dc.contributor.author | Bhattacharya, G.C. | |
dc.contributor.author | Chaubey, A.K. | |
dc.contributor.author | Murty, G.P.S. | |
dc.contributor.author | Rao, D.G. | |
dc.contributor.author | Scherbakov, V.S. | |
dc.contributor.author | Lygin, V.A. | |
dc.contributor.author | Philipenko, A.I. | |
dc.contributor.author | Bogomyagkov, A.P. | |
dc.date.accessioned | 2009-05-08T11:56:19Z | |
dc.date.available | 2009-05-08T11:56:19Z | |
dc.date.issued | 1992 | |
dc.identifier.citation | Oceanogarphy of the Indian Ocean. Ed. by: Desai, B.N., 503-509p. | |
dc.identifier.uri | http://drs.nio.org/drs/handle/2264/3037 | |
dc.description.abstract | Based on the analysis of some additional magnetic profiles, an updated correlation and identification of the sea-floor spreading type magnetic lineations in the northeastern Arabian Sea is presented. The anomaly 24 A-B sequence, characterisEd. by double troughed shape, is the most conspicuous anomaly identifiable across the entire area. Identification and correlation is suggested for: (1) well developed anomaly 23, and (2) some of the hitherto unidentified isolated prominent anomalies, which were considered to be of sea-floor spreading origin by earlier workers. A new fracture zone is proposed west of 64 degrees E long. and minor alteration in the locations of the previously postulated fracture zones is suggested. Estimated half spreading rates between anomalies 23 and 28 vary from 4.5 to 9.1 cm y sup(-1) | |
dc.language.iso | en | |
dc.publisher | Oxford and IBH, New Delhi | |
dc.rights | Copyright [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.title | Marine magnetic anomalies in the northeastern Arabian Sea | |
dc.type | Conference Article | |