塔里木盆地台盆区天然气生成动力学模拟与成藏研究
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摘要
针对塔里木盆地台盆区海相天然气多源多期成藏的特点,本论文对台盆区主要烃源岩与原油进行了封闭金管高压釜热模拟实验,获取了可靠的天然气组分与碳同位素数据,开展了天然气生成与碳同位素分馏动力学模拟研究,并结合GC—MS与PVT模拟方法,研究了原油裂解气的生成机理与保存特征,探讨了原油裂解气与干酪根裂解气形成过程的差异性及两类气体的判识标准。在此基础上,利用动力学方法对典型海相天然气藏的成因与成藏模式进行了研究与探讨,对今后高成熟海相地区的天然气勘探具有重要的指导意义。本研究取得如下主要成果与认识:
1、获取了典型干酪根与油样主要气态烃组分的生成与裂解动力学参数及甲烷碳同位素动力学参数。这些参数能较好拟合实验数据,可应用到地质条件下的生气与碳同位素动力学模拟。
2、原油裂解成气与干酪根裂解成气的差异主要体现在前者早期的裂解气以C_(2-5)重烃为主,其后期裂解是原油裂解气甲烷的主要来源,而干酪根裂解气甲烷主要来自干酪根本身的裂解;(δ~(13)C_2-δ~(13)C_3)与δ~(13)C_1交汇图能有效区分两类裂解气,可作为区分两类气体的依据之一。
3、原地原油裂解气藏的形成与保存主要受储层含油饱和度、盆地温压场、地质系统开放程度及构造作用等多个因素的综合控制。
4、英南2井侏罗系气藏为干酪根裂解气与原油裂解气的混合气,干酪根裂解气主要来源于寒武—下奥陶地层,原油裂解气主要来源于中上奥陶统上部。气藏主要充注时间在第三纪之后,属于次生深源气藏。
5、桑南地区天然气主要属干酪根裂解气、气源岩是位于LN46井至构造高部位的中下寒武统烃源岩。凝析油主要来源于早期寒武系古油藏的裂解及中上奥陶统烃源岩,气藏从三叠纪末期开始聚气,主成藏期在第三纪之后。
δ
which, generally, is a function of oil saturation of reservoir, temperature, pressure, geological sealing degree and structural uplifting.4. The gases in YN2 gas pool are a mixture of kerogen gas and oil cracking gas. The kerogen gas results from the Cambrian-lower Ordovician strata while the oil cracking gas is mainly derived from the cracking of oil in paleo oil pools in the upper part of the mid-upper Ordovician strata. The YN2 gas pool was charged mainly after the Tertiary period and is a secondary gas pool with deeper sources.5. The gases in Sang-nan gas pools are mainly composed of kerogen gas from mid-lower Cambrian strata with major source areas from the slopes to the structural high, i.e. from LN46 and LN59 in the southwest and southeast slopes, respectively, to LG13 in the structural high. In addition to the mid-upper Ordovician source rocks, the cracking of Cambrian oils in paleo oil pools is an alternative source for the condensates. Approximately, the effective gas accumulation initiated at the end of Triassic period, but the major charging occurred after the Tertiary period.
1、获取了典型干酪根与油样主要气态烃组分的生成与裂解动力学参数及甲烷碳同位素动力学参数。这些参数能较好拟合实验数据,可应用到地质条件下的生气与碳同位素动力学模拟。
2、原油裂解成气与干酪根裂解成气的差异主要体现在前者早期的裂解气以C_(2-5)重烃为主,其后期裂解是原油裂解气甲烷的主要来源,而干酪根裂解气甲烷主要来自干酪根本身的裂解;(δ~(13)C_2-δ~(13)C_3)与δ~(13)C_1交汇图能有效区分两类裂解气,可作为区分两类气体的依据之一。
3、原地原油裂解气藏的形成与保存主要受储层含油饱和度、盆地温压场、地质系统开放程度及构造作用等多个因素的综合控制。
4、英南2井侏罗系气藏为干酪根裂解气与原油裂解气的混合气,干酪根裂解气主要来源于寒武—下奥陶地层,原油裂解气主要来源于中上奥陶统上部。气藏主要充注时间在第三纪之后,属于次生深源气藏。
5、桑南地区天然气主要属干酪根裂解气、气源岩是位于LN46井至构造高部位的中下寒武统烃源岩。凝析油主要来源于早期寒武系古油藏的裂解及中上奥陶统烃源岩,气藏从三叠纪末期开始聚气,主成藏期在第三纪之后。
δ
which, generally, is a function of oil saturation of reservoir, temperature, pressure, geological sealing degree and structural uplifting.4. The gases in YN2 gas pool are a mixture of kerogen gas and oil cracking gas. The kerogen gas results from the Cambrian-lower Ordovician strata while the oil cracking gas is mainly derived from the cracking of oil in paleo oil pools in the upper part of the mid-upper Ordovician strata. The YN2 gas pool was charged mainly after the Tertiary period and is a secondary gas pool with deeper sources.5. The gases in Sang-nan gas pools are mainly composed of kerogen gas from mid-lower Cambrian strata with major source areas from the slopes to the structural high, i.e. from LN46 and LN59 in the southwest and southeast slopes, respectively, to LG13 in the structural high. In addition to the mid-upper Ordovician source rocks, the cracking of Cambrian oils in paleo oil pools is an alternative source for the condensates. Approximately, the effective gas accumulation initiated at the end of Triassic period, but the major charging occurred after the Tertiary period.
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