Abstract
The Curie depth map of India compiled from MAGSAT data has been used for preparing the lithosphere thickness and the surface heat flow density maps of the Indian Craton, utilizing the concept of magnetothermometry. The lithosphere thicknesses of the major Indian geological units/provinces, as obtained from the prepared map, are found to be in reasonably good agreement with the previously published values for these regions. Also, the surface heat flow density values obtained from the prepared maps closely follow the previously published results. The maps are useful in providing first order estimates of lithosphere thickness and surface heat flow density of the important geological units/provinces of India.
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References
Gupta, M.L., S.B. Singh, S.R. Sharma and V.K. Saxena, 1982, Geothermal studies in Peninsular India and parts of Himalaya, Geophys. Res. Bull. 20, 293–305.
Mahadevan, T.M., 1994, Deep continental structure of the India: A review, Geol. Soc. Ind. Mem. 28, 33–97.
Mayhew, A.M., 1982, Application of satellite magnetic anomaly data to Curie isotherm mapping, J. Geophys. Res. 87, 4846–4854.
Mishra, D.C., 1984, Magnetic anomalies — the India and Antarctica, Earth Planet. Sci. Lett. 71, 173–180.
Negi, J.G., P.K. Agarwal and O.P. Pandey, 1987, Large variation of Curie depth and lithospheric thickness beneath the Indian subcontinent and a case for magnetothermometry, Geophys. J. Roy. Astron. Soc. 88, 763–775.
Shankar, R., 1988, Heat flow map of the India and discussions on its geological and economic significance, The Indian Minerals 48, 89–110.
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Sarkar, R.K., Saha, D.K. A note on the lithosphere thickness and heat flow density of the Indian Craton from MAGSAT data. Acta Geophys. 54, 198–204 (2006). https://doi.org/10.2478/s11600-006-0017-8
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DOI: https://doi.org/10.2478/s11600-006-0017-8