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891.
扬子陆核与陆缘新元古代岩浆事件对比及其构造意义——来自黄陵和汉南侵入杂岩ELA-ICPMS锆石U-Pb同位素年代学的约束 总被引:28,自引:12,他引:16
本文报道分别位于扬子克拉通核部和北缘的黄陵及汉南新元古代侵入杂岩体的惰性气体激光剥蚀-等离子体质谱(ELA-ICPMS)锆石U-Pb年代学研究及其构造意义分析.定年数据显示,黄陵地区的三斗坪、大老岭岩套分别形成于794±7和795±8Ma;晓峰浅成岩岩套形成于744±22Ma,不仅与震旦系莲沱组底部火山岩年龄相同,且同期热事件普遍记录于杂岩体内其它岩套.汉南杂岩体中五堵门岩体形成于789±10Ma,在分析误差范围内与三斗坪、大老岭岩套相同;天平河岩形成于863±10Ma,这是在扬子北缘首次识别出这期岩浆作用.在扬子陆核和北缘侵入杂岩中还分别发现了≈860Ma和945~931Ma的捕获锆石.此外,740Ma的后期热事件同样记录于汉南杂岩体,表明扬子陆块内部和北缘共同经历了790Ma的峰期中酸性岩浆作用和≈740Ma的后期强烈热改造事件,即事件具有克拉通范围的性质.与天平河岩体岩性相似、年龄相同的侵入岩体已在攀西多处地区发现,说明空间上860Ma岩浆作用在扬子北缘和西缘可能具延续性.作者认为,"晋宁期"具造山性质的构造运动开始的时间应以830Ma为限,于≈790Ma达到了以壳内物质重熔为主的大规模岩浆侵入事件的峰期,并在≈740Ma以短期内地壳运动由剧烈抬升向快速沉降的构造转换为造山作用结束的标志.本次研究成果为探讨扬子克拉通新元古代大规模岩浆作用与同期全球构造事件的相互关系提供了重要的同位素年代学约束. 相似文献
892.
S, C, O, H Isotope Data and Noble Gas Studies of the Maoniuping LREE Deposit, Sichuan Province, China: A Mantle Connection for Mineralization 总被引:3,自引:2,他引:1
TIAN Shihong DING Tiping MAO Jingwen LI Yanhe YUAN Zhongxin Institute of Mineral Resources Chinese Academy of Geological Sciences Beijing Key Laboratory of Isotope Geology Ministry of Land Resources Beijing China University of Geosci 《《地质学报》英文版》2006,80(4):540-549
The Maoniuping REE deposit, located about 22 km to the southwest of Mianning, Sichuan Province, is the second largest light REE deposit in China, subsequent to the Bayan Obo Fe-Nb-REE deposit in the Inner Mongolia Autonomous Region. Tectonically, it is located in the transitional zone between the Panxi rift and the Longmenshan-Jinpingshan orogenic zone. It is a carbonatite vein-type deposit hosted in alkaline complex rocks. The bastnaesite-barite, bastnaesite-calcite, and bastnaesite-microcline lodes are the main three types of REE ore lodes. Among these, the first lode is distributed most extensively and its REE mineralization is the strongest. Theδ34Sv-CDT values of the barites in the ore of the deposit vary in a narrow range of +5.0 to +5.1‰in the bastnaesite-calcite lode and +3.3 to +5.9‰in the bastnaesite-barite lode, showing the isotopic characteristics of magma-derived sulfur. Theδ13Cv-PDB values and theδ518OV-SMOW values in the bastnaesite-calcite lode range from -3.9 to -6.9‰and from +7.3 to +9.7‰, respectively, which fall into the range of "primary carbonatites", showing that carbon and oxygen in the ores of the Maoniuping deposit were derived mainly from a deep source. Theδ13Cv-PDB values of fluid inclusions vary from -3.0 to -5.6‰, with -3.0 to -4.0‰in the bastnaesite-calcite lode and -3.0 to -5.6‰in the bastnaesite-barite lode, which show characteristics of mantle-derived carbon. TheδDv-SMOW values of fluid inclusions range from -57 to -88‰, with -63 to -86‰in the bastnaesite-calcite lode and -57 to -88‰in the bastnaesite-barite lode, which show characteristics of mantle-derived hydrogen. Theδ18OH2OV-SMOW values vary from +7.4 to +8.6‰in the bastnaesite calcite lode, and +6.7 to +7.8‰in the bastnaesite-barite lode, almost overlapping the range of +5.5 to +9.5‰for magmatic water. The 4He content, R/Ra ratios are (13.95 to 119.58×10-6 (cm3/g)STP and 0.02 to 0.11, respectively, and 40Ar/36Ar is 313±1 to 437±2. Considering the 4He increase caused by high contents of radioactive elements, a mantle-derived fluid probably exists in the inclusions in the fluorite, calcite and bastnaesite samples. The Maoniuping deposit and its associated carbonatite-alkaline complex were formed in 40.3 to 12.2 Ma according to K-Ar and U-Pb data. All these data suggest that large quantities of mantle fluids were involved in the metallogenic process of the Maoniuping REE deposit through a fault system. 相似文献
893.
Single-Doppler Radar Observations of a High Precipitation Supercell Accompanying the 12 April 2003 Severe Squall Line in Fujian Province
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In this study,single Doppler radar data were used to examine the structure and evolution of a high precipitation(HP) supercell embedded in a cold front near Jianyang,Fujian Province on 12 April 2003.The synoptic environment was characterized by high humidity at low levels,moderate CAPE(convective available potential energy;1601 J kg~(-1)),moderate wind shear(22 m s~(-1) in 0-5 km),and veering of the horizontal winds with height,similar to those HP supercells previously observed in midlatitudes.In additio... 相似文献
894.
采用等温溶解平衡法研究了288K时Li+,Mg2+//SO42-,B4O72--H2O四元体系的固液相平衡关系,测定了该四元体系在288K时平衡液相的溶解度和密度。依据实验测定的平衡溶解度数据及对应的平衡固相,绘制了该四元体系的平衡相图及密度组成图。研究结果表明:交互四元体系Li+,Mg2+//SO42-,B4O27--H2O288K时平衡相图中有2个共饱点,5条单变量曲线,4个结晶区对应的平衡固相分别为Li2B4O7.3H2O,Li2SO4.H2O,MgB4O7.9H2O和MgSO4.7H2O。 相似文献
895.
针对四川盆地下三叠统飞仙关组层序地层存在多种不同划分方案,以高精度层序地层学理论与方法为指导,以蜀南地区飞仙关组台地相碎屑岩和碳酸盐岩为研究对象,以野外露头剖面、岩芯、钻井、测井、地震等资料为基础,综合应用岩性突变面、沉积相转换面、沉积物空间堆积样式的变化、早期成岩变化、电测井曲线特征以及地震反射特征等标志,识别出不同级次的11个层序界面,据此将本区飞仙关组划分为2个三级层序(TSQ1和TSQ2)和10个四级层序,其中TSQ1可细分出6个四级层序,TSQ2可再分出4个四级层序,并将其与传统地层单位进行对比:三级层序TSQ1和TSQ2分别对应于飞一段+飞二段地层和飞三段+飞四段地层。通过层序地层对比和层序地层格架的建立,指出这些层序在全区均具有良好的可对比性和等时性,每个层序均具有快速海侵到缓慢海退的特点,均由海侵体系域和高位体系域构成,未发现低位体系域和凝缩段。层序与储层关系的研究表明,四级层序Ⅲ和Ⅷ是台内鲕滩这种有利储集相带的主要发育层位,所形成的滩相鲕粒灰岩储层与高位体系域的向上变浅序列和早期暴露及其所导致的大气淡水淋溶改造有关,平面上集中分布于中东部地区。 相似文献
896.
On the DB gap of white dwarf evolution:effects of hydrogen mass fraction and convective overshooting
Jie Su Yan Li National Astronomical Observatories/Yunnan Observatory Chinese Academy of Sciences Kunming China Graduate University of Chinese Academy of Sciences Beijing 《中国天文和天体物理学报》2010,10(3)
We investigate the spectral evolution of white dwarfs by considering the effects of hydrogen mass in the atmosphere and convective overshooting above the convection zone.Our numerical results show that white dwarfs with MH~10-16M⊙ show the DA spectral type between 46000■Teff■26000K and the DO or DB spectral type may appear on either side of this temperature range.White dwarfs with10-15M⊙ appear as DA stars until they cool to Teff~31000K;from then on they will evolve into DB white dwarfs as a result of conve... 相似文献
897.
The simultaneous photometric and spectroscopic observations of the spotted G dwarf AP149 in the young open cluster α Persei are analyzed here.We reconstruct the observed light curves with a two-starspot model by means of a light curve modeling technique,and find that the active regions shift oppositely along longitude on a time scale of one day.Combining with the observational data obtained by other groups,we discuss the evolution of spotted regions in the photosphere,and find that its starspots evolve not ... 相似文献
898.
Bo Wang Zhan-Wen Han National Astronomical Observatories/Yunnan Observatory Chinese Academy of Sciences Kunming China Graduate University of Chinese Academy of Sciences Beijing 《中国天文和天体物理学报》2010,10(3)
Type Ia supernovae(SNe Ia)play an important role in the study of cosmic evolution,especially in cosmology.There are several progenitor models for SNe Ia proposed in the past years.By considering the effect of accretion disk instability on the evolution of white dwarf(WD)binaries,we performed detailed binary evolution calculations for the WD+red-giant(RG)channel of SNe Ia,in which a carbon-oxygen WD accretes material from a RG star to increase its mass to the Chandrasekhar mass limit.According to these calcu... 相似文献
899.
Jarken Esimbek 《中国天文和天体物理学报》2010,10(2)
We collect 3249 OH maser sources from the literature published up to April 2007, and compile a new catalog of OH masers. We look for the exciting sources of these masers and their infrared properties from IRAS and MSX data, and make a statistical study. MSX sources associated with stellar 1612 MHz OH masers are located mainly above the blackbody line; this is caused by the dust absorption of stellar envelopes, especially in the MSX A band. The mid-IR sources associated with stellar OH masers are concentrate... 相似文献
900.
Zhong-Mu Li Cai-Yan Mao Ru-Heng Li Ru-Xi Li Mao-Cai Li College of Physics Electronic Information Dali University Dali China National Astronomical Observatories Chinese Academy of Sciences Beijing 《中国天文和天体物理学报》2010,10(2)
Binary stars are common in star clusters and galaxies, but the detailed effects of binary evolution are not taken into account in some color-magnitude diagram (CMD) studies. This paper studies the CMDs of twelve globular clusters via binarystar stellar populations. The observational CMDs of the star clusters are compared to those of binary-star populations, and then the stellar metallicities, ages, distances and reddenings of these star clusters are obtained. The paper also tests the different effects of bi... 相似文献