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IUGG XXIV General Assembly July 2-13, 2007 Perugia, Italy<br />

(S) - <strong>IASPEI</strong> - International Association of Seismology and Physics of the Earth's<br />

Interior<br />

JSS016 Poster presentation 2355<br />

Gas-hydrates: a future potential source of energy in India<br />

Dr. Kalachand Sain<br />

Marine Geophysical Group National Geophysical Research Institute<br />

KALACHAND SAIN National Geophysical Research Institute, Uppal Road, Hyderabad - 500 007, India<br />

The energy-demand in developing countries like is growing very fast compared to industrial countries of<br />

the world. At present we import more than ~70% of our energy requirement and major discovery of<br />

hydrocarbons have not taken place during the last couple of decades. Since the economic growth with<br />

our huge population depends heavily on the energy security, we are desperately looking for an alternate<br />

form of energy. Gas-hydrates seem to be the best alternative. Gas-hydrates are crystalline from of<br />

water and low molecular weight hydrocarbons (mainly methane), and are formed at high pressure and<br />

low temperature in the outer continental margins and permafrost regions. These have attracted the<br />

global attention due to their wide-spread occurrences and potential as future major energy resources.<br />

Parameters such as bathymetry, seafloor temperature, sedimentary thicknesses, rate of sedimentation,<br />

total organic carbon content etc. indicate good prospects of gas-hydrates in the huge continental<br />

margins of . The methane gas stored in the form of gas-hydrates and underlying free-gas within our<br />

exclusive economic zone is estimated to be of the order of trillion meter cube, which can take care of<br />

our energy requirements for several tens of decades. The National Gas Hydrates Programs under the<br />

aegis of the Ministry of Petroleum & Natural Gas and the Ministry of Earth Sciences have initiated a lot<br />

of scientific plans and technological advancement for the exploration and exploitation of gas-hydrates.<br />

As a member of the national program, we are mainly involved in finding out the prospective zones and<br />

evaluating the resource potential using geophysical (seismic) data. Gas-hydrates are mostly detected by<br />

identifying an anomalous reflector, known as the bottom simulating reflectors or BSR on seismic data<br />

based on its characteristic features. We identified BSRs on available seismic data in the Kerala-Konkon,<br />

Krishna-Godavari andMahanadi basins and the Andaman region. The recent drilling expedition at the<br />

identified locations of gas-hydrates occurrences delineated a rich gas-hydrates deposit in the Krishna-<br />

Godavari basin. The Mahanadi basin and the Andaman region have been found very prospective for<br />

gas-hydrates. Much of the deep-water regions are yet to be explored. New data sets with suitable<br />

parameters are to be acquired to comprehend the lateral/areal extension of gas-hydrates, and assess<br />

their resource potential along the margins of Indian continent. As gas-hydrates are not stable at NTP,<br />

the existing technique, generally used for conventional hydrocarbons, cannot be used for exploitation. A<br />

concerted effort is going on in this direction. With the growth of technology, it is expected that methane<br />

from below the gas-hydrates can be exploited economically in near future. It may take a decade or so<br />

to produce gas from gas-hydrates. Therefore, it is high time to map the prospective zones of gashydrates<br />

and evaluate the resource potential. For this purpose, we have developed several seismic tools<br />

like traveltime tomography; waveform inversion; AVO inversion; AVO attributes; quality factors, seismic<br />

attributes etc. and will demonstrate their application to multi-channel marine seismic reflection data. We<br />

will also show that studies of quality factor and proxies like pockmark and gas escape features (like<br />

faulting or gas-chimney) offer indirect evidences for the identification of gas-hydrates in absence of<br />

BSR. As pure gas-hydrates have much higher seismic velocities than that of host sediments, presence of<br />

gas-hydrates increases seismic velocities, whereas free-gas below the hydrates-bearing sediments<br />

reduces the seismic velocity. Thus estimating accurate velocities using waveform tomography followed<br />

by rock physics modeling or invoking effective medium theory provide an excellent tool for quantifying<br />

gas-hydrates and/or free-gas across a BSR.

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