K.en
dc.contributor.authorMather, T.en
dc.contributor.authorPyle, D.en
dc.contributor.authorDi Carlo, I.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italiaen
dc.contributor.departmentISTOen
dc.contributor.departmentISTOen
dc.contributor.departmentCRPGen
dc.contributor.departmentUnipaen
dc.contributor.departmentMassachusset universityen
dc.contributor.departmentUnipaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Palermo, Palermo, Italiaen
dc.contributor.departmentMcGill Universityen
dc.contributor.departmentHarwall Campusen
dc.contributor.departmentUniversity of Oxforden
dc.contributor.departmentUniversity of Oxforden
dc.contributor.departmentISTOen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
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.deptMassachusset university-
crisitem.author.deptUniversità di Palermo-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Palermo, Palermo, Italia-
crisitem.author.deptMcGill University-
crisitem.author.deptHarwall Campus-
crisitem.author.deptDepartment of Earth Sciences, University of Oxford-
crisitem.author.deptEarth Science Department, University of Oxford, UK-
crisitem.author.deptCNRS Orleans, Francia-
crisitem.author.orcid0000-0001-9124-5027-
crisitem.author.orcid0000-0003-3175-5425-
crisitem.author.orcid0000-0001-6955-1685-
crisitem.author.orcid0000-0002-0254-6539-
crisitem.author.orcid0000-0002-6570-9673-
crisitem.author.orcid0000-0003-4259-7303-
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.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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