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Coal seam gas distribution and hydrodynamics of the Sydney Basin, NSW, Australia

机译:澳大利亚新南威尔士州悉尼盆地的煤层气分布和流体动力学

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This paper reviews various coal seam gas (CSG) models that have been developed for the Sydney Basin, and provides an alternative interpretation for gas composition layering and deep-seated CO_2 origins. Open file CSG wells, supplemented by mine-scale information, were used to examine trends in gas content and composition at locations from the margin to the centre of the basin. Regionally available hydrochemistry data and interpretations of hydrodynamics were incorporated with conventional petroleum well data on porosity and permeability. The synthesised gas and groundwater model presented in this paper suggests that meteoric water flow under hydrostatic pressure transports methanogenic consortia into the subsurface and that water chemistry evolves during migration from calcium-rich freshwaters in inland recharge areas towards sodium-rich brackish water down-gradient and with depth. Groundwater chemistry changes result in the dissolution and precipitation of minerals as well as affecting the behaviour of dissolved gases such as CO_2. Mixing of carbonate-rich waters with waters of significantly different chemistries at depth causes the liberation of CO_2 gas from the solution that is adsorbed into the coal matrix in hydrodynamically closed terrains. In more open systems, excess CO_2 in the groundwater (carried as bicarbonate) may lead to precipitation of calcite in the host strata. As a result, areas in the central and eastern parts of the basin do not host spatially extensive CO_2 gas accumulations but experience more widespread calcite mineralisation, with gas compositions dominated by hydrocarbons, including wet gases. Basin boundary areas (commonly topographic and/or structural highs) in the northern, western and southern parts of the basin commonly contain CO_2-rich gases at depth. This deep-seated CO_2-rich gas is generally thought to derive from local to continental scale magmatic intrusions, but could also be the product of carbonate dissolution or acetate fermentation.
机译:本文回顾了为悉尼盆地开发的各种煤层气(CSG)模型,并为天然气成分分层和深层CO_2来源提供了另一种解释。开放文件的CSG井,加上矿山规模的信息,被用来检查从盆地边缘到盆地中心位置的天然气含量和组成趋势。将地区可获得的水化学数据和流体动力学解释与有关孔隙度和渗透率的常规石油井数据结合在一起。本文提出的合成气和地下水模型表明,在静水压力下的大气水流将产甲烷的联合体运入地下,并且在从内陆补给区的富含钙的淡水向富含钠的微咸水向下迁移的过程中,水化学演化。与深度。地下水的化学变化导致矿物的溶解和沉淀,并影响溶解气体(如CO_2)的行为。在深度上将富含碳酸盐的水与化学性质明显不同的水混合会导致从溶液中释放出CO_2气体,该溶液在水动力封闭的地形中被吸附到煤基质中。在更开放的系统中,地下水中过量的CO_2(以碳酸氢盐形式携带)可能导致方解石在宿主岩层中沉淀。结果,该盆地中部和东部地区的区域内没有大量的CO_2气藏,但方解石矿化更为普遍,气体成分以碳氢化合物(包括湿气)为主。盆地北部,西部和南部部分的盆地边界区域(通常是地形和/或构造高点)通常在深处含有富含CO_2的气体。人们普遍认为这种深层的富含CO_2的气体来自局部到大陆范围的岩浆侵入,但也可能是碳酸盐溶解或醋酸盐发酵的产物。

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