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Tectonic shortening and gravitational spreading in the Gulf of Cadiz accretionary wedge: Observations from multi-beam bathymetry and seismic profiling
Authors:Marc-André Gutscher  Stephane Dominguez  Graham K. Westbrook  Pascal Gente  Nathalie Babonneau  Thierry Mulder  Eliane Gonthier  Rafael Bartolome  Joaquim Luis  Filipe Rosas  Pedro Terrinha
Affiliation:1. Department of Earth Sciences, Utrecht University, Utrecht, Netherlands;2. Repsol, Madrid, Spain;3. ONHYM, Rabat, Morocco;4. Department of Geology, University of Salamanca, Salamanca, Spain;1. IDL – Instituto Dom Luíz, Faculdade de Ciências da Universidade de Lisboa, Edifício C1, Campo Grande, 1749-016 Lisboa, Portugal;2. IPMA – Instituto Português do Mar e da Atmosfera, Rua C do Aeroporto, 1749-077 Lisboa, Portugal;3. EMEPC – Estrutura de Missão para a Extensão da Plataforma Continental, Rua Costa Pinto 65, 2770-047 Paço de Arcos, Portugal;4. CSIC, Instituto de Ciencias del Mar, GMC, Passeig Marítim de la Barceloneta 37-49, E-08003 Barcelona, Spain;5. IGME – Instituto Geológico y Minero de España, Rios Rosas 23, 28003 Madrid, Spain;1. Univ. Lille, CNRS, Univ. Littoral Cote d''Opale, UMR 8187, LOG, Laboratoire d''Océanologie et de Géosciences, F-59 000 Lille, France;2. Instituto Oceanográfico de la Armada (INOCAR), Av. 25 de Julio, Guayaquil, Ecuador
Abstract:The Gulf of Cadiz lies astride the complex plate boundary between Africa and Eurasia west of the Betic-Rif mountain belt. We report on the results of recent bathymetric swathmapping and multi-channel seismic surveys carried out here. The seafloor is marked by contrasting morphological provinces, spanning the SW Iberian and NW Moroccan continental margins, abyssal plains and an elongate, arcuate, accretionary wedge. A wide variety of tectonic and gravitational processes appear to have shaped these structures. Active compressional deformation of the wedge is suggested by folding and thrusting of the frontal sedimentary layers as well as basal duplexing in deeper internal units. There is evidence for simultaneous gravitational spreading occurring upslope. The very shallow mean surface and basal slopes of the accretionary wedge (1° each) indicate a very weak decollement layer, geometrically similar to the Mediterranean Ridge accretionary complex. Locally steep slopes (up to 10°) indicate strongly focused, active deformation and potential gravitational instabilities. The unusual surface morphology of the upper accretionary wedge includes “raft-tectonics” type fissures and abundant sub-circular depressions. Dissolution and/or diapiric processes are proposed to be involved in the formation of these depressions.
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