dc.creatorMorosini, Augusto Francisco
dc.creatorChristiansen, Rodolfo Omar
dc.creatorEnriquez, Eliel
dc.creatorPagano Género, Diego Sebastián
dc.creatorPerón Orrillo, Juan Matías
dc.creatorOrtiz Suarez, Ariel Emilio
dc.creatorMartínez, Myriam Patricia
dc.creatorMuñoz, Brian Lucas
dc.creatorRamos, Gabriel Alejandro
dc.date.accessioned2022-01-21T13:07:46Z
dc.date.accessioned2022-10-15T16:31:06Z
dc.date.available2022-01-21T13:07:46Z
dc.date.available2022-10-15T16:31:06Z
dc.date.created2022-01-21T13:07:46Z
dc.date.issued2020-11
dc.identifierMorosini, Augusto Francisco; Christiansen, Rodolfo Omar; Enriquez, Eliel; Pagano Género, Diego Sebastián; Perón Orrillo, Juan Matías; et al.; Architecture and kinematics of the Famatinian deformation in the Sierra Grande de San Luis: A record of a collisional history at 33° S latitude; Pergamon-Elsevier Science Ltd; Journal of South American Earth Sciences; 105; 11-2020; 1-30
dc.identifier0895-9811
dc.identifierhttp://hdl.handle.net/11336/150467
dc.identifier1873-0647
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4409512
dc.description.abstractAn improved understanding of the evolution of the Famatinian basement in the Sierra Grande de San Luis (SGSL) in Argentina is presented. Combining geological, geophysical and petrological data, a 3D inversion model for the basement rocks and their shear zones in the study area was constructed. The inversion model and the ground data show that the main deformation mechanism that affected the metamorphic complexes is related to a significant number of shear zones which delineate the architecture of the basement. Results suggest that the regional scale shear system (~40 km wide and ~120 km long) and the internal structural elements of the different tectonic domains are the product of an important crustal shortening. A contractional tectonic framework related to the indentation of the Cuyania/Precordillera microcontinent on the western Gondwana margin is proposed to be the cause of the tectonic mechanisms that led to a pop-up megastructure in the western sector of the SGSL and the closing of the Famatinian backarc.
dc.languageeng
dc.publisherPergamon-Elsevier Science Ltd
dc.relationinfo:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S0895981120305290?via%3Dihub
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1016/j.jsames.2020.102986
dc.rightshttps://creativecommons.org/licenses/by-nc-nd/2.5/ar/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.subjectGRAVITY/MAGNETIC DATA
dc.subjectPOP-UP STRUCTURE
dc.subjectSHEAR ZONE SYSTEM
dc.subjectSTRUCTURAL ANALYSIS
dc.subjectTECTONIC EVOLUTION
dc.titleArchitecture and kinematics of the Famatinian deformation in the Sierra Grande de San Luis: A record of a collisional history at 33° S latitude
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:ar-repo/semantics/artículo
dc.typeinfo:eu-repo/semantics/publishedVersion


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