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A 3D velocity model built by a joint Bayesian inversion of over 20 years of radial receiver functions and ambient noise Rayleigh waves. The model includes velocity uncertainties in the crust and upper mantle and is intended as a foundation for future higher-resolution models. It was authored by Bin He and last updated in May 2026.
Data files are in NC, PY, TXT, DAT, and GZ formats; users may need specific tools to process these.