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ADVANCEMENTS IN CARBON-OXYGEN SURVEILLANCE OF THE DEEPWATER GULF OF MEXICO MARS WATERFLOOD

机译:墨西哥火星水域深水湾碳氧监测的进展

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The primary purpose of the Mars (Mississippi Canyon807) waterflood in the deepwater of the Gulf of Mexico(GOM) is to increase recovery efficiency in three mainreservoirs. A robust surveillance logging program hasbeen conducted in the field since 1996. Measurementshave included strain, flow profile, reservoir layerpressure, casing inspection, and multi-component fluidsaturation evaluations. The fluid saturation surveillanceresults derived from log measurements have historicallybeen based on original porosity estimates. More recentanalysis techniques have included reductions inporosity due to compaction to better understand fluiddistributions and eliminate anomalous saturationindications. The newly developed modeling canobserve and more accurately identify injected seawaterat the observation wells. This fluid identification isaccomplished through recently developed interpretationmethods using pulsed neutron sensors includinginelastic carbon-oxygen (C/O mode) and capture sigma(∑ mode). The method is demonstrated with severalMars examples including discussion of interpretations.Surveillance of the Mars field is critical to optimizingrecovery. The cased hole logging data are integratedwith other subsurface data, including 4D seismic,additional openhole logs from new wells, productiondata, and injection data. This dataset allows the team toproperly operate existing wells, identify additionalopportunities, and plan future activities. Carbon-oxygenand sigma surveillance has provided an understandingof the fluid changes within the reservoirs under theinfluence of compaction, water injection and aquifermovement. Through experiences in several reservoirs,anomalous tri-fluid (oil, native formation water andinjected waterflood seawater) saturation estimates wereidentified. The proper evaluation of multiple fluids isdependent on the porosity of the rock matrix system.After application of measured strain and porosityreduction modeling, estimates obtained were morerepresentative than what conventional analysis wouldderive. While log measurements investigate the nearwellbore, reservoir modeling can predict a compactionprofile spanning from most dramatic in the nearwellbore region to lesser impact further in the reservoir.Techniques are demonstrated that help identify fluidand porosity changes in the volume observed by thepulsed neutron tool.Selected Mars well log examples are described in detailto highlight the results of compaction and fluidsaturation with time. This discussion is focused on bestpractices learned during the 14 year surveillanceprogram. Included are highlights on how recent logresponses have encouraged the development of moreadvanced methods of interpretation. In some cases theinterpretation became problematic since log responsesdid not indicate a unique solution. The new techniquespresented have provided more accurate multi-fluidvolumetric evaluation and assisted in quantification ofcompaction estimates in wells lacking strainsurveillance. Potential added benefits from this recentmethod include fluid saturation evaluation in complexlithology reservoirs with enhanced recovery. The newmethod better defines fluid types and allows a moreindependent determination of porosity reduction. Theuse of improved methods will hopefully increaseinterest in reservoir surveillance and allow waterfloodsto be operated more effectively.
机译:火星(密西西比峡谷)的主要目的 807)墨西哥湾深水区的注水 (GOM)是提高回收效率的三个主要方面 水库。强大的监视日志记录程序具有 自1996年以来在该领域进行。 包括应变,流量分布,储层 压力,套管检查和多组分流体 饱和度评估。流体饱和度监测 历史上从对数测量得出的结果 根据原始孔隙率估算得出。更近 分析技术包括减少 压实导致的孔隙率,以更好地理解流体 分布并消除异常饱和 适应症。新开发的建模可以 观察并更准确地识别注入的海水 在观察井。此流体标识为 通过最近开发的解释完成 使用脉冲中子传感器的方法,包括 非弹性碳氧(C / O模式)并捕获sigma (∑模式)。该方法用几个例子来说明 火星的例子包括对解释的讨论。 火星场的监视对于优化火星至关重要 恢复。套管井测井数据已集成 以及其他地下数据,包括4D地震, 新井,生产中的其他裸眼测井 数据和注入数据。该数据集使团队能够 正确操作现有油井,确定其他油井 机会,并计划未来的活动。碳氧 Sigma监视提供了一个了解 下储层内流体的变化 压实,注水和含水层的影响 移动。通过几个水库的经验, 异常三流体(石油,天然地层水和 注入注水海水的饱和度估算值是 确定。对多种流体的正确评估是 取决于岩石基质系统的孔隙度。 施加测得的应变和孔隙率后 减少建模,获得的估计更多 比常规分析更具代表性 派生。测井调查附近 井眼,油藏建模可以预测压实度 轮廓从最近最戏剧性的 井眼区域对储层的影响较小。 演示了有助于识别流体的技术 和孔隙率的变化所观察到的体积 脉冲中子工具。 详细介绍了选定的火星测井实例 突出压实和流动的结果 随着时间的推移饱和。讨论重点是 在14年的监视中学习到的实践 程序。其中包括有关最近的日志记录的亮点 回应鼓励更多的发展 先进的解释方法。在某些情况下 自日志响应以来,解释变得有问题 并不表示唯一的解决方案。新技术 提出了提供更准确的多流体 体积评估并协助量化 缺乏应变的井中的压实估计 监视。最近的这项工作可能带来的额外好处 方法包括复杂地层的流体饱和度评估 具有提高采收率的岩性油藏。新的 方法可以更好地定义流体类型,并允许更多 独立确定孔隙率的降低。这 改进方法的使用有望增加 对水库监控感兴趣并允许注水 以便更有效地进行操作。

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