Effect of Shale Reservoir Characteristics on Shale Oil Movability in the Lower Third Member of the Shahejie Formation,Zhanhua Sag

To reveal the effect of shale reservoir characteristics on the movability of shale oil and its action mechanism in the lower third member of the Shahejie Formation(Es3l), samples with different features were selected and analyzed using N2 adsorption, high-pressure mercury injection capillary pressure(MICP), nuclear magnetic resonance(NMR), high-speed centrifugation, and displacement image techniques. The results show that shale pore structure characteristics control shale oil movability directly. Movable oil saturation has a positive relationship with pore volume for radius > 2 μm, as larger pores often have higher movable oil saturation, indicating that movable oil is present in relatively larger pores. The main reasons for this are as follows. The relatively smaller pores often have oil-wetting properties because of organic matter, which has an unfavorable effect on the flow of oil, while the relatively larger pores are often wetted by water, which is helpful to shale oil movability. The rich surface provided by the relatively smaller pores is beneficial to the adsorption of immovable oil. Meanwhile, the relatively larger pores create significant pore volume for movable oil. Moreover, the larger pores often have good pore connectivity. Pores and fractures are interconnected to form a complex fracture network, which provides a good permeability channel for shale oil flow. The smaller pores are mostly distributed separately;thus, they are not conducive to the flow of shale oil. The mineral composition and fabric macroscopically affect the movability of shale oil. Calcite plays an active role in shale oil movability by increasing the brittleness of shale and is more likely to form micro-cracks under the same stress background. Clay does not utilize shale oil flow because of its large specific surface area and its block effect. The bedding structure increases the large-scale storage space and improves the connectivity of pores at different scales, which is conducive to the movability of shale oil.     

重庆地区夏季一次降水过程及增雨潜力的数值模拟分析

利用国家气象中心GRAPES人工增雨云系模式,选取2008年7月4日重庆地区一次降水过程进行数值模拟,分析了重庆地区降雨天气的水汽分布、云系宏微观分布、云中微物理转化和增雨潜力等特征。结果表明：本次降水大气过程中,重庆地区水汽含量极为丰富,水汽分布与地形分布呈明显的对应关系,低层水汽输送较大,整层水汽通量较高,有明显水汽辐合,云中液态水对地面降水影响很大。西南气流和地形共同作用为重庆地区液态水的形成提供了有利条件,在东北部山区迎风坡处大量水汽累积抬升,易形成丰富的液态水。重庆东北部地区水汽向云水转化较强,过冷液态水含量丰富,冰晶含量少,0℃层附近水汽垂直通量较大,降水效率较低,有较大的增雨潜力。     

蒙古塔木察格盆地塔南凹陷下白垩统层序结构类型、控制因素与层序发育模式

利用录井及地震反射资料,采用层序地层学原理对蒙古塔木察格盆地塔南凹陷下白垩统地层层序进行了划分和对比,划分出了4个三级层序（SQ1-SQ4）。在此基础上,结合盆地的构造演化特点,研究了层序结构特征,划分了层序类型,其中,SQ1和SQ2为初始裂谷期湖泊层序,SQ3为裂谷深陷期层序,SQ4为裂谷后过渡层序。层序的结构主要受构造沉降方式控制,塔南凹陷不同时期构造沉降方式不同,形成了3种层序发育模式,即简单箕状斜坡模式、差异沉降构造反转模式、坳陷型层序发育模式,不同的层序发育模式,其地层岩性圈闭的发育和分布不同。     

Intraplate deformation and 3D rheological structure of the Rhine Rift System and adjacent areas of the northern Alpine foreland

The lithosphere of the Northern Alpine foreland has undergone a polyphase evolution during which interacting stress-induced intraplate deformation and upper mantle thermal perturbations controlled folding of the thermally weakened lithosphere. In this paper we address relationships among deeper lithospheric processes, neotectonics and surface processes in the Northern Alpine foreland with special emphasis on tectonically induced topography. We focus on lithosphere memory and neotectonics, paying special attention to the thermo-mechanical structure of the Rhine Graben System and adjacent areas of the northern Alpine foreland lithosphere. We discuss implications for mechanisms of large-scale intraplate deformation and links with surface processes and topography evolution.     

采用土工合成材料的新型护岸结构的动态数值模拟

固化土和土工格栅护岸工法（SG-WALL工法）是一种采用固化土和土工格栅加固港口护岸结构的新型工法。它的抗震性能已经通过一系列振动台试验得到了确认。为了能够数值再现SG-WALL结构在地震荷载作用下的动力反应,对SG-WALL结构的振动台试验进行了动态数值模拟研究。试验和模拟结果的对比表明,数值模拟方法能够再现SG-WALL结构在振动荷载作用下的主要动力特征。模拟结果还表明：固化土的长度对SG-WALL抗震性能起到重要的影响;土工格栅的最大拉应变发生在与排桩的连接处,并且沿着远离排桩的方向逐渐减小。     

辽南庄河地区栗子房变质核杂岩的发现及意义

在区域地质调查资料基础上,根据宏观与微观构造测量,通过分析区域岩浆活动性及其测年资料等,揭示了在辽南庄河栗子房地区存在另一个变质核杂岩构造,即栗子房变质核杂岩。该核杂岩具有3层结构和5个部分,即由新太古代变质深成岩及中生代花岗岩侵入体构成的下盘、由不同层次的构造岩组成的中部拆离断层带以及由前寒武纪沉积盖层和白垩纪伸展盆地构成的上盘。栗子房变质核杂岩形成于早白垩世,运动方向为上盘相对下盘由NWW向SEE方向运动,与辽南金州变质核杂岩和万福变质核杂岩在几何学、运动学极性和形成时间等方面具有很多相似性,形成于同一动力学背景。该变质核杂岩的厘定可为阐明华北克拉通东部晚中生代岩石圈减薄过程及岩石圈的力学和流变学属性提供依据。同时,变质核杂岩与金矿床成矿关系密切,栗子房变质核杂岩的拆离断层带附近可作为下一步金矿勘查的重点工作区,成矿潜力较大。     

TEM study of a special grain boundary in a synthetic K-feldspar bicrystal: Manebach Twin

 A monoclinic KAlSi₃O₈ feldspar Manebach twin boundary was synthesized by diffusion bonding and examined using high-resolution transmission electron microscopy. The sharp (001) twin boundary is straight and free of strain. The boundary width is smaller than d₀₀₁. There is no rigid body shift observed at the twin boundary, and the feldspar structure is arranged symmetrically across (001). The twin boundary structure consists of bridged tetrahedral crankshafts, which are characteristic of the feldspar lattice. The grain boundary structure is in good agreement with the geometrical model of Taylor et al. (1934). The grain boundary composition of K_1/2H_1/2AlSi₃O₈ differs from their model. Received: 13 February 2002 / Accepted: 24 December 2002 Acknowledgements We thank M. Rühle, S. Hutt, J. Mayer, A. Strecker and U. Salzberger at MPI, Stuttgart, for their support and valuable advice in preparing TEM sections of bicrystals.     

Characteristics of Radar Echo Parameters and Microphysical Structure Simulation of a Short-Time Heavy Precipitation Supercell

By using the conventional observations, radar data, NCEP/NCAR FNL 1°×1° reanalysis data and numerical simulation data and with the construction and calculation of radar echo parameters, this paper presents the structural characteristics and physical processes of a short-time heavy precipitation supercell that occurred in the squall line process in Shanxi Province on 24 June 2020. The results show that this squall line event occurred in front of a surface cold front,combined with infiltration of ...     

Dynamical response to supernova-induced gas removal in spiral galaxies with dark matter halo

We investigate the dynamical response, in terms of disc size and rotation velocity, to mass loss by supernovae in the evolution of spiral galaxies. A thin baryonic disc having the Kuzmin density profile embedded in a spherical dark matter halo having a density profile proposed by Navarro, Frenk & White is considered. For the purpose of comparison, we also consider the homogeneous and   r ⁻¹  profiles for dark matter in a truncated spherical halo. Assuming for simplicity that the dark matter distribution is not affected by mass-loss from discs and the change of baryonic disc matter distribution is homologous, we evaluate the effects of dynamical response in the resulting discs. We found that the dynamical response only for an adiabatic approximation of mass-loss can simultaneously account for the rotation velocity and disc size as observed particularly in dwarf spiral galaxies, thus reproducing the Tully–Fisher relation and the size versus magnitude relation over the full range of magnitude. Furthermore, we found that the mean specific angular momentum in discs after the mass-loss becomes larger than that before the mass-loss, suggesting that the mass-loss would most likely occur from the central disc region where the specific angular momentum is low.