东准噶尔双泉金矿LA-ICP-MS锆石U-Pb测年及赋矿岩石地球化学特征

为了解双泉金矿成矿时代及成矿环境,分别对双泉金矿含金石英脉和赋矿岩石进行采样测试分析。高精度LA-ICP-MS锆石U-Pb法测年结果表明,双泉金矿含金石英脉加权平均206Pb/238U年龄为(303.53±0.79)Ma,代表了含金石英脉形成年龄,属晚石炭世前后挤压推覆构造体系产物。与双泉金矿主成矿期年龄对比,结合矿区成矿条件及黄铁矿、毒砂等矿物形态特征,认为该金矿的形成不是一期结果,而是经历了预富集、富集的演化历程。赋矿岩石地球化学分析结果表明,岩石的SiO2、K2O、CaO(SiO2=58.82%~89.25%,K2O=1.12%~4.47%,CaO=0.52%~4.47%)含量高,Na2O含量低(Na2O=0.43%~1.76%),A/CNK值大于1,δ值小于3.3,属过铝质、钙碱性岩石,具富钾钙、贫钠镁特点;Ba相对Rb,Th亏损,K2O含量接近活动陆缘K2O含量,TiO2含量与岛弧TiO2含量接近,推断岩体形成于活动陆缘或岛弧环境;稀土元素具弱的负Eu、负Ce异常,(La/Sm)N值较(Gd/Yb)N值大,轻稀土元素分馏程度高于重稀土元素,表明岩浆具壳幔混熔特点。东准噶尔后碰撞阶段早石炭世至二叠纪晚期发生的陆-陆碰撞造山及伸展张弛构造运动可能是造成此结果的主要构造因素。     

http://www.sciencedirect.com/science/article/pii/S1674987114000668

Microbial diversity in the hydrate-containing (sites SH3B and SH7B) and-free (sites SH1B, SH5B, SH5C) sediments collected from the Shenhu area of the South China Sea (SCS) was investigated using 16S rR...     

中国喀斯特天坑研究起源、进展与展望

喀斯特天坑是20世纪末首先在中国南方峰丛和峰林喀斯特地区中发现的一种特殊且宏大的地表负地形,由于具有独特的科学价值和旅游价值,自被发现以来便引起了国内外地貌学者和地质学者的高度关注。对于喀斯特天坑(tiankeng)能否显著区别于其它普通漏斗,而成为一种独立的喀斯特地貌类型,国内外学者已从形态学、成因学、演化发生学等方面进行了深入探究,但仍未取得完全共识。国内外学者在其分类、形成与演化机制、发育条件、地质年代判定、岩溶生态环境等一系列问题上,也进行了较深入的探讨与激烈的争论。同时,对于喀斯特天坑价值的讨论以及开发与保护方面的研究也正引起国内外学者越来越多的关注。为此,论文围绕中国喀斯特天坑的研究阶段、研究进展、价值和开发与保护等主要议题进行了系统性的梳理与评述,进而提出中国喀斯特天坑当前研究中存在的问题和未来的研究方向。     

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。     

基于测月雷达机制月壤相对介电常数反演方法模拟研究

嫦娥三号卫星于2013年12月2日发射,并成功着陆月球,其巡视器上搭载的测月雷达实现了首次雷达就位探测月球。基于测月雷达的探测机制,给出了两种计算月壤相对介电常数的方法,标定件标定法和双天线时延法,并通过仿真验证了两种计算方法的有效性,文中同时给出了两种计算方法存在的局限性,为后期基于嫦娥三号雷达数据进行月球次表层的介电特性反演提供了重要依据。     

江西省森林和植被碳汇价值研究

江西生态优势明显,森林覆盖率居全国前列,研究植被生态系统碳汇价值是应对气候变化和生态文明建设的具体体现。基于森林资源清查资料,研究了2001—2016年江西省森林碳汇价值;基于卫星遥感数据反演获取植被生态系统净初级生产力(NPP),评估了2000—2016年江西各设区市(县)植被碳汇分布特征。结果表明:1)2016年江西省森林碳储量价值为980.30亿元,植被和森林碳汇价值均呈上升趋势。2)江西省植被碳汇价值增加率为4.55亿元/a,2016年约为823.53亿元,每公顷所创造的碳汇经济价值为4930.67元,比2000年增加了11%。3)2016年各设区市植被碳汇价值排名前三位的分别是赣州、吉安和上饶,排名后三位的是新余、鹰潭和萍乡,单位面积固碳价值排名前三位的为赣州、吉安和抚州,排名后三位的是南昌、九江和鹰潭,其排名与森林面积和森林覆盖率有较大关系。     

A diagnostic study of the southern hemisphere summer circulation of the CCC general circulation model

Abstract

The medium‐scale wave regime, consisting largely of zonal wavenumbers 5–7, frequently dominates the summer Southern Hemisphere tropospheric circulation. We perform a diagnostic study of this circulation as simulated by the Canadian Climate Centre (CCC) general circulation model (GCM). The analysis of Hövmöller diagrams, space‐time and zonal wavenumber spectra shows that the CCC GCM is able to simulate the observed medium‐scale wave regime.

The zonally averaged meridional eddy heat and momentum transports and the associated baroclinic and barotropic energy conversions are also examined. The distributions of the transports on the vertical plane agree well with the observations. After comparison with the observed December‐January‐February 1979 distributions, some quantitative differences remain: the heat transport is too weak aloft and too large near the surface, whereas the momentum transport tends to be too weak. The baroclinic and barotropic conversions show a maximum in the medium‐scale waves. The time evolution of the Richardson number of the mean flow suggests that the medium‐scale wave is due to a baroclinic instability.     

A Research on the Imaging Strategy and Imaging Simulation of Toutatis in the Chang’e-2 Flyby Mission

For the Chang’e-2 extended mission of asteroid exploration, the illumination conditions for imaging the asteroid Toutatis are calculated in this paper according to the orbital parameters of both the Chang’e-2 detector and the asteroid, as well as the incident angles of sunlight. On this basis, it is suggested to take photographs after flyby, and the orientation of the camera's optical axis in the coordinate system deflned by Earth's mean equator and equinox at J2000.0 is proposed to be (118.02°, 22.03°). Based on the shape model of Toutatis determined by the foreign radar data, the orientation of the asteroid in the inertial space is calculated at the rendezvous time. Using the Oren-Nayar diffuse-reflection model and the relative positions among the sun, the asteroid, and the detector, together with the cameras orientation, the imaging simulations are performed on the starry sky background respectively at the distances of 300 km, 500 km, and 1000 km from the asteroid after flyby. The results of simulations are verified further by the optical images of Toutatis obtained in the mission.