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Assessment of gas-hydrate saturations in the Makran accretionary prism using the offset dependence of seismic amplitudes
2010
Geophysics
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11 We estimate the saturations of gas hydrate and free gas based on measurements of 12 seismic reflection amplitude versus offset (AVO) for a bottom simulating reflector (BSR) 13 coupled with rock physics modeling. We apply the approach to data from a seismic line in the 14 Makran accretionary prism in the Arabian Sea. The results reveal lateral variations of gas 15 hydrate and free gas saturations between 4-29% and 1-7.5%, respectively, depending on the 16 rock physics model used to relate
doi:10.1190/1.3315861
fatcat:4ppxvam5e5f4nhpo2vfqsx6bui