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Testing the directional recording ability of natural chemical remanent magnetisations using historical sediments

dc.contributor.authorBaker, Evelyn B.en
dc.contributor.authorMuxworthy, Adrian R.en
dc.contributor.authorHeslop, Daviden
dc.date.accessioned2025-12-17T07:40:57Z
dc.date.available2025-12-17T07:40:57Z
dc.date.issued2025-11-10en
dc.description.abstractRocks containing magnetic minerals capture the Earth's magnetic field during their formation and growth, and acquire a chemical remanent magnetisation (CRM). However, the ability of magnetic minerals in sediments to accurately record the direction of the Earth's magnetic field during CRM acquisition has yet to be field tested. In this study, the directional recording ability of CRMs in nature was tested using historical salt marsh sediments from Norfolk, UK. Our results find greigite is the dominant remanence carrier in the salt marsh sediments. Evidence for this includes a gyroremanent magnetisation acquired during alternating field demagnetisation and abundant authigenic iron sulphides identified in SEM-EDX analysis. These iron sulphides appeared as clusters and framboids of equidimensional grains. This morphology is typical of natural iron sulphides. SEM analysis shows these grains on the surface of existing grains and within cracks, indicating that the iron sulphides grew authigenically. During the authigenic growth of greigite, it will acquire a grain-growth CRM of the geomagnetic field. A consistent direction (declination 356°, inclination 68°) with an α 95 of 8° was found throughout the sediments. This direction is indistinguishable from the average geomagnetic field direction during greigite formation for the last 100 years. Therefore, the CRM carried by greigite has accurately recorded the Earth's field direction. This is the first study to directly demonstrate that natural grain-growth CRMs reliably record magnetic field direction.en
dc.description.sponsorshipE.B.B was sponsored by a Science and Technology Facilities Council PhD scholarship 2295497 and acknowledges funding from the UKRI Research Frontier Guarantee program EP/Y014375/1 . D.H. was supported by The Australian Research Council grant DP220102167 . We thank Jack Turney and Alex Lipp for their assistance in the field. We thank Chuang Xuan for the use of the palaeomagnetic laboratory at the University of Southampton, and Yuxi Jin for helping with these measurements. We thank Richard Harrison for the use of the palaeomagnetic laboratory at University of Cambridge, and Hassan Aftab Sheikh for helping with these measurements. We also thank Andrew Roberts for the suggestion of the locality.en
dc.description.statusPeer-revieweden
dc.format.extent11en
dc.identifier.issn0012-821Xen
dc.identifier.otherORCID:/0000-0001-8245-0555/work/198504551en
dc.identifier.scopus105021108303en
dc.identifier.urihttps://hdl.handle.net/1885/733795699
dc.language.isoenen
dc.provenanceThis is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/).en
dc.rights © 2025 The Author(s).en
dc.sourceEarth and Planetary Science Lettersen
dc.subjectChemical remanent magnetisationen
dc.subjectgreigiteen
dc.subjectpalaeomagnetismen
dc.titleTesting the directional recording ability of natural chemical remanent magnetisations using historical sedimentsen
dc.typeJournal articleen
dspace.entity.typePublicationen
local.contributor.affiliationBaker, Evelyn B.; Imperial College Londonen
local.contributor.affiliationMuxworthy, Adrian R.; Imperial College Londonen
local.contributor.affiliationHeslop, David; Climate and Ocean Geoscience, Research School of Earth Sciences, ANU College of Science and Medicine, The Australian National Universityen
local.identifier.citationvolume672en
local.identifier.doi10.1016/j.epsl.2025.119718en
local.identifier.pure63397c3e-78f4-4719-a694-d3f1926be6a9en
local.identifier.urlhttps://www.scopus.com/pages/publications/105021108303en
local.type.statusPublisheden

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