这样的分布是很不寻常的，因为银河中心区域的气体是相对均匀的分布。
Such a distribution is highly unusual because gas in the inner region of the galaxy is relatively evenly distributed.
来自地震剖面的强烈反映表明在气体水合物区域的基础之上存在不均匀受力的情况。
Strong reflections from seismic profiles indicate a discontinuity at the base of the gas hydrate zone.
当气体介质等温、均匀时，分别计算气体介质的普朗克平均吸收系数、有效吸收系数和壁面入射平均吸收系数。
While the gas medium is isothermal uniformed, the dissertation calculates the effective absorption coefficient, the Planck-mean absorption coefficient and the wall-incident mean coefficient.
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