dc.creatorLisé Pronovost, Agathe
dc.creatorSt Onge, Guillaume
dc.creatorGogorza, Claudia Susana
dc.creatorHaberzettl, Torsten
dc.creatorPreda, Michel
dc.creatorKliem, Pierre
dc.creatorFrancus, Pierre
dc.creatorZolitschka, Bernd
dc.creatorThe PASADO Science Team
dc.date.accessioned2018-04-10T20:23:52Z
dc.date.accessioned2018-11-06T14:46:00Z
dc.date.available2018-04-10T20:23:52Z
dc.date.available2018-11-06T14:46:00Z
dc.date.created2018-04-10T20:23:52Z
dc.date.issued2013-02
dc.identifierLisé Pronovost, Agathe; St Onge, Guillaume; Gogorza, Claudia Susana; Haberzettl, Torsten; Preda, Michel; et al.; High-resolution paleomagnetic secular variations and relative paleointensity since the Late Pleistocene in southern South America; Pergamon-Elsevier Science Ltd; Quaternary Science Reviews; 71; 2-2013; 91-108
dc.identifier0277-3791
dc.identifierhttp://hdl.handle.net/11336/41606
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1890008
dc.description.abstractPaleomagnetic inclination, declination and relative paleointensity were reconstructed from the sediments of Laguna Potrok Aike in the framework of the International Continental scientific Drilling Program (ICDP) Potrok Aike maar lake Sediment Archive Drilling prOject (PASADO). Here we present the u-channel-based full vector paleomagnetic field reconstruction since 51.2 ka cal BP. The relative paleointensity proxy (RPI) was built by normalising the natural remanent magnetisation with the anhysteretic remanent magnetisation using the average ratio at 4 demagnetisation steps part of the ChRM interval (NRM/ARM10–40 mT). A grain size influence on the RPI was removed using a correction based on the linear relationship between the RPI and the median destructive field of the natural remanent magnetisation (MDFNRM). The new record is compared with other lacustrine and marine records and stacks from the mid- to high-latitudes of the Southern Hemisphere, revealing consistent millennial-scale variability, the identification of the Laschamp and possibly the Mono Lake geomagnetic excursions, and a direction swing possibly associated to the Hilina Pali excursion at 20 ka cal BP. Nonetheless, a global-scale comparison with other high-resolution records located on the opposite side of the Earth and with various dipole field references hint at a different behaviour of the geomagnetic field around southern South America at 46 ka cal BP.
dc.languageeng
dc.publisherPergamon-Elsevier Science Ltd
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1016/j.quascirev.2012.05.012
dc.relationinfo:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S0277379112001990
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/restrictedAccess
dc.subjectICDP-PROJECT PASADO
dc.subjectLAGUNA POTROK AIKE
dc.subjectPALEOMAGNETISM
dc.subjectRELATIVE PALEOINTENSITY
dc.titleHigh-resolution paleomagnetic secular variations and relative paleointensity since the Late Pleistocene in southern South America
dc.typeArtículos de revistas
dc.typeArtículos de revistas
dc.typeArtículos de revistas


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