南海神湖 W17 井岩心沉积物的综合特征及其对甲烷水合物动力学的影响

0 ENERGY & FUELS
Yan Li , Chenlu Xu , Jianxi Zhu , Hongfeng Lu , Yunting Liu , Yuhang Gu , Zhejun Pan , Praveen Linga , Zhenyuan Yin
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引用次数: 0

摘要

天然气水合物(NGH)被认为是一种巨大的非常规能源,在满足未来能源需求方面前景广阔。在神狐地区(位于中国南海北坡),对天然气水合物进行了一系列深入研究,如勘探、钻探和两次现场生产试验。海洋沉积物岩心的岩性特征及其对甲烷水合物(MH)形成的影响相对未知,值得进一步研究。在本研究中,我们对位于南中国海第一个 NGH 油田生产附近的取芯井神湖 W17 井回收的岩心沉积物进行了一系列岩性表征。岩心沉积物被归类为粘土质粉砂,中位粒度为6.91微米,主要由粘土矿物、石英和方解石组成。根据 X 射线衍射分析,粘土矿物的主要成分分别为伊利石-直闪石层、伊利石、绿泥石和高岭石。岩芯沉积物的孔隙率为 32.5%,根据汞侵入测试,渗透率为 7.8 mD。根据扫描电镜和 QEMSCAN 分析,确定了四种类型的原生孔隙:粒间孔隙、晶间孔隙、粒内孔隙和与海洋化石有关的孔隙。此外,还研究了回收的岩心沉积物(0-40 wt%)对 MH 形成动力学的影响,并通过形态观察阐明了 MH 与岩心沉积物的相互作用。在有 SCS 岩心沉积物存在的情况下,诱导时间明显缩短至 20 分钟。在最大气体吸收量为 134.1 Vg-Vw-1 时,观察到两阶段的 MH 形成行为:(a) 最初的 MH 形成于气-液界面,MH 向上生长,细粒沉积物迁移;(b) 第二阶段 MH 显著生长,MH 和岩心沉积物分层形成。MH 形成的毛细管通道促进了岩心沉积物的迁移,而岩心沉积物的迁移又为 MH 的形成提供了额外的气液接触面积。该研究为了解神湖岩心沉积物在 MH 形成过程中的作用提供了宝贵的见解,这对于理解储层中 NGH 的空间异质性以及设计合适的生产策略至关重要。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Comprehensive characterizations of core sediments recovered from Shenhu W17 well in South China sea and its impact on methane hydrate kinetics

Comprehensive characterizations of core sediments recovered from Shenhu W17 well in South China sea and its impact on methane hydrate kinetics
Natural Gas Hydrates (NGH) is considered a vast unconventional energy source that holds significant promise in addressing future energy demands. In Shenhu area (located at northern slope of the South China Sea, SCS), there has been conducted a series of further studies of NGH such as exploration, drilling, and twice field production testing. The lithological characteristics of cores from marine sediments and their influence on methane hydrate (MH) formation are relatively unknown and merits further investigation. In this study, we conducted a chain of lithological characterization on the core sediments recovered from Shenhu W17 well, the coring well which located near the 1st NGH field production in SCS. The core sediments are classified as clayey-silt, its median grain size is 6.91 μm, comprising primarily clay minerals, quartz, and calcite. According to X-ray diffraction analysis, the main content of clay minerals is illite-smectite layers, illite, chlorite, and kaolinite, respectively. Porosity of the core sediments is 32.5% and the permeability is 7.8 mD based on mercury intrusion tests. Four types of primary pores are identified based on SEM and QEMSCAN analysis: intergranular pore, intercrystalline pore, intragranular pore, and pores associated with marine fossils. Moreover, the influence of the recovered core sediments (0–40 wt%) on MH formation kinetics were examined with morphology observed to elucidate the MH-core sediments interaction. The induction time was reduced significantly to ∼20 min in the presence of SCS core sediments. A two-stage MH formation behavior is observed with a maximum gas uptake of 134.1 Vg·Vw−1: (a) an initial MH formation at the gas-liquid interface with MH upward growth and fine-grain sediments migration; and (b) a second stage of significant MH growth with layered formation of MH and core sediments. The capillary channels of MH formed facilities the migration of core sediments, which in turn provides additional gas-liquid contact area for MH formation. The study provides valuable insights on the role Shenhu core sediments in MH formation, which is essential for understanding the spatial heterogeneity of NGH in reservoir and for designing suitable production strategy.
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