青海同仁县江里沟斑岩-矽卡岩型铜钨钼矿床辉钼矿Re-Os同位素年龄及其成矿意义     

张涛  张德会  杨兵  张辉  喻晓 《地质学报》2015,89(2):355-364

西秦岭同德—泽库多金属成矿带是青海省重要的矿产集中区之一,位于西秦岭北缘斑岩-矽卡岩型铜、钼、金成矿带的最西端。江里沟矿床是该区的重要组成部分,为一个典型的斑岩型-矽卡岩型铜钨钼矿床。本文利用Re-Os同位素定年方法对江里沟铜钨钼矿床进行了成矿时代测定,获得了5件样品辉钼矿的Re-Os同位素模式年龄范围为219.5±3.1~222.2±4.0Ma,等时线年龄为224.3±7.3Ma。矿区二长花岗岩SHRIMP锆石UPb年龄测定结果表明岩石存在两个期次结晶年龄232±4Ma和214±4Ma,矿区花岗岩可能是两个期次岩浆活动的产物。根据斑岩型矿床矿化晚于成矿母岩的特征,认为江里沟矿床成矿时代属晚三叠世,与矿区232Ma期次的岩浆侵入活动关系密切,成矿晚于成岩约8Ma,成矿与成岩时代基本一致,是西秦岭印支期构造-岩浆活动的产物。本次研究可以大致确定岗察复式岩体周边矿床成矿时限为243.8~214Ma,与区域西秦岭—东昆仑三叠纪构造岩浆作用和成矿时代一致,构成西秦岭北缘斑岩-矽卡岩型铜-钼-金成矿系统的一部分。  相似文献   

Re–Os and U–Pb Geochronology of Porphyry and Skarn Types Copper Deposits in Jilin Province,NE China          下载免费PDF全文

Yong Zhang  Shu–Wen Xing  Quan–Heng Song  Yan Wang  Zheng–Tao Yu  Xiao–Hui Du  Yu–Bo Ma  Zeng–Jie Zhang 《Resource Geology》2015,65(4):394-404

Jilin Province in NE China lies on the eastern edge of the Xing–Meng Orogenic Belt. Mineral exploration in this area has resulted in the discovery of numerous large, medium, and small sized Cu, Mo, Au, and Co deposits. To better understand the formation and distribution of both the porphyry and skarn types Cu deposits of the region, we examined the geological characteristics of the deposits and applied zircon U–Pb and molybdenite Re–Os isotope dating to constrain the age of the mineralization. The Binghugou Cu deposit yields a zircon U–Pb age for quartz diorite of 128.1 ± 1.6 Ma; the Chang'anpu Cu deposit yields a zircon U–Pb age for granite porphyry of 117.0 ± 1.4 Ma; the Ermi Cu deposit yields a zircon U–Pb age for granite porphyry of 96.8 ± 1.1 Ma; the Tongshan Cu deposit yields molybdenite Re–Os model ages of 128.7 to 130.2 Ma, an isochron age of 129.0 ± 1.6 Ma, and a weighted mean model age of 129.2 ± 0.7 Ma; and the Tianhexing Cu deposit yields molybdenite Re–Os model ages of 113.9 to 115.2 Ma, an isochron age of 114.7 ± 1.2 Ma, and a weighted mean model age of 114.7 ± 0.7 Ma. The new ages, combined with existing geochronology data, show that intense porphyry and skarn types Cu mineralization was coeval with Cretaceous magmatism. The geotectonic processes responsible for the genesis of the Cu mineralization were probably related to lithospheric thinning. By analyzing the accumulated molybdenite Re–Os, zircon U–Pb, and Ar–Ar ages for NE China, it is concluded that the Cu deposits formed during multiple events coinciding with periods of magmatic activity. We have identified five phases of mineralization: early Paleozoic (~476 Ma), late Paleozoic (286.5–273.6 Ma), early Mesozoic (~228.7 Ma), Jurassic (194.8–137.1 Ma), and Cretaceous (131.2–96.8 Ma). Although Cu deposits formed during each phase, most of the Cu mineralization occurred during the Cretaceous.  相似文献   

川北早寒武世碳酸盐岩台缘斜坡沉积特征及变形构造形成机制探讨   总被引：2，自引：2，他引：0       下载免费PDF全文

沈骋  谭秀成  李凌  施开兰  苏成鹏  连承波  黎虹玮  肖笛 《古地理学报》2015,17(3):321-334

基于对川北米仓山西部旺苍县鼓城乡唐家河下寒武统仙女洞组露头剖面的观察与镜下分析发现,仙女洞组下段由生物碎屑泥晶灰岩(L)、粉砂质泥岩(M)、似瘤状砾屑灰岩(L')、角砾灰岩(R)、藻凝块灰岩(A)和含生屑钙质砂岩(S)组合而成,其以角砾灰岩、似瘤状砾屑灰岩和藻凝块灰岩为特征,且发育异地岩块和滑塌变形构造。进一步分析认为:L-M岩石组合为正常的斜坡环境低能沉积;L'-R岩石组合中的角砾灰岩为上斜坡生物灰泥丘崩坍滑动至下部而形成的,似瘤状砾屑灰岩可能是由于L-M岩石组合快速沉积导致沉积物失稳滑动变形、上斜坡生物灰泥丘崩落角砾致使的差异压实和滑动、以及后期物质成分差异引起的压溶作用等共同作用的结果,从而使灰质层发生破碎并被泥质包围形成断续的砾屑状,甚至轻微的位移,进而形成条带特征不明显的杂乱变形构造;微生物岩(Mb)组合为上斜坡的灰泥丘沉积;S-M岩石组合为斜坡上部的浊流沉积。根据上述分析结果建立米仓山西部仙女洞组碳酸盐岩台缘斜坡沉积模式,表明仙女洞组沉积早期米仓山西部存在台缘斜坡相沉积。  相似文献   

新疆阿尔泰青河-富蕴地区晚新生代隆升-剥露过程——来自磷灰石裂变径迹的证据     

徐芹芹  季建清  孙东霞  赵磊 《地质通报》2015,34(5):834-844

前人已经对阿尔泰造山带中—新生代的陆内造山作用进行了大量的研究工作,但对中国境内阿尔泰山的隆升过程特别是晚新生代以来的隆升研究程度较弱。阿尔泰山现今的构造面貌究竟是何时定格的,目前仍没有确切的认识。对阿尔泰青河—富蕴地区花岗岩与片麻岩5件样品进行了磷灰石裂变径迹研究,获得了该区晚新生代以来的隆升—剥露信息,并探讨了该区的热史演化过程与阿尔泰山现代地貌的形成。样品的磷灰石裂变径迹年龄为18.7±1.6~22.7±2.2Ma,封闭径迹长度分布在11.6±1.2~13.1±1.4μm之间。热史模拟表明,阿尔泰青河—富蕴地区具有四阶段演化模式:28Ma以前的稳定阶段、28~18Ma的快速冷却阶段、18~8Ma的稳定阶段、8~6Ma以来的快速冷却阶段。8~6Ma以来是本区剥露的最快时期,这一阶段的隆升造就了现代阿尔泰山的地貌,而且也存在于中国西部的其他造山带。2期主要的快速隆升—剥露事件均与青藏高原的隆升阶段有很好的对应关系,应该是对印度—欧亚板块碰撞的响应。  相似文献   

系外行星大气研究现状     

田蕾  季江徽 《天文学进展》2015,(1):27-43

探测系外行星的最终目的是为了寻找系外生命和宣居行星,而系外行星大气是人们了解行星宜居特性的窗口,所以系外行星大气的研究至关重要。近10年来,系外行星大气的理论研究和观测都发展迅速。受观测技术限制,目前观测到大气的系外行星主要是用凌星法探测到的热木星和超级地球,还有用直接成像法探测到的离主星较远的年轻气态巨行星。力求在系外行星大气领域飞速发展之际,对该领域研究现状做简明介绍。首先介绍系外行星大气的观测方法,随后介绍热木星和超级地球的大气概况和研究现状,最后对系外行星大气探测的有关项目进行简要介绍,以展示未来系外行星大气研究的前景。  相似文献   

The inner solar system cratering record and the evolution of impactor populations   总被引：1，自引：0，他引：1  

Robert G.Strom  Renu Malhotra  Zhi-Yong Xiao  Takashi Ito  Fumi Yoshida  Lillian R Ostrach 《天文和天体物理学研究(英文版)》2015,(3):407-434

We review previously published and newly obtained crater size-frequency distributions in the inner solar system. These data indicate that the Moon and the terrestrial planets have been bombarded by two populations of objects. Population 1,dominating at early times, had nearly the same size distribution as the present-day asteroid belt, and produced heavily cratered surfaces with a complex, multi-sloped crater size-frequency distribution. Population 2, dominating since about 3.8–3.7 Gyr,had the same size distribution as near-Earth objects(NEOs) and a much lower impact flux, and produced a crater size distribution characterized by a differential –3single-slope power law in the crater diameter range 0.02 km to 100 km. Taken together with the results from a large body of work on age-dating of lunar and meteorite samples and theoretical work in solar system dynamics, a plausible interpretation of these data is as follows. The NEO population is the source of Population 2 and it has been in near-steady state over the past ～ 3.7–3.8 Gyr; these objects are derived from the main asteroid belt by size-dependent non-gravitational effects that favor the ejection of smaller asteroids. However, Population 1 was composed of main belt asteroids ejected from their source region in a size-independent manner, possibly by means of gravitational resonance sweeping during orbit migration of giant planets;this caused the so-called Late Heavy Bombardment(LHB). The LHB began some time before ～3.9 Gyr, peaked and declined rapidly over the next ～ 100 to 300 Myr,and possibly more slowly from about 3.8–3.7 Gyr to ～2 Gyr. A third crater population(Population S) consisted of secondary impact craters that can dominate the cratering record at small diameters.  相似文献   

Machine Learning-based Weather Support for the 2022 Winter Olympics     

Jiangjiang XIA  Haochen LI  Yanyan KANG  Chen YU  Lei JI  Lve WU  Xiao LOU  Guangxiang ZHU  Zaiwen Wang  Zhongwei YAN  Lizhi WANG  Jiang ZHU  Pingwen ZHANG  Min CHEN  Yingxin ZHANG  Lihao GAO  Jiarui HAN 《大气科学进展》2020,37(9):927-932

正1.A key support for the 2022 Winter Olympics The XXIV Olympic Winter Games are scheduled to take place from 4 to 22 February 2022, followed by the Paralympic Games from 4 to 13 March, in Beijing and towns in the neighboring Hebei Province, China. Weather plays an extremely important role in the outcome of the games (Chen et al., 2018). It can not only cause a difference between a medal or not, but affect the safety of athletes. Success of the Winter Olympics will greatly depend on weather conditions at the outdoor competition venues, dealing with many weather elements including the snow surface temperature, apparent tem-  相似文献   

Specific Relationship between the Surface Air Temperature and the Area of the Terra Nova Bay Polynya,Antarctica   总被引：1，自引：0，他引：1  

Yifan DING  Xiao CHENG  Xichen LI  Mohammed SHOKR  Jiawei YUAN  Qinghua YANG  Fengming HUI 《大气科学进展》2020,37(5):532-544

Antarctic polynyas play an important role in regional atmosphere?ice?ocean interactions and are considered to help generate the global deep ocean conveyer belt.Polynyas therefore have a potential impact on the Earth’s climate in terms of the production of sea ice and high-salinity shelf water.In this study,we investigated the relationship between the area of the Terra Nova Bay polynya and the air temperature as well as the eastward and northward wind based on the ERA5 and ERAInterim reanalysis datasets and observations from automatic weather stations during the polar night.We examined the correlation between each factor and the polynya area under different temperature conditions.Previous studies have focused more on the effect of winds on the polynya,but the relationship between air temperature and the polynya area has not been fully investigated.Our study shows,eliminating the influence of winds,lower air temperature has a stronger positive correlation with the polynya area.The results show that the relationship between the polynya area and air temperature is more likely to be interactively influenced.As temperature drops,the relationship of the polynya area with air temperature becomes closer with increasing correlation coefficients.In the low temperature conditions,the correlation coefficients of the polynya area with air temperature are above 0.5,larger than that with the wind speed.  相似文献   

Seasonal and Sub-Seasonal Circulation Anomalies Associated with Persistent Rainy Days in 2018/2019 Winter in Shanghai,China     

Wei Wang  Fei Xin  Xiao Pan  Ying Zhang  Tim Li 《Acta Meteorologica Sinica》2020,34(2):304-314

Shanghai experienced the longest rainy days in 2018/2019 winter since 1988. The physical cause of such an unusual climate condition was investigated through the diagnosis of observational data. From a seasonal perspective, a long persistent rainy winter was often associated with an El Niño condition in the equatorial Pacific. This abnormal oceanic condition induces a remote teleconnection pattern with pronounced low-level southerly anomalies over East China. The wind anomalies transported moisture from tropical oceans and caused persistent rainfall in East Asia. Meanwhile, the local rainfall time series exhibited a strong quasi-biweekly oscillation (QBWO). Three persistent rainy events were identified in the 2018/2019 winter and they all occurred during the active phase of the QBWO. The first two events were associated with a low pressure anomaly west of Shanghai. Southerly anomalies associated with the low pressure system advected high mean moisture into central eastern China, leading to the persistent rainfall there. The third event was associated with a high pressure anomaly in lower troposphere to the east of Shanghai, which induced anomalous southerlies to its west, favoring the occurrence of rainfall in Shanghai. The result suggests the importance of high-frequency variability in affecting seasonal rainfall anomalies.  相似文献   

从FY-4A卫星遥感数据和GFS资料估算全天空状况下的地表长波辐射通量     

闵敏  吴晓 《气象》2020,46(3):336-345

本文介绍一种利用FY-4A成像仪遥感数据和全球预报系统(GFS)资料估算全天空地表长波辐射通量的反演方法。该方法通过辐射传输模拟和统计回归计算建立云天地表下行长波辐射通量的反演模式,并基于GFS资料处理云覆盖地区的地表上、下行长波辐射通量。这种全天空状况下两种通量的反演结合了FY-4A晴空地表长波辐射业务产品和本文反演模式处理的云天地表上、下行长波辐射通量。2018年9月1日的处理结果与Aqua/CERES同类产品相对比,精度为:RMSE=20.52 W·m^-2,R=0.9481,Bias=3.3 W·m^-2(夜间地表下行辐射通量对比);RMSE=25.58 W·m^-2,R=0.9096,Bias=5.4 W·m^-2(白天地表下行辐射通量对比);RMSE=10.97 W·m^-2,R=0.9762,Bias=-3.3 W·m^-2(夜间地表上行辐射通量对比);RMSE=19.97 W·m^-2,R=0.9283,Bias=5.0 W·m^-2(白天地表上行辐射通量对比)。这些结果表明本文发展的方法能够反演出精度较好的云天上下行长波辐射通量资料,为今后利用FY-4后续星处理生成全天空状况下的地表长波辐射通量产品奠定了理论基础。  相似文献