Novel Reservoir Sand Grain Size Map Based on Open Hole Gamma Ray Log as Im-Proved ThruTubing Sand Screen Size Selection Guideline on Tunu Multi-Layer Un-Consolidated Gas Reservoir

Rahman Setiadi, Yulianto Jong, Nur Mahfudhin, Mutawif Ilmi Muwaffaqih, Albert Richal Dading
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引用次数: 2

Abstract

Tunu is one of Mahakam fields with majority gas production. The depositional nature of fluvial with minimum tidal influence results in the signature of delta sedimentation by hundred layers of gas-bearing sand lenses as pay zone. They are constructed of unconsolidated clean and shaly sand reservoirs at the shallower burial and higher consolidation at deeper burial due to compaction and diagenesis. The unconsolidated section requires sand control as mandatory means to unlock it safely. The combined challenge of numerous sand layers and marginal reserves makes it economically impossible to perform regular detailed physical sand grain assessment by individual conventional coring completed with Laser Particle Sieve Analysis (LPSA). An economic approach is through performing sand bailing. However, the bailed sand dry-sieve results were confusing with wide particle size distribution (PSD) curve variation from several well samples. Referring to this PSD uncertainty, installing straddled thru-tubing screen in front of the reservoir as sand control resulted in good production and plugged indication at the beginning of the initiative by utilizing a similar screen opening size. Thus, a new fit-for-purpose methodology was required. A study to predict sand grain size on each reservoir target was initiated by analyzing three available shallow reservoir cores in Mahakam, which could cover most of Tunu's shallow sedimentation type. The result was that most of the sand grain size distribution on each sample core correlated with their calculated shale volume content (v-shale). Lower v-shale is respected to larger sand grain size. Unconsolidated Tunu Shallow reservoir doesn't contain any specific radioactive minerals. Thus, v-shale could be easily calculated from gamma-ray logs, which are always available on each reservoir target at any drilled wells. The relationship between sand grain size and v-shale was gathered on a single map. The map was then validated by historical screen installation. Positive results were seen when screen size selection respects specific patterns on the generated sand map at the v-shale value of perforation intervals. Thru-tubing screen installation campaign was continued following the new sand map reference. It could deliver more than 80% successful installation with no plugging or sand at a new perforated reservoir when no screen integrity issue due to erosion was encountered. This novel approach allowed better prediction of thru-tubing screen opening size requirements and perforation interval selection in Tunu unconsolidated reservoir and was successfully expanded in offshore Mahakam field at similar facies.
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基于裸眼伽马测井的新型储层砂粒度图——改进的突努多层未固结气藏过油管筛砂粒度选择准则
Tunu是Mahakam的主要气田之一。潮汐影响最小的河流沉积性质,形成了以百层含气砂透镜体为产层的三角洲沉积特征。浅层埋深处为未固结的洁净泥质砂储层,深层因压实作用和成岩作用形成较高的固结砂储层。未固结段需要防砂作为安全解锁的强制手段。大量砂层和边际储量的综合挑战使得通过激光颗粒筛分析(LPSA)完成单个常规取心来进行常规详细的物理砂粒评估在经济上是不可能的。一种经济的方法是通过进行沙坑。然而,由于几口井样品的粒径分布(PSD)曲线变化较大,因此,脱砂干筛结果令人困惑。考虑到这种PSD的不确定性,在储层前面安装跨式过油管筛管防砂,通过使用类似的筛管开口尺寸,获得了良好的生产效果,并在作业开始时显示出堵塞迹象。因此,需要一种新的适合目的的方法。通过分析Mahakam地区三个可用的浅层储层岩心,对每个储层目标层的砂粒度进行了预测研究,这些岩心可以覆盖Tunu的大部分浅层沉积类型。结果表明,每个样品岩心上的大部分砂粒度分布与其计算的页岩体积含量(v-shale)相关。下v型页岩的砂粒尺寸较大。未固结土努浅层储层不含任何特定的放射性矿物。因此,v型页岩可以很容易地从伽马射线测井曲线中计算出来,这些测井曲线在任何一口井的每个储层目标上都是可用的。将砂岩粒度与v型页岩的关系集中在一张图上。然后通过历史屏幕安装验证该地图。当筛管尺寸选择符合射孔段v-页岩值上生成的砂图的特定模式时,可以看到积极的结果。根据新的砂图参考,继续进行过油管筛管安装工作。在新射孔油藏中,如果没有因侵蚀而导致筛管完整性问题,该系统的安装成功率可达80%以上,无堵塞或出砂。这种新方法可以更好地预测Tunu松散油藏的过油管筛管开孔尺寸要求和射孔间隔选择,并成功推广到类似相的海上Mahakam油田。
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