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71.
综合1:5万区调成果,系统阐述了赣西北地区双桥山群的沉积学特征,认为是一套形成于滨海-半深海环境的重力流沉积体系,基本发育-系列重力流沉积相单元,即块状混杂砾岩相,正递变砾岩相,经典浊积岩相等,对各单元基本层序特征进行了总结论述,并结合地球化学特征及粒度分析成果探讨了沉积环境。  相似文献   
72.
东营中央洼陷带缓坡远岸浊积扇体系序列及其含油气性   总被引:3,自引:0,他引:3  
通过对东营中央洼陷带沙三段浊积砂体的物源和成因类型分析认为该区在沙三段沉积时期形成了南部物源和东部物源共同起作用的沉积格局。其中,南部的物源影响了整个中央洼陷带,沙三段共形成5套规模较大的缓坡远岸浊积扇序列;而东部的物源只影响东营三角洲前缘的局部地区,形成了一些规模较小的滑塌浊积扇。同时指出梁家楼地区沙三段上亚段底部发育的缓坡远岸浊积扇属于较罕见的大型低位扇体系,并认为东营中央洼陷带沙三段下亚段也具有该类成因扇体的发育条件,其勘探潜力优于沙三段中、上亚段,发现大型的、以缓坡远岸浊积扇为储层的岩性油藏的可能性较大。  相似文献   
73.
在川西北壤塘地区三叠系西康群海底扇填图实践的基础上 ,从海底扇的沉积特征入手 ,对填图中存在的问题及区调方法、内容进行了分析与探讨 ,提出了岩相—基本层序—组 (地层 )的海底扇填图新方法。  相似文献   
74.
洼陷中浊积岩沉积特征及油气富集规律研究   总被引:13,自引:1,他引:13       下载免费PDF全文
随着油气勘探的不断深入,我国东部地区主要含油气盆地勘探的主要目标逐渐转为一些较复杂的隐蔽油气藏,尤其是盆内的次级洼陷,已成为勘探的重要地区。多年的勘探实践表明,对于我国东部的陆相箕状盆地,洼陷中含油气是必然规律。在洼陷内最重要的油藏类型是砂体岩性与构造—岩性油藏,并且绝大多数为浊流成因。本文以山东济阳坳陷与昌潍坳陷的德南、牛庄、利津、博兴等几个洼陷为例,介绍洼陷生油条件的地震研究方法与三角洲—浊积扇体系中浊积岩发育区的沉积特征、油气富集规律及地震综合研究方法。  相似文献   
75.
笔者通过海平面变化曲线与碳氧同位素曲线比较,发现两者曲线基本吻合,碳同位素曲线显示的海平面变化更接近露头层序地层的海平面变化;氧同位素曲线与露头层序海平面变化大体一致。局部出现相反结论。碳同位素曲线对沉积环境变化较氧同位素曲线更敏感。通过两者曲线研究,说明运用稳定同位素曲线变化可作为浊积岩层序地层学研究的一个研究手段。  相似文献   
76.
Abstract The outer parts of a number of small Late Jurassic sandy deep‐water fans in the northern North Sea are dominated by the stacked deposits of co‐genetic sandy and muddy gravity flows. Sharp‐based, structureless and dewatered sandstone beds are directly overlain by mudclast breccias that are often rich in terrestrial plant fragments and capped by thin laminated sandstones, pseudonodular siltstones and mudstones. The contacts between the clast‐rich breccias and the underlying sandstones are typically highly irregular with evidence for liquefaction and upward sand injection. The breccias contain fragments (up to metre scale) of exotic lithologies surrounded by a matrix that is extremely heterogeneous and strewn with multiphase and variably sheared sand injections and scattered coarse and very coarse sand grains (often coarser than in the immediately underlying sand bed). Markov chain analysis establishes that the breccias consistently overlie sandstones, and the character of the breccias and their external contacts rule out a post‐depositional origin via in situ liquefaction, intrastratal flowage or bed amalgamation and disruption. The breccias are interpreted as debrites that rode on a water‐rich sand bed just deposited by a co‐genetic concentrated gravity current. As such, they are referred to as ‘linked debrites’ to distinguish them from debrites emplaced in the absence of a precursor sand bed. The distinction is important, because these linked debris flows can achieve significant mobility through entrainment of both water and sediment from beneath, and they ride on a low‐friction carpet of liquefied sand. This explains the paradox presented by fan fringes in which there are common debrites, when conventional thinking might predict that deposits of low‐concentration gravity currents should be more important here. In fact, evidence for transport by low‐concentration turbidity currents is rare in these systems. Several possible mechanisms might explain the formation of linked flows, but the ultimate source of both sandy and clast‐rich flow components must be in shallower water on the basin margin (the debrites are not triggered from distal slopes). Flow partitioning may have occurred by upslope erosion and retardation of the mudclast‐charged portion of an erosional sandy density current, partial flow transformation of a precursor debris flow and/or hydraulic segregation and reconcentration of the flaky clasts and carbonaceous matter during transport. Linked debrites are not restricted to small sand‐rich fans, and similar mechanisms may be responsible for the long runout of debris flows in other systems. The recognition of a distinct class of linked debrites is of wider importance for facies prediction, reservoir heterogeneity and even carbon fluxes and sequestration on continental margins.  相似文献   
77.
The partitioning of different grain-size classes in gravity flow deposits is one of the key characteristics used to infer depositional processes. Turbidites have relatively clean sandstones with most of their clay deposited as part of a mudstone cap or as a distal mudstone layer, whereas sand-bearing debrites commonly comprise mixtures of sand grains and interstitial clay; hybrid event beds develop alternations of clean and dirty (clay-rich) sandstones in varying proportions. Analysis of co-genetic mudstone caps in terms of thickness and composition is a novel approach that can provide new insight into gravity flow depositional processes. Bed thickness data from the ponded Castagnola system show that turbidites contain more clay overall than do hybrid event beds. The Castagnola system is characterized by deposits of two very different petrographic types. Thanks to this duality, analyses of sandstone and mudstone composition allow inference of which proportion of the clay in each of the deposit types was acquired en route. In combination with standard sedimentological observations the new data allow insight into the likely characteristics of their parent flows. Clean turbidites were deposited by lower concentration, long duration, erosive, muddy turbidity currents which were more efficient at fractionating clay particles away from their basal layer. Hybrid event beds were deposited by shorter duration, higher-concentration, less-erosive sandier flows which were less efficient at clay fractionation. The results are consistent with data from other turbidite systems (for example, Marnoso-arenacea). The approach represents a new method to infer the controls on the degree of clay partitioning in gravity flow deposits.  相似文献   
78.
IODP367/368航次在南海北部深海盆地多个站位发现上中新统厚达数百米的大规模深海浊积岩。采用碎屑锆石U-Pb年龄谱系分析方法对U1500站上中新统浊积砂体进行源汇对比分析。研究结果表明U1500站上中新统浊积岩碎屑锆石年龄谱系与其西侧琼东南盆地和北侧珠江口盆地中新世沉积物特征类似。多维排列分析(MDS)结果也显示,该站位样品与珠江口盆地、琼东南盆地沉积物关系密切,表明南海北部深海盆地内厚达数百米的上中新统浊积砂体为南海北部物源和南海西部物源混合堆积形成。南海西部陆源输入物质以浊流搬运的方式,沿中央峡谷从西到东搬运至南海东部深海盆地;南海北部珠江物源以重力流的形式,经南海北部陆坡峡谷搬运至深海盆地中,两种来源的沉积物在深海盆地发生混合沉积,形成U1500站厚达数百米的浊积砂体。南海北部深海盆地厚层浊积砂体物质来源的准确识别,对深刻理解南海新生代盆地的构造演化、沉积物充填过程、物源演变以及古地理特征均具有重要意义。  相似文献   
79.
In the Nile deep-sea turbidite system (NDSTS), the province fed by the Rosetta branch of the Nile delta is characterised by the recurrent activity of gravity processes. Seven mass-transport deposits (MTDs) were recognised from the upper to the mid slope, downstream from imbricated scars (~ 30 km-long, ~ 200 m high) running along the shelf edge nearby the Rosetta canyon. Extending on surfaces between 200 and 5000 km2, with estimated volumes from 3 to 500 km3, these MTDs represent about 40% (up to 90% locally) of the total Pleistocene–Holocene sedimentary thickness. Three types of MTDs can be distinguished on the basis of their scale. Each has also a distinctive internal configuration and distribution within the Rosetta depositional setting. Age estimates of two MTDs point towards relationships between climate and submarine mass failures through sea-level changes, sediment supply, or a combination of both. Additionally, the presence of gas in the sediment and earthquake shaking may have concurred to trigger large-scale failures on the low slope angles (1°–2°) of the Rosetta area.  相似文献   
80.
A complete transect of a fossil carbonate ramp slope has been reconstructed using outcrop data from the Lower-Middle Eocene Anotz Formation in the western Pyrenees. The Anotz Formation contains four calciclastic (mostly bioclastic) members encased within hemipelagic marl/limestone alternations, each calciclastic member representing a submarine fan system. Individual fans are composed of a gullied upper slope, a leveed feeder channel, a channelized lobe area, an unconfined lobe zone and a peripheral lobe fringe that grades downcurrent into basinal deposits. Quantitative data on the dimensions and degree of lateral continuity and vertical connectivity of the Anotz calciclastic fan elements are presented. These data provide information for a better understanding of the intrinsic nature of calciclastic submarine fans and to model their reservoir potential. The long-term evolution of the Anotz carbonate slope was generally progradational, as evidenced by the four discrete episodes of calciclastic-fan development. The location of the fans was controlled by the synsedimentary tectonic activity of the Pamplona fault, which created a slope valley along which the reworked shallow-water calciclastic sediments were funnelled. In addition, episodic basinward tilting of the shallow-water carbonate ramp, linked to the development of the South Pyrenean foreland basin, switched on and off the process of calciclastic resedimentation and determined the growth or abandonment of the fan systems.  相似文献   
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