Please use this identifier to cite or link to this item: https://cir.cenieh.es/handle/20.500.12136/3181
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dc.contributor.authorDinis, R.-
dc.contributor.authorFont, E.-
dc.contributor.authorCarmo, J.-
dc.contributor.authorTrindade, R.-
dc.contributor.authorReboleira, A.S.P.S.-
dc.contributor.authorHasözbek, Altuğ-
dc.contributor.authorJiménez Barredo, Fernando-
dc.contributor.authorParés, Josep María-
dc.contributor.authorCarvalho, E.-
dc.date.accessioned2024-03-12T12:12:04Z-
dc.date.issued2023-
dc.identifier.citationXIII MAGIBER, 2023, 41-44es_ES
dc.identifier.urihttps://cir.cenieh.es/handle/20.500.12136/3181-
dc.descriptionPonencia presentada en: XIII MAGIBER, 25-28 de julio 2023, Porto, Portugales_ES
dc.description.abstractSpeleothems magnetism has been used for the study of short-lived variations in the Earth's magnetic field (CMT) as well as climate. In this work, two speleothems from the Estremenho Limestone Massif of Portugal were studied, to obtain information about the variation of the CMT. Paleomagnetic data (natural remanent magnetization), measurement of magnetic properties (FORC), and U-Th dating were performed, as well as the calculation of relative paleointensity, through the Pseudo-Thellier method. Paleomagnetic results indicate that stalagmites recorded a stable remnant magnetization of primary origin (contemporaneous with stalagmite precipitation) and indicate magnetite as the main carrier of magnetization in stalagmites. U-Th dating provided an age range in one of the stalagmites (114.7 ±1.5 ky BP; 109.6 ±1.7 ky BP; 106.3 ±1.6 ky BP), compatible with the Blake geomagnetic excursion age. The relative paleointensity curve shows a pattern of variation very similar to the reference curves for this time interval, however, the magnetic data obtained do not indicate the presence of the occurrence of the Blake excursion. This suggests an older age for this geomagnetic excursion, or a secondary magnetization origin. Further research is needed to unravel this discrepancy.es_ES
dc.description.sponsorshipThis work was supported by the SAMEPA project funded by FCT (ref. PTDC/CTA-GEO/0125/2021; MITEXPL/ACC/0023/2021; UIDB/00329/2020; /UIDB/50019/2020) and is part of the Ph.D. grant of Rafael Dinis (FCT-10216.2022.BD).es_ES
dc.language.isoenes_ES
dc.rightsinfo:eu-repo/semantics/openAccesses_ES
dc.subjectSpeleothemses_ES
dc.subjectPaleomagnetismes_ES
dc.subjectClimatees_ES
dc.subjectMagnetic Mineralogyes_ES
dc.subjectBlake Geomagnetic Excursiones_ES
dc.titlePaleomagnetism and Relative Paleointensity of two stalagmites from the Estremenho Limestone Massif, Portugales_ES
dc.title.alternativePaleomagnetismo e paleointensidade relativa de duas estalagmites do Maciço Calcário Estremenho, Portugales_ES
dc.typePresentationes_ES
dc.typeOtheres_ES
dc.relation.publisherversionhttps://sge.usal.es/comisiones/memorias_paleomagnetismo/PDFS_Comis_paleomag_MAGIBER_XIII_porto.pdfes_ES
dc.date.available2024-03-12T12:12:04Z-
Appears in Collections:Congresos, encuentros científicos y estancias de investigación



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