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The influence of pore structure on P- & S-wave velocities in complex carbonate reservoirs with secondary storage space

机译:孔结构对P-和P的影响具有二级存储空间的复杂碳酸盐岩油藏的横波速度

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Secondary storage spaces with very complex geometries are well developed in Ordovician carbonate reservoirs in the Tarim Basin, which is taken as a study case in this paper. It is still not clear how the secondary storage space shape influences the P- & S-wave velocities (or elastic properties) in complex carbonate reservoirs. In this paper, three classical rock physics models (Wyllie timeaverage equation, Gassmann equation and the Kuster-Toks?z model) are comparably analyzed for their construction principles and actual velocity prediction results, aiming at determining the most favourable rock physics model to consider the influence of secondary storage space shape. Then relationships between the P- & S-wave velocities in carbonate reservoirs and geometric shapes of secondary storage spaces are discussed from different aspects based on actual well data by employing the favourable rock physics model. To explain the influence of secondary storage space shape on V _(P)- V _(S) relationship, it is analyzed for the differences of S-wave velocities between derived from common empirical relationships (including Castagna’s mud rock line and Greenberg-Castagna V _(P)- V _(S) relationship) and predicted by the rock physics model. We advocate that V _(P)- V _(S) relationship for complex carbonate reservoirs should be built for different storage space types. For the carbonate reservoirs in the Tarim Basin, the V _(P)- V _(S) relationships for f ractured, fractured-cavernous, and fractured-hole-vuggy reservoirs are respectively built on the basis of velocity prediction and secondary storage space type determination. Through the discussion above, it is expected that the velocity prediction and the V _(P)- V _(S) relationships for complex carbonate reservoirs should fully consider the influence of secondary storage space shape, thus providing more reasonable constraints for prestack inversion, further building a foundation for realizing carbonate reservoir prediction and fluid prediction.
机译:塔里木盆地奥陶系碳酸盐岩储层发育几何形状非常复杂的二次储藏空间,以本文为研究案例。尚不清楚次级储藏空间的形状如何影响复杂碳酸盐岩储层中的纵波和横波速度(或弹性特性)。本文比较了三种经典岩石物理模型(Wyllie时间平均方程,Gassmann方程和Kuster-Toks?z模型)的构造原理和实际速度预测结果,旨在确定最有利的岩石物理模型来考虑二次存储空间形状的影响。然后,利用有利的岩石物理模型,根据实际油井数据,从不同方面探讨了碳酸盐岩储层中的P波和S波速度与次生储藏空间的几何形状之间的关系。为了解释次要存储空间形状对V _(P)-V _(S)关系的影响,分析了常见经验关系(包括Castagna的泥岩线和Greenberg-Castagna)得出的S波速度之间的差异。 V_(P)-V_(S)关系),并由岩石物理模型预测。我们主张,应针对不同的存储空间类型建立复杂碳酸盐岩储层的V_(P)-V_(S)关系。对于塔里木盆地碳酸盐岩油藏,在速度预测和次生储藏空间的基础上,分别建立了压裂,裂缝-空洞和裂缝-孔洞型油藏的V_(P)-V_(S)关系。类型确定。通过以上讨论,可以预期,复杂碳酸盐岩储层的速度预测和V_(P)-V_(S)关系应充分考虑次生储集空间形状的影响,从而为叠前反演提供更合理的约束条件,进一步为实现碳酸盐岩储层预测和流体预测奠定基础。

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