Evolution of Polytropic Reimann Disks in Halos     

M. G. Abrahamyan 《Astrophysics》2004,47(4):555-567

The equilibrium of elliptical Riemann disks with a polytropic equation of state and their evolution under the influence of viscosity and gravitational radiation inside spheroidal halos with a relative surface mass density k. The evolutionary trajectory of a disk inside a halo with k<0.5, which is analogous to the evolution of an isolated disk, differs from that of a disk inside a denser halo.  相似文献   

广西岩溶区金属硫化物矿床风化与元素表生迁移特征     

农毅平 《南方国土资源》1996,(3)

对广西岩溶区三个铅锌硫化物矿床风化带观测结果表明，中低山岩溶区硫化物矿床具有更强烈的风化淋滤作用，但次生晕面积较小；岩溶平原区硫化物矿床风化与元素表生迁移特征较相似于非岩溶区的情况，表现在可产生较宽的ｐＨ偏低带和较大面积的次生晕  相似文献   

On the origin of high-eccentricity halo stars     

C.B. Brook  D. Kawata  B.K. Gibson  C. Flynn 《Astrophysics and Space Science》2003,284(2):845-848

The present-day chemical and dynamical properties of the Milky Way are signatures of the Galaxy's formation and evolution. Using a self consistent chemodynamical evolution code we examine these properties within the currently favoured paradigm for galaxy formation – hierarchical clustering within a CDM cosmology. Our Tree N-body/Smoothed Particle Hydrodynamics code includes a self-consistent treatment of gravity, hydrodynamics, radiative cooling, star formation, supernova feedback and chemical enrichment. Two models are described which explore the role of small-scale density perturbations in driving the evolution of structure within the Milky Way. The relationship between metallicity and kinematics of halo stars are quantified and the implications for galaxy formation discussed. While high-eccentricity halo stars have previously been considered a signature of `rapid collapse', we suggest that many such stars may have come from recently accreted satellites. This revised version was published online in August 2006 with corrections to the Cover Date.  相似文献   

Catch per unit effort, foraging efficiency, and parental investment in breeding great cormorants (Phalacrocorax carbo carbo)     

Gremillet  David 《ICES Journal of Marine Science》1997,54(4):635-644

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苏北盐城凹陷复合含油气系统   总被引：1，自引：0，他引：1  

宋宁  朱霞  林春明  赵彦彦 《海洋地质前沿》2003,19(12):18-22

苏北盐城凹陷含油气系统可划分为上、下2个复合含油气系统。上复合含油气系统，即Pz、K2p、K2t(生)-K2t、E1f1(储)一E1f1 E1f2(盖)，古生界、中生界浦口组和泰州组为烃源岩层，泰州组和阜宁组一段为储集层，阜宁组一段顶部至二段暗色泥岩为区域盖层，油气沿深大断裂运移，油气成藏关键时刻在古近纪晚期至新近纪早期，有利勘探区在深大断裂附近的中、新生界发育地区；下复合含油气系统，即Pz、K2p(生)-Pz、K2p(储)-K2p3 K2p4(盖)，油气通过断层或不整合运移，油气大量生成的关键时刻为古近纪早期，该系统中气藏分布在古生界被中生界覆盖地区。  相似文献   

徽县头滩子地区土壤金异常晕与金矿化特征          下载免费PDF全文

董佑仁  辛存林 《甘肃地质》2008,(2):56-60

通过区域地质的研究,分析了头滩子地区的土壤金异常晕,该区土壤晕分布与构造展布方向一致,金异常晕对地层的选择性不明显。指出了构造、热液、地层岩性三位一体控制着金的矿化与成矿。特别是断裂构造是金矿化的必要条件。  相似文献   

浙北双溪坞群的构造特征及地质意义   总被引：1，自引：0，他引：1  

竺国强  陈梓军 《高校地质学报》1996,2(1):58-64

本文在野外地质工作基础上,通过对双溪坞群的岩层对比和构造分析,认为本区的双溪坞群与上覆地层间在构造样式上的存在着较大差异。双溪坞群的章村组和北组具有相似的地质特征,为同一火山放心回的产物。神功运动使早期形成的双溪坞群褶皱造山,开怀 竖线型平臣褶皱构造,并受后期构造的叠加改造,形成轴向北东的叠加褶皱构造格局。  相似文献   

主砂体及其构造改造样式的盆地产铀远景评价判据     

陈祖伊  郭庆银  刘红旭 《铀矿地质》2005,21(3):152-160

本文在介绍并分析美国和前苏联总结的砂岩型铀矿区域评价判据的基础上, 引入当今碎屑岩沉积学和盆地地球动力学方面的若干新进展, 提出以主砂体及其随后经历的构造改造样式相结合的盆地产铀远景评价判据和以分析区域构造活动史和原型盆地演化相结合的盆地产铀远景评价模式。最后以潮水盆地为例, 具体分析了盆地各个时代盖层容存后生铀矿化的可能性, 指出盆地中的主要找矿目标层位和远景成矿地段。  相似文献   

Sulfur Content and Isotopic Ratio of Cambro-Ordovician Carbonate Rocks from South Korea: A Possible Source for Mesozoic Magmatic-hydrothermal Ore Sulfur     

Shunso ISHIHARA  Myung–Shik JIN  Yoshimichi KAJIWARA 《Resource Geology》2002,52(1):41-48

Abstract: Carbonate rocks of Cambrian (18 samples) and lower-middle Ordovician (11 samples) ages from South Korea were analyzed for sulfur contents of structurally substituted sulfate (SSS) and sulfides and their δ³⁴S values. The δ³⁴S values of SSS ranging from +25.9 to +45.2 permil, are averaged as +33.6 and +33.5 permil for the Cambrian and Ordovician rocks, respectively, which indicate high δ³⁴S values of the Cambro-Ordovician seawater. The SSS contents in the carbonate rocks are low being 2.9 to 17.3 ppm S (averaged as 7.0 ppm S). Sulfide sulfur, on the contrary, is much abundant containing 3 to 1,880 ppm S and the δ³⁴S values range widely between –17.6 and +31.1 permil. Sulfide sulfur of the studied rocks excluding impure carbonates has an average content of 187 ppm S and δ³⁴S value of +12.8 permil (n=24). The estimated δ³⁴S (sulfate–sulfide) values, which range from 13.8 to 25.4 permil in general with a few exceptions from 36.5 up to 52.3 permil for some impure carbonates, may provide evidence for the persistent oceanic anoxia with its temporary recovery during the Cambro-Ordovician time.
The SSS and sulfide sulfurs have often higher δ³⁴S values than the Mesozoic-Cenozoic ore sulfur (Ishihara et al., 2000). Since carbonate rocks are very reactive with circulating hydrothermal ore solution, high δ³⁴S values of the Korean ore deposits might be caused to some extent by ³⁴S enrichment from the host carbonates, resulting in the low SSS contents observed.  相似文献   

锡铁山铅锌矿地质特征、矿床成因及找矿标志   总被引：4，自引：1，他引：4  

李如满  汪树栋 《矿产与地质》2003,17(3):218-221

通过找矿工作的实践，认为锡铁山铅锌矿床是由火山喷流沉积—后期热液叠加改造富集的块状硫化物多金属矿床。区域上NW—SE向早古生代形成的裂谷带，三级盆地内沉积的晚奥陶世滩间山群的大理岩与绿片岩系是表区找矿的最佳区段。而绢云绿泥斜长片岩、含碳质绢云绿泥片岩、白色大理岩、条带状大理岩是铅锌矿的最重要的找矿标志。  相似文献