应用能谱扫描电镜与X射线衍射等分析技术研究西藏扎西康铅锌矿中伴生元素锰的赋存状态

西藏扎西康铅锌多金属矿床是我国首次发现的喷流沉积-热泉水改造型锰铁锑铅锌银矿床,已有研究表明矿床中除了铅锌矿还伴生有银、锑、铜、硫、锰、砷等多种元素。本文在化学多元素分析和光学显微镜镜下鉴定的基础上,结合能谱扫描电子显微镜和X射线衍射分析等手段对扎西康铅锌矿中伴生组分Mn的含量、矿物种类、嵌布和包裹等特性进行了研究。分析结果表明,原生矿石的主要成矿元素Pb和Zn的含量分别为6.00%和4.00%,伴生元素Mn的含量平均达到4.36%;原生矿石中的主要矿物为方铅矿、闪锌矿,其次为黄铁矿、毒砂和菱锰矿等。原生矿石中伴生元素Mn主要以独立的菱锰矿和铁菱锰矿形式存在,与闪锌矿和方铅矿密切共生,是成矿早期重要的载矿矿物,嵌布在石英、黄铁矿、闪锌矿和毒砂的粒间、边部及空隙间,其次以类质同象形式赋存于菱铁矿和菱锌矿中。进一步对扎西康铅锌矿选冶产物中的伴生元素Mn的含量和赋存状态进行研究,研究表明Mn具有较高的综合利用价值,在原生矿石、铅精矿、锌精矿和尾矿中的质量分数分别为4.36%、0.51%、0.95%和5.36%,显示Mn很少一部分进入铅精矿和锌精矿,而绝大部分进入尾矿;Mn在尾矿中仍主要以菱锰矿形式存在,存在形式与原生矿石相比未发生改变,可通过强磁选工艺从铅锌尾矿中综合回收利用Mn。     

红外光谱/扫描电镜等现代大型仪器岩石矿物鉴定技术及其应用

传统的光学显微镜由于分辨率、放大倍数的限制,对于细微颗粒的定性分析不准确,矿物的定量分析存在一定的误差,对纳米-微米级矿物形貌及结构特征的观察束手无策。随着油气勘探及地质找矿的不断深入,需要提供岩石中所有矿物、孔隙及微量元素的信息,因此整合傅里叶红外光谱仪、X射线衍射仪、拉曼光谱仪、扫描电镜的优点,建立以大型仪器为基础的岩石矿物鉴定方法是当前地质工作的需要。红外光谱光谱范围为7500~370 cm-1,能对固、液、气样品中含量高于30%的矿物进行快速、准确的定性分析;主要用于有机质分析,其次还可对部分具有极性键的无机化合物及金属氧化物进行分析。X射线衍射仪能快速地对样品中含量大于15%的矿物进行较为准确的定量分析;现今主要用于各类晶质矿物的定性分析,同时也可对碳酸盐岩矿物等不含水矿物进行定量分析。拉曼光谱仪光谱范围为200~1000 nm,空间分辨率为横向0.5μm、纵向2μm,通过对包裹体进行测试能直接获得成岩过程中的温度、压力、流体成分等信息;目前主要用于流体包裹体成分的测试,其次还可对分子极化度会发生变化的液态、粉末及固体样品进行定性分析。扫描电镜分辨率达到1 nm,能清晰地观察到纳米-微米级矿物的形貌特征及矿物的结构特征;主要用于纳米-微米级的任何非磁性固体矿物的形貌及相关关系的观察。通过大型仪器建立的岩石矿物鉴定方法具有更高的分辨率,显著地提高了岩矿鉴定的精准度,大大拓宽了岩矿鉴定的范围(如鉴定纳米/微米级的矿物、矿物的不同变种等),能够全面、精准地提供岩石矿物的矿物含量和矿物组成、客观准确的成岩作用信息、清晰的矿物微观形貌及结构特征,而且仪器功能相互重叠,测试结果相互验证,保证了测试结果的可靠性。与传统光学显微镜鉴定方法相比,现代大型仪器岩石矿物鉴定技术为揭示矿物间的共生、反应、演化、岩石的成因、沉积/成岩环境等提供了依据,为地质工作提供准确、全面的矿物定性定量、组构特征及成岩作用等信息,为地质工作的顺利完成奠定了坚实的基础。     

陆生植物氮同位素组成与气候环境变化研究进展

近年来,由于植物氮同位素组成(δ15N)记载了气候环境变化的信息,因而被广泛应用于全球变化研究中,成为古气候环境再造和了解现代气候环境变化信息的有力工具。然而,人们对气候环境引起的δ15N变化及其指示的气候环境意义并不完全清楚,这就有可能限制植物δ15N在古气候环境变化等领域研究中的应用。在概述植物氮同位素分馏和植物不同氮源的氮同位素分布的基础上,分析了温度、降水、大气CO2浓度和海拔高度等气候环境因子对陆生植物δ15N的影响以及它们的关系。指出了目前研究中存在的问题及其研究前景,认为在全球变化研究中利用植物氮同位素技术不仅可以重建古气候环境(如重建大气CO2浓度变化),揭示历史时期温度、降水的变化,而且还可以在一定的时间和空间上综合反映生态系统氮循环的特征。     

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Tidal pattern instabilities on multi-moon planets

The equilibrium tide-generating forces in the lunar orbital plane of a planet of radius R are calculated for the case of N moons of mass Mi orbiting the planet at instantaneous polar coordinates (Di, αi). For the case of a single moon, there are only two high tides. For the case of two moons, it is found that there can exist a critical lunar orbital distance at which two high tides become unstable with respect to formation of three high tides. Bifurcation diagrams are presented which depict how the angular positions of the high and low tides on the planet vary with the lunar distances and lunar separation angle. Tidal stability diagrams, which illustrate the stability regions for various tidal patterns as a function of lunar distances and lunar separation angle, are presented for various values of D₂/D₁ and M₂/M₁. Generally speaking, the aforementioned tidal instability, and hence the propensity for formation of three high tides on a two-moon planet, exists over a significant range of lunar distances and separation angles provided that M₂/M₁∼³(D₂/D₁). For the case of N>2 moons, the tidal stability diagram becomes more complex, revealing a diversity of potential tidal patterns.     

Layering stratigraphy of eastern Coprates and northern Capri Chasmata, Mars

Distinct competent layers are observed in the slopes of eastern Coprates Chasma, part of the Valles Marineris system on Mars. Our observations indicate that the stratigraphy of Coprates Chasma consists of alternating thin strong layers and thicker sequences of relatively weak layers. The strong, competent layers maintain steeper slopes and play a major role in controlling the overall shape and geomorphology of the chasmata slopes. The topmost competent layer in this area is well preserved and easy to identify in outcrops on the northern rim of Coprates Chasma less than 100 m below the southern Ophir Planum surface. The volume of the topmost emplaced layer is at least 70 km³ and may be greater than 2100 km³ if the unit underlies most of Ophir Planum. The broad extent of this layer allows us to measure elevation offsets within the north rim of the chasma and in a freestanding massif within Coprates Chasma where the layer is also observed. Rim outcrop morphology and elevation differences between Ophir and Aurorae Plana may be indicative of the easternmost extent of the topmost competent layer. These observations allow an insight into the depositional processes that formed the stratigraphic stack into which this portion of the Valles Marineris is carved, and they present a picture of some of the last volcanic activity in this area. Furthermore, the elevation offsets within the layer are evidence of significant subsidence of the massif and surrounding material.     

纳米计量学的基础技术组件

为了满足ASTROD激光宇航动力学任务慨念计划的高精度要求 ,以及实现新质量标准 ,我们开始进行次纳米激光测长与纳米定位控制的研究。本文将回顾我们在清华大学与工研院测量中心的研究成果 ,介绍如何利用外差式激光干涉仪、挠性微动台与压电陶瓷 ,进行次纳米激光测长与纳米定位控制。此研究成果将做为ASTROD计划中 ,无拖曳航天技术的研发基础。之后讨论如何将纳米定位控制系统与扫描穿隧显微镜进行整合 ,完成计量型扫描穿隧显微镜 ,进一步将微结构的测量尺寸直接追溯至长度标准。     

Derivation of planetary topography using multi-image shape-from-shading

In many cases, the derivation of high-resolution digital terrain models (DTMs) from planetary surfaces using conventional digital image matching is a problem. The matching methods need at least one stereo pair of images with sufficient texture. However, many space missions provide only a few stereo images and planetary surfaces often possess insufficient texture.This paper describes a method for the generation of high-resolution DTMs from planetary surfaces, which has the potential to overcome the described problem. The suggested method, developed by our group, is based on shape-from-shading using an arbitrary number of digital optical images, and is termed “multi-image shape-from-shading” (MI-SFS). The paper contains an explanation of the theory of MI-SFS, followed by a presentation of current results, which were obtained using images from NASA's lunar mission Clementine, and constitute the first practical application with our method using extraterrestrial imagery. The lunar surface is reconstructed under the assumption of different kinds of reflectance models (e.g. Lommel-Seeliger and Lambert). The represented results show that the derivation of a high-resolution DTM of real digital planetary images by means of MI-SFS is feasible.     

利用扫描电镜-电子探针研究四川杨柳坪镍铜硫化物矿床铂钯的赋存状态及沉淀机制

本文利用电子探针和配备能谱分析功能的扫描电镜对四川杨柳坪镍-铜硫化物矿床中铂钯的赋存状态进行了研究。结果表明,铂以独立矿物相砷铂矿和自然铂存在;钯以碲化物、碲铋化物、碲锑化物、锑化物及自然钯独立矿物相存在,也以类质同象形式分布在碲镍矿中(钯含量约10%),另外还以锑铋钯碲矿、六方锑碲钯矿、碲钯矿独立矿物相存,并以类质同象形式分布在Vavrinite(钯含量5%)和砷铂矿(钯含量1%~5%)中。杨柳坪矿床中铂钯元素沉淀与贱金属矿物(BMS)及晚期热液蚀变矿物蛇纹石、方解石密切相关,其沉淀经历了3个阶段:1早期高温阶段(1200~900℃),铂钯元素沉淀并包裹在BMS中;2中期中高温阶段(650~250℃),分离结晶作用使铂钯元素沉淀并分布BMS矿物的边部,同时该阶段热液来源的铂钯元素沉淀于BMS粒间;3晚期热液蚀变阶段(500~300℃),热液蚀变作用引起铂钯元素沉淀在蚀变矿物中或嵌布在BMS裂隙。本文研究成果为认识该矿床及同类型镍-铜硫化物矿床的铂钯成矿过程提供了新的依据。     

赣东北朱溪铜钨矿区花岗闪长斑岩LA-ICP-MS锆石U-Pb定年及地质意义

赣东北朱溪超大型铜钨矿位于江南古岛弧带塔前—赋春成矿带中段,该矿床的发现可进一步验证"南钨北扩"观点并对"南钨北铜"格局提出挑战,但前人对与朱溪铜钨矿成矿作用有关的花岗岩缺少精确的年代学研究,导致对其地球动力学背景理解不够深入。本研究通过详细的野外调查、岩心编录和岩矿鉴定,并利用激光剥蚀电感耦合等离子体质谱(LA-ICP-MS)锆石U-Pb法对朱溪铜钨矿区侵入元古代双桥山岩群中的铜矿化花岗闪长斑岩进行测年,获得了锆石206Pb/238U加权平均年龄为847.2±9.4 Ma(MSWD=0.111),代表了其侵位结晶的年龄,属新元古代。分析认为:朱溪铜钨矿区铜矿化花岗闪长斑岩是新元古代早期华南古洋壳俯冲消减及扬子陆块与华夏陆块发生碰撞作用下的岩浆产物,这次岩浆活动与区域上塔前—赋春成矿带成矿作用关系密切,并为钦—杭成矿带提供了成矿物质基础。本次对其成岩年龄的限定,为研究朱溪超大型铜钨矿矿床提供了新证据。