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1.
东非海岸主要含油气盆地属典型大陆裂谷层序和被动陆缘层序叠合的断坳型盆地,是在冈瓦纳大陆裂解及印度洋扩张的区域构造演化背景下形成的,均经历了卡鲁裂谷期、马达加斯加漂移期和被动大陆边缘期三期构造演化。但是,南、北盆地在构造及沉积演化特征及石油地质条件、油气分布上存在较大差异,北部盆地早期受特提斯洋海侵影响,沉积发育了侏罗系潟湖相盐岩、浅海相泥页岩,而南部盆地处于强烈火山作用区,二者油气富集规律存在差异,烃源岩、储盖组合由北向南年代逐渐变新,目前北部油气发现明显更为丰富。初步分析认为,构造环境不同使得烃源岩发育北富南贫,断裂及塑性岩体作用形成的通源断层和有利圈闭存在差异,导致了东非大陆边缘南、北部盆地油气成藏上的不同。 相似文献
2.
宽扎盆地油气地质特征 总被引：1，自引：0，他引：1
安哥拉宽扎盆地是典型被动大陆边缘盆地,完整经历了前裂谷阶段、裂谷阶段、过渡阶段及漂移阶段等4个构造演化阶段,形成了盐下、盐间和盐上3套沉积层序,并各自形成含油气系统。在对宽扎盆地构造演化、沉积特征及油气成藏条件进行分析后认为:宽扎盆地盐下、盐间和盐上3套沉积层序的油气成藏主控因素分别为拉伸断陷、盐隆起及盐构造运动;宽扎盆地盐下有利勘探区为盆地东部白垩系地堑构造区,盐间有利勘探区为盆地中东部盐隆发育部位,盐上有利勘探区为盆地东部古近系和新近系地堑发育部位;宽扎盆地今后勘探工作重点应放在盆地东部白垩系地堑构造区的盐下碳酸盐岩储层目标。 相似文献
3.
台西南盆地的构造演化与油气藏组合分析 总被引：14，自引：2，他引：14
杜德莉 《海洋地质与第四纪地质》1994,14(3):5-18
本文根据台西南盆地的地质、地球物理资料，对台西南盆地的地壳结构、基底特征、沉积厚度、断裂构造等基本地质构造特征＾［１］作了研究，探讨了台西南盆地的构造发展演化及及油气藏组合。认为该盆地的构造演化为幕式拉张。幕式拉张可分为三大张裂幕，相应的热沉降作用使盆地在不同的张裂幕时期发展为断陷，裂陷，裂拗－拗陷。它们分别与板块作用下的区域构造运动阶段相对应，说明区域构造运动不但控制了盆地的发展演化，同时也制约 相似文献
4.
《海洋地质与第四纪地质》2016,(4)
远东鄂霍茨克海域发育多个新生代弧后盆地,这些盆地是西太平洋边缘海盆的重要组成部分,介绍了鄂霍茨克海域的地质结构和构造特征,探讨了海域内盆地形成的动力机制来源及构造演化阶段的划分。认为太平洋板块与欧亚板块碰撞引发区域上挤压与引张作用在时间上相互消长的效应、深部软流圈上涌,共同引发鄂霍茨克海域内多期次弧后扩张作用,导致海域内弧后裂谷盆地的发育;同时,周边板块碰撞导致大型走滑断裂发育和构造反转,对盆地的形成进行改造;共同控制了弧后沉积盆地的形成与演化。盆地构造演化可以划分为4个阶段,即基底拼合阶段(J-K2前)、基底褶皱-张裂变形阶段(K2-E1早期)、盆地裂陷-拗陷作用阶段(E1-N1)及构造反转阶段(N2-第四纪)。 相似文献
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南海北部深水区东西构造差异性及其动力学机制 总被引：1，自引：0，他引：1
南海北部深水区位于南海洋陆转换带,构造运动活跃,构造特征复杂。同时,南海北部深水区石油、天然气、天然气水合物等矿产资源丰富。因此,加强南海北部深水盆地构造特征分析,揭示南海北部陆缘构造属性与南海形成演化机制,对于南海深部过程演变研究、油气资源评价与地质灾害防治等具有重要的意义。本论文通过对南海北部深水区陆架-陆坡结构、盆地构造特征与演化规律的分析,指出研究区东西存在明显的构造差异性,并分析了其动力学机制。南海北部深水区东部陆架-陆坡结构为宽洼窄隆型,而西部为窄洼宽隆型。东部珠江口盆地深水凹陷均为半地堑结构,剖面上呈不对称的箕状;西部琼东南盆地除北礁凹陷为南段北超的小型半地堑外,其它凹陷均为地堑结构,为南北双断式沉积体系。在构造演化方面,东部中中新世末结束裂后期进入新构造活动期,白云凹陷构造活动性增强,表现为快速的沉降和显著的晚期断裂作用;而西部晚中新世末才进入新构造活动期,深水区表现为快速沉积作用,断裂活动较弱。 相似文献
6.
琼东南盆地华光凹陷构造特征及沉积充填 总被引：4，自引：0，他引：4
南海北部大陆边缘发育多个新生代含油气盆地。近年来,在南海北部珠江口盆地南部深水区陆续发现大中型气藏,证实了该区油气地质条件优越。琼东南盆地南部深水区与珠江口盆地深水区具有相似的构造沉积演化史,油气地质条件相似,具有形成大中型油气藏的地质条件,因此十分有必要开展该区的构造特征及沉积充填研究。基于近年来新采集的高精度地震资料,对华光凹陷构造特征进行详细分析,认为区内发育4种伸展构造样式,分别是地堑、半地堑、多米诺式半地堑和地垒;经历两个构造演化阶段,形成"下断上拗"的双层结构特征,相应发育两个期次的正断层。下构造层古近系受裂陷作用控制,断层发育,地层分布受断裂控制明显,上构造层新近系-第四系构造活动微弱,断层不发育,地层变形小且沉积厚度趋于稳定。华光凹陷古近系为河湖相-海陆过渡相沉积,其中下渐新统崖城组煤系地层是琼东南盆地勘探证实的主要烃源岩层系,上渐新统陵水组是主要储层发育时期,新近系-第四系为浅海-半深海-深海相沉积,其中中新统储层发育,上中新统及以上海相泥岩是良好的盖层。因此,华光凹陷具有良好的生储盖组合。 相似文献
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《海洋地质前沿》2017,(2)
西纳土纳盆地是发育在东南亚巽他克拉通内的裂谷盆地,也是印度尼西亚重要的含油气盆地。运用盆地分析及石油地质学的理论与方法,对盆地构造—沉积演化及主力烃源岩、储集层及盖层等成藏要素进行综合研究,系统总结油气成藏特征及分布规律,并通过对比分析指出构造演化与沉积充填差异是造成盆地内烃源岩演化、储集层发育、油气成藏特征差异的主控因素。研究表明,油气可采储量区域上集中在Anambas地堑和Penyu次盆东北部,主要油气田(藏)类型包括挤压背斜、披覆构造和地层—构造型;层系上,油气主要储集于上渐新统和下中新统。盆地内远景地层圈闭以上始新统—下渐新统Belut组冲积扇相砂砾岩和上渐新统—下中新统Gabus—下Arang组河流下切谷砂岩为有利储层,勘探程度低,资源潜力较大。 相似文献
8.
《海洋地质与第四纪地质》2016,(2)
根据莺歌海盆地区域地质背景与古新近系构造沉积演化特征,结合钻井资料和前人烃源岩研究及生烃模拟实验结果,深入研究了不同层位烃源岩尤其是古近系烃源岩地球化学特征,重点剖析了烃源条件及高温高压环境中有机质热演化成烃特点。研究表明,中新统海相陆源烃源岩分布较广泛,其有机质干酪根类型属Ⅱ2—Ⅲ型,处在成熟-高熟大量生气阶段,为盆地浅层及中深层天然气气藏主要烃源岩;始新统及渐新统湖相及煤系亦是盆地重要烃源岩,主要分布在盆地西北部及与琼东南盆地毗邻的东南部,其生源母质类型属偏腐殖型,且处于成熟-高熟/裂解气阶段,具有较大生烃潜力。基于盆地构造沉积演化特点与烃源条件分析,结合近年来天然气勘探成果与有利油气富集区带综合评价,预测盆地临高反转构造带及临高海口-昌化区是勘探古近系烃源供给之油气有利富集区;莺东斜坡以及靠近琼东南盆地1号断裂带附近区域亦是勘探古近系烃源供给之油气的重要勘探领域。同时中深层深部高温超压九大构造圈闭系列则是勘探发现大中型天然气田群建成特大气区的主战场。 相似文献
9.
南沙海域区域地质构造 总被引：25，自引：1，他引：24
以多年来在南沙海域的海洋地质－地球物理综合考察所取得的资料为基础,分析研究了区内的地球物理场特征、深部地壳结构、基底性质、断裂构造等,其中断裂构造划分出正断裂、逆冲断裂和走滑断裂３个系统,区域上划分出３大块体和６个地块。叠置在不同地壳类型和基底之上或不同构造部位的１３个主要的大中型新生代盆地,具有沉积厚度大、盆地类型多、规模大的特点,是多种盆地原型的叠覆盆地,也是油气资源的重要场所。 相似文献
10.
太平洋板块、印度板块和欧亚板块的演化对中国东部古近纪沉积盆地的沉降及充填具有控制作用。讨论了我国东部新生代断陷盆地群的深部构造背景,在相对统一的板块构造背景中初步分析了陆缘断陷盆地和陆内断陷盆地的形成演化与周边板块主要构造运动事件的关系,并对这种关系的一致性进行了简要讨论。在此基础上,对不同构造演化阶段内的陆缘和陆内断陷盆地的沉积建造特点和沉降中心迁移规律进行了对比分析,对位于中国东部复杂构造体制内不同位置的陆缘与陆内断陷盆地每个构造演化阶段的沉积响应特征及其一致性和差异性进行了初步研究。将东部陆内和陆缘断陷盆地的沉积建造渐变特征或变异规律与深部构造过程表现进行综合分析,对深入理解我国东部陆相断陷盆地群系的盆间关系,深入认识新生代断陷盆地浅部过程与深部过程之间的耦合具有重要理论意义。 相似文献
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12.
《Deep Sea Research Part I: Oceanographic Research Papers》1999,46(10):1779-1792
Many of the deep basins filled by hot brines in the Red Sea have not been investigated since their discovery in the early 1970s. Twenty years later, in September 1992, six of these deeps were revisited. The temperature and salinity of the Suakin, Port Sudan, Chain B, and Nereus deeps ranged from 23.25 to 44.60°C and from 144 to 270‰. These values were approximately the same in 1972, indicating that the budget of heat and salt was quite balanced. We measured strong gradients of properties in the transition zone between brines and overlying seawater. The contribution of salinity to the density gradient was more than one order of magnitude higher than the opposite contribution of temperature across the seawater–brine interface. Therefore the interface was extemely stable, and the transfer of properties across it was considered to be controlled mostly by molecular diffusion. We calculate that the diffusional transport of salt from the brines to seawater cannot affect significantly the salinity of the brines over a 20 year period, which agrees with the observations. The brine pools can persist for centuries with no salt input. Therefore, the persisence of brines does not correspond to a steady balance between diffusional loss and continuous input of hydrothermal solutions. Deeps that experience only episodical hydrothermal brine supplies may persist for a long time with salt inherited from past inputs. The theoretical loss of heat by diffusion from the brine to seawater was higher than the observed decrease in temperature of the brine pool during the 20 year period of observation. We calculated that the heat flux out of the pools into the overlying seawater was compensated by a heat flux into the pools of about 250–600 mW/m2. This range of values corresponds to bottom heat flow values that have been reported earlier for the axial zone of the Red Sea. In contrast to the other brine pools, the temperature and salinity of the Valdivia Deep brine increased by 4.1°C and 10‰, respectively, between 1972 and 1992, which is explained by present-day hydrothermal brine discharge. 相似文献
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14.
察尔汗盐湖地下卤水动态规律研究 总被引：2，自引：0，他引：2
建立了描述采卤过程中地下卤水运动规律的数学模型,并用有限元素法进行了数值迭代求解。在此基础上,用等值线比较法,根据1988年3月—1989年6月间65个观测点上每月一次的地下卤水的水位观测数据,对首采区中312个剖分节点上的渗透系数等水文地质参数进行了修正和反求。经修正反求后地下卤水水位的模拟值与实测值之间的相对误差由原来的14．3％改善为7.7％。 相似文献
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The densities of artificial and real Red Sea brines have been measured at 25°C with a vibrating tube densimeter. Measurements were also made on mixtures of Red Sea brines with seawater and pure water. The results have been used to characterize the density—composition relations of waters across the interface of brine and average Red Sea waters. The results for the real and artificial brines are in reasonable agreement.The composition of the brines and mixtures with seawater have been characterized by conductivity measurements of weight diluted samples. The conductivity salinities were found to be conservative to within for the mixtures.The densities of brines and mixtures of brines and seawater were estimated from apparent molal volume data using Young's rule. The calculated densities for all of the solutions were found to be in good agreement with the measured values, demonstrating the applicability of Young's rule to concentrated natural waters. 相似文献
17.
R. Hekinian J. Francheteau V. Renard R. D. Ballard P. Choukroune J. L. Cheminee F. Albarede J. F. Minster J. L. Charlou J. C. Marty J. Boulegue 《Marine Geophysical Researches》1983,6(1):1-14
A submersible study of a fast spreading (12 cm yr-1) Mid-Ocean ridge segment (East Pacific Rise near 12°50′ N) led to the discovery of intense hydrothermal activity. Twenty four sites with active vents and sixty inactive hydrothermal deposits were found within a narrow graben averaging about 300 m in width along a 20 km long segment of the ridge crest. The graben is floored with fresh basaltic sheet flows including collapsed pits or lava lake structures. From both deep towed camera stations and manned submersible observations, it is estimated that the average spacing between the ridge axis hydrothermal deposits averaging in size 10–50 m in diameter lies between 100 to 200 m. The hydrothermal deposits found in the central graben are believed to have formed rapidly (on the order of a few decades). Detailed investigations of one active site have enabled us to witness the growth of an active chimney which increased its height by 40 cm in 5 days i.e. 8 cm per day. Extensive hydrothermal deposits were discovered on an off-axis seamount located 6 km East of the ridge axis. The hydrothermal deposits found on both the ridge axis and on the seamount are similar in composition and consist essentially of zinc, copper and iron mineral phases. Chemical studies conducted on the venting fluids (320°C) showed that the concentration of the dissolved major metal ions (Fe, Mn, and Zn) is about 0.10–0.13 gl-1. If we accept an average flow rate of 10ls-1 based on visual observations the mass of metallic products spewing out from an active chimney must be about 100 kg per day. 相似文献
18.
A marine controlled source electromagnetic (CSEM) campaign was carried out in the Gulf of Mexico to further develop marine electromagnetic techniques in order to aid the detection and mapping of gas hydrate deposits. Marine CSEM methods are used to obtain an electrical resistivity structure of the subsurface which can indicate the type of substance filling the pore space, such as gas hydrates which are more resistive. Results from the Walker Ridge 313 study (WR 313) are presented in this paper and compared with the Gulf of Mexico Gas Hydrate Joint Industry Project II (JIP2) logging while drilling (LWD) results and available seismic data. The hydrate, known to exist within sheeted sand deposits, is mapped as a resistive region in the two dimensional (2D) CSEM inversion models. This is consistent with the JIP2 LWD resistivity results. CSEM inversions that use seismic horizons provide more realistic results compared to the unconstrained inversions by providing sharp boundaries and architectural control on the location of the resistive and conductive regions in the CSEM model. The seismic horizons include: 1) the base of the gas hydrate stability zone (BGHSZ), 2) the top of salt, and 3) the top and bottom of a fine grained marine mud interval with near vertical hydrate filled fractures, to constrain the CSEM inversion model. The top of salt provides improved location for brines, water saturated salt, and resistive salt. Inversions of the CSEM data map the occurrence of a ‘halo’ of conductive brines above salt. The use of the BGHSZ as a constraint on the inversion helps distinguish between free gas and gas hydrate as well as gas hydrate and water saturated sediments. 相似文献
19.
Catherine Pierre Germain Bayon Marie-Madeleine Blanc-Valleron Jean Mascle Stéphanie Dupré 《Geo-Marine Letters》2014,34(2-3):253-267
On the passive margin of the Nile deep-sea fan, the active Cheops mud volcano (MV; ca. 1,500 m diameter, ~20–30 m above seafloor, 3,010–3,020 m water depth) comprises a crater lake with hot (up to ca. 42 °C) methane-rich muddy brines in places overflowing down the MV flanks. During the Medeco2 cruise in fall 2007, ROV dives enabled detailed sampling of the brine fluid, bottom lake sediments at ca. 450 m lake depth, sub-surface sediments from the MV flanks, and carbonate crusts at the MV foot. Based on mineralogical, elemental and stable isotope analyses, this study aims at exploring the origin of the brine fluid and the key biogeochemical processes controlling the formation of these deep-sea authigenic carbonates. In addition to their patchy occurrence in crusts outcropping at the seafloor, authigenic carbonates occur as small concretions disseminated within sub-seafloor sediments, as well as in the bottom sediments and muddy brine of the crater lake. Aragonite and Mg-calcite dominate in the carbonate crusts and in sub-seafloor concretions at the MV foot, whereas Mg-calcite, dolomite and ankerite dominate in the muddy brine lake and in sub-seafloor concretions near the crater rim. The carbonate crusts and sub-seafloor concretions at the MV foot precipitated in isotopic equilibrium with bottom seawater temperature; their low δ13C values (–42.6 to –24.5‰) indicate that anaerobic oxidation of methane was the main driver of carbonate precipitation. By contrast, carbonates from the muddy lake brine, bottom lake concretions and crater rim concretions display much higher δ13C (up to –5.2‰) and low δ18O values (down to –2.8‰); this is consistent with their formation in warm fluids of deep origin characterized by 13C-rich CO2 and, as confirmed by independent evidence, slightly higher heavy rare earth element signatures, the main driver of carbonate precipitation being methanogenesis. Moreover, the benthic activity within the seafloor sediment enhances aerobic oxidation of methane and of sulphide that promotes carbonate dissolution and gypsum precipitation. These findings imply that the coupling of carbon and sulphur microbial reactions represents the major link for the transfer of elements and for carbon isotope fractionation between fluids and authigenic minerals. A new challenge awaiting future studies in cold seep environments is to expand this work to oxidized and reduced sulphur authigenic minerals. 相似文献
20.
Stéphanie Dupré Jean Mascle Jean-Paul Foucher François Harmegnies John Woodside Catherine Pierre 《Geo-Marine Letters》2014,34(2-3):153-168
The Menes caldera is a fault-controlled depression (~8 km in diameter) at ~3,000 m water depth in the western province of the Nile deep-sea fan off NW Egypt, comprising seven mud volcanoes (MVs) of which two are active. Based on multichannel and chirp seismic data, temperature profiles, and high-resolution bathymetric data collected during the 2000 Fanil, 2004 Mimes and 2007 Medeco2 expeditions, the present study investigates factors controlling MV morphology, the geometry of feeder channels, and the origin of emitted fluids. The active Cheops and Chephren MVs are 1,500 m wide with subcircular craters at their summits, about 250 m in diameter, generally a few tens of metres deep, and filled with methane-rich muddy brines with temperatures reaching 42 °C and 57 °C respectively. Deployments of CTDs and corers with attached temperature sensors tracked these warm temperatures down to almost 0.5 km depth below the brine lake surface at the Cheops MV, in a feeder channel probably only a few tens of metres wide. Thermogenic processes involve the dissolution of Messinian evaporites by warm fluids likely sourced even deeper, i.e. 1.7 and 2.6 km below the seabed at the Cheops and Chephren MVs respectively, and which ascend along listric faults. Seepage activity appears broadly persistent since the initiation of mud volcanism in the Early Pliocene, possibly accompanied by lateral migration of feeder channels. 相似文献