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首页> 外文期刊>Geological Journal >Geochemical and stable carbon isotope composition variations of natural gases in tight sandstones from the West Sichuan Basin, China
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Geochemical and stable carbon isotope composition variations of natural gases in tight sandstones from the West Sichuan Basin, China

机译:中国四川盆地西部砂岩中天然气的地球化学和稳定碳同位素组成变化

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> Recent exploration has revealed the great potential of gas resources, complicated gas distributions and geochemical characteristics of natural gases in tight sandstones of the West Sichuan Basin, China (WSBC). The chemical, stable carbon and light hydrocarbon compositions of natural gases from WSBC were investigated to assess the genesis, sources, and migration pattern leading to variations in the geochemical and stable carbon isotope compositions. The analysis shows that the natural gas in the Jurassic tight sandstones occurs as dry gas or wet gas in some places; however, most of the gas in the deep Triassic tight sandstones is apparently dry gas. Carbon isotope distributions increased in the order δ 13 C 1 ??δ 13 C 2 ??δ 13 C 3 ??δ 13 C 4 . The light hydrocarbon content increased in the order of chain (i.e. non‐cyclic) alkanes, cycloalkanes, and aromatic hydrocarbons. Relatively high ethane carbon isotope values and methylcyclohexane contents indicated the presence of lacustrine coal‐formed gases. The Jurassic natural gas is in a lower thermally mature stage and possibly originated from a mixture of T 3 X 3 and T 3 X 5 black mudstones. The deep Triassic natural gas was possibly originated in the deep source rocks because the gas has a relatively higher thermal maturity. Positive correlations between burial depth and methane content, dryness coefficient, δ 13 C 1 , and δ 13 C 1 –δ 13 C 2 for the deep Triassic gas suggest that the migration distance was short and the source was nearby or the gas accumulated in situ . The chemical compositions and geological studies revealed that the fractionation of the Jurassic natural gases in a tight reservoir was predominantly caused by vertical migration rather than the maturity of the local source rocks. Copyright ? 2016 John Wiley & Sons, Ltd.
机译: >最近的探索揭示了天然气资源的巨大潜力,复杂的天然气分布中国四川盆地三川砂岩中天然气的地球化学特征(WSBC)。研究了来自WSBC的天然气的化学,碳和光烃组合物,以评估导致地球化学和稳定的碳同位素组合物的变化的成因,来源和迁移模式。分析表明,侏罗纪紧身砂岩中的天然气在某些地方作为干气或湿气体发生;然而,深度三叠系紧密砂岩中的大部分气体显然是干燥的气体。碳同位素分布在Δ 13℃的顺序增加δ 13℃ 1 13/13 / sup> c 2 α& ?δ 13 c 3 α&δ 13 c 4 。光环含量按环(即非环状)烷烃,环烷烃和芳烃的顺序增加。相对较高的乙烷碳同位素值和甲基环己烷含量表明存在曲线煤成型气体。侏罗纪天然气在较低的热成熟台中,可能源自T 3 x 3 和t 3 x 的混合物5 黑色泥岩。由于气体具有相对较高的热成熟度,因此可能起源于深源岩石。埋藏深度和甲烷含量之间的正相关,干燥系数,δ 13 / sup> 1 1 ,Δ 13 c 1 -Δ 13 c 2 对于深度三叠气体,表明迁移距离短,源位于附近或气体累积原位累积。化学成分和地质研究表明,侏罗纪天然气在紧密水库中的分馏主要是由垂直迁移引起的,而不是当地来源岩的成熟度。版权? 2016年John Wiley& SONS,LTD。

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