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dc.contributor.authorBorlina, Cauê S.-
dc.contributor.authorLima, Eduardo A.-
dc.contributor.authorFeinberg, Joshua M.-
dc.contributor.authorJaqueto, Plinio-
dc.contributor.authorLascu, Ioan-
dc.contributor.authorTrindade, Ricardo I. F.-
dc.contributor.authorFont, Eric-
dc.contributor.authorSánchez-Moreno, Elisa M.-
dc.contributor.authorDimuccio, Luca Antonio-
dc.contributor.authorYokoyama, Yusuke-
dc.contributor.authorParés, Josep María-
dc.contributor.authorWeiss, Benjamin P.-
dc.contributor.authorDorale, Jeffrey A.-
dc.date.accessioned2024-07-18-
dc.date.accessioned2024-10-10T09:08:47Z-
dc.date.issued2024-10-
dc.identifier.citationGeochemistry, Geophysics, Geosystems, 2024, 25(10), e2024GC011594es_ES
dc.identifier.issn1525-2027-
dc.identifier.urihttps://cir.cenieh.es/handle/20.500.12136/3331-
dc.description.abstractSpeleothems are mineral deposits capable of recording detrital and/or chemical remanent magnetization at annual timescales. They can offer high-resolution paleomagnetic records of short-term variations in Earth's magnetic field, crucial for understanding the evolution of the dynamo. Owing to limitations on the magnetic moment sensitivity of commercial cryogenic rock magnetometers (∼10−11 Am2), paleomagnetic studies of speleothems have been limited to samples with volumes of several hundreds of mm3, averaging tens to hundreds of years of magnetic variation. Nonetheless, smaller samples (∼1–10 mm3) can be measured using superconducting quantum interference device (SQUID) microscopy, with a sensitivity better than ∼10−15 Am2. To determine the application of SQUID microscopy for obtaining robust high-resolution records from small-volume speleothem samples, we analyzed three different stalagmites collected from Lapa dos Morcegos Cave (Portugal), Pau d'Alho Cave (Brazil), and Crevice Cave (United States). These stalagmites are representative of a range of magnetic properties and have been previously studied with conventional rock magnetometers. We show that by using SQUID microscopy we can achieve a five-fold improvement in temporal resolution for samples with higher abundances of magnetic carriers (e.g., Pau d'Alho Cave and Lapa dos Morcegos Cave). In contrast, speleothems with low abundances of magnetic carriers (e.g., Crevice Cave) do not benefit from higher resolution analysis and are best analyzed using conventional rock magnetometers. Overall, by targeting speleothem samples with high concentrations of magnetic carriers we can increase the temporal resolution of magnetic records, setting the stage for resolving geomagnetic variations at short time scales.es_ES
dc.description.sponsorshipThis work was partially supported by the National Science Foundation (NSF) Grants EAR-2044806, EAR-2044535, and EAR-2044506, Fundação para a Ciência e a Tecnologia (FCT-Portugal, PTDC/CTA-GEO/0125/2021 and MIT-EXPL/ACC/0023/2021), and the MIT-Portugal Seed Fund. CSB thanks The Morton K. Blaustein Scholars Fund. EMSM acknowledges the project BU037P23 of the Junta de Castilla y León and the European Research and Development Fund. Fieldwork and speleothem sampling in Portugal were authorized by Instituto da Conservação da Natureza e das Florestas (ICNF I.P.), under the responsibility of LD and supported by CEGOT I&D Unit (FCT-Portugal, UIDP/GEO/04084/2020_UC). Fieldwork and speleothem collection in Brazil were authorized by the Instituto Brasileiro do Meio Ambiente e dos Recursos Renováveis, and we thank the Centro Nacional de Pesquisa e Conservação de Cavernas (CECAV/ICMBio) for providing permission to collect stalagmite samples.es_ES
dc.language.isoenes_ES
dc.publisherAmer Geophysical Uniones_ES
dc.rightsinfo:eu-repo/semantics/openAccesses_ES
dc.rightsAtribución-NoComercial-SinDerivadas 4.0 Estados Unidos de América (CC BY-NC-ND 4.0)*
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/deed.es*
dc.subjectPaleomagnetismes_ES
dc.subjectMagnetic microscopyes_ES
dc.subjectSpeleothemses_ES
dc.subjectEarth's magnetic fieldes_ES
dc.titleObtaining High-Resolution Magnetic Records From Speleothems Using Magnetic Microscopyes_ES
dc.typeArticlees_ES
dc.identifier.doi10.1029/2024GC011594-
dc.relation.publisherversionhttps://doi.org/10.1029/2024GC011594es_ES
dc.date.available2024-10-10T09:08:47Z-
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