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dc.contributor.authorKrishna, K.S.
dc.contributor.authorMurty, G.P.S.
dc.contributor.authorSrinivas, K.
dc.contributor.authorRao, D.G.
dc.date.accessioned2009-05-08T11:56:16Z
dc.date.available2009-05-08T11:56:16Z
dc.date.issued1992
dc.identifier.citationGeo-Marine Letters, Vol.12; 7-13p.
dc.identifier.urihttp://drs.nio.org/drs/handle/2264/3031
dc.description.abstractThe northern parts of the Prathap and Laccadive Ridge system, eastern Arabian Sea, consist of three parallel basement ridge peaks at varied depths. The topographic highs are associated with either well developed or subdued magnetic signatures. Model studies, constrainEd. by seismic results, determine the varied nature and depth to the top of the causative basement bodies. Similarities of the geophysical signatures of the ridges and their structural resemblance perhaps point to their common origin. Hence we propose that the Prathap Ridge complex may be a part of the Chagos-Laccadive Ridge system and formed because of the Reunion hotspot activity
dc.language.isoen
dc.publisherSpringer
dc.rightsCopyright [1992]. All efforts have been made to respect the copyright to the best of our knowledge. Inadvertent omissions, if brought to our notice, stand for correction and withdrawal of document from this repository.
dc.titleMagnetic studies over the northern extension of the Prathap ridge complex, eastern Arabian sea
dc.typeJournal Article


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