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Simulation of Multicomponent Gas Flow and Condensation in Marcellus Shale Reservoir

机译:Marcellus Shale水库多组分气体流动和凝结的模拟

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The Marcellus shale formation, with more than 463 trillion cubic feet (Tcf) of recoverable gas in Pennsylvania and West Virginia, will play a critical role in providing clean energy, environmental sustainability, and increased security for our nation. However, due to recent low gas prices, most of the operating companies have slowed down their activities in dry gas areas and refocused their attention in oil and condensate production from liquid-rich regions. This change in production plans requires detailed investigation of gas condensate bank developments and saturation dynamics in shale gas reservoirs that change greatly depending on reservoir rock and fluid properties and also operating conditions. An advanced level of understanding of the parameters affecting gas condensate phase behavior is necessary in order to make accurate predictions of these changes. Phase behavior and critical properties of gas condensate in shale gas reservoirs is significantly different than that of gas condensate as bulk in the PVT cell. It is highly affected by shale pore size distribution leading to changes in gas compressibility, viscosity, formation volume and original gas in place calculations. In addition to pore size effect, fluid composition, natural and hydraulic fractures, reservoir anisotropy, rock compressibility and number of horizontal wells and their operating conditions could also significantly impact the condensate bank developments and saturation dynamics. To quantify the importance of these parameters experimental design model, i.e., Plackett-Burman, implemented following a systematic approach for two different cases (single well cylindrical model and actual Marcellus shale gas reservoir). Detailed uncertainty analysis of different parameters using Marcellus shale gas reservoir model show the significance of reservoir fluid composition, matrix anisotropy, rock compressibility and hydraulic fracture spacing on condensate bank developments where the pore size confinement effects has been ignored. They also show that gas condensation is not only a near wellbore phenomenon but it can happen deep into the reservoir causing severe formation damage. However, considering the nano-pore size characteristics of Marcellus shale gas reservoir by assuming average 2 nm pore size distribution the modified critical properties and fluid behavior, results in significant reduction in condensate saturations around the wellbore and inside the reservoir. This significantly alleviates the formation damage that has been seen in the absence of nano-pore wall confinement effects. Based on our study, critical properties and phase behavior of reservoir fluid under pore wall confinements have the most significant impact on production strategies and stimulation design for Marcellus shale gas reservoirs.
机译:在宾夕法尼亚州和西弗吉尼亚和西弗吉尼亚州拥有超过463万亿立方英尺(TCF)的Marcellus页岩形成将在提供清洁能源,环境可持续性和增加我们国家的安全性方面发挥关键作用。然而,由于近期的低气体价格,大多数运营公司都在干燥气体地区的活动放缓,并从富含液体地区重新分为他们的石油和冷凝水生产。这种生产计划的变化需要详细调查页岩气藏的气体冷凝水库开发和饱和动力学,这取决于储层岩石和流体性能以及操作条件。需要对影响气体凝结物相行为的参数的先进的理解水平是为了做出这些变化的准确预测。气体储层气体冷凝物的相位行为和关键特性显着不同于PVT细胞中块状的气体冷凝物的特性。它受到页岩孔径分布的影响,导致气体可压缩性,粘度,地层体积和原始气体的变化。除孔径效果外,流体组成,天然和液压骨折,储层各向异性,岩石压缩性和水平井的数量以及其运行条件也可能会显着影响冷凝物银行的开发和饱和动态。为了量化这些参数的重要性,实验设计模型,即Plackett-Burman,在两个不同案例的系统方法之后实施(单井圆柱形模型和实际Marcellus页岩气藏)。使用Marcellus页岩气储层模型的不同参数的详细不确定性分析表明储层流体组成,基质各向异性,岩石压缩性和液压骨折间距对孔径限制效应忽略的凝析液的显着性。他们还表明,气体凝结不仅是近井筒现象,而且它可能会深入储层导致严重的形成损伤。然而,考虑到Marcellus页岩气储层的纳米孔尺寸特性通过假设平均2nm孔径分布改性的关键性质和流体行为,导致井筒周围的冷凝物饱和性显着降低,并且在储层内部显着降低。这显着减轻了在没有纳米孔壁限制效应的情况下已经看到的形成损伤。基于我们的研究,孔隙壁限制下储层液体的关键特性和相位行为对Marcellus页岩气藏的生产策略和刺激设计产生了最大的影响。

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