松辽盆地南部泉头组砂岩型铀矿成矿条件分析

通过对松辽盆地南部泉头组砂岩型铀成矿条件分析认为: 泉头组半干旱的亚热带古气候对成矿有利。河流相和三角洲相沉积具有形成厚大砂体的条件。砂体较为发育, 单层砂体厚度可达42 m。虽砂体中有机质含量较低, 但泉头组下部含煤层中的烃类可通过断裂构造及不整合面上升进入砂体, 弥补还原剂的不足。工业铀矿孔的发现反映出泉头组有铀的大规模富集。总之, 泉头组是松辽盆地南部一个重要的找矿目的层, 找矿意义重大。     

云南大姚地区上白垩统马头山组六苴段中亚段

上白垩统马头山组六苴段中亚段(K2ml2)是云南六苴砂岩型铜矿区内含铜层位之一.六苴段中亚段含铜砂岩Mo、Cd、As、Cu等亲硫元素富集.微量元素多富集于浅色砂岩中,向紫色砂岩一侧逐渐亏损,呈现分带特征.铜矿石V/(V+Ni)值大于0.7,反映缺氧环境的特点.稀土元素总量(∑REE)101.71×106～157.55×10-6,稀土元素分配模式为Eu、Ce亏损-轻稀土元素富集型.从铜矿石→浅色矿化砂岩→浅色无矿砂岩,随着铜含量的降低,Mo、Cd、As、Hg平均含量逐渐降低,∑REE与高场强元素Nb、Zr、Hf、Th平均含量逐渐升高.六苴段中亚段砂岩具"矿源层"的特征,铜矿石与围岩具物源一致性,铜矿石在弱碱性、还原条件下由砂岩经水-岩作用形成,与六苴铜矿床(K2ml1)成矿机理相似.小河地段纵向上从北向南,六苴段中亚段中铜矿化的能力逐渐减弱,推测矿化带在走向上向西(紫色砂岩一侧)发生了偏移.     

临南洼陷带滩坝砂岩储层分布

临南洼陷带沙四段滨浅湖滩坝相成因的砂体广泛发育,近年来已成为该区十分重要的勘探后备阵地。但该区火成岩发育,地震资料品质较差,滩坝砂的分布发育不清,不利于勘探部署。在深化研究沙四上亚段古地貌、沉积特征的基础上,运用频谱分解等技术提高地震资料分辩率,综合利用了正演及属性分析等技术,对滩坝砂岩的发育范围进行了预测,取得了良好的效果,为该层系油藏的勘探提供了可靠的依据。     

Control of tectonic setting and large-scale faults on the basin-scale distribution of deformation bands in porous sandstone (Provence,France)

From outcrops located in Provence (South-East France), we describe the distribution, the microstructures, and the petrophysical properties of deformation band networks related to both contractional and extensional tectonic events. In contraction, pervasively distributed networks of reverse-sense compactional shear bands are observed in all folded sand units of the foreland, whereas localized networks of clustered reverse-sense shear bands are only observed close to a large-scale thrust. In extensional setting, networks of clustered normal-sense shear bands are generally observed adjacent to map-scale faults (100 m–10 km scale), although some randomly distributed bands are also observed between these faults. Normal-sense cataclastic faults, i.e. zone of deformation bands containing a localized slip-surface, are also observed to be restricted to sand units, suggesting that faults initiated in the sands during extension, but not during contraction. Shear bands and faults show cataclastic microstructures with high-permeability reduction whereas compactional shear bands show crush microbreccia or protocataclastic microstructures with moderate permeability reduction. This basin-scale analysis underlines the major role of tectonic settings (thrust-fault versus normal-fault andersonian-stress regime) and the influence of inherited large-scale faults on the formation/localization of low-permeability shear bands. We also provide a geometrical analysis of the band network properties (spacing, thickness, shear/compaction ratio, degree of cataclasis, petrophysical properties) with respect to the median grain size, porosity and grain sorting of host sand. This analysis suggests that grain size, although less important than stress-state conditions and the presence of large-scale faults, has a non-negligible effect on band network geometry. No correlations are observed between the grain sorting, porosity and band network geometry.     

鄂北致密薄储层地震响应特征分析

鄂尔多斯盆地北部大牛地气田塔巴庙区块致密薄层发育。利用岩石物理等数据的物性参数,对不同储集条件下的薄层、薄互层进行地震正演分析。结果表明:在薄层特别是薄互层条件下,叠前波场响应特征十分复杂,有别于常规AVO类型的变化规律,且含气层和干层的响应特征有明显差异。根据叠前地震波场的响应特征和不同的变化规律可以细化薄层研究,进一步识别储集类型。     

河北省石家庄市南部污灌区厚层包气带污染物自然衰减的微生物作用潜力评价

本次研究的目的是利用传统的培养技术和现代的磷脂脂肪酸PLFA(Phosphor Lipid Fatty Acid)技术、Biolog技术、16 S rRNA基因变性梯度凝胶电泳DGGE(Denaturing Gradient Gel Electrophoresis)及测序技术,调查石家庄市南部污灌区厚近30 m包气带微生物含量、分布、活性和多样性,评价污灌区厚层包气带污染物自然衰减的微生物作用潜力。包气带沉积物样品通过岩芯钻探获得,用于物理、化学和微生物分析。结果显示,土壤层(5~20 cm)微生物含量高,活性高,代谢类型多,可培养的异养菌与自养菌、好氧异养菌、兼性厌氧异氧菌和专性厌氧异养菌共存;土壤层下伏包气带微生物含量较低,活性降低,代谢类型减少,可培养的细菌主要是好氧性异养菌、兼性厌氧异养菌和好氧自养菌,而且随岩性而变化,在砂层和重粘土层含量低,活性低,而在亚粘土层含量和活性大。研究结果指示土壤层具有很高的污染物生物自然衰减潜力,而且下伏包气带仍有这种潜力,特别是下部溶解有机碳DOC(Dissolved Organic Carbon)含量高的层位潜力更大。     

Matrix‐rich and associated matrix‐poor sandstones: Avulsion splays in slope and basin‐floor strata

A common facies observed in deep‐water slope and especially basin‐floor rocks of the Neoproterozoic Windermere Supergroup (British Columbia, Canada) is structureless, coarse‐tail graded, medium‐grained to coarse‐grained sandstone with from 30% to >50% mud matrix content (i.e. matrix‐rich). Bed contacts are commonly sharp, flat and loaded. Matrix‐rich sandstone beds typically form laterally continuous units that are up to several metres thick and several tens to hundreds of metres wide, and commonly adjacent to units of comparatively matrix‐poor, scour‐based sandstone beds with large tabular mudstone and sandstone clasts. Matrix‐rich units are common in proximal basin‐floor (Upper Kaza Group) deposits, but occur also in more distal basin‐floor (Middle Kaza Group) and slope (Isaac Formation) deposits. Regardless of stratigraphic setting, matrix‐rich units typically are directly and abruptly overlain by architectural elements comprising matrix‐poor coarse sandstone (i.e. channels and splays). Despite a number of similarities with previously described matrix‐rich beds in the literature, for example slurry beds, linked debrites and co‐genetic turbidites, a number of important differences exist, including the stratal make‐up of individual beds (for example, the lack of a clean sandstone turbidite base) and their stratigraphic occurrence (present throughout base of slope and basin‐floor strata, but most common in proximal lobe deposits) and accordingly suggest a different mode of emplacement. The matrix‐rich, poorly sorted nature of the beds and the abundance and size of tabular clasts in laterally equivalent sandstones imply intense upstream scouring, most probably related to significant erosion by an energetic plane‐wall jet or within a submerged hydraulic jump. Rapid energy loss coupled with rapid charging of the flow with fine‐grained sediment probably changed the rheology of the flow and promoted deposition along the margins of the jet. Moreover, these distinctive matrix‐rich strata are interpreted to represent the energetic initiation of the local sedimentary system, most probably caused by a local upflow avulsion.     

酒东盆地红山地区下白垩统新民堡群灰白色蚀变带特征及其与铀成矿的关系

研究区位于酒东盆地东北缘红山地区。通过对下白垩统新民堡群后生氧化改造作用的研究,认为灰白色弱氧化、强水解蚀变带是层间氧化带的一部分。铁和有机质是沉积岩中常见的色素,当含氧水进入目的层砂体时,砂体中的有机质、低价铁(Fe2+)等化合物被氧化,导致岩石褪色;同时氧化作用导致砂岩中长石水解,形成以高岭石为主的白色黏土矿物,使岩石增白。增白与褪色的双重作用是砂岩总体上变白的重要原因,其所形成的灰白色蚀变岩位于强氧化的紫红色-黄色蚀变亚带与灰色原生岩石带之间的一定范围内。铀矿化(体)产在弱氧化、强水解灰白色砂岩与原生灰色砂岩界面附近偏灰色岩石一侧[1-2]。灰白色蚀变带与铀成矿关系密切,可作为区域性白垩系砂岩型铀矿的找矿标志之一。     

银河系厚盘恒星元素丰度研究

自20世纪80年代开始的观测表明,银河系存在厚盘结构,但其形成机制至今还是一个没有解决的问题。近年来很多工作发现,厚盘恒星的α元素丰度随金属丰度的变化趋势与薄盘不同, 这种不同还表现在Al、Mn、Zn、中子俘获元素等其他元素上。结合年龄、运动学参数研究, 恒星元素丰度可以对银河系厚盘形成机制提供观测依据。     

银河系厚盘的本地空间密度

本文利用北银极天区的现代恒星计数资料，采用标准的银河系模型，通过恒星统计积分方程对参数值组合模型的亮度函数进行计数分析，证明了银河系厚盘恒星成份存在的必要性，并进一步得出太阳附近厚盘成份的空间密度的最佳期望值为薄盘密度的０．０４１．