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Detalhes Referência

Tipo
Artigos em Revista

Tipo de Documento
Artigo Completo

Título
Is the Ibero-Armorican Arc primary or secondary? An analysis of the contraction required to form it by vertical axis rotation

Participantes na publicação
Josep Maria Casas (Author)
Joan Guimerà (Author)
Joaquina Alvarez-Marron (Author)
Ícaro Días da Silva (Author)
Dep. Geologia
IDL

Resumo
Different models have been proposed to explain the formation of the Ibero-Armorican Arc (IAA), as being primary or secondary (rotational). Secondary arc formation models require significant vertical axis rotations at the end of the Variscan orogeny. Estimates of the north-south (present coordinates) amount of contraction (horizontal shortening) needed for these rotations range from 54% to 91%, at the core or at the SE tip of the arc, near the present-day Mediterranean coast, respectively. These estimates are compared with coeval deformational structures developed in three areas of the orogen, one in the autochthonous hinterland in the southern branch of the arc, the second in the Cantabrian Zone foreland fold-and-thrust belt in the core of the arc, and the third in the SE continuation of the south branch of the Ibero- Armorican Arc, in the present-day Iberian Chain. From this analysis it follows that the shortening associated with late Variscan deformation is much less than that needed to explain the formation of the Ibero-Armorican Arc from a former linear orogen by means of vertical axis rotation. We therefore propose that the geometry of the arc should be re-evaluated. We discuss the paleomagnetic data purported to support the secondary origin, as well as the role of late-Variscan regional strike-slip faults in modifying the geometry of the Iberian and Armorican massifs. Our analysis suggests that the IAA formed mainly from a primary non-rotational margin-controlled curvature, slightly modified by ca. 5-20% of superposed contraction during late Carboniferous and/or Alpine times.

Data de Submissão/Pedido
2021-05-28
Data de Aceitação
2022-01-17
Data de Publicação
2022-01-21

Suporte
Journal of the Geological Society

Identificadores da Publicação
ISSN - 0016-7649

Editora
Geological Society of London

Página Final
065

Identificadores do Documento
DOI - https://doi.org/10.1144/jgs2021-065
URL - http://dx.doi.org/10.1144/jgs2021-065

Identificadores de Qualidade
SCIMAGO Q1 (2020) - 1.429 - Geology
Web Of Science Q2 (2020) - 3.8 - GEOSCIENCES, MULTIDISCIPLINARY - SCIE
Web Of Science Q2 (2019) - 3.100 - GEOSCIENCES, MULTIDISCIPLINARY - SCIE
SCOPUS Q1 (2019) - 5.2 - Geology
SCIMAGO Q1 (2019) - 1.532 - Geology
CITESCORE (2020 onward) Q1 (2020) - 5.7 - Geology


Exportar referência

APA
Josep Maria Casas, Joan Guimerà, Joaquina Alvarez-Marron, Ícaro Días da Silva, (2022). Is the Ibero-Armorican Arc primary or secondary? An analysis of the contraction required to form it by vertical axis rotation. Journal of the Geological Society, ISSN 0016-7649. eISSN . http://dx.doi.org/10.1144/jgs2021-065

IEEE
Josep Maria Casas, Joan Guimerà, Joaquina Alvarez-Marron, Ícaro Días da Silva, "Is the Ibero-Armorican Arc primary or secondary? An analysis of the contraction required to form it by vertical axis rotation" in Journal of the Geological Society, 2022. 10.1144/jgs2021-065

BIBTEX
@article{54258, author = {Josep Maria Casas and Joan Guimerà and Joaquina Alvarez-Marron and Ícaro Días da Silva}, title = {Is the Ibero-Armorican Arc primary or secondary? An analysis of the contraction required to form it by vertical axis rotation}, journal = {Journal of the Geological Society}, year = 2022, }