西湖凹陷西次凹古近系花港组—平湖组深层油气成藏过程

西湖凹陷西次凹古近系花港组和平湖组深层油气资源丰富，是东海陆架盆地勘探开发新领域，受储层差异致密化影响，油气成藏机理复杂。为了厘清西次凹深层油气成藏过程，本文通过流体包裹体岩相学特征、显微测温、激光拉曼光谱、包裹体所含油气地球化学等实验分析，结合构造演化、地层埋藏史、热史等，开展了系统的储层特征、油气成藏期次、成藏过程研究。结果表明，花港组深层（>4000 m）和平湖组储层均已致密化，溶蚀孔隙是主要的储集孔隙类型；花港组和平湖组均发育两期油气包裹体，早期含油包裹体较多，晚期以天然气包裹体为主，成藏时间分别为龙井运动期和冲绳运动期，以晚期天然气成藏最为关键。包裹体中油气地球化学特征类似，反映生烃母质以高等植物生源为主，低等生物为辅，与平湖组煤系烃源岩特征一致。冲绳运动叠加平湖组生气增压是晚期天然气成藏的主要动力，此时H10段及以上储层未致密化。根据储层致密化与成藏时序匹配关系可将西次凹M构造深层油气藏类型划分为常规型、先成藏后致密型、先致密后成藏型和边成藏边致密型4种。本文成果可为研究区下一步致密砂岩气的勘探开发部署提供重要的理论依据。     

商河县馆陶组热储地热尾水回灌可行性研究

从回灌热储层条件、动力场特征、水化学及库容条件等方面,研究了商河县地热回灌地质条件。结合区内地热资源开发利用现状与回灌工程技术条件,对商河县地热尾水回灌的可行性进行了研究,认为在现有条件下,可逐步推行地热尾水回灌。     

西峰油田三叠系延长组长2_2砂层组沉积相分析

通过对西峰油田三叠系延长组长22砂层组的泥岩颜色、岩石类型、沉积构造、生物化石、沉积层序以及单井相等的研究,认为延长组长22油层主要沉积相为正常三角洲沉积。三角洲平原是该区三角洲砂体堆积的主体。可进一步辨别出分流河道、天然堤、分流间湾及决口扇4个微相。     

川西上三叠统须家河组超致密砂岩储层评价

川西须家河组超致密砂岩中发育多种储层类型,天然气产出能力各异。针对须家河组超致密砂岩整体孔渗关系差,以孔隙度为基础、单定量孔渗关系模型评价精度低的特点,以微观孔隙结构与储集物性关系深入分析为基础,建立了以渗透率为基础,利用与多种储集类型相配置的孔渗多定量关系模型,分别确定了不同储集类型的不同下限,提高了超致密砂岩储层的评价水平。     

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。     

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.