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Ccte d'Ivoire-Ghana margin: seismic imaging of passive rifted crust adjacent to a transform continental margin
Authors:C Peirce  R B Whitmarsh  R A Scrutton  B Pontoise  F Sage  J Mascle
Institution:Department of Geological Sciences, University of Durham, Science Laboratories, South Road, Durham, DH1 3LE, UK;Institute of Oceanographic Sciences, Deacon Laboratory, Brook Road, Wormley, Godalming, Surrey, GU8 5UB, UK;Department of Geology and Geophysics, Grant Institute, West Mains Road, Edinburgh, EH9 3JW, UK;ORSTOM—Laboratoire de Géodynamique sous Marine, BP 48, 06230 Villefranche sur mer, France;GEMCO—Laboratoire de Géodynamique sous Marine, BP 48, 06230 Villefranche sur mer, France
Abstract:During May 1990 and January-February 1991, an extensive geophysical data set was collected over the Côte d'Ivoire-Ghana continental margin, located along the equatorial coast of West Africa. The Ghana margin is a transform continental margin running subparallel to the Romanche Fracture Zone and its associated marginal ridge—the Côte d'Ivoire-Ghana Ridge. From this data set, an explosive refraction line running ~ 150 km, ENE-WSW between 3°55'N, 3°21'W and 4°23'N, 2°4'W, has been modelled together with wide-angle airgun profiles, and seismic reflection and gravity data. This study is centred on the Côte d'Ivoire Basin located just to the north of the Côte d'Ivoire-Ghana Ridge, where bathymetric data suggest that a component of normal rifting occurred, rather than the transform motion observed along the majority of the equatorial West African margin.
Traveltime and amplitude modelling of the ocean-bottom seismometer data shows that the continental Moho beneath the margin rises in an oceanward direction, from ~ 24 km below sea level to ~ 17 km. In the centre of the line where the crust thins most rapidly, there exists a region of anomalously high velocity at the base of the crust, reaching some 8 km in thickness. This higher-velocity region is thought to represent an area of localized underplating related to rifting. Modelling of marine gravity data, collected coincident with the seismic line, has been used to test the best-fitting seismic model. This modelling has shown that the observed free-air anomaly is dominated by the effects of crustal thickness, and that a region of higher density is required at the base of the crust to fit the observed data. This higher-density region is consistent in size and location with the high velocities required to fit the seismic data.
Keywords:continental margin  Côte d'Ivoire-Ghana  OBS  seismic structure
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