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

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。     

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

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。     

The inner solar system cratering record and the evolution of impactor populations

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.     

新降雪密度估算方法研究进展

降雪深度预报是北方地区冬季气象服务的重点和难点,新降雪密度估算是降雪深度预报的关键技术。本文回顾了新降雪密度估算中需要着重考虑的气象要素,并对国内外广泛使用的几类新降雪密度估算方法进行了详细的介绍和对比,在此基础上,评述几种估算方法的特点、局限性以及它们之间的承接联系,并对未来新降雪密度估算的发展方向进行了展望。主要结论为:(1)温度、风速、湿度的垂直分布及太阳辐射、降水量是影响新降雪密度的重要气象要素。(2)目前被广泛应用的新降雪密度估算方法有设为常数法、建立公式法、后处理诊断法和基于微物理过程法等四类,四种方法各具特点和局限性,且存在着上下承接关系。(3)较为科学的后处理诊断法和基于微物理过程法有着各自的相对优势也有着难以克服的不足,未来新降雪密度的估算需要在这两种方法的相互促进、共同提高中逐步发展。     

夏季江淮地区降水的气候变化研究进展

针对夏季江淮地区降水的气候变化进行了文献综述和展望。首先回顾了中国大陆东部夏季降水进退研究情况,然后重点概述了中国大陆东部降水气候变化的研究成果、江淮梅雨气候变化和该地区夏季极端降水的研究成果、中国大陆中东部对流降水与层状降水的气候变化研究现状,随后对引起江淮地区夏季降水气候变化的影响机理研究做了回顾。文章最后指出未来要加强五个方面的研究,即江淮地区降水气候变化的综合机理研究、天气学研究、大气污染作用研究、云物理学研究和观测技术方法研究。     

ECMWF集合预报统计量在江西降水预报中的检验分析

利用江西省93个国家气象观测站降水量资料,对2014年ECMWF集合预报降水统计量进行逐6 h和24 h晴雨检验、降水分级检验及区域性暴雨检验。结果表明:1)10%、25%、Mode、融合、最小值在晴雨预报准确率方面较控制预报更有参考价值。2)对于全年降水分级检验,10%、25%、Mode、融合、最小值这5个统计量在小雨的预报方面较控制预报更有参考价值;中位数、概率对中雨的ETS评分要略高于控制预报;90%、75%、概率对大雨预报比控制预报好。对于暴雨预报,最大值、90%、融合比控制预报好;融合、最大值对大暴雨落区的指示意义不大,但对大暴雨量级降水的可能性可以供预报员参考。3)对于区域性暴雨预报,90%、融合、最大值的预报技巧比控制预报高,最大值虽然空报较严重,但对降水量级有一定的指示意义。集合预报各统计量对于强降水过程爆发或发展阶段的预报效果不如降水过程成熟期或末期好。     

A new lunar absolute control point: established by images from the landing camera on Chang'e-3

The establishment of a lunar control network is one of the core tasks in selenodesy, in which defining an absolute control point on the Moon is the most important step. However, up to now, the number of absolute control points has been very sparse. These absolute control points have mainly been lunar laser ranging retroreflectors, whose geographical location can be observed by observations on Earth and also identified in high resolution lunar satellite images. The Chang'e-3(CE-3) probe successfully landed on the Moon, and its geographical location has been monitored by an observing station on Earth. Since its positional accuracy is expected to reach the meter level, the CE-3 landing site can become a new high precision absolute control point. We use a sequence of images taken from the landing camera, as well as satellite images taken by CE-1 and CE-2, to identify the location of the CE-3 lander. With its geographical location known, the CE-3 landing site can be established as a new absolute control point, which will effectively expand the current area of the lunar absolute control network by 22%, and can greatly facilitate future research in the field of lunar surveying and mapping, as well as selenodesy.     

Isolation and biological characteristics of aerobic marine magnetotactic bacterium YSC-1

1 INTRODUCTION Magnetotactic bacteria are able to respond and orient along the direction of terrestrial or artificial magnetic field, a behavior referred to as magneto- taxis. In the majority of magnetotactic bacteria, the magnetosomes are 25–120 nm in d…     

国标图纸的分片输出

本文阐述了国标图纸分片输出的意义与方法；通过举例，ＡｕｔｏＣＡＤ用户能够容易地掌握使用本文中所述的分片输出方法，用小幅面图形输出设备绘制大幅面的工程技术图纸。