Central Indian tectonics revisited using aeromagnetic data

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dc.contributor.author Rajaram, M.
dc.contributor.author Anand, S.P.
dc.date.accessioned 2015-07-06T11:00:59Z
dc.date.accessioned 2021-02-12T10:51:44Z
dc.date.available 2015-07-06T11:00:59Z
dc.date.available 2021-02-12T10:51:44Z
dc.date.issued 2003
dc.identifier.citation Earth Planets Space, v.55/4, p. e1-e4, 2003, doi: 10.1186/BF03351743 en_US
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/206
dc.description.abstract Aeromagnetic data, covering 600,000 km2 of Central India, have been analysed for the first time to throw light on the various tectonic blocks of the region, ranging in age from the Archean to the present. Existing geotectonic models are based on inadequate data and studies of relatively small regions. From the aeromagnetic data, we use the analytic signal and Euler deconvolution, to elucidate the subsurface structure of the region and redefine the tectonic elements. Contrary to the belief that the Central Indian shear defines the edge of the Central Indian craton, we find that the Sukinda thrust merges with the Tan shear to demarcate the edge of the Bastar and Eastern Ghat blocks by a shear that extends for approximately 1000 km in length. We call this the Main Peninsular shear. Magnetic anomaly data can thus play a crucial role in understanding the tectonic elements of a region with large surface cover. en_US
dc.language.iso en en_US
dc.subject Aeromagnetic anomalies en_US
dc.subject Analytic signal en_US
dc.subject Euler solutions en_US
dc.subject Peninsular India en_US
dc.subject Tectonic elements en_US
dc.title Central Indian tectonics revisited using aeromagnetic data en_US
dc.type Article en_US
dc.identifier.accession 090709


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