中缅毗邻区金腊Pb-Zn-Ag多金属矿田元素、稳定同位素和流体包裹体地球化学   总被引：4，自引：0，他引：4  

陈永清  黄静宁  卢映祥  夏庆霖  孙明祥  李建荣 《地球科学》2009,34(4):585-594

跨越中缅边境的金腊铅-锌-银多金属矿田包括南腊和金厂两处铅锌银矿床, 大地构造上处于保山-掸泰地块东缘, 勐统-耿马-西盟元古宙-古生代被动大陆边缘活动带南段.通过对容矿围岩、与矿化有关的花岗岩和矿石元素地球化学以及矿石硫、铅同位素和流体包裹体的研究, 结论如下: (1) 与同类岩石相比, 与矿化有关的花岗岩普遍富集Pb、Zn、Cu、Au、Sn、W等成矿元素, 其中钾长花岗斑岩与Pb-Zn-Ag矿化关系最密切. (2) 铅同位素表明, 矽卡岩型致密块状矿石铅同位素比值(206Pb/204Pb、207Pb/204Pb和208Pb/204Pb) 皆低于热液充填型角砾状矿石和似层状硅化白云岩型矿石, 意味着形成于岩体接触带的矽卡岩型矿石相对形成于远离岩体的热液充填型角砾状矿石和似层状硅化白云岩型矿石含有更低的放射性成因铅. (3) 铅-锌-银矿化主要经历了两个成矿期: 矽卡岩化成矿期和中低温热液成矿期, 前者主要形成铅-锌-铜(金) 矿化, 后者主要形成铅-锌-银矿化; 中低温热液成矿期又可划分为两个成矿阶段: 中温成矿阶段(200~290℃) 和低温成矿阶段(140~200℃), 前者主要形成交代充填型硅化角砾岩矿体, 后者主要形成层间破碎带充填型硅化矿体. (4) 金腊铅锌矿床、保山-镇康地块某些铅锌矿床和昌宁-孟连火山岩带的铅锌矿床, 虽然产于不同的地质构造单元, 但矿石铅同位素组成却具有类似的特征, 而且矿化皆与喜马拉雅期侵位的花岗岩密切相关.这表明: 虽然上述矿床产出于不同的地质构造单元, 但成矿皆与喜马拉雅期构造岩浆活动具有某种内在联系.   相似文献   

Helium, Argon, and Xenon Isotopic Compositions of Ore-formingFluids in Jinding-Baiyangping Polymetallic Deposits,Yunnan, Southwest China   总被引：13，自引：0，他引：13  

XUE Chunji  WANG Denghong  CHEN Yuchuan  YANG Jianmin  YANG Weiguang 《《地质学报》英文版》2000,74(3):521-528

The Jinding superlarge lead and zinc deposit has attracted the attention of geologists of the world and its metallogenesis has long been in dispute. This paper takes the Jinding deposit and the Baiyangping Cu-Ag-Co deposit which was recently found at about 30 km north of Jinding as one ore belt, and, based on researches on the helium, argon, and xenon isotopic compositions of primary inclusions in ore-forming solutions of the main stage, the authors have found that the 3He/4He ratio of the ore-forming fluid is 2.7′ 10- 6 (varying from 0.19 to 1.97 Ra), the 4He/40Ar ratio (0.24- 3.12) is close to the mantle characteristic ratio, and the xenon isotopic composition and evolution show characters of the mantle xenon. The above results reveal the characteristics of mantle source and crust-mantle fluid mixing (mantle helium reaching 32%) and the metallogenic contributions of the deep processes in the Jinding-Baiyangping ore belt.  相似文献   

Emanation-Sedimentary Metallogenic Series and Models of the Proterozoic Rift in the Kangdian Axis     

QIN Dexian  LIU ChunxueKunming University of Science  Engineering  Kunming  Yunnan 《《地质学报》英文版》2000,74(3):466-472

The Kangdian axis basement can be divided into two tectonic layers. The lower tectonic layer is the crystalline basement which is made up of the Archaean Dibadu Formation and early Proterozoic Dahongshan Group. The former is a kata-metamorphic basic volcano-sedimentary formation of the old geosyncline (old continental nucleus), and the latter is a medium-grade metamorphosed alkali-rich basic volcanic (emanation)-sedimentary formation of the Yuanjiang-Dahongshan marginal rift. They are in disconformable contact. The upper tectonic layer is the folded basement, and made up of the middle-late Proterozoic Kunyang Group. It is the result of Dongchuan-Yuanjiang intercontinental rifting with discordant contract with the underlying and overlying strata. Along with the evolution of Proterozoic from early to late, four types of emanation-sedimentary deposits in the Kangdian axis rift were formed in turn: (1) emanation-sedimentary iron-copper-gold deposits related to basic volcanic rocks in the Yuanmou-Dahongshan  相似文献   

A possible explanation for the electron/positron excess of ATIC/PAMELA     

Rui-Zhi Yang  Jin Chang  Jian Wu Purple Mountain Observatory  Chinese Academy of Sciences  Nanjing  China 《中国天文和天体物理学报》2010,10(1)

Results from PAMELA and ATIC indicate that the Kaluza-Klein type dark matter particles could be the annihilation source of the observed excess of electrons and positrons.Assuming the existence of a nearby black hole with 10000–100000 solar masses and a point source boost algorithm,we apply the standard propagation model and find that the results fit the data well.  相似文献   

A Probable Short Decimetric Type Ⅰ-like Noise Storm: Associated with Type Ⅲ Bursts?     

Rui-Xiang Xie  Min Wang  Yi-Hua YanNational Astronomical Observatories  Yunnan Observatory  Chinese Academy of Sciences  Kunming  National Astronomical Observatories  Chinese Academy of Sciences  Beijing 《中国天文和天体物理学报》2005,(1)

A rare Type I-like noise storm was observed with the solar radio spectrometers (1.0-2.0 GHz and 2.60-3.8 GHz) at National Astronomical Observatories of China (NAOC) on September 23, 1998. We concentrate on checking the Type I-like noise storm occurred in the decay phase of a Type Ⅳ radio burst. This noise storm consists of many Type I bursts and isolated Type Ⅲ or Type Ⅲ pair bursts. It has a bandwidth of ≤0.5 GHz. The duration of each Type I burst is of the order of 100-300 ms. The total duration is greater than 11 minutes. The circular polarization  相似文献   

太阳物理学中的分形和混沌   总被引：1，自引：0，他引：1  

环遵祥  吴铭蟾 《天文学进展》1996,14(4):286-296

对非线性科学的两个重要分支；分形和混沌在太阳物理学中的应用情况作了综述信要内容包括；太阳活动混沌性的揭示；对太阳活动混沌性的可能解释－太阳非线性发电机理论；一些太阳现象的分形描述；耀斑的自组织临界行为研究，最后给出了作者对这一领域工作前景的展望。  相似文献   

前兆地电阻率资料处理的剥皮法   总被引：2，自引：1，他引：2       下载免费PDF全文

毛先进  钱家栋 《地震学报》2001,24(6):645-650

在台址下电阻率分层均匀的前提下，针对我国绝大多数前兆地电台单极距观测的事实与现状，提出一种试图从这种观测所获得的视电阻率时间序列中识别电阻率表层变化和深部变化的等效模型方法．分析表明，在保持布极方式和观测结果不变的前提下，任意多层的地电结构都可以视为一个二层地电结构——等效模型．本文中，等效模型上层的地电参数（电阻率和厚度）与实际模型第一层相同，下层的地电参数（电阻率）则根据等效要求，由实际模型第二层及其以下各层的地电参数经计算得到，因此，等效模型的下层包含了实际模型第二层及其以下各层的综合影响．初步研究表明，这种方法是可行的．   相似文献   

岩石破坏前的短临应变前兆研究   总被引：5，自引：1，他引：5  

许昭永  杨润海  赵晋明  华培忠  王彬  梅世蓉 《地震研究》2001,24(3):191-196

采用新型应变仪观测岩样在破坏孕育过程中岩样表面测点的应变变化，结果除了长趋势变化，破坏前几秒的特征变化外，在破坏前百分之几秒至十分之几秒还有突变和拢动等特征变化。  相似文献   

不同震级范围的地震频度和频度比     

蔡静观  吴惠芝 《地震地磁观测与研究》1992,(6)

讨论了云南地区不同震级范围的小震频度在强震前的时间进程曲线,发现在介质比较破碎地区,震级偏小的地震频度显示出较明显的强震前孕震系统的非线性阶段,而在介质比较完整的地区,则震级偏大的地震频度反应较明显。为此,引入了频度比的概念,结果表明,强震孕震区的频度比表现为在强震前2—4年,持续增加或持续降低,在强震前1—2年,呈(增加后)降低或(降低后)增加的异常变化,曲线形态出现拐点。对频度比在实际预报工作中的预报能力,也进行了讨  相似文献   

陕西汛期降水与前期大气环流遥相关型的联系   总被引：1，自引：0，他引：1  

高智  谢双亭 《南京气象学院学报》1992,15(4):576-583

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