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低渗透油藏CO2驱过程中含水率变化规律 总被引:1,自引:0,他引:1
通过国内外多个油田水驱后实施CO2驱的矿场实例研究,发现注入CO2后很多油井存在含水率下降的现象;这种现象发生在CO2驱的整个开发阶段,包括注气初期阶段CO2未到达生产井、生产井见气阶段以及高气油比阶段。重点讨论了生产井见气前的开发规律,在该阶段油藏内以油水两相渗流为主,不受三相渗流作用的影响。通过现场动态反应并结合室内细管和长岩心实验,揭示了CO2与油、水2种介质的相互作用,得到了两个结论:第一是始于低含水阶段的CO2驱过程中气体穿越地层水驱替地层油到达生产井;第二是始于高含水阶段的CO2驱替规律在不同级别低渗透岩心中的差异非常明显:对于特低渗岩心,CO2突破前的采出程度占CO2驱总采出程度的73.27%,CO2突破后的采出程度占26.73%,对于一般低渗岩心,CO2突破前的采出程度仅占CO2驱总采出程度的16.72%,而CO2突破后的采出程度占到了CO2驱总采出程度的83.28%。 相似文献
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Kathleen C. Benison Deidre LaClair Jessica Walker 《Earth and Planetary Science Letters》2008,270(3-4):330-337
Physical sedimentology experiments have shown that sulfuric acid solutions may have formed some surface features seen on Mars. Recent data returned from Mars show the presence of jarosite, sulfate salts, hematite, phyllosilicates, and opaline silica, all of which precipitate from some terrestrial sulfuric acid solutions. There is a plethora of geochemical, mineralogical, and sedimentological data indicative of past sulfuric acid systems on Mars, but there has never been a comprehensive study published regarding sulfuric acid as a physical sedimentological agent. In the laboratory, we ran liquids of various compositions over sediments in order to test how these liquids entrain, transport, and deposit sediments. Pure water and concentrated sulfuric acid solutions produced the same general features, such as channels, gullies, and alluvial fans. However, sulfuric acid solutions yielded some distinct sedimentary features not produced by pure water runs. These features, narrow, deeply incised channels of consistent widths, rounded discrete fans, and air bubble “craters”, are similar to some Martian landscape features. These experimental results indicate that acid solutions should be considered a possible sedimentological agent on Mars. 相似文献
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王旺庄水源地是淄博市晴纶工程的后备水源地,设计供水能力20000m^2/d。利用Ritz有限元数值分析方法。结合单纯性线性规划,在完成了对山东省淄博市临淄区王旺庄一朱台地段的淄博市腈纶工程水源地的水文地质模型建造的基础上,成功地对水源地进行地下水开采模拟,同时对该水源地的未来10年开采作了两种大气降水条件下的地下水动态预测。为腈纶工程水源地地下水开采提供了充分的设计依据。 相似文献
117.
Takehiro Koyaguchi Bettina Scheu Noriko K. Mitani Oleg Melnik 《Journal of Volcanology and Geothermal Research》2008
When a highly viscous bubbly magma is sufficiently decompressed, layer-by-layer fracturing propagates through the magma at a certain speed (fragmentation speed). On the basis of a recent shock tube theory by Koyaguchi and Mitani [Koyaguchi, T., Mitani, N. K., 2005. A theoretical model for fragmentation of viscous bubbly magmas in shock tubes. Journal of Geophysical Research 110 (B10), B10202. doi:10.1029/2004JB003513.], gas overpressures at the fragmentation surface are estimated from experimental data on fragmentation speed in shock tube experiments for natural volcanic rocks with various porosities. The results show that gas overpressure at the fragmentation surface increases as initial sample pressure increases and sample porosity decreases. We propose a new fragmentation criterion to explain the relationship between the gas overpressure at the fragmentation surface, the initial pressure and the porosity. Our criterion is based on the idea that total fragmentation of highly viscous bubbly magmas occurs when the tensile stress at the midpoint between bubbles exceeds a critical value. We obtain satisfactory agreement between our simulation and experiment when we assume that the critical value is inversely proportional to the square root of bubble wall thickness. This fragmentation criterion suggests that long micro-cracks or equivalent flaws (e.g., irregular-shaped bubbles) that reach the midpoints between bubbles are a dominant factor to determine the bulk strength of the bubbly magma. 相似文献
118.
The influence of tropical Indian Ocean warming on the Southern Hemispheric stratospheric polar vortex 总被引:1,自引:0,他引:1
ShuangLin Li 《中国科学D辑(英文版)》2009,52(3):323-332
During the past decades, concurrent with global warming, most of global oceans, particularly the tropical Indian Ocean, have
become warmer. Meanwhile, the Southern Hemispheric stratospheric polar vortex (SPV) exhibits a deepening trend. Although previous
modeling studies reveal that radiative cooling effect of ozone depletion plays a dominant role in causing the deepening of
SPV, the simulated ozone-depletion-induced SPV deepening is stronger than the observed. This suggests that there must be other
factors canceling a fraction of the influence of the ozone depletion. Whether the tropical Indian Ocean warming (IOW) is such
a factor is unclear. This issue is addressed by conducting ensemble atmospheric general circulation model (AGCM) experiments.
And one idealized IOW with the amplitude as the observed is prescribed to force four AGCMs. The results show that the IOW
tends to warm the southern polar stratosphere, and thus weakens SPV in austral spring to summer. Hence, it offsets a fraction
of the effect of the ozone depletion. This implies that global warming will favor ozone recovery, since a warmer southern
polar stratosphere is un-beneficial for the formation of polar stratospheric clouds (PSCs), which is a key factor to ozone
depletion chemical reactions.
Supported by National Natural Science Foundation of China (Grant Nos. 40775053 and 90711004), National Basic Research Program
of China (Grant No. 2009CB421401), and Innovation Key Program of Chinese Academy of Sciences (Grant Nos. KZCXZ-YW-Q11-03,
KZCZ2-YW-Q03-08) 相似文献
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针对华北地区农业生产水平和农业干旱特点 ,于 1 996~ 1 998年进行了农业干旱监测预测、秸秆覆盖、底墒科学利用、有限水胁迫效应、深松、多功能防旱剂和有限灌溉等单项农业干旱防御技术试验研究 .在它们的防旱机理、功能和操作技术方面取得了较好的效果 .在此基础上 ,在干旱严重的 1 998~ 1 999年冬小麦生育期内 ,在河南郑州郊区、山东泰安郊区和河北固城 ,根据各地条件因地制宜地对上述技术进行组装配套集成示范试验 .结果表明 ,综合应用这些技术具有较显著的抗旱增产效能 ,小麦增产 1 0 .1 %~ 36.0 % ,耗水量减少 1 .0 %~ 1 9.0 % ,水分利用效率提高 1 0 .6%~ 60 .0 % . 相似文献