Moho depth and equivalent elastic thickness of the lithosphere over the Vema Channel: A new evidence of an aborted ridge
Autor(a) principal: | |
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Data de Publicação: | 2018 |
Outros Autores: | , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1016/j.jsames.2017.12.011 http://hdl.handle.net/11449/179701 |
Resumo: | We investigate the Vema Channel in terms of spatial variations of the elastic thickness (Te) in the frame of the thin plate flexure model using the convolutive method. The modeling of the Moho in terms of the thin plate flexure model is done by a least squares approximation of the Moho obtained from gravity inversion. The flexure is calculated by the convolution of the crustal load with the point-load flexure response curves. The RMS difference between the gravity and flexure Moho surfaces is minimized by varying the Te by inverse modeling. The result is a solution of the flexed crust that is in best agreement with the long-wavelength component of the gravity field. The flexure Moho depths vary between 12 and 18 km and agree well with those obtained from gravity inversion. The spatial variations of Te range from 2 to 30 km and have a good correlation with the geological interpretation for an aborted ridge near Vema Channel, called in this paper as the Vema Aborted Ridge (VAR). The occurring of seamounts appears to be correlated to a weak and deformed region. Attempts of crustal breakup are marked by high Te values (30 km) while lower values (3–12 km) are found for the suggested aborted ridge. The VAR is on Isochron of 93 Ma and shows symmetrical older along both sides of its axis. Asymmetric magnetic anomalies are found over the ridge and may be related to upper-extended continental crust broken by the Vema. |
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Moho depth and equivalent elastic thickness of the lithosphere over the Vema Channel: A new evidence of an aborted ridgeAborted ridgeExtinct spreading centerFlexural analysisFlexural rigiditySouth Atlantic evolutionWe investigate the Vema Channel in terms of spatial variations of the elastic thickness (Te) in the frame of the thin plate flexure model using the convolutive method. The modeling of the Moho in terms of the thin plate flexure model is done by a least squares approximation of the Moho obtained from gravity inversion. The flexure is calculated by the convolution of the crustal load with the point-load flexure response curves. The RMS difference between the gravity and flexure Moho surfaces is minimized by varying the Te by inverse modeling. The result is a solution of the flexed crust that is in best agreement with the long-wavelength component of the gravity field. The flexure Moho depths vary between 12 and 18 km and agree well with those obtained from gravity inversion. The spatial variations of Te range from 2 to 30 km and have a good correlation with the geological interpretation for an aborted ridge near Vema Channel, called in this paper as the Vema Aborted Ridge (VAR). The occurring of seamounts appears to be correlated to a weak and deformed region. Attempts of crustal breakup are marked by high Te values (30 km) while lower values (3–12 km) are found for the suggested aborted ridge. The VAR is on Isochron of 93 Ma and shows symmetrical older along both sides of its axis. Asymmetric magnetic anomalies are found over the ridge and may be related to upper-extended continental crust broken by the Vema.Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)São Paulo State University – UNESP Institute of Geosciences and Exact Sciences, C.P. 178Geological Survey of Brazil – CPRM/DISEGESão Paulo State University – UNESP/UNESPetro Institute of Geosciences and Exact Sciences, C.P. 178São Paulo State University – UNESP Institute of Geosciences and Exact Sciences, C.P. 178São Paulo State University – UNESP/UNESPetro Institute of Geosciences and Exact Sciences, C.P. 178CAPES: 88887.091710 2014-01Universidade Estadual Paulista (Unesp)Geological Survey of Brazil – CPRM/DISEGEConstantino, Renata Regina [UNESP]Costa, Iago Sousa LimaHackspacher, Peter Christian [UNESP]de Souza, Iata Anderson [UNESP]2018-12-11T17:36:25Z2018-12-11T17:36:25Z2018-03-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article133-142application/pdfhttp://dx.doi.org/10.1016/j.jsames.2017.12.011Journal of South American Earth Sciences, v. 82, p. 133-142.0895-9811http://hdl.handle.net/11449/17970110.1016/j.jsames.2017.12.0112-s2.0-850443958252-s2.0-85044395825.pdf10401359359087340000-0003-2125-3050Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengJournal of South American Earth Sciences0,829info:eu-repo/semantics/openAccess2023-10-28T06:07:45Zoai:repositorio.unesp.br:11449/179701Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T16:15:13.458144Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Moho depth and equivalent elastic thickness of the lithosphere over the Vema Channel: A new evidence of an aborted ridge |
title |
Moho depth and equivalent elastic thickness of the lithosphere over the Vema Channel: A new evidence of an aborted ridge |
spellingShingle |
Moho depth and equivalent elastic thickness of the lithosphere over the Vema Channel: A new evidence of an aborted ridge Constantino, Renata Regina [UNESP] Aborted ridge Extinct spreading center Flexural analysis Flexural rigidity South Atlantic evolution |
title_short |
Moho depth and equivalent elastic thickness of the lithosphere over the Vema Channel: A new evidence of an aborted ridge |
title_full |
Moho depth and equivalent elastic thickness of the lithosphere over the Vema Channel: A new evidence of an aborted ridge |
title_fullStr |
Moho depth and equivalent elastic thickness of the lithosphere over the Vema Channel: A new evidence of an aborted ridge |
title_full_unstemmed |
Moho depth and equivalent elastic thickness of the lithosphere over the Vema Channel: A new evidence of an aborted ridge |
title_sort |
Moho depth and equivalent elastic thickness of the lithosphere over the Vema Channel: A new evidence of an aborted ridge |
author |
Constantino, Renata Regina [UNESP] |
author_facet |
Constantino, Renata Regina [UNESP] Costa, Iago Sousa Lima Hackspacher, Peter Christian [UNESP] de Souza, Iata Anderson [UNESP] |
author_role |
author |
author2 |
Costa, Iago Sousa Lima Hackspacher, Peter Christian [UNESP] de Souza, Iata Anderson [UNESP] |
author2_role |
author author author |
dc.contributor.none.fl_str_mv |
Universidade Estadual Paulista (Unesp) Geological Survey of Brazil – CPRM/DISEGE |
dc.contributor.author.fl_str_mv |
Constantino, Renata Regina [UNESP] Costa, Iago Sousa Lima Hackspacher, Peter Christian [UNESP] de Souza, Iata Anderson [UNESP] |
dc.subject.por.fl_str_mv |
Aborted ridge Extinct spreading center Flexural analysis Flexural rigidity South Atlantic evolution |
topic |
Aborted ridge Extinct spreading center Flexural analysis Flexural rigidity South Atlantic evolution |
description |
We investigate the Vema Channel in terms of spatial variations of the elastic thickness (Te) in the frame of the thin plate flexure model using the convolutive method. The modeling of the Moho in terms of the thin plate flexure model is done by a least squares approximation of the Moho obtained from gravity inversion. The flexure is calculated by the convolution of the crustal load with the point-load flexure response curves. The RMS difference between the gravity and flexure Moho surfaces is minimized by varying the Te by inverse modeling. The result is a solution of the flexed crust that is in best agreement with the long-wavelength component of the gravity field. The flexure Moho depths vary between 12 and 18 km and agree well with those obtained from gravity inversion. The spatial variations of Te range from 2 to 30 km and have a good correlation with the geological interpretation for an aborted ridge near Vema Channel, called in this paper as the Vema Aborted Ridge (VAR). The occurring of seamounts appears to be correlated to a weak and deformed region. Attempts of crustal breakup are marked by high Te values (30 km) while lower values (3–12 km) are found for the suggested aborted ridge. The VAR is on Isochron of 93 Ma and shows symmetrical older along both sides of its axis. Asymmetric magnetic anomalies are found over the ridge and may be related to upper-extended continental crust broken by the Vema. |
publishDate |
2018 |
dc.date.none.fl_str_mv |
2018-12-11T17:36:25Z 2018-12-11T17:36:25Z 2018-03-01 |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://dx.doi.org/10.1016/j.jsames.2017.12.011 Journal of South American Earth Sciences, v. 82, p. 133-142. 0895-9811 http://hdl.handle.net/11449/179701 10.1016/j.jsames.2017.12.011 2-s2.0-85044395825 2-s2.0-85044395825.pdf 1040135935908734 0000-0003-2125-3050 |
url |
http://dx.doi.org/10.1016/j.jsames.2017.12.011 http://hdl.handle.net/11449/179701 |
identifier_str_mv |
Journal of South American Earth Sciences, v. 82, p. 133-142. 0895-9811 10.1016/j.jsames.2017.12.011 2-s2.0-85044395825 2-s2.0-85044395825.pdf 1040135935908734 0000-0003-2125-3050 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Journal of South American Earth Sciences 0,829 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
133-142 application/pdf |
dc.source.none.fl_str_mv |
Scopus reponame:Repositório Institucional da UNESP instname:Universidade Estadual Paulista (UNESP) instacron:UNESP |
instname_str |
Universidade Estadual Paulista (UNESP) |
instacron_str |
UNESP |
institution |
UNESP |
reponame_str |
Repositório Institucional da UNESP |
collection |
Repositório Institucional da UNESP |
repository.name.fl_str_mv |
Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP) |
repository.mail.fl_str_mv |
|
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1808128624474193920 |