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New Acoustic Log Data Interpretation for Gas-bearing Shaly Sands

机译:含气纹理沙滩的新型声学日志数据解释

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Acoustic wave propagation in a sandstone formation depends on porosity, mineralogy, rock matrix elastic moduli, and fluid saturation. The wave velocities are directly linked to pore space compressibility, which forms the basis of many acoustic interpretation methods for identifying gas-bearing sands, e.g., Castagna’s cross-plot method and Murphy et al.’s modulus decomposition method, etc. The latter method detects the presence of gas by comparing acoustic log data with synthetic data computed for full saturated water, oil and water conditions. A basic assumption of this method is that the ratio of the bulk and shear moduli under gas-saturation is invariant for sandstones. This assumption limits the application of this method only to the clean sand scenario. For shaly sands with significant clay content, this moduli ratio is not a constant value, and the interpretation based on the constant ratio assumption may become invalid. We developed a new acoustic interpretation method for gas indication in the shaly sandstone formation. This method determines the variation of the dry frame bulk-to-shear moduli ratio by calibrating it in a water-bearing zone. This calibration establishes the correlation between the moduli ratio and shale content. The established correlation is then applied throughout the zone of interest to calculate pore fluid bulk modulus and gas saturation. The calculation result enables a direct interpretation of gas-bearing sands. To apply this method, acoustic compressional and shear velocity, gamma ray, and density log data are required. In case there is no water-bearing zone for the calibration, default ratio values can be used. This method has been successfully tested in several wells. Two examples are used to demonstrate the method and its application. In both examples, the new results are compared with those from Murphy et al.’s method to demonstrate the marked improvement of the new method for shaly sands. Neutron and density results and resistivity log data further validate the new results.
机译:砂岩形成中的声波繁殖取决于孔隙率,矿物学,岩石基质弹性模量和流体饱和度。波速度直接连接到孔隙空间可压缩性,这构成了许多声学解释方法的基础,用于识别含气砂,例如Castagna的交叉图方法和Murphy等人。的模量分解方法。后一种方法通过将声学日志数据与用于全饱和水,油和水条件计算的合成数据进行比较来检测气体的存在。这种方法的基本假设是砂岩堆气饱和下的散装和剪切模量的比例是砂岩的不变。该假设仅限于清洁沙子场景的方法。对于具有显着粘土含量的Shaly Sands,这种模拟比不是恒定值,并且基于恒定比率假设的解释可能变得无效。我们开发了一种新的气体指示在Shary砂岩形成中的气体指示。该方法通过在含水区中校准它来确定干式框架抗剪切模率比的变化。该校准建立了模拟比和页岩内容之间的相关性。然后在整个感兴趣的区域中施加建立的相关性以计算孔隙流体散装模量和气体饱和度。计算结果可以直接解释含气砂。为了应用这种方法,需要声学压缩和剪切速度,伽马射线和密度日志数据。如果没有用于校准的含水区,则可以使用默认比率值。这种方法已在几个井中成功测试。使用两个例子来证明方法及其应用。在两个例子中,将新结果与来自Murphy等人的方法进行比较。证明谢利砂砂的新方法的方法的方法。中子和密度结果和电阻率日志数据进一步验证了新结果。

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