南秦岭主要类型热水沉积岩的REE地球化学   总被引：1，自引：0，他引：1  

薛春纪  马国良  隗合明  曾章仁 《地球科学与环境学报》1996,(3)

南秦岭泥盆纪沉积柱中产有多种类型海底热水沉积岩．它们的ΣＲＥＥ偏低（平均６３．０９×１０－６），ＲＥＥ配分曲线平缓右倾，Ｌａ／Ｙｂ＝２～８，Ｃｅ亏损，总体上与海水相似。产于Ｓｅｄｅｘ含矿层中的热水沉积岩具有正Ｅｕ异常，与现代海底热液及红海热液沉积物可比；而产在Ｓｅｄｅｘ含矿层以下地层中的热水沉积岩Ｅｕ亏损，与ＥＰＲ热液沉积物相似。ＲＥＥ地球化学研究和岩石学研究结果一致，支持热水沉积岩ＲＥＥ来源于海水及部分下伏沉积柱（包括基底），含矿热水沉积岩是盆地热演化到一定阶段具有一定深度和规模的循环对流体系在海底的化学沉积，而Ｓｅｄｅｘ含矿层以下地层中的热水沉积岩则是浅部热水对流循环的海底显示．成岩和变质作用对岩石的ＲＥＥ未造成影响。  相似文献   

Diagenetic Sequences Analysis of Fuyu Reservoir in Qijia - Gulong Depression, Northern Songliao Basin     

YAN Jianping  LIU Li  Zhang Xinrong  Ma Yanping 《世界地质(英文版)》2002,5(1)

Five paragenetic associations are recognized in Fuyu reservoir of Qijia - gulong depression of Daqing oil field: 1 )detrital illite permeation, glauconite and pyrite precipitation; 2 ) feldspar dissolution, kaolinite precipitation and the incipient quartz overgrowths; 3 ) early calcite cements; 4 ) postdate quartz overgrowths and pore - filling quartz, authigenetic illite and chlorite formation, feldspar overgrowths, petroleum injections, K - feldspar and calcite cement dissolution; 5) pore - filling calcite and calcite replacement.  相似文献   

论丽水运动     

马武平 《浙江国土资源》1997,(1)

本文以翔实的地质资料，就丽水以南吴弄口盆地的永康群与丽水南明山一带丽水盆地的天台群之间呈角度不整合接触关系，及其地层层序作了全面论述，认为它们之间存在一次重要意义的地壳运动──丽水运动。  相似文献   

矿业开发与生态环境一体化     

张军营  孔小卫  徐莉  岳喜平 《河南国土资源》2001,(3)

概述了矿业开发与生态环境的关系 ,矿业开发与生态环境一体化的原则和组织 ,国内外现状和发展趋势 ,对河南省矿业生态环境存在问题及其原因进行了综合分析 ,论述了矿业开发与生态环境一体化的准则与前景 ,提出今后工作建议。  相似文献   

星系形成的半解析模型研究进展     

康熙 《天文学进展》2005,23(2):135-143

基于目前流行的冷暗物质等级成团理论的星系形成的半解析模型取得了很大进展．在引入一系列合理的关于重子物质物理过程的假设，如气体冷却、恒星形成率、超新星能量反馈以后，结合N体数值模拟，星系形成的半解析模型一方面能较成功地预言许多与观测符合的近邻星系的性质，如光度函数、星系的两点相关函数、Thlly-Fisher关系、星系团中椭圆星系的颜色一星等关系等；另一方面还能较成功地预言宇宙的恒星形成历史，以及一部分高红移星系的性质，如Lyman-Break星系的数目随红移的分布．但是最近一些观测表明，半解析模型在高红移预言的大质量星系较少，且红星系数目也较观测少．重点讨论半解析模型成功与不足之处，并指出解决这些问题可能的途径。  相似文献   

Estimates of AGN Black Hole Mass and Minimum Variability Timescale   总被引：4，自引：0，他引：4  

Guang-Zhong Xie  Luo-En Chen Huai-Zhen Li  Li-Sheng Mao  Hong Dai  Zhao-Hua Xie  Li Ma  Shu-Bai Zhou National Astronomical Observatories  Yunnan Observatory  Chinese Academy of Science  Kunming  Yunnan Astrophysics Center  Yunnan University  Kunming Physics Department  Yunnan Normal University  Kunming Physics Department  Yuxi Normal College  Yuxi Graduate University of Chinese Academy of Sciences  Beijing 《中国天文和天体物理学报》2005,5(5):463-470

Black hole mass is one of the fundamental physical parameters of active galactic nuclei (AGNs), for which many methods of estimation have been proposed. One set of methods assumes that the broad-line region (BLR) is gravitationally bound by the central black hole potential, so the black hole mass can be estimated from the orbital radius and the Doppler velocity. Another set of methods assumes the observed variability timescale is determined by the orbital timescale near the innermost stable orbit around the Schwarzschild black hole or the Kerr black hole, or by the characteristic timescale of the accretion disk. We collect a sample of 21 AGNs, for which the minimum variability timescales have been obtained and their black hole masses (Mσ) have been well estimated from the stellar velocity dispersion or the BLR size-luminosity relation. Using the minimum variability timescales we estimated the black hole masses for 21 objects by the three different methods, the results are denoted by Ms, Mk and Md, respectively. We compared each of them with Mσindividually and found that: (1) using the minimum variability timescale with the Kerr black hole theory leads to small differences between Mσand Mk, none exceeding one order of magnitude, and the mean difference between them is about 0.53 dex; (2) using the minimum variability timescale with the Schwarzschild black hole theory leads to somewhat larger difference between Mσand Ms: larger than one order of magnitude for 6 of the 21 sources, and the mean difference is 0.74 dex; (3) using the minimum variability timescale with the accretion disk theory leads to much larger differences between Mσand Md, for 13 of the 21 sources the differences are larger than two orders of magnitude; and the mean difference is as high as about 2.01 dex.  相似文献   

微波爆发区的日冕磁场研究     

周爱华  傅其骏 《天文学进展》1996,14(4):297-301

回顾了日冕磁的研究历史，介绍了我们首镒提出的日冕磁场的微波诊断方法及其应用的带来的启迪，提出进一步开展日冕磁场及其相关研究的建议。  相似文献   

A model of rotating hotspots for the 3 : 2 frequency ratio of high-frequency quasi-periodic oscillations in black hole X-ray binaries     

Ding-Xiong Wang  Yong-Chun Ye  Guo-Zheng Yao  Ren-Yi Ma 《Monthly notices of the Royal Astronomical Society》2005,359(1):36-42

  相似文献   

Parallels plane projection and its geometric features     

Zhou  ChengHu  Ma  Ting  Yang  Liao  Qin  Biao 《中国科学:地球科学(英文版)》2007,50(1):176-180

A new equivalent map projection called the parallels plane projection is proposed in this paper. The transverse axis of the parallels plane projection is the expansion of the equator and its vertical axis equals half the length of the central meridian. On the parallels plane projection, meridians are projected as sine curves and parallels are a series of straight, parallel lines. No distortion of length occurs along the central meridian or on any parallels of this projection. Angular distortion and the proportion of length along meridians (except the central meridian) introduced by the projection transformation increase with increasing longitude and latitude. A potential application of the parallels plane projection is that it can provide an efficient projection transformation for global discrete grid systems.

  相似文献   

天鹅座X-1硬X射线的能量谱     

马宇蒨  李光华  张承模  钱跃民  肖谦益  陆柱国  吴枚  戴长江  李惕碚  顾逸东  张希元 《中国天文和天体物理学报》1989,(4)

1985年9月22日,我们用空间硬X射线望远镜HAPI-2,在我国的高空气球上,对天鹅座X-1进行了观测,望远镜几何面积为140cm~2,观测能区20—200keV,空间定向精度±0.2°。获得的硬X射线能谱陡,总辐射能流LX～1.0×1~(37)erg/sec,低于常规态。本文将介绍望远镜的性能和观测过程,能谱分析的结果,并对当时天鹅座X-1可能的“态”进行讨论。  相似文献