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Petrography,mineralogy, and geochemistry of lunar meteorite Sayh al Uhaymir 300

Abstract— We report here the petrography, mineralogy, and geochemistry of lunar meteorite Sayh al Uhaymir 300 (SaU 300). SaU 300 is dominated by a fine‐grained crystalline matrix surrounding mineral fragments (plagioclase, pyroxene, olivine, and ilmenite) and lithic clasts (mainly feldspathic to noritic). Mare basalt and KREEPy rocks are absent. Glass melt veins and impact melts are present, indicating that the rock has been subjected to a second impact event. FeNi metal and troilite grains were observed in the matrix. Major element concentrations of SaU 300 (Al₂O₃ 21.6 wt% and FeO 8.16 wt%) are very similar to those of two basalt‐bearing feldspathic regolith breccias: Calcalong Creek and Yamato (Y‐) 983885. However, the rare earth element (REE) abundances and pattern of SaU 300 resemble the patterns of feldspathic highlands meteorites (e.g., Queen Alexandra Range (QUE) 93069 and Dar al Gani (DaG) 400), and the average lunar highlands crust. It has a relatively LREE‐enriched (7 to 10 x CI) pattern with a positive Eu anomaly (?11 x CI). Values of Fe/Mn ratios of olivine, pyroxene, and the bulk sample are essentially consistent with a lunar origin. SaU 300 also contains high siderophile abundances with a chondritic Ni/Ir ratio. SaU 300 has experienced moderate terrestrial weathering as its bulk Sr concentration is elevated compared to other lunar meteorites and Apollo and Luna samples. Mineral chemistry and trace element abundances of SaU 300 fall within the ranges of lunar feldspathic meteorites and FAN rocks. SaU 300 is a feldspathic impact‐melt breccia predominantly composed of feldspathic highlands rocks with a small amount of mafic component. With a bulk Mg# of 0.67, it is the most mafic of the feldspathic meteorites and represents a lunar surface composition distinct from any other known lunar meteorites. On the basis of its low Th concentration (0.46 ppm) and its lack of KREEPy and mare basaltic components, the source region of SaU 300 could have been within a highland terrain, a great distance from the Imbrium impact basin, probably on the far side of the Moon.     

东昆仑纳赤台地区构造时空格架及成矿地质背景分析

纳赤台地区位于东昆仑成矿带中段,为解决该区域重要成矿带基础地质矿产等方面的问题,开展了1:5万基础地质矿产调查。结果显示: 区内构造强应变带和糜棱岩化带交替频繁出现,脆—韧性剪切带中强片理化及糜棱岩化、S-C组构、旋转碎斑和不对称褶皱等构造现象常见,EW向、NWW向构造发育; 新识别出的构造形迹和新发现的一些金铜铅锌等矿点及矿化线索,与区域上绝大多数矿床、矿点分布实例及EW向、NWW向线性构造带产出较一致,表明构造与成矿存在着直接或间接的关系。EW向、NWW向为主的构造与多金属矿床在时空和成因上有着密切的关系,昆仑河韧性剪切带形成时代为中—晚志留世(432~423 Ma),同区内新发现的二道沟白钨矿、铜金山钨锡矿的成矿时代较接近,认为该区域找矿潜力较大。     

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不同太阳、月亮坐标算法对GNSS部分系统误差的影响研究

研究天文年历、JPL星历计算的太阳、月亮坐标的差异及对GNSS导航定位的影响。结果表明,不同星历计算的太阳坐标差异最大为5×10⁸ m,月亮坐标差异最大为3×10⁶ m。天文年历与DE421计算的星固系X方向之间的夹角最大达30′（Y方向与X方向类似）。太阳坐标差异引起的相位绕转改正之间的差异最大达0.3 mm,卫星天线相位中心偏差改正之间的差异最大达3 mm。太阳、月亮坐标差异导致固体潮改正之间的差异最大达3 mm。经实测GPS数据验证,不同星历计算的太阳、月亮坐标差异对PPP的影响可以忽略,建议在PPP中采用计算效率高的天文年历。     

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????2008???????87??95????????ν?????????IGS????????????????GPS??????????????????????????????IGS?????????????????????????????y???????40??IGS????????????GPS??????????????????????????侫???????4.9??3.6??3.4 cm????IGS?????????????GPS??????????????????????????????????????????????????????????????????IGS??????????IGS?????ν????????????????????     

基于SEM图像的既有地基红黏土颗粒微观结构及分形特征研究

采用IPP（Image-Pro Plus）图像分析软件对贵州省贵阳市某工厂三种既有地基红黏土SEM图像的信息进行提取和处理,定性描述和定量分析土体的微观结构,并引入分形理论分析SEM图像,提出在IPP软件中获取颗粒三维分形维数的计算方法。结果表明:（1）抗剪强度参数随微观颗粒数、颗粒形态比的增大而增大,随颗粒平均面积的增大而减小;（2）颗粒分布及形态均具有明显的分形特征,分形维数介于2~3之间,抗剪强度参数均随颗粒分布及形态分维值的增大而增大;（3）与构建三维模型的方法相比,利用IPP软件计算土颗粒三维分形维数的方法具有可行性,简单易操作,结果可靠。      

流动站与参考站不同采样率GPS数据的处理策略

针对GPS流动站与参考站采用不同采样率的特殊应用情况,当观测数据不同步时,采用历元间的相位差分计算流动站的高精度“伪距”,进而单独进行导航定位解算;当流动站与参考站观测数据同步时,采用双差模式。该方案不但充分利用了观测数据,而且可以节省数据采集和传输及运算的成本。飞机导航试验的数据解算表明,采用这种方法,流动站的定位精度可以达到cm级,而且位置更新率较高。     

基于站间单差相位绕转数据估计测站天线旋转速率的方法研究

相位绕转在GNSS定位中是一种误差源,但包含接收机天线旋转的有用信息。提出了一种基于站间单差相位绕转观测数据估计测站天线旋转速率的方法。首先由无几何距离观测值的变化判断天线旋转的开始与结束时间,然后利用单颗卫星站间差分的无几何距离观测值求出测站的天线旋转角度,以及单颗卫星的测站天线旋转速率,最后将所有卫星计算的测站天线旋转速率按照高度角加权平均得到最终的天线旋转速率。通过精心设计实验方案,经实测数据验证,该方法可以精确地估计测站天线的旋转速率,在本实验中,天线旋转平均速率估计精度约为0.5°/s。     

一种加速精密单点定位收敛的新方法

将自适应选权滤波应用到参数估计中,对于合理地选取未知参数及其方差-协方差阵的初值,提出了利用选权拟合的方法。算例结果表明,采用新方法单点定位可以在较短的时间内达到dm甚至cm级的精度。