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dc.contributor.authorChávez Segura, René
dc.contributor.authorFlores Márquez, Elsa Leticia
dc.contributor.authorSuriñach Cornet, Emma
dc.contributor.authorGalindo Zaldívar, Jesús 
dc.contributor.authorRodríguez Fernández, José
dc.contributor.authorMaldonado, Andrés
dc.date.accessioned2014-06-02T07:48:22Z
dc.date.available2014-06-02T07:48:22Z
dc.date.issued2007
dc.identifier.citationChávez Segura, R.; et al. Combined use of the GGSFT data base and on board marine collected data to model the Moho beneath the Powell Basin, Antarctica. Geologica Acta, 5(4): 323-335 (2007). [http://hdl.handle.net/10481/32075]es_ES
dc.identifier.issn1695-6133
dc.identifier.issn1696-5728
dc.identifier.urihttp://hdl.handle.net/10481/32075
dc.description.abstractThe Powell Basin is a small oceanic basin located at the NE end of the Antarctic Peninsula developed during the Early Miocene and mostly surrounded by the continental crusts of the South Orkney Microcontinent, South Scotia Ridge and Antarctic Peninsula margins. Gravity data from the SCAN 97 cruise obtained with the R/V Hespérides and data from the Global Gravity Grid and Sea Floor Topography (GGSFT) database (Sandwell and Smith, 1997) are used to determine the 3D geometry of the crustal-mantle interface (CMI) by numerical inversion methods. Water layer contribution and sedimentary effects were eliminated from the Free Air anomaly to obtain the total anomaly. Sedimentary effects were obtained from the analysis of existing and new SCAN 97 multichannel seismic profiles (MCS). The regional anomaly was obtained after spectral and filtering processes. The smooth 3D geometry of the crustal mantle interface obtained after inversion of the regional anomaly shows an increase in the thickness of the crust towards the continental margins and a NW-SE oriented axis of symmetry coinciding with the position of an older oceanic spreading axis. This interface shows a moderate uplift towards the western part and depicts two main uplifts to the northern and eastern sectors.es_ES
dc.description.sponsorshipWe are thankful to the Hespérides Working Group who provided some original data. CGL2004-05646/ANT and University of Barcelona and DGIA-UNAM Interchange program financed this study. The CONACyT, Mexico, also supported Dr. E. L. Flores-Márquez and R.E. Chávez stays at the Universidad de Barcelona.es_ES
dc.language.isoenges_ES
dc.publisherUniversidad de Barcelona; Instituto de Ciencias de la Tierra Jaume Almeraes_ES
dc.rightsCreative Commons Attribution-NonCommercial-NoDerivs 3.0 Licensees_ES
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es_ES
dc.subjectGravity es_ES
dc.subjectInverse theoryes_ES
dc.subjectAntartic Peninsulaes_ES
dc.subjectPowell Basines_ES
dc.subjectMarine geophysicses_ES
dc.titleCombined use of the GGSFT data base and on board marine collected data to model the Moho beneath the Powell Basin, Antarcticaes_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses_ES


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