Tectonic shortening and gravitational spreading in the Gulf of Cadiz accretionary wedge: Observations from multi-beam bathymetry and seismic profiling

被引:38
作者
Gutscher, Marc-Andre [1 ]
Dominguez, Stephane [2 ]
Westbrook, Graham K. [3 ]
Gente, Pascal [1 ]
Babonneau, Nathalie [1 ]
Mulder, Thierry [4 ]
Gonthier, Eliane [4 ]
Bartolome, Rafael [5 ]
Luis, Joaquim [6 ]
Rosas, Filipe [7 ]
Terrinha, Pedro [8 ]
机构
[1] Univ Brest, CNRS, UMR Domaines Ocean 6538, Inst Univ Europeen Mer, F-29280 Plouzane, France
[2] Univ Montpellier 2, CNRS, F-34095 Montpellier 5, France
[3] Univ Birmingham, Birmingham B15 2TT, W Midlands, England
[4] Univ Bordeaux, EPOC, UMR5805, Bordeaux, France
[5] CMIMA, Barcelona, Spain
[6] Univ Algarve, Algarve, Portugal
[7] Univ Lisbon, IDL, P-1699 Lisbon, Portugal
[8] INETI, Dept Marine Geol, Alfragide, Portugal
关键词
Iberia; Morocco; Accretionary wedge; Decollement; Gravitational spreading; WESTERN MEDITERRANEAN RIDGE; PLATE BOUNDARY; LISBON-EARTHQUAKE; GIBRALTAR ARC; MUD VOLCANOS; GEODYNAMIC EVOLUTION; FRONTAL ACCRETION; EASTERN SEGMENT; SUBDUCTION ZONE; IBERIAN MARGIN;
D O I
10.1016/j.marpetgeo.2007.11.008
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
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 degrees each) indicate a very weak decollement layer, geometrically similar to the Mediterranean Ridge accretionary complex. Locally steep slopes (up to 10 degrees) 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 (C) 2008 Elsevier Ltd. All rights reserved
引用
收藏
页码:647 / 659
页数:13
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