A crustal model along 39°S from a seismic refraction profile- ISSA 2000

The results of a seismic refraction profile across the Southern Andes at 39°S from the Chilean Pacific coast to the Argentinean Neuquén Basin are presented here. A 2-D crustal velocity model was derived from traveltime forward modeling of the correlated phases on shot-sections from shot-points in th...

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Autores principales: Araneda,Manuel, Asch,Günter, Bataille,Klaus, Bohm,Mirjam, Bruhn,Carsten, Giese,Peter, Lüth,Stefan, Quezada,Jorge, Rietbrock,Andreas, Wigger,Peter
Lenguaje:English
Publicado: Servicio Nacional de Geología y Minería (SERNAGEOMIN) 2003
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Acceso en línea:http://www.scielo.cl/scielo.php?script=sci_arttext&pid=S0716-02082003000100006
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spelling oai:scielo:S0716-020820030001000062003-10-21A crustal model along 39°S from a seismic refraction profile- ISSA 2000Araneda,ManuelAsch,GünterBataille,KlausBohm,MirjamBruhn,CarstenGiese,PeterLüth,StefanQuezada,JorgeRietbrock,AndreasWigger,Peter Seismic refraction Crustal structure Southern Chile The results of a seismic refraction profile across the Southern Andes at 39°S from the Chilean Pacific coast to the Argentinean Neuquén Basin are presented here. A 2-D crustal velocity model was derived from traveltime forward modeling of the correlated phases on shot-sections from shot-points in the Pacific Ocean and in the Chilean Main Cordillera. The crustal velocity model is characterized by lower average velocities in the fore-arc than in the arc. A typical continental Moho was not observed under the fore-arc, under the arc the Moho could only be inferred from teleseismic receiver function studies. The oceanic Moho was observed down to ca. 45 km depth under the continental fore-arc. Using additional structural and seismic data, the velocity model was extrapolated to the west and to the east, and this model was converted into a rough density model. The gravity, computed from this density model, is consistent with the free-air and Bouguer gravity. A crustal thickness of ca. 40 km is inferred for the magmatic arc. Gradually decreasing average velocities of the continental crust from east to west are proposed to be due to the influence of the intrusion of the North Patagonian batholith in the east and of decreasing age of the accretionary wedge together with underplating of subducted sediments at the base of the continental crust in the west.info:eu-repo/semantics/openAccessServicio Nacional de Geología y Minería (SERNAGEOMIN)Revista geológica de Chile v.30 n.1 20032003-07-01text/htmlhttp://www.scielo.cl/scielo.php?script=sci_arttext&pid=S0716-02082003000100006en10.4067/S0716-02082003000100006
institution Scielo Chile
collection Scielo Chile
language English
topic Seismic refraction
Crustal structure
Southern Chile
spellingShingle Seismic refraction
Crustal structure
Southern Chile
Araneda,Manuel
Asch,Günter
Bataille,Klaus
Bohm,Mirjam
Bruhn,Carsten
Giese,Peter
Lüth,Stefan
Quezada,Jorge
Rietbrock,Andreas
Wigger,Peter
A crustal model along 39°S from a seismic refraction profile- ISSA 2000
description The results of a seismic refraction profile across the Southern Andes at 39°S from the Chilean Pacific coast to the Argentinean Neuquén Basin are presented here. A 2-D crustal velocity model was derived from traveltime forward modeling of the correlated phases on shot-sections from shot-points in the Pacific Ocean and in the Chilean Main Cordillera. The crustal velocity model is characterized by lower average velocities in the fore-arc than in the arc. A typical continental Moho was not observed under the fore-arc, under the arc the Moho could only be inferred from teleseismic receiver function studies. The oceanic Moho was observed down to ca. 45 km depth under the continental fore-arc. Using additional structural and seismic data, the velocity model was extrapolated to the west and to the east, and this model was converted into a rough density model. The gravity, computed from this density model, is consistent with the free-air and Bouguer gravity. A crustal thickness of ca. 40 km is inferred for the magmatic arc. Gradually decreasing average velocities of the continental crust from east to west are proposed to be due to the influence of the intrusion of the North Patagonian batholith in the east and of decreasing age of the accretionary wedge together with underplating of subducted sediments at the base of the continental crust in the west.
author Araneda,Manuel
Asch,Günter
Bataille,Klaus
Bohm,Mirjam
Bruhn,Carsten
Giese,Peter
Lüth,Stefan
Quezada,Jorge
Rietbrock,Andreas
Wigger,Peter
author_facet Araneda,Manuel
Asch,Günter
Bataille,Klaus
Bohm,Mirjam
Bruhn,Carsten
Giese,Peter
Lüth,Stefan
Quezada,Jorge
Rietbrock,Andreas
Wigger,Peter
author_sort Araneda,Manuel
title A crustal model along 39°S from a seismic refraction profile- ISSA 2000
title_short A crustal model along 39°S from a seismic refraction profile- ISSA 2000
title_full A crustal model along 39°S from a seismic refraction profile- ISSA 2000
title_fullStr A crustal model along 39°S from a seismic refraction profile- ISSA 2000
title_full_unstemmed A crustal model along 39°S from a seismic refraction profile- ISSA 2000
title_sort crustal model along 39°s from a seismic refraction profile- issa 2000
publisher Servicio Nacional de Geología y Minería (SERNAGEOMIN)
publishDate 2003
url http://www.scielo.cl/scielo.php?script=sci_arttext&pid=S0716-02082003000100006
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