纳土纳盆地东北部碎屑储层

D. Mulyono
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引用次数: 0

摘要

东纳土纳盆地由几个次盆区组成,这些次盆区形成于第三纪渐新世至早中新世,是与南海张开有关的伸展作用的结果。在靠近金枪鱼地块的北部地区,出现了几个小的渐新世半地堑。沉积物呈NE-SW走向,厚度相对均匀,厚度小于2600 ft,区域厚度向东向盆地中心增长。而在中新世下,一次更为明显的伸展活动扩大了原有的半地堑,形成了以碎屑层序为主的大型生长断裂相关沉积包体。中新世中期的海相条件导致了碳酸盐的发育,这种发育一直持续到中新世晚期,地震观测到一些非常大的与礁有关的碳酸盐堆积。晚中新世,该区受右旋张拉作用进一步变形,形成了大量的NE-SW正断层。随后是一段平静期,上覆的上新世慕达组海相页岩和碎屑沉积。渐新统和中新统下段受构造控制的局部厚层序显示出良好的烃源/储/封对发育潜力。东纳图纳盆地的勘探始于20世纪70年代,主要针对Terumbu组碳酸盐岩聚集,这很容易在现有的二维地震数据上绘制。其中最重要的发现是1973年AGIP发现的超巨型D α气田,含超过220 TCF,含+/- 71% CO2。然而,2D地震数据无法很好地成像下伏碎屑,而且许多钻井的位置也不适合测试Arang和Gabus下伏碎屑剖面。2014年,Premier Oil在Kuda Laut-1井和Singa Laut-1井的Gabus和Lower Terumbu碎屑岩中发现了油气,证实了这些层段的勘探潜力。2021年第三季度至第四季度,另外两口井对金枪鱼油田的发现进行了评估,确认存在富含凝析油产量高的湿气,但也遇到了先前发现的气柱的油环。主要储层为下特伦布浅海生物扰动泥质砂岩(Kuda Laut上盘构造)和Gabus河道砂岩(Singa Laut下盘构造)。常规岩心、大量电缆数据和DST显示,这两个储层的性质非常不同。目前正在进行井后分析,以进一步表征这些储层及其所含流体的特征,其结果将对Tuna油田的商业开发至关重要。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Clastic Plays in The North East Natuna Basin
The East Natuna Basin comprises several sub-basinal areas which formed during the Tertiary as a result of extension relating to the opening of the South China Sea during the Oligocene and Early Miocene. Several small Oligocene half-grabens occur in the northern part of the area close to where the Tuna Block is located. They have a NE-SW trend and the sediments are relatively uniform in thickness, less than 2,600 ft thick, with regional thickness growth to the east towards the basin center. However in the Lower Miocene a more pronounced extensional episode enlarged the existing half grabens and generated large growth fault related sediment packages consisting predominantly of clastic sequences. Marine conditions in the Mid Miocene gave rise to carbonate development which continued to the latest Miocene with some very large reef related carbonate build-ups observed on seismic. In Late Miocene this area underwent further deformation caused by right lateral transtension which produced numerous NE-SW normal faults. This was then followed by a period of quiescence and deposition of the overlying Pliocene Muda Formation marine shales and clastics. The tectonically controlled, locally thick sequences of the Oligocene and Lower Miocene sediments indicate good potential for source and reservoir/seal pair rocks. Exploration in the East Natuna Basin began in the 1970’s, mainly targeting the Terumbu Formation carbonate buildups, which were easily mapped on the available 2D seismic data. Some discoveries were made and the most significant of which was the supergiant D Alpha gas field discovery by AGIP in 1973 containing over 220 TCF including +/- 71% CO2. However, the underlying clastics were not well imaged by the 2D seismic data and many of the wells drilled were not optimally located for testing the underlying Arang and Gabus clastic sections. The discovery of hydrocarbons in the Gabus and Lower Terumbu clastics in the Kuda Laut-1 and Singa Laut-1 wells by Premier Oil in 2014 confirmed the exploration potential of these intervals. The discoveries now known as the Tuna Field were appraised by two additional wells in Q3-Q4 2021 confirming the presence of rich wet gas with a high condensate yield, but also encountering oil rims, to the previously discovered gas columns. The main reservoirs are Lower Terumbu shallow marine bioturbated shaly sandstones in the Kuda Laut hanging wall structure and Gabus fluvial channel sandstones in the Singa Laut footwall structure. These two reservoirs exhibit very different properties as indicated by conventional cores, extensive wireline data and the DST’s. Post well analysis is ongoing to further characterize these reservoirs and the fluids contained, the results of which will be critical for the commercial development of the Tuna field.
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