贺兰山群早元古代花岗岩的地质特征和岩石谱系单位划分

通过对呼鲁斯太幅和古拉本幅的１／５万区域地质调查工作，对该地区太古代贺兰山群中－高级变质岩中早元古代花岗岩进行了岩石谱系单位的划分和填图。在此基础上，从花岗岩的地质学、岩石学、岩石化学和地球化学等方面进行了较系统的详细研究，把早元古代花岗岩划分出７个单元，并将其中的５个单元归并为两个超单元。     

激发极化法在早前寒武纪变质岩系找水中的应用

通过对在早前寒武纪变质岩系进行抗旱找水中利用地球物理勘探定井的实例分析,阐述了利用激发极化法在早前寒武纪变质岩分布区辨认含水层,确定含水层埋深,最终确定较好井位的方法。该方法对解决早前寒武纪变质岩系的干旱缺水现状有广泛深远的意义。     

关于2×2块矩阵在除环上群逆的注记

针对分块矩阵在除环上群逆的表示,在证明中使用的引理并不能根据所给条件判定得到分块矩阵群逆的存在性,采用举反例的方法说明存在的问题,进而通过在原有题设中添加了一个条件,证明了分块矩阵的群逆存在,从而更正了定理内容。利用一个新引理和分块矩阵的子矩阵的秩之间的关系证明得到2×2块矩阵在除环上群逆表示的一个新的结果.     

山东省昌乐县新生代火山口新发现及旅游地质意义

昌乐蓝宝石闻名遐尔，但蕴藏蓝宝石的火山岩及火山群却少有人知。昌乐县境内几十个由新近纪临胸群牛山组尧山组玄武岩构成的山包，大都是古火山口(颈)。近期，在北岩镇南开出的古火山口(颈)，其玄武岩柱状节理的扇状展布和罕见的两次熔岩喷发交切遗迹，比以往已开发的乔官镇团山子古火山口更为奇特和壮观。火山地貌景观区历来是人们向往的旅游胜地，对昌乐古火山群旅游资源，应加大开发和保护力度，使其尽快成为人们观赏地质奇观、增长科学知识的基地。发展地质旅游将促进当地经济的腾飞。     

山地城市公交系统服务在老年人群体中分配公平性评价

公交系统作为一种面向公众全体尤其是弱势群体的公共服务设施,其公平性对于促进宜居城市与公交都市建设具有较大的现实意义.本研究考虑山地城市地形变化的影响,提出了一类测度公交站点实际服务范围的新方法来修正公交服务供给公平性评价模型,并以贵阳市为例,对贵阳市公交系统服务供给在老年群体中分配的公平性进行分析.研究结果表明:①山地...     

丹凤地区刘岭群倒转变质带及其地质意义

根据变质矿物组合和变质带的特征,结合变形构造研究,认为丹凤地区的刘岭群曾遭受过中压相系的变质作用,随后又被褶皱及剪切推覆作用改造,使变质带倒转、变薄。文章认为,本区刘岭群在时代上不能与西部邻区的中泥盆统地层对比。     

Importance of footing–soil separation on dynamic stiffness of piled embedded footings

Different phenomena such as soil consolidation, erosion, and scour beneath an embedded footing supported on piles may lead to loss of contact between soil and the pile cap underside. The importance of this separation on the dynamic stiffness and damping of the foundation is assessed in this work. To this end, a numerical parametric analysis in the frequency domain is performed using a rigorous three‐dimensional elastodynamic boundary element–finite element coupling scheme. Dimensionless plots relating dynamic stiffness functions computed with and without separation effects are presented for different pile–soil configurations. Vertical, horizontal and rocking modes of oscillation are analyzed for a wide range of dimensionless frequencies. It is shown that the importance of separation is negligible for frequencies below those for which dynamic pile group effects start to become apparent. Redistribution of stiffness contributions between piles and footing is also addressed. Copyright © 2009 John Wiley & Sons, Ltd.     

The mass of the Andromeda galaxy

This paper argues that the Milky Way galaxy is probably the largest member of the Local Group. The evidence comes from estimates of the total mass of the Andromeda galaxy (M31) derived from the three-dimensional positions and radial velocities of its satellite galaxies, as well as the projected positions and radial velocities of its distant globular clusters and planetary nebulae. The available data set comprises 10 satellite galaxies, 17 distant globular clusters and nine halo planetary nebulae with radial velocities. We find that the halo of Andromeda has a mass of together with a scalelength of 90 kpc and a predominantly isotropic velocity distribution. For comparison, our earlier estimate for the Milky Way halo is Although the error bars are admittedly large, this suggests that the total mass of M31 is probably less than that of the Milky Way . We verify the robustness of our results to changes in the modelling assumptions and to errors caused by the small size and incompleteness of the data set.
Our surprising claim can be checked in several ways in the near future. The numbers of satellite galaxies, planetary nebulae and globular clusters with radial velocities can be increased by ground-based spectroscopy, while the proper motions of the companion galaxies and the unresolved cores of the globular clusters can be measured using the astrometric satellites Space Interferometry Mission ( SIM ) and Global Astrometric Interferometer for Astrophysics ( GAIA ). Using 100 globular clusters at projected radii 20 R 50 kpc with both radial velocities and proper motions, it will be possible to estimate the mass within 50 kpc to an accuracy of 20 per cent. Measuring the proper motions of the companion galaxies with SIM and GAIA will reduce the uncertainty in the total mass caused by the small size of the data set to 22 per cent.     

圈闭地形内斜坡破坏的多期性和规律性

本文以黄河上游某拟建水电站坝址场地为例,论证了圈闭地形内斜坡破坏的多期性和规律性问题。在充分的野外调查和室内研究资料的基础上,将区内的斜坡破坏分为两期,即第一期为已经失稳的老滑坡群;第二期为发育在第一期滑坡群圈闭状破裂壁之后的正处于蠕动和破坏阶段的变形坡体,进而将第一期的滑坡分为两个强度次序。同时,还揭示了圈闭地形内斜坡破坏的规律性,即随着期和序次的增高,斜坡破坏面积增大,滑坡个数增多,规模减小,强度降低,滑距变短,滑体破碎程度变弱。最后指出,上述多期性和规律性应具有普遍性意义。     

OGC WCS系统若干关键实现技术研究

由于栅格数据种类繁多,处理过程复杂,目前还没有一种软件能为他们提供完善的WCS。研究表明,针对具体的数据源设计和实现WCS是比较好的解决方案。研究针对MODIS数据,参照OGC WCS实现规范,在充分分析WCS数据处理与服务流程的基础上,总结了WCS系统实现的技术要点,研究和探讨了系统实现中的若干关键技术问题,包括元数...