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991.
本文通过对湘南经向构造带北段的遥感地质解译,发现了具有环形影象特征的古盆、古盆盆缘及其附近爆花点状影象的古岩溶,并阐述了它们在空间分布上与铀矿化有着较为密切的关系。文章在分析该区经向构造紧密褶断带和新华夏系构造强烈活动的基础上,强调了构造体系的复合。从而展示了古盆、古岩溶空间分布上的构造有利部位。华南多数大、中型铀矿床、在空间分布上显示了与NNE向中、新生代断拗红盆有着某种内在联系,作者就断拗红盆对铀成矿的机理进行了探索。并提出在该区一定的标高和距断拗红盆的一定范围内为理想的找矿区域。 相似文献
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董兆祥 《吉林大学学报(地球科学版)》1987,(1)
针对风化岩体仍无理想的定量分带方法这一研究现状与工程建筑需要的矛盾,提出了对能够检测工程环境岩体风化程度的各种物理力学、矿物学和声学指标进行方差分析和特殊的“动态方差分析”方法,可对岩体风化带的划分进行定量评价,达到某一试验结果下的最佳分带效果。还结合应用实例讨论了不同地质条件下分带计算过程的相应变化和应用效果。最后指出,工程岩体分类亦可借鉴本文的研究方法。 相似文献
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Summary The earthquakes of 19 September 1985 (18.2° N, 102.7° W and a magnitude of 8.1 Richter scale) and of 20 (17.6° N, 101.8° W and a magnitude of 7.5 Richter scale) September 1985, caused the total or partial destruction of more than 2000 structures in Mexico City. The most affected areas are located along the fringes of and bordering old roadways, earthworks (dikes), aquaducts and pre-hispanic population centres. Ancient construction artificially modified the sedimentation in the basin of the Mexico Valley Lakes making the sub-soil of Mexico City more rigid near to the surface, and producing deviations of the surface seismic waves (Rayleigh waves and Love waves). Also, when earthquakes occur on the Pacific coast, seismic waves travel quickly through plutonic, metamorphics and continental and marine rocks of different ages, having high seismic velocities. When the seismic waves enter the poorly consolidated lake sediments having low seismic velocities in the Mexico City Basin, they produce an energy buildup that causes the phenomenon called magnification.There exists a direct relation between the amplification mentioned above and the presence of rigid bodies that are buried in the sub-soil. The length of these bodies is of the order of tens of kilometres horizontally with thicknesses less than 50 metres. These Rigid Barriers produce reflections and refractions of the surface waves along their borders with destructive consequences for the buildings. A correlation between the buildings and the houses damaged and destroyed and the location of the prehispanic construction on the sub-soil has been made which shows that the most damage happened in the borders of old roadways (i.e. Tlalpan road), perimeter walls (i.e. San Lazaro), aqueducts (i.e. Chapultepec Avenue), pyramids (i.e. Templo Mayor) and population centres (i.e. Tlaltelolco). 相似文献
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北京小汤山地区第四系深层地下水氟含量普遍超标, 严重制约区域供水。在收集整理基础地质、水文地质、地热地质资料基础上, 开展第四系高氟地下水与地热水之间关系研究工作。研究表明: 小汤山地区位于复式背斜的核部区域, 该区热储层与第四系地层直接接触并形成水力“天窗”, 受构造应力影响在热储层发育大量张性裂隙, 加之上覆第四系盖层结构松散且厚度较薄, 导致该区成为地热富集带; 在高温高压环境下, 地热水中氟化物含量普遍较高, 地热水上涌同第四系深层地下水发生热流-冷流的混合作用, 导致第四系深层地下水中氟化物含量升高, 形成第四系高氟地下水。 相似文献
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Sean C Solomon Author Vitae 《Earth and Planetary Science Letters》2003,216(4):441-455
The planet Mercury, a difficult object for study by astronomical observation and spacecraft exploration alike, poses multiple challenges to our general understanding of the inner planets. Mercury’s anomalously high uncompressed density implies a metal fraction of 60% or more by mass, an extreme outcome of planetary formational processes common to the inner solar system. Whether that outcome was the result of chemical gradients in the early solar nebula or removal by impact or vaporization of most of the silicate shell from a differentiated protoplanet can potentially be distinguished on the basis of the chemical composition of the present crust. Our understanding of the geological evolution of Mercury and how it fits within the known histories of the other terrestrial planets is restricted by the limited coverage and resolution of imaging by the only spacecraft to have visited the planet. The role of volcanism in Mercury’s geological history remains uncertain, and the dominant tectonic structures are lobate scarps interpreted as recording an extended episode of planetary contraction, issues that require global imaging to be fully examined. That Mercury has retained a global magnetic field when larger terrestrial planets have not stretches the limits of standard hydromagnetic dynamo theory and has led to proposals for a fossil field or for exotic dynamo scenarios. Hypotheses for field generation can be distinguished on the basis of the geometry of Mercury’s internal field, and the existence and size of a fluid outer core on Mercury can be ascertained from measurements of the planet’s spin axis orientation and gravity field and the amplitude of Mercury’s forced librations. The nature of Mercury’s polar deposits, suggested to consist of volatile material cold-trapped on the permanently shadowed floors of high-latitude impact craters, can be tested by remote sensing of the composition of Mercury’s surface and polar atmosphere. The extremely dynamic exosphere, which includes a number of species derived from Mercury’s surface, offers a novel laboratory for exploring the nature of the complex and changing interactions among the solar wind, a small magnetosphere, and a solid planet. Recent ground-based astronomical measurements and several new theoretical developments set the stage for the in-depth exploration of Mercury by two spacecraft missions within the coming decade. 相似文献
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