DI029-0002
A radially anisotropic Shear wave velocity structure of the Himalaya

Wednesday, 16 December 2020
Poster
Rupak Banerjee, Indian Institute of Science Education and Research Kolkata, Kolkata, India, Shubham Sharma, Helmholtz Centre Potsdam GFZ German Research Centre for Geosciences, Potsdam, Germany, Supriyo Mitra, Indian Institute of Science Education and Research Kolkata, Department of Earth Sciences, Kolkata, India and Sn Bhattacharya, Lihospheric Study Centre, New Delhi, India
Abstract:
A precise shear wave velocity (Vs) structure is a first-order proxy to understand the structural, thermal and deformational configurations of the lithosphere. We use surface wave data from the Dolakha Nepal earthquake recorded by 8 stations in Jammu and Kashmir Himalaya (JAKSNET) to compute fundamental mode Rayleigh and Love wave dispersion curves. We perform joint inversion of the two datasets to obtain radially anisotropic shear-wave velocity model (VSH and VSV) for the Himalayan lithosphere. Dispersion curves have been computed between 15 and 90 s period using the multiple filter analysis. The individual source-receiver dispersion curves have been averaged by error weighting to obtain the mean and standard deviation at discrete periods. The starting model for the joint inversion is constructed by combining CRUST1.0 and PREM, for the crust and upper mantle structure, respectively. In the inversion, the model space is exhaustively explored using Genetic Algorithms (GA), and the synthetic dispersion curves are computed using Thomson-Haskell method with reduced delta matrix, where depth decay factors (r1 and r2) are complex conjugates. The free parameters in the inversion are horizontally polarized compressional and shear wave velocities (VPH and VSH), layer thickness (h) and Vs anisotropy represented by Xi (ξ=VSH2/VSV2). The misfit between the calculated and observed datasets are iteratively minimised to obtain the best fitting model. Results reveal variation of ξ as a function of depth. The lower crust has ξ<1, which results from VSV being faster than VSH. However, in the upper mantle ξ >1, and hence VSH is greater than VSV. This change of ξ from the lower crust to the upper mantle points to deformational decoupling.