石油与天然气地质 ›› 2024, Vol. 45 ›› Issue (1): 185-199.doi: 10.11743/ogg20240113
张宝收1(), 张本健1, 汪华1, 陈践发2, 刘凯旋2, 豆霜1, 戴鑫1, 陈双玲1
收稿日期:
2023-07-27
修回日期:
2023-12-05
出版日期:
2024-02-01
发布日期:
2024-02-29
第一作者简介:
张宝收(1976—),男,高级工程师,油气成藏、油气资源评价与氦气成藏机理。E‑mail: zhangbaos-tlm@petrochina.com.cn。
基金项目:
Baoshou ZHANG1(), Benjian ZHANG1, Hua WANG1, Jianfa CHEN2, Kaixuan LIU2, Shuang DOU1, Xin DAI1, Shuangling CHEN1
Received:
2023-07-27
Revised:
2023-12-05
Online:
2024-02-01
Published:
2024-02-29
摘要:
氦气成藏长期以来研究较少,成藏条件与成藏机理还不十分清楚,氦源岩类型和形成条件争议较大。通过解剖含氦-富氦的金秋气田认为:①金秋气田氦气含量主要分布在0.05 %~0.10 %,平均为0.07 %,部分井含量超过0.10 %,最高为0.20 %。同位素分析认为氦气为壳源成因,没有幔源的贡献。②金秋气田是一个典型以中生界沉积岩为氦源岩的含氦-富氦气田。上三叠统须家河组和侏罗系具有较高的铀、钍元素含量和较大的地层厚度,在金秋地区具有较高的氦气生气强度,是形成含氦-富氦气藏的氦源基础。氦气应该主要来源于侏罗系储层,而非上三叠统须家河组烃源岩层系。③金秋气田含氦-富氦气田的形成受3个主要因素控制,具有高氦气生气强度的氦源岩提供了很好的物质基础;具有适度充注强度的烃类气体的存在有利于氦气富集;地层抬升剥蚀温、压下降导致的原位溶解氦气脱溶作用是氦气富集的有益补充。
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