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Signatures of Reductive Magnetic Mineral Diagenesis From Unmixing of First-Order Reversal Curves

dc.contributor.authorRoberts, Andrew P.
dc.contributor.authorZhao, Xiang
dc.contributor.authorHarrison, Richard J
dc.contributor.authorHeslop, David
dc.contributor.authorMuxworthy, Adrian R
dc.contributor.authorRowan, J. Christopher
dc.contributor.authorLarrasoaña, Juan C.
dc.contributor.authorFlorindo, Fabio
dc.date.accessioned2021-12-02T22:30:20Z
dc.date.available2021-12-02T22:30:20Z
dc.date.issued2018
dc.date.updated2020-11-23T11:54:18Z
dc.description.abstractDiagenetic alteration of magnetic minerals occurs in all sedimentary environments and tends to be severe in reducing environments. Magnetic minerals provide useful information about sedimentary diagenetic processes, which makes it valuable to use magnetic properties to identify the diagenetic environment in which the magnetic minerals occur and to inform interpretations of paleomagnetic recording or environmental processes. We use a newly developed first‐order reversal curve unmixing method on well‐studied samples to illustrate how magnetic properties can be used to assess diagenetic processes in reducing sedimentary environments. From our analysis of multiple data sets, consistent magnetic components are identified for each stage of reductive diagenesis. Relatively unaltered detrital and biogenic magnetic mineral assemblages in surficial oxic to manganous diagenetic environments undergo progressive dissolution with burial into ferruginous and sulfidic environments and largely disappear at the sulfate‐methane transition. Below the sulfate‐methane transition, a weak superparamagnetic to largely noninteracting stable single domain (SD) greigite component is observed in all studied data sets. Moderately interacting stable SD authigenic pyrrhotite and strongly interacting stable SD greigite are observed commonly in methanic environments. Recognition of these characteristic magnetic components enables identification of diagenetic processes and should help to constrain interpretation of magnetic mineral assemblages in future studies. A key question for future studies concerns whether stable SD greigite forms in the sulfidic or methanic zones, where formation in deeper methanic sediments will cause greater delays in paleomagnetic signal recording. Authigenic pyrrhotite forms in methanic environments, so it will usually record a delayed paleomagnetic signal.en_AU
dc.description.sponsorshipThis work was supported financially by the Australian Research Council through grant DP160100805, by the European Research Council under the European Union’s Seventh Framework Programme (FP/2007–2013)/ERC grant agreement number 320750, and by the National Institute of Advanced Industrial Science and Technology, Ministry of Economy, Trade and Industry, Japanen_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn2169-9313en_AU
dc.identifier.urihttp://hdl.handle.net/1885/254489
dc.language.isoen_AUen_AU
dc.provenancehttps://v2.sherpa.ac.uk/id/publication/11081..."The Published Version can be archived in a Non-Commercial Institutional Repository" from SHERPA/RoMEO site (as at 3/12/2021). An edited version of this paper was published by AGU. Copyright (2018) American Geophysical Union.en_AU
dc.publisherWiley Blackwellen_AU
dc.relationhttp://purl.org/au-research/grants/arc/DP160100805en_AU
dc.rights© 2018. American Geophysical Unionen_AU
dc.sourceJournal of Geophysical Research: Solid Earthen_AU
dc.titleSignatures of Reductive Magnetic Mineral Diagenesis From Unmixing of First-Order Reversal Curvesen_AU
dc.typeJournal articleen_AU
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue6en_AU
local.bibliographicCitation.lastpage4522en_AU
local.bibliographicCitation.startpage4500en_AU
local.contributor.affiliationRoberts, Andrew, College of Science, ANUen_AU
local.contributor.affiliationZhao, Xiang, College of Science, ANUen_AU
local.contributor.affiliationHarrison, Richard J, University of Cambridgeen_AU
local.contributor.affiliationHeslop, David, College of Science, ANUen_AU
local.contributor.affiliationMuxworthy, Adrian R, Imperial College Londonen_AU
local.contributor.affiliationRowan, J. Christopher, Kent State Universityen_AU
local.contributor.affiliationLarrasoaña, Juan C., Área de Cambio Global, IGME, Oficina de Proyectos de Zaragozaen_AU
local.contributor.affiliationFlorindo, Fabio, Instituto Nazionale di Geofisica e Vulcanologiaen_AU
local.contributor.authoruidRoberts, Andrew, u4817957en_AU
local.contributor.authoruidZhao, Xiang, u5047067en_AU
local.contributor.authoruidHeslop, David, u4919989en_AU
local.description.notesImported from ARIESen_AU
local.identifier.absfor040406 - Magnetism and Palaeomagnetismen_AU
local.identifier.absfor040299 - Geochemistry not elsewhere classifieden_AU
local.identifier.absseo970104 - Expanding Knowledge in the Earth Sciencesen_AU
local.identifier.ariespublicationa383154xPUB10459en_AU
local.identifier.citationvolume123en_AU
local.identifier.doi10.1029/2018JB015706en_AU
local.identifier.scopusID2-s2.0-85050238031
local.publisher.urlhttps://www.wiley.com/en-gben_AU
local.type.statusPublished Versionen_AU

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