鄂尔多斯盆地延长组湖盆中部长6厚层砂体成因分析

笔者对鄂尔多斯盆地湖盆中部地区延长组长6物源分析、沉积相类型、坡折带控砂、砂体分布规律等进行了研究。东北、西南两大物源提供了充足的物质基础,发育三角洲牵引流作用的沉积砂岩和重力搬运的浊积砂岩,主要为叠置水下分流河道、河口砂坝-水下分流河道和滑塌浊积岩等不同类型的砂体组合,形成了垂直湖岸线和平行湖岸线展布的巨型厚砂岩分布带。     

Mass-transport deposits on the Rosetta province (NW Nile deep-sea turbidite system, Egyptian margin): Characteristics, distribution, and potential causal processes

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.     

广西丹池盆地泥盆系浊积岩和硅质岩的特征及构造意义

对广西丹池地区泥盆系浊积岩和硅质岩的沉积特征、岩石化学成分和形成机制的研究表明,它们是在受同生断裂控制的深水拗陷盆地中,由浊流和热水沉积而形成的沉积岩石。相同类型岩石的分布特征表现南盘江晚古生代沉积盆地呈浅海“台地”和深海“槽沟”相间排列的构造格局,其形成和演化与滇黔桂地体和云开地体的碰撞拼贴造山作用以及造山后地壳的蠕散拉伸作用有关。     

湘黔桂浅变质岩区含金建造及其与金矿的关系

湘黔桂相邻区中、新元古界浅变质岩系的含金建造多为斜坡-盆地相、深水-较深水、远源-中源的浊流沉积,常富含凝灰质、碳质及硫化物,属于活动大陆边缘地壳强烈拉伸环境的产物,形成于扬子古大陆裂陷和再度裂陷时期.中、新元古代火山活动为其提供了丰富的成矿物质,多数成为原生含金建造,个别成为衍生含金建造.这些含金建造在形成之后,先后遭受了区域埋深变质作用、区域动力变质作用,以及脆韧性、脆性剪切作用,最终形成了变质细碎屑岩型金矿.     

灾变事件地层斜坡滑塌（带）堆积的特征——以滇西保山地区上三叠统南梳坝组为例

保山地块保山地区三叠系上统南梳坝组研究程度较差,以往的资料多侧重于岩石地层、生物地层的研究,沉积环境资料甚少。通过1∶5万保山幅等8幅区域地质调查,在南梳坝组中发现了灰岩滑塌岩块、下超面、饥饿沉积、水道砾岩、粒序层理、复理石韵律及槽模、沟模等一系列非常重要的沉积相资料,认为其沉积环境为斜坡-盆地环境,总体为一套浊积岩,其中的同沉积＂褶皱＂、同沉积断层、大量的滑塌面、各种类型的滑塌褶皱组成了3条较大规模的滑塌带,是斜坡环境的沉积物在地震作用触发下形成的,剖面结构＂不合理＂,明显具有灾变事件地层的特征。灰岩滑塌岩块有极浓的油气味,显示出生储存油气的良好环境。因此,重塑三叠系上统南梳坝组的古地理环境,不仅对发展沉积学、地层学有重要意义,而且对于寻找烃源岩也有重要的现实意义。     

东濮凹陷濮卫环洼带沙三段沉积体系及储层发育规律

为了提高东濮凹陷濮卫环洼带隐蔽油气藏的勘探精度,以层序地层学理论和瓦尔特相律为指导,通过钻井岩芯、测井和地震的三元分析法,综合构造-地层分析,在东濮凹陷濮卫环洼带沙三段共识别出湖底扇、滨浅湖砂坝-风暴、低位盐湖、三角洲、深湖-半深湖等五种沉积体系,分析了主要储层发育期沉积体系的时空展布特征,探讨了层序地层体制下沙三段的沉积体系发育模式及储层发育规律,指出环洼带东部及北部水下河道与坡折带的交汇处是储层的主要发育地带,其沉积体系主要为湖底扇、三角洲沉积体系.     

Dynamics of Saturn's magnetodisk near Titan's orbit: Comparison of Cassini magnetometer observations from real and virtual Titan flybys

We analyze the variability of the ambient magnetospheric field along Titan's orbit at 20.3 Saturn radii. However, while our preceding study (Simon et al., 2010) focused on Cassini magnetometer observations from the 62 Titan flybys (TA-T62) between October 2004 and October 2009, the present work discusses magnetic field data that were collected near Titan's orbit when the moon was far away. In analogy to the observations during TA-T62, the magnetospheric fields detected during these 79 “virtual” Titan flybys are strongly affected by the presence of Saturn's bowl-shaped and highly dynamic magnetodisk current sheet. We therefore provide a systematic classification of the magnetic field observations as magnetodisk current sheet or lobe-type scenarios. Among the 141 (62 real+79 virtual) crossings of Titan's orbit between July 2004 and December 2009, only 17 encounters (9 real+8 virtual) took place within quiet, magnetodisk lobe-type fields. During another 50 encounters (21 real+29 virtual), rapid transitions between current sheet and lobe fields were observed around the moon's orbital plane. Most of the encounters (54=22 real+32 virtual) occurred when Titan's orbit was embedded in highly distorted current sheet fields, thereby invalidating the frequently applied idealized picture of Titan interacting with a homogeneous and stationary magnetospheric background field. The locations of real and virtual Titan flybys are correlated to each other. Each of the 62 real Titan flybys possesses at least one virtual counterpart that occurred shortly before or after the real encounter and at nearly the same orbital position. A systematic comparison between Cassini magnetometer observations from the real Titan flybys and their virtual companions suggests that there is no clear evidence of Titan exerting a significant level of control on the vertical oscillatory motion of the magnetodisk near its orbit.     

东营中央洼陷带缓坡远岸浊积扇体系序列及其含油气性

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。     

青海省贵南县过马营一带早中三叠世隆务河组沉积特征

青海贵南县过马营一带隆务河组为一套典型的浊流沉积,对此套浊积岩的沉积特征进行研究。通过对过马营一带隆务河组浊积岩的岩石组合特征、地层层序及鲍玛层序特征分析,探讨其沉积环境特征,并与典型浊积扇模式对比,建立沉积模型。综合分析认为,隆务河组由下向上的3个段分别位于浊积扇的外扇、中扇、内扇,其中中扇辫状河道发育。此研究对于西秦岭造山带的沉积环境分析及构造演化具有重要的意义。     

Discovery of an outcropping Mass Transport Deposit (MTD) in the Palaeogene subalpine synclines of southeastern France: Implications on flexural sub-basin deformation

We document the sedimentary facies of a large Mass Transport Deposit (MTD) within the sand-rich sediment gravity flow-dominated deposits of the Eocene–Oligocene south-western Alpine forelands (Annot Sandstone system). The MTD with an approximated volume of several hundreds of cubic kilometres fills a sub-basin located in the Mont-Tournairet confined sub-basin. Autochthonous facies are very typical sediment gravity-flow deposits (thin-bedded classical turbidites and thick-bedded hyperconcentrated to concentrated flow deposits) that stratigraphically belong to the Annot Sandstone infill. Slumps and internal metre-large fold axes of the deformed stratigraphic intervals indicate a main transport direction towards the northwest. The seafloor instability that led to the mass-flow events within the Mont-Tournairet sub-basin could have been favoured by high sedimentation rates in a small, confined and tectonically active sub-basin, possibly enhanced by local structural deformation associated with the Triassic evaporites on the eastern side of the Mont-Tournairet confined basin. The presence of the MTD suggests that a period of increased flexural subsidence rate and basin deformation occurred in this portion of the subalpine foreland basin. Therefore, the MTD forms a stratigraphic marker of a period of tectonic activity.