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Short Note |
1 Bullard Laboratories
University of
Cambridge
Cambridge CB3 OEZ, United Kingdom
(S.M., K.P.)
2 Indian Institute of
Astrophysics
Bangalore, India 560 037
(V.K.G.)
3 Center for Mathematical Modelling and
Computer Simulations
Bangalore, India 560 037
(V.K.G.)
4 National Geophysical Research
Institute
Hyderabad, India 500 007
(S.S.R.)
* Present address: Department of Geology and Geophysics, Indian Institute of Technology, Kharagpur, India 721 302.
We investigate the upper mantle shear-wave speed structure beneath the south
Indian shield by measuring and modeling fundamental mode Rayleigh wave
phase-velocity dispersion. Observed phase velocities for the south Indian shield
closely match those observed for the Canadian shield. We constrain the south
Indian crust using published receiver function results and invert the dispersion
data for upper mantle shear-wave structure. The
155-km-thick seismic
lithosphere of the south Indian shield is composed of a 35 km-thick, two-layer
crust and a
120-km-thick, high-velocity upper mantle lid. Beneath the Moho
the average Sn wave speed is
4.7 km
sec1. Both Sn travel times data and the
dispersion data suggest a positive sub-Moho shear-wave speed gradient. Beneath
the seismic lithosphere there is a low- velocity layer where the shear-wave
speed drops to
4.4 km sec1.
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