A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2018; you can also visit the original URL.
The file type is
Assessment of gas-hydrate saturations in the Makran accretionary prism using the offset dependence of seismic amplitudes
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 relatedoi:10.1190/1.3315861 fatcat:4ppxvam5e5f4nhpo2vfqsx6bui