Crustal velocity structure of the Deccan Volcanic Province, Indian Peninsula, from observed surface wave dispersion

被引:4
|
作者
Suresh, Gaddale [1 ]
Teotia, Satbir S. [2 ]
Bhattacharya, Sankar N. [1 ]
机构
[1] Indian Meteorol Dept, Seismol Div, New Delhi, India
[2] Kurukshetra Univ, Dept Geophys, Kurukshetra 132119, Haryana, India
关键词
INVERSION; SUBCONTINENT;
D O I
10.4401/ag-6540
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Through inversion of fundamental mode group velocities of Love and Rayleigh waves, we study the crustal and subcrustal structure across the central Deccan Volcanic Province (DVP), which is one of the world's largest terrestrial flood basalts. Our analysis is based on broadband seismograms recorded at seismological station Bhopal (BHPL) in the central India from earthquakes located near west coast of India, with an average epicentral distance about 768 km. The recording station and epicentral zone are situated respectively on the northern and southern edges of DVP with wave paths across central DVP. The period of group velocity data ranges from 5 to 60 s for Rayleigh waves and 5 to 45 s for Love waves. Using the genetic algorithm, the observed data have been inverted to obtain the crust and subcrustal velocity structure along the wavepaths. Using this procedure, a similar velocity structure was also obtained earlier for the northwestern DVP, which is in the west of the present study region. Comparison of results show that the crustal thickness decreases westward from central DVP (39.6 km) to northwestern DVP (37.8 km) along with the decrease of thickness of upper crust; while the thickness of lower crust remains nearly same. From east to west S-wave velocity in the upper crust decreases by 2 to 3 per cent, while P-wave velocity in the whole crust and subcrust decreases by 3 to 6 per cent. The P- and S-wave velocities are positively correlated with crustal thickness and negatively correlated with earth's heat flow. It appears that the elevated crustal and subcrustal temperature in the western side is the main factor for low velocities on this side.
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页数:8
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