The role of smectites in the electrical conductivity of active hydrothermal systems: electrical properties of core samples from Krafla volcano, Iceland

dc.contributorHáskóli Íslandsen_US
dc.contributorUniversity of Icelanden_US
dc.contributor.authorLévy, L
dc.contributor.authorGibert, B
dc.contributor.authorSigmundsson, Freysteinn
dc.contributor.authorFlóvenz, Ólafur G.
dc.contributor.authorHersir, Gylfi
dc.contributor.authorBriole, P
dc.contributor.authorPezard, PA
dc.contributor.departmentJarðvísindastofnun (HÍ)en_US
dc.contributor.departmentInstitute of Earth Sciences (UI)en_US
dc.contributor.schoolVerkfræði- og náttúruvísindasvið (HÍ)en_US
dc.contributor.schoolSchool of Engineering and Natural Sciences (UI)en_US
dc.date.accessioned2019-10-03T11:42:55Z
dc.date.available2019-10-03T11:42:55Z
dc.date.issued2018-08-18
dc.descriptionPublisher's version (útgefin grein)en_US
dc.description.abstractThe underground circulation of hot water, of interest for geothermal energy production, is often indirectly inferred from the presence of minerals formed by hydrothermal alteration at different temperatures. Clay minerals, such as smectite and chlorite, can be mapped from the surface using electrical soundings and give information about the structure of the geothermal system. Here, we investigate the specific role of smectite in the electrical response of igneous basaltic rocks and evaluate what physical processes make smectite a better electrical conductor than surrounding minerals. Laboratory measurements of cation exchange capacity (CEC), mineralogy, porosity and electrical conductivity are presented for 88 core samples from four boreholes at the Krafla volcano, Northeast Iceland. CEC is found to be a reliable measure of the smectite weight fraction in these volcanic samples, through a comparison with an independent quantification of the smectite content using Rietveld refinements of X-ray diffraction patterns. The bulk electrical conductivity, measured at fluid conductivities in the range 0.02–11.7 S m−1, increases non-linearly with the fluid conductivity for samples with high smectite content. This non-linear variation is fitted with a function and a model for a conduction process through connected interlayer spaces within smectite. The process differs from electrical double layer conduction, which involves only cations on the crystal edges of smectite, not in the interlayer spaces. The laboratory results can help refine interpretations of electrical soundings in the context of geothermal exploration.en_US
dc.description.sponsorshipThis research was supported by the IMAGE FP7 EC project (Integrated Methods for Advanced Geothermal Exploration, grant agreement no. 608553) and by a PhD grant from Paris Sciences et Lettres.en_US
dc.description.versionPeer Revieweden_US
dc.format.extent1558-1582en_US
dc.identifier.citationL Lévy, B Gibert, F Sigmundsson, ÓG Flóvenz, GP Hersir, P Briole, PA Pezard, The role of smectites in the electrical conductivity of active hydrothermal systems: electrical properties of core samples from Krafla volcano, Iceland, Geophysical Journal International, Volume 215, Issue 3, December 2018, Pages 1558–1582, https://doi.org/10.1093/gji/ggy342en_US
dc.identifier.doi10.1093/gji/ggy342
dc.identifier.issn0956-540X
dc.identifier.issn1365-246X (eISSN)
dc.identifier.journalGeophysical Journal Internationalen_US
dc.identifier.urihttps://hdl.handle.net/20.500.11815/1291
dc.language.isoenen_US
dc.publisherOxford University Press (OUP)en_US
dc.relation.ispartofseriesGeophysical Journal International;215(3)
dc.relation.urlhttp://academic.oup.com/gji/article-pdf/215/3/1558/25808251/ggy342.pdfen_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectElectrical propertiesen_US
dc.subjectHydrothermal systemsen_US
dc.subjectJarðhitakerfien_US
dc.subjectJarðhitien_US
dc.subjectRafleiðnien_US
dc.titleThe role of smectites in the electrical conductivity of active hydrothermal systems: electrical properties of core samples from Krafla volcano, Icelanden_US
dc.typeinfo:eu-repo/semantics/articleen_US
dcterms.license© The Author(s) 2018. Published by Oxford University Press on behalf of The Royal Astronomical Society. This article is published and distributed under the terms of the Oxford University Press, Standard Journals Publication Model (https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model)en_US

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