首页> 外文期刊>American Journal of Science >GENERALIZATION OF GAS HYDRATE DISTRIBUTION AND SATURATION IN MARINE SEDIMENTS BY SCALING OF THERMODYNAMIC AND TRANSPORT PROCESSES
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GENERALIZATION OF GAS HYDRATE DISTRIBUTION AND SATURATION IN MARINE SEDIMENTS BY SCALING OF THERMODYNAMIC AND TRANSPORT PROCESSES

机译:通过热力学和运输过程的尺度化来估算海洋沉积物中的天然气水合物分布和饱和度

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Gas hydrates dominated by methane naturally occur in deep marine sediment along continental margins. These compounds form in pore space between the seafloor and a sub-bottom depth where appropriate stability conditions prevail. However, the amount and distribution of gas hydrate within this zone, and free gas below, can vary significantly at different locations. To understand this variability, we develop a one-dimensional numerical model that simulates the accumulation of gas hydrates in marine sediments due to upward and downward fluxes of methane over time. The model contains rigorous thermodynamic and component mass balance equations that are solved using expressions for fluid flow in compacting sediments. The effect of salinity on gas hydrate distribution is also included. The simulations delineate basic modes of gas hydrate distribution in marine sediment, including systems with no gas hydrate, gas hydrate without underlying free gas, and gas hydrate with underlying free gas below the gas hydrate stability zone, for various methane sources. The results are scaled using combinations of dimensionless variables, particularly the Peclet number and Damkohler number, such that the dependence of average hydrate saturation on numerous parameters can be summarized using two contour maps, one for a biogenic source and one for upward flux from a deeper source. Simulations also predict that for systems at steady state, large differences in parameters like seafloor depth, seafloor temperature and geothermal gradient cause only small differences in average hydrate saturation when examined with scaled variables, although important caveats exist. Our model presents a unified picture of hydrate accumulations that can be used to understand well-characterized gas hydrate systems or to predict steady-state average hydrate saturation and distribution at locations for which seismic or core data are not available.
机译:甲烷为主的天然气水合物自然存在于大陆边缘的深海沉积物中。这些化合物形成在海底和次要深度之间的孔隙空间中,其中适当的稳定性条件占优势。但是,该区域内气体水合物的数量和分布以及下方的游离气体在不同位置可能有很大差异。为了理解这种可变性,我们开发了一个一维数值模型,该模型可以模拟由于甲烷随时间向上和向下流动而在海洋沉积物中产生的天然气水合物。该模型包含严格的热力学和组分质量平衡方程,可使用压实沉积物中的流体流动表达式来求解。盐度对天然气水合物分布的影响也包括在内。该模拟描述了海洋沉积物中气体水合物分布的基本模式,包括对于各种甲烷源而言,无气体水合物的系统,没有底层自由气的天然气水合物以及在天然气水合物稳定区以下的带有底层自由气的天然气水合物。使用无因次变量(尤其是Peclet数和Damkohler数)的组合对结果进行缩放,以便可以使用两个等高线图来总结平均水合物饱和度对众多参数的依赖性,其中一个用于生物源,一个用于从深处向上的通量。资源。模拟还预测,对于处于稳态的系统,使用比例变量进行检查时,海底深度,海底温度和地热梯度等参数的较大差异仅会导致平均水合物饱和度的较小差异,尽管存在一些重要警告。我们的模型提供了水合物堆积的统一图景,可用于了解特征明确的天然气水合物系统或预测稳态平均水合物饱和度以及在没有地震或岩心数据的位置处的分布。

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