首页> 外文期刊>Applied Geochemistry: Journal of the International Association of Geochemistry and Cosmochemistry >Identification of gas inflow zones in the COSC-1 borehole (Jamtland, central Sweden) by drilling mud gas monitoring, downhole geophysical logging and drill core analysis
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Identification of gas inflow zones in the COSC-1 borehole (Jamtland, central Sweden) by drilling mud gas monitoring, downhole geophysical logging and drill core analysis

机译:通过钻井泥气监测,井下地球物理测井和钻孔核心分析识别COSC-1钻孔(贾姆特兰,瑞典中部)的气体流入区

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On-line monitoring of drilling mud gas was for the first time applied during continuous wireline coring of the COSC-1 borehole (Jamtland, central Sweden) to analyse formation gases and to identify inflow gas zones. Nearly complete gas records were obtained with 3 m depth resolution from 662 m (installation of the separator for gas extraction) to 1709 m and 6 m resolution from 1709 m to 2490 m depth (COSC-1 final depth: 2496 m) for H-2, CH4, CO2, and He. Between 662 m and 1400 m, both He and CH4 form broad peaks superimposed by several spike-like features. Zones with gas spikes coincide with high resistivity intervals from dual laterolog (DLL) geophysical borehole logging and show fractures in borehole televiewer (BHTV) images, drill core scans, and visual core inspection. Therefore, we assume gas inflow through open fractures where DLLd/DLLs ratios >1.5 imply the presence of free gas. The correlation between helium and DLLd/DLLs ratios no longer appears at depths greater than similar to 1550 m, probably because the formation gases are dissolved in formation fluids at higher pressure. Below 1550 m depth, the He concentration drops significantly, whereas the CH4 concentration remains relatively high and H-2 and CO2 reach maximum values. The high amount of H-2 and CH4 at depths below 1616 m, from where friction between the casing and the drill string was reported, imply that these gases are most certainly artificially generated at depths below 1616 m and at least partly of artificial origin at shallower depths.
机译:钻井泥气的在线监测是在COSC-1钻孔(瑞典中部)的连续有线上衣期间施加的第一次应用于分析地层气体并识别流入气体区。从662米(用于气体萃取分离器的分离器安装)到1709米和6米的分辨率,从1709米到2490米深度(COSC-1最终深度:2496米),获得几乎完全的气体记录2,CH4,CO2和他。在662米和1400米之间,他和CH4都形成宽峰,叠加了几种类似的穗状花序。具有气体尖峰的区域与双侧面(DLL)地球物理钻孔测井的高电阻率间隔一致,在钻孔电视机(BHTV)图像中显示骨折,钻头核心扫描和视觉核心检查。因此,我们假设通过开口骨折的气体流入,其中DLLD / DLL比率> 1.5意味着存在自由气体。氦气和DLLD / DLLS比率之间的相关性不再出现在大于相似的深度至1550μm,可能是因为在更高的压力下形成形成气体溶解在地层流体中。低于1550米的深度,他浓度显着下降,而CH4浓度仍然相对较高,H-2和CO2达到最大值。从报道壳体和钻柱之间的摩擦下方的深度低于1616μm的高量H-2和CH4,意味着这些气体最肯定会人工地在1616米以下的深度处产生,并且至少部分地是人工来源浅的深度。

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