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gas hydrate - CCOP

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Q-values computed from the zero-offset Mallik data by the spectral ratio method are shown in<br />

Figure 7. The depths of reflections marked ‘A’, ‘B’, and ‘C’ in Figure 6 is indicated. As shown<br />

in Figure 7, the <strong>gas</strong> <strong>hydrate</strong> zone has low Q-factor and the variation in Q-factors matches very<br />

well with the boundaries of the <strong>gas</strong> <strong>hydrate</strong> zone. Moreover, at the depth of reflection ‘B’, the<br />

Q-factor becomes large compared to those of surrounding formations.<br />

Q-factor<br />

0 100 200 300 400 500<br />

500<br />

600<br />

Depth (m)<br />

700<br />

800<br />

900<br />

1000<br />

Top of <strong>gas</strong> <strong>hydrate</strong> zone<br />

Coal seam in <strong>gas</strong> <strong>hydrate</strong> zone<br />

1100<br />

Bottom of <strong>gas</strong> <strong>hydrate</strong> zone<br />

1200<br />

Figure 7. Q factors extracted from the zero-offset VSP data at Mallik 3L-38 well<br />

by using the spectral ratio method.<br />

Frequency-dependent Q-factors were computed by the modified spectral ratio method for the<br />

Mallik zero-offset data although the results are not shown here. The Q-factors for all layers<br />

showed lower values compared to those obtained by the spectral ratio method. Further<br />

preprocessing and analysis are needed to get more precise Q-factors by the modified spectral<br />

ratio method.<br />

CONCLUSIONS<br />

The algorithm of the spectral ratio method and the modified spectral method were developed<br />

and applied to synthetic data sets and the zero-offset data at Mallik 3L-38 <strong>gas</strong> <strong>hydrate</strong><br />

production research well. The frequency-independent Q-factors from the synthetic data<br />

obtained by using the spectral ratio method provide the information on the pattern of the<br />

change in Q-factors along the depth. While the computed Q-factors approach the true values<br />

for the layers of low Q-factors, they deviate from the true values for the layers of high Q-<br />

factors. In the layers with large Q values, the differences of the frequency spectrums of traces<br />

are very small and it makes the computation of Q-factors very unstable. The variation of the<br />

Q-factors extracted from the zero-offset VSP data at Mallik 3L-38 well by the spectral ratio<br />

method agrees well with the boundaries of the layers, including the <strong>gas</strong> <strong>hydrate</strong> zone,<br />

described in the reflection image. The results of applying the modified spectral ratio method,<br />

which provides frequency-dependent Q-factors, show very unstable Q-factors for some layers<br />

in the synthetic data and the Mallik data. Further analysis and research are required to obtain<br />

more precise Q-factors by the modified spectral ratio method.<br />

New Energy Resources in the <strong>CCOP</strong> Region - Gas Hydrates and Coalbed Methane 41

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