Geothermal investigations in the 1993 Latur earthquake area, Deccan Volcanic Province, India

Authors
Citation
S. Roy et Rum. Rao, Geothermal investigations in the 1993 Latur earthquake area, Deccan Volcanic Province, India, TECTONOPHYS, 306(2), 1999, pp. 237-252
Citations number
63
Categorie Soggetti
Earth Sciences
Journal title
TECTONOPHYSICS
ISSN journal
00401951 → ACNP
Volume
306
Issue
2
Year of publication
1999
Pages
237 - 252
Database
ISI
SICI code
0040-1951(19990615)306:2<237:GIIT1L>2.0.ZU;2-M
Abstract
Heat flow measurements have been made in four boreholes in the epicentral a rea of the Latur earthquake (M-w 6.2, 1993) in the southeastern part of the Cretaceous-Eocene Deccan Volcanic Province (DVP), central India. Three of these, located 4 to 8 km from the surface rupture zone near Killari, were a bout 180 m deep and yielded heat flow values in the range 33 to 40 mW m(-2) . A hole was specially drilled in the surface rupture zone and penetrating the entire 338 m Deccan basalt cover and a further 271 m into the Archaean granite-gneiss basement. Temperature gradients over both the basaltic as we ll as the ganite-gneiss sections, which have a large thermal conductivity c ontrast, yielded a consistent heat flow value of 43 mW m(-2). Earlier measu rements at Koyna, the site of another stable continental region (SCR) earth quake (M-w 6.3, 1967) in the western part of the DVP, and at another locali ty, Loner, in the central part of the DVP had yielded heat flow values of 4 1 mW m(-2) and 47 mW m(-2), respectively. Thus the southern part of the DVP is characterised by a low heat flow regime, similar to that over the Archa ean Dhanwar province immediately to the south. The 617 m deep hole at Killa ri provided an opportunity for carrying out measurements of radioactive hea t production on core samples of the 271 m long basement section. Thirty-nin e core samples of the migmatitic gneisses and the granites encountered in t he 271 m long basement section of KLR-1 were analysed for U, Th and K, and resulted in estimates of heat production of 0.5 and 2.6 mu W m(-3), respect ively, for the two types. A crustal heat production model is envisaged, wit h the thicknesses of the gneisses and the granites constrained from availab le pressure estimates in the Dharwar craton, and also considering a 17 km ' granitic' upper crust and a 20 km 'granulitic' lower crust based on deep se ismic sounding data. Using this crustal heat production model and the heat flow value of 43 mW m(-2), the estimated crustal temperatures imply a deep (>30 km) brittle-ductile transition. Even though heat flow-crustal temperat ure considerations allow for deeper, crustal earthquake foci, most of the M -w > 6 events of the last three decades in the Australian and Indian SCRs s how shallow foci (<10 km). This calls for seeking possible mechanisms for f rictional failure to take place in the top part of a crust which is largely brittle. (C) 1999 Elsevier Science B.V. All rights reserved.