吉林陨石球粒的结构及构造

comparatively evident chondritie structure is observed in the Jilin meteorite. Chondrules range from 0.2 to 3mm in diameter, averaging 0.6mm. Chondrules can be divided into the following types according to the principal minerals crystallized and structure-texture characteristics: (1) Olivine chondrules. In terms of their structure they can be subdivided into prophyritic, grated, barred, sub swirlling internal flow and granular chondrulcs; (2) Orthopyroxene ahondrules. Textural types found are fan-like, radial,parallel fibrous, porphyritic and irregular; (3) Olivineorthopyroxene chondrules; (4)Glass or devitrified chondrules; (5) Ni-Fe chondrules and (6) Troilite-olivine chondrules. Among them, porphyritic and granular olivine chondrules and various kinds of radial orthopyroxene chondrules are most common. In addition, also have been recognized the overlapping of two or more chondrules and chondrules coated with glassy crust. The structure and texture of chondrules indicate that they were originated from molten silicate droplets through rapid cooling prior to the formation of the meteorite parent body. Rapid fusion may be induced on the surface of a few solidified chondrules by solar impulse wave or nebula lightning and, if rapid cooling followed, this would give rise to the appearance of glassy crust. Collision between chondrulcs may result in a variety of chondrule fragments and crystal debris. In some cases, collision is also considered to be responsible for the entrench, inclusion and overlapping textures in ehondrules. After the formation of the meteorite parent body recrystallization of chondrules may take place as a result of thermal metamorphism.     

吉林陨石中包裹体特征，形成温度及其意义的探讨

Glass and gas inclusions have been observed in olivine and other minerals in 30 doubly polished tin sections of Jilin meteorites, indicating that there must have been melting And condensation stages during the process of meteorite formation. Temperatures of formation have been determined by homogenization and quenching runs,giving 1050-200℃ and 502℃ for glass and gas inclusions respectively, Meanwhile,the fibrous radial crystals of pyroxene have been notieed to grow when heated over 800℃. These observations are in general agreement with the available experimental data and theoretical calculations regarding meteorite.     

中天山马鞍桥石炭纪沉积特征及构造意义

出露于中天山马鞍桥、巴仑台北的石炭纪地层属于大塘阶晚期至威宁期碳酸盐和碎屑岩的混合沉积。沉积特征和微量元素标志显示该套地层主体为潮坪-泻湖相沉积,仅顶部为河湖相沉积。砂岩的元素地球化学特征以及骨架颗粒的百分含量均显示,该套地层的蚀源区为岛弧火山岩系和中酸性花岗岩系的中天山微板块。有足够的证据表明该套地层形成于中天山微板块与南天山弧后盆地碰撞的挤压背景,即前陆盆地中,构造和海平面变化是该套充填物的主要控制因素。     

CAWS600型自动气象站维护和常见故障判断

简要介绍CAWS600型自动气象站的基本组成、仪器检测的一般方法，具体介绍电源系统、采集系统、传感器的日常维护和注意事项；针对自动站在其运行中出现的常见故障，进行原因分析，并找出解决办法。     

甘肃金川铜镍矿石中MgO对浮选的影响

金川铜镍矿浮选精矿中MgO高,影响闪速熔炼。对金川主力矿山二矿区矿石中MgO分布特征与赋存状态的研究,分析影响浮选过程中MgO难以抑制原因。认为矿石本身MgO含量高、矿石蚀变严重、含镁矿物自然可浮性的良好是造成精矿中MgO高的主要原因。提出研究含镁矿物的浮选特性和矿石的矿物组成特点是精矿降镁的前提。     

天山托洋峰花岗质岩石的同位素地球化学特征

分析了西天山托木尔峰地区花岗质岩石和基底岩石的稀土元素,微量元素以及Ｏ、Ｐｂ、Ｓｒ、Ｎｄ同位素组成。本区北部伊犁地块基底岩石的Ｎｄ同位素模式年龄约为１．９Ｇａ,南部南天山褶皱带的约为０．７０５到０．７３３）表明本区花岗质岩石主要为地壳溶融产物。Ｏ、Ｐｂ、Ｓｒ、Ｎｄ同位素组成批示位于伊犁地块和南天山褶皱带的花岗岩源区岩石的Ｎｄ模式年龄都相当于伊犁地壳,但源区性质不同,前者源区δ＾１８Ｏ低,μ值低,Ｔ     

隔震结构中非经典阻尼影响及最佳阻尼比分析

本文采用双自由度非比例阻尼振动模型描述基础隔震体系,用拉普拉斯变换方法获得其地震时域响应的近似解析解,借助于应谱理论分析了非比例阻尼对隔震体系中的上部结构层间最大剪力及隔震层最大位移等响应值的影响,探寻了隔震系统最佳阻尼比的取值范围。     

陨石氧同位素组成及其地学意义

介绍了各类陨石氧同位素组成的特点,对陨石氧同位素组成的主要成因观点进行了评述,结合地球的原始物质组成,讨论了陨石氧同位素组成的地球科学意义。     

厦门东侧海域浮游植物的种类组成与分布

共鉴定厦门东侧海域浮游植物４３属１１１种,其主体是广温性种类（５６种）,占浮游植物总种数的５０％。主要优势种的季节性演替明显。四季浮游植物的平均细胞总量达３６５００千个／ｍ＾３,最重要的优势种是施链角毛藻（Ｃｈａｅｔｏｃｅｒｏｓｃ ｃｕｒｖｉｓｅｔｕｓ）（占总量的５３．３％）和中肋骨条藻（Ｓｋｅｌｅｔｏｎｅｍａ ｃｏｓｔａｔｕｍ）（占２０．０）。浮游植物的繁盛时期在春、夏两季,但高峰期出现在春季,不同于相邻的厦门外港和厦门西港。