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Rock physics modeling for assessing gas hydrate and free gas: a case study in the Cascadia accretionary prism

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Abstract

We investigate the estimation of gas hydrate and free gas concentration using various rock physics models in the Cascadia accretionary prism, which is one of the most intensively studied regions of natural gas hydrate occurrences. Surface seismic reflection data is the most useful and cost-effective in deriving seismic velocity, and hence estimating gas hydrate and free gas across a BSR with depth, if a proper background (without gas hydrate and free gas) velocity is chosen. We have used effective medium theory of Helgerud et al. (EMTH) and, a combination of self-consistent approximation and differential effective medium (SCA-DEM) theory coupled with smoothing approximation for crystalline aggregate. Using the SCA-DEM (non-load-bearing) and EMTH (load-bearing) modeling, we calculate the average saturations of gas hydrate as 17 and 19%, respectively within ~100 m thick sedimentary column using velocity, derived from the surface seismic data. The saturations of gas hydrate are estimated as 15 and 18% using the SCA-DEM, and 20 and 25% using EMTH from the logging-while-drilling and wire-line sonic velocities, respectively. Estimations of gas hydrate from Poisson’s ratio are in average 50% for EMTH and 10% for SCA-DEM theory. We obtain the maximum saturation of free gas as 1–2% by employing the SCA-DEM theory either to seismic or sonic velocities, whereas the free-gas saturation varies between 0.1 and 0.4% for EMTH model. The gas hydrate saturation estimated from the sonic velocity and the free gas saturation derived from both the seismic and sonic velocities using the SCA-DEM modeling match quite well with those determined from the pressure core data in the study region.

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Acknowledgments

We are grateful to the Director, NGRI for his kind consent to publish this work, and two anonymous reviewers for their suggestions to improve the quality of the paper. The Ministry of Earth Sciences, Delhi and the Department of Science & Technology, Delhi are acknowledged for financial support to the gas hydrate program at NGRI.

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  1. National Geophysical Research Institute (Council of Scientific and Industrial Research), Uppal Road, Hyderabad, 500 606, India

    Kalachand Sain, Ranjana Ghosh & Maheswar Ojha

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  1. Kalachand Sain
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  2. Ranjana Ghosh
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Correspondence to Kalachand Sain.

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Sain, K., Ghosh, R. & Ojha, M. Rock physics modeling for assessing gas hydrate and free gas: a case study in the Cascadia accretionary prism. Mar Geophys Res 31, 109–119 (2010). https://doi.org/10.1007/s11001-010-9086-9

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