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91.
多步分解法初步研究石英砂中甲烷水合物p-T稳定条件   总被引:1,自引:0,他引:1  
设计加工了一套研究海底沉积物水合物稳定条件实验装置,采用多步加热分解的方法对不同孔隙度的石英砂沉积物甲烷水合物相态平衡点(p-T稳定条件)进行了初步研究。为校验实验装置和实验方法,首先对甲烷水合物在十二烷基硫酸钠(SDS)溶液中的生成和分解过程进行了研究,获得的实验数据与文献数据吻合得很好。在此基础上,以4种不同粒径(96~180μm、180~380μm、212~380μm和380~830μm)的石英砂为介质,分别研究了甲烷水合物的p-T稳定条件。结果表明,实验测得的数据与纯水溶液中的结果基本一致,说明在实验所用的不同粒径石英砂构成的孔隙尺度内,毛细管作用对水合物相态点的影响可以忽略。  相似文献   
92.
孔隙压力对煤岩基质解吸变形影响的试验研究   总被引:1,自引:0,他引:1  
煤层气开采过程中,伴随着煤层气不断地吸附、解吸和渗流,煤体产生变形,极易导致煤和瓦斯突出事故。以晋城天地王坡煤矿为例,通过实验室内试验,模拟煤层气在复杂地层漫长的形成和逐渐开采过程,得到了孔隙压力与解吸量、应变的变化关系,并拟合得出其相应关系表达式,揭示了一些新的规律:(1)初期解吸速度较快,解吸量随时间的增长而不断增加,后期解吸速度减缓,解吸量逐渐趋于稳定;(2)孔隙压力与解吸量、应变呈现抛物线曲线关系,随孔隙压力的升高,吸附和膨胀变形占主导,其值均在增大;(3)存在最小孔隙压力值,随孔隙压力的增大,解吸时间增长,孔隙压力越小,吸附解吸规律越不明显,对于晋城天地王坡煤矿3#煤样,该值在1.0MPa左右;(4)不同加载方式对解吸量和变形量影响较大,先部分加载吸附后全部载荷解吸结果同比加全部载荷吸附解吸结果高13%~77%。试验结果可为煤层气(CBM)抽放安全和煤与瓦斯突出防治提供理论依据。  相似文献   
93.
根据内蒙古额济纳旗地区X井白垩系额济纳旗组、侏罗系麻木乌苏组、古生界顶面风化壳等不同层段的油气显示特征和钻井泥浆烃类气体组分、甲烷C同位素的分析结果,认为侏罗系和白垩系油气显示特征相同,为油与气显示,气体样品的干燥系数(C1/C总)为0.80~0.87,甲烷C同位素δ13C1为-48.19‰~-50.87‰,表现了低成熟热解气的特征;古生界风化壳为气显示,天然气干燥系数(C1/C总)为0.91~0.92,甲烷C同位素δ13C1为-21.56‰~-30.91‰,表现了高成熟热解气的特征。该井及邻区的中生界、古生界烃源岩干酪根类型及其演化程度具有显著的差别,中生界烃源岩以低成熟混合型干酪根为主,古生界烃源岩为成熟—高成熟(或过成熟)的混合型-腐泥型干酪根。表明该区存在以中生界侏罗系—白垩系低成熟烃源岩为油气源的油气系统和古生界高成熟(或过成熟)烃源岩为气源的油气系统,指示了古生界油气资源前景。  相似文献   
94.
根据内蒙古额济纳旗地区X井白垩系额济纳旗组、侏罗系麻木鸟苏组、古生界顶面风化壳等不同层段的油气显示特征和钻井泥浆烃类气体组分、甲烷C同位素的分析结果,认为侏罗系和白垩系油气显示特征相同,为油与气显示,气体样品的干燥系数(C_1/C_总)为0.80~0.87,甲烷C同位素δ~(13)C_1为-48.19‰~-50,87‰,表现了低成熟热解气的特征;古生界风化壳为气显示,天然气干燥系数(C_1/C_总)为0.91~0.92,甲烷C同位素δ~(13)C_1为-21.56‰-30.91‰,表现了高成熟热解气的特征.该井及邻区的中生界、古生界烃源岩干酪根类型及其演化程度具有显著的差别,中生界烃源岩以低成熟混合型干酪根为主,古生界烃源岩为成熟-高成熟(或过成熟)的混合型-腐泥型干酪根.表明该区存在以中生界侏罗系-白垩系低成熟烃源岩为油气源的油气系统和古生界高成熟(或过成熟)烃源岩为气源的油气系统,指示了古生界油气资源前景.  相似文献   
95.
Water is a necessary element during gas hydrate formations. Therefore, by analyzing water depletion changes in media, the reaction characteristics of methane hydrate in media can be studied. In this study, two water sources supplying some liquid water which may be consumed by the methane hydrate formation reactions were designed and assembled. Using them, the full formation processes of methane hydrate was studied. Experimental results show the following: If heat released from nucleation reaction of methane hydrate is diffused rapidly, the nucleation ratios will be enhanced discernibly. While the hydrate is formed, a force is generated that sucks fresh water from the source into the vicinity of the hydrate, slowing down the cementation process and causing some hydrate grain dissociation. As a result of cementation differences, the hydrate reaction processes with different water sources present linear or quadratic equation characteristics. After a few repeated dissociation and formation processes of some hydrate grains caused by the fresh water, the gas amounts contained in hydrate will be significantly enhanced.  相似文献   
96.
沉积物孔隙毛细管压力与甲烷水合物饱和度关系研究   总被引:1,自引:1,他引:0  
To better understand the relationship between the pore capillary pressure and hydrate saturation in sediments, a new method was proposed. First, the phase equilibria of methane hydrate in fine-grained silica sands were measured. As to the equilibrium data, the pore capillary pressure and saturation of methane hydrate were calculated. The results showed that the phase equilibria of methane hydrates in fine-grained silica sands changed due to the depressed activity of pore water caused by the surface group and negatively charged characteristic of silica particles as well as the capillary pressure in small pores together. The capillary pressure increased with the increase of methane hydrate saturation due to the decrease of the available pore space. However, the capillary-saturation relationship could not yet be described quantitatively because of the stochastic habit of hydrate growth.  相似文献   
97.
基于微孔充填模型的页岩储层吸附动力学特征分析   总被引:1,自引:0,他引:1       下载免费PDF全文
微孔填充是吸附质分子在吸附剂纳微孔隙中、较高平衡压力下表现出来的一种吸附特征,以此为基础发展起来的热
力学理论在确定吸附剂微观结构及吸附性能研究方面起到了巨大推动作用。基于此,该文重点探讨了甲烷在页岩中吸附时
填充率θ、特征能量E、特征系数n、微分吸附功A 、吸附热Q、吸附焓ΔH 及吸附熵ΔS 的变化关系。结果表明:特征系数n
取1较为适当;温度升高特征能量E 值略降,3组样品E 值范围4.14~5.63 kJ/mol;随着θ 的不断增加,A ,Q ,|ΔH |及|
ΔS |等参数值逐渐降低,各能量参数随吸附进行而发生较为规律的变化,无突变。结果认为,热力学参数一定程度上代表
了TOC 及Ro 等参数的综合效应,受单一因素干扰性不强。将计算的Q 及ΔS 等热力学参数与四川盆地志留系龙马溪组页岩的
相应参数进行了对比,进一步表明四川盆地该套龙马溪组页岩具有巨大的页岩气勘探和开发潜力。  相似文献   
98.
The Huanghebei Coalfield, one of the coal production bases in North China, was considered as a coalfield without coal‐bed methane (CBM) during past decades. In recent years, however, CBM has been discovered in coal‐bearing successions. In order to understand the CBM geological characteristics and accumulation process in this area, fifteen coal samples were collected and analyzed with respect to coal maceral and reflectance. The result shows that the gas distribution is uneven and the content varies in different areas even for the same coal bed. The storage of CBM is affected by geological factors such as burial depth, geological structures, and magmatic intrusion, among which the former two are more important in the formation of CBM. Deep burial of coal beds with the presence of cap‐rock mudstone can seal CBM. The CBM is also accumulated and preserved at the place where normal faults are distributed. Magmatic intrusion causes contact metamorphism and controls the CBM formation by heating the coal‐bearing successions. The obtained data indicate the geological conditions in northeastern Zhaoguan Mine are preferable for CBM formation and conservation; recent exploration estimates the CBM geological reserves up to 282.16 Mm3 and average of reserve abundance at 0.1662 × 108 m3 km?2. The Changqing Mine is a potential prospect in terms of CBM exploration since its geological conditions (structures and burial depth) are similar to the Zhaoguan Mine and its cap rock is even better.  相似文献   
99.
何宏  李红霞  张科  陶小晚  蔡春芳 《地质科学》2014,49(4):1327-1336
塔中地区奥陶系天然气成因多样;Ⅰ号坡折带中东部奥陶系天然气以高干燥系数、 甲烷同位素值重为特征;与塔深1井寒武系原油裂解气接近;应主要来自寒武系原油裂解气成因。寒武系贫H2S、 高成熟原油裂解气在喜马拉雅山期时;气侵奥陶系油气藏;得到了以下主要证据的支持: 1)天然气甲烷δ13C值大多比Chung et al.(1988)天然气模式甲烷δ13C值计算值高3‰以上;2)干燥系数与甲烷δ13C值大体上具有正相关关系;3)天然气干燥系数与H2S含量大体上具有负相关关系。这些特征表明;存在贫H2S、 相对富13C甲烷为主的干气与富H2S、 相对贫13C甲烷的湿气混合作用。奥陶系中H2S-δ34S 值为14‰~20‰;远低于中深1井寒武系原地热化学硫酸盐还原作用(TSR)成因的H2S(33‰);支持了奥陶系中H2S并不是来源于寒武系古油气藏。于是提出;来自寒武系贫H2S的干气在喜马拉雅山期对良里塔格组和鹰山组油气藏发生了气洗;油气藏的气/油比值增大、 导致了原油蜡含量增高、 甲烷δ13C值发生正偏移。  相似文献   
100.
The Junction gold deposit, in Western Australia, is an orogenic gold deposit hosted by a differentiated, iron‐rich, tholeiitic dolerite sill. Petrographic, microthermometric and laser Raman microprobe analyses of fluid inclusions from the Junction deposit indicate that three different vein systems formed at three distinct periods of geological time, and host four fluid‐inclusion populations with a wide range of compositions in the H2O–CO2–CH4–NaCl ± CaCl2 system. Pre‐shearing, pre‐gold, molybdenite‐bearing quartz veins host fluid inclusions that are characterised by relatively consistent phase ratios comprising H2O–CO2–CH4 ± halite. Microthermometry suggests that these veins precipitated when a highly saline, >340°C fluid mixed with a less saline ≥150°C fluid. The syn‐gold mineralisation event is hosted within the Junction shear zone and is associated with extensive quartz‐calcite ± albite ± chlorite ± pyrrhotite veining. Fluid‐inclusion analyses indicate that gold deposition occurred during the unmixing of a 400°C, moderately saline, H2O–CO2 ± CH4 fluid at pressures between 70 MPa and 440 MPa. Post‐gold quartz‐calcite‐biotite‐pyrrhotite veins occupy normal fault sets that slightly offset the Junction shear zone. Fluid inclusions in these veins are predominantly vapour rich, with CO2?CH4. Homogenisation temperatures indicate that the post‐gold quartz veins precipitated from a 310 ± 30°C fluid. Finally, late secondary fluid inclusions show that a <200°C, highly saline, H2O–CaCl2–NaCl–bearing fluid percolated along microfractures late in the deposit's history, but did not form any notable vein type. Raman spectroscopy supports the microthermometric data and reveals that CH4–bearing fluid inclusions occur in syn‐gold quartz grains found almost exclusively at the vein margin, whereas CO2–bearing fluid inclusions occur in quartz grains that are found toward the centre of the veins. The zonation of CO2:CH4 ratios, with respect to the location of fluid inclusions within the syn‐gold quartz veins, suggest that the CH4 did not travel as part of the auriferous fluid. Fluid unmixing and post‐entrapment alteration of the syn‐gold fluid inclusions are known to have occurred, but cannot adequately account for the relatively ordered zonation of CO2:CH4 ratios. Instead, the late introduction of a CH4–rich fluid into the Junction shear zone appears more likely. Alternatively, the process of CO2 reduction to CH4 is a viable and plausible explanation that fits the available data. The CH4–bearing fluid inclusions occur almost exclusively at the margin of the syn‐gold quartz veins within the zone of high‐grade gold mineralisation because this is where all the criteria needed to reduce CO2 to CH4 were satisfied in the Junction deposit.  相似文献   
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