江西利山金矿床地质特征及控矿构造

本文较系统地阐述了利山金矿床的各项地质特征，并重点就控矿构造问题进行了总结讨论，认为ＮＷＷ向断裂带严格控制了所有金矿体的产出。ＮＮＥ、ＮＮＷ向断裂与ＮＷＷ向断裂带的交汇部位控制了富矿段的产出。在此基础上初步探讨了矿床成因及找矿方向，这对该地区的找矿评价和开发均具有实际意义     

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.     

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。     

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.     

大庆宋芳屯油田肇35区块葡萄花油层非均质性研究

从储层宏观与微观非均质性入手,分别研究了肇35区块葡萄花油层的层内、层间、平面和微观非均质性特征及主控因素,研究区层内非均质性主要受到沉积构造、渗透率韵律以及夹层分布等的影响;从物性和隔层分布特征方面分析了层间非均质性特征,自下而上葡萄花油层非均质性呈现弱→强→弱的变化趋势;平面非均质性特征受砂体及沉积微相展布影响较大,沿河道延伸方向非均质性较好。研究区主要发育正常粒间孔、缩小粒间孔和粒内溶蚀孔,整体上储层微观孔隙结构发育良好。从不同方面分析了研究区非均质性对剩余油分布的影响,沉积微相类型和成岩作用是控制储层非均质性的主因素。最终对葡萄花油层主力小层进行储层评价,预测了有利储层的发育面积和分布范围,为下一步的勘探开发提供一定的依据。     

格型钢板桩结构有限元数值分析

以有限元软件ABAQUS作为分析平台,建立波浪荷载作用下格型钢板桩结构稳定性及应力分析的三维弹塑性有限元分析模型。格型钢板桩采用壳体单元模拟,在相邻板桩之间设置铰接连接器模拟板桩之间的相对转动;土体采用Mohr-Coulomb本构模型模拟,在格型钢板桩与其内、外土体之间设置接触面单元模拟它们之间的滑移、张裂和闭合。结合某实际工程,研究结构的破坏模式、失稳特性和应力分布特性,分析参数变化对结构稳定性和环向拉力的影响,并对格内土体的剪切变形进行分析,建议格型钢板桩锁口拉力的验算断面。结果表明,铰接连接器的设置对于结构稳定性影响不大,但对环向拉力有一定影响;格内土体的剪切变形主要发生在格体中轴处,符合太沙基法结论。     

黔东地区变质核杂岩构造及其控矿作用

黔东地区的变质核杂岩构造其变质核杂岩为中元古界四堡群、梵净山群变质基底,其主滑脱面发育于新元古界底部的甲路组,同时在下江群、板溪群中出现一系列次级滑脱面,在其上的早古生代地层中则发育伸展剥离正断层系统。该类型构造形成于加里东期末,是该区加里东造山期后隆升背景的产物。变质核杂岩构造与该地区的金、铜、铅、锌、锑及汞等矿产关系十分密切,它们分别受控于主滑脱带、次级滑脱带及伸展剥离正断层系统,且在剖面上矿物组合、成矿温度出现有规律变化,反映出该地区金及多金属矿产是受控于变质核杂岩构造的一个完整的、相互有机联系的成矿系统。     

The 2dF Galaxy Redshift Survey: luminosity dependence of galaxy clustering

We investigate the dependence of the strength of galaxy clustering on intrinsic luminosity using the Anglo-Australian two degree field galaxy redshift survey (2dFGRS). The 2dFGRS is over an order of magnitude larger than previous redshift surveys used to address this issue. We measure the projected two-point correlation function of galaxies in a series of volume-limited samples. The projected correlation function is free from any distortion of the clustering pattern induced by peculiar motions and is well described by a power law in pair separation over the range     . The clustering of     galaxies in real space is well-fitted by a correlation length     and power-law slope     . The clustering amplitude increases slowly with absolute magnitude for galaxies fainter than M *, but rises more strongly at higher luminosities. At low luminosities, our results agree with measurements from the Southern Sky Redshift Survey 2 by Benoist et al. However, we find a weaker dependence of clustering strength on luminosity at the highest luminosities. The correlation function amplitude increases by a factor of 4.0 between     and −22.5, and the most luminous galaxies are 3.0 times more strongly clustered than L * galaxies. The power-law slope of the correlation function shows remarkably little variation for samples spanning a factor of 20 in luminosity. Our measurements are in very good agreement with the predictions of the hierarchical galaxy formation models of Benson et al.