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dc.contributor.authorCalvo Rathert, Manuel 
dc.contributor.authorBógalo Román, Mª Felicidad 
dc.contributor.authorMorales, J.
dc.contributor.authorGoguitchaichvili, Avto
dc.contributor.authorLebedev, Vladimir A.
dc.contributor.authorVashakidze, George T.
dc.contributor.authorGarcía Redondo, Natalia
dc.contributor.authorHerrero, E.
dc.date.accessioned2021-11-08T11:30:47Z
dc.date.available2021-11-08T11:30:47Z
dc.date.issued2021-02
dc.identifier.issn2169-9313
dc.identifier.urihttp://hdl.handle.net/10259/6117
dc.description.abstractSixteen rhyolitic and dacitic Cretaceous and Paleocene-Eocene lavas from the Lesser Caucasus have been subjected to paleomagnetic and multimethod paleointensity experiments to analyze the variations of the Earth's magnetic field. Paleointensity experiments were performed with two methods. Thellier-type experiments with the IZZI method on 65 specimens (nine flows) yielded 15 successful determinations and experiments with the multispecimen method on 14 samples (seven flows) yielded two successful determinations. The joint analysis of the results obtained with both methods produced a mean FuK = (19.9 ± 3.7) µT for upper Cretaceous and FPg = (20.7 ± 3.3) µT for Paleogene sites. Low virtual axial dipole moments for the Cretaceous (3.4 × 1022 Am2) and Paleogene (3.5 × 1022 Am2) samples support the idea of a lower average dipole moment during periods of stable polarity of the Earth magnetic field. Mean flow paleomagnetic directions did not match expected upper Cretaceous to Paleogene directions calculated from the European Apparent Polar Wander Path. While inclination results roughly agreed with expected values, a group of sites showed nearly North-South paleodeclinations (D = 1.1° ± 14.2°), and another group displayed eastward deviated paleodeclinations (D = 72.9° ± 26.6°). These results suggest the occurrence of nearly vertical-axis rotations, probably as a result of continental collision since Oligocene. In addition to paleomagnetic and palaeointensity analyses, new K-Ar absolute age determinations have been performed on three of the studied sites, yielding Late Cretaceous ages (78.7 ± 1.7, 79.7 ± 1.6, and 83.4 ± 1.8 Ma (2σ)).en
dc.description.sponsorshipProject PID2019-105796GB-100/AEI/10.13039/501100011033 (Agencia Estatal de Investigación, Spain). M. Calvo-Rathert acknowledges funding from the Fulbright Commission and the Spanish Ministry of Science, Innovation, and Universities for a research stay at Hawaii University at Manoa. A. Goguitchaichvili acknowledges financial support from UNAM-PAPIIT no. IN101920. N. García-Redondo acknowledges financial support from Junta de Castilla y León and the European Research Development Fund (ERDF). EHB acknowledges financial support for laboratory maintenance and measurements to SOEST-HIGP and National Science Foundation grants. These is SOEST 11143 and HIGP 2420 contribution.en
dc.format.mimetypeapplication/pdf
dc.language.isoengen
dc.publisherAmerican Geophysical Union (AGU)en
dc.relation.ispartofJournal of geophysical research. Solid earth. 2021, V. 126, n. 2, e2020JB020019en
dc.subjectCaucasusen
dc.subjectCretaceousen
dc.subjectK-Ar datingen
dc.subjectPaleointensityen
dc.subjectPaleomagnetismen
dc.subjectRock magnetismen
dc.subject.otherMagnetismoes
dc.subject.otherMagnetismen
dc.subject.otherGeologíaes
dc.subject.otherGeologyen
dc.subject.otherFísicaes
dc.subject.otherPhysicsen
dc.titleAn Integrated Paleomagnetic, Multimethod- Paleointensity, and Radiometric Study on Cretaceous and Paleogene Lavas From the Lesser Caucasus: Geomagnetic and Tectonic Implicationsen
dc.typeinfo:eu-repo/semantics/articlees
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses
dc.relation.publisherversionhttps://doi.org/10.1029/2020JB020019
dc.identifier.doi10.1029/2020JB020019
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersiones


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