SIMS Pb/Pb dating of Zr-rich minerals in lunar meteorites Miller Range 05035 and LaPaz Icefield 02224:Implications for the petrogenesis of mare basalt

Miller Range (MIL) 05035 and LaPaz Icefield (LAP) 02224 are unbrecciated lunar basalt meteorites. In this report, we studied their petrography and mineralogy and made in situ uranogenic Pb/Pb dating of Zr-rich minerals. Petrography and mineralogy of these two lunar meteorites are consistent with previous investigations. The zirconolite Pb/Pb age of MIL 05035 is 3851±8 Ma (2σ), in excellent agreement with previous reports. This age suggests that MIL 05035 could be paired with Asuka 881757, a low-Ti mare basalt meteorite. The magmatic event related to MIL 05035 was probably due to the late heavy impact bom- bardment on the moon around 3.9 Ga. One baddeleyite grain in LAP 02224 shows a large variation of Pb/Pb age, from 3109±29 to 3547±21 Ma (2σ), much older than the whole-rock age of the same meteorite (~3.02±0.03 Ga). The other baddeleyite grain in LAP 02224 has an age of 3005±17 Ma (2σ). The result indicates that the minimum crystallization age of LAP 02224 is ~3.55 Ga and the younger ages could reflect late thermal disturbance on U-Pb system.     

丽江高美古的气象条件

综述云南丽江高美古的天文台选址经过、自然环境、云量、大气水汽积分含量和其他气象要素观测的结果     

新型天气预报业务系统框架

在兰州区域气象中心ＤＥＣ业务网络下运行的新型天气预报业务系统,对西北地区东部的重要天气,按中短期预报时效,以模块的方式建立预报系统;以引进人工智能神经元网络技术,预报甘肃省降水天气。该系统经试运行,具有业务实用性强、预报效果较好等特点     

盘古山钨矿成矿流体特征及其地质意义

盘古山钨矿是一个石英脉型钨多金属矿床,在赣南地区的钨矿床中尤为著名。本文在详细的流体包裹体岩相学研究的基础上,对该矿床主成矿阶段黑钨矿-黄铁矿-石英脉和黑钨矿-辉铋矿-石英脉中含矿石英脉中的流体包裹体做了显微测温及拉曼探针分析。结果显示,该矿床流体包裹体类型复杂,不同类型包裹体均一温度及盐度差异较大,反映了复杂的流体特征;包裹体组合复杂,各类型包裹体常叠加在一起,不同分布特征的包裹体组合的均一温度存在明显区别。其中NaCl-H2O气液(Ⅰ型)包裹体均一温度分布范围为100~370℃,大致可划分为三个温度区间,即270~370℃高温区、230~270℃中温区及100~210℃低温区;盐度均10wB%NaCleq.,主要集中在1wB%NaCleq.和4~6wB%NaCleq.之间。相对而言,含CO2三相(Ⅱ型)包裹体的均一温度普遍高于Ⅰ型包裹体,主要集中在220~250℃、260~350℃之间;而盐度相对较低,集中在2~5 wB%NaCleq.之间。所有这些包裹体特征都表明成矿流体具有多期次性,可能反映本区存在多期次的矿化作用。利用含CO2三相包裹体的部分均一温度与最终均一温度计算出成矿流体的捕获压力36.3~97.8 Mpa,平均压力72.2 Mpa,按静岩压力换算成最小成矿深度为1.4~3.76 km,平均为2.78 km。对各类包裹体的激光拉曼探针测试表明:成矿流体中除水、CO2外,还含有少量的CH4和N2。盘古山钨矿的各类流体包裹体的综合特征研究表明,流体的不均一捕获作用可能是盘古山钨矿床石英脉型钨矿形成的主要机制。     

富铯矿物及其在核废物地质处置上的意义

自然界中最常见的铯矿物主要有铯沸石、富铯的云母类矿物和富铯的绿柱石类矿物,它们产于稀有金属花岗岩和LCT(Lithium-Cesium-Tantalum)型稀有金属伟晶岩脉体的中心部位或围岩接触带附近,形成于初始富含铯和挥发组份、处于稳定构造环境且经过高度演化分异的原始花岗质岩浆.由于天然富铯矿物中铯含量一般可达15%,它们的合成相可作为核废料中放射性元素137Cs的前景载体相,而且富铯矿物各自的化学成分和结构等矿物学特征,对137Cs核废物载体相及相应的深埋藏地质环境的选择和载体相在不同地质环境下的行为预测都有较好的指导意义.     

基于数字滑坡技术的暴雨滑坡、泥石流预警、监测模型研究

中国学者在暴雨滑坡、泥石流预测预报研究领域取得的成果为采用数字滑坡技术进行暴雨滑坡、泥石流预警、监测模型研究提供了宝贵的基础,应用数字滑坡技术建立暴雨滑坡、泥石流预测模型的原则是：（1）必须在滑坡、泥石流形成条件理论指导下;（2）应了解研究区地质环境及滑坡、泥石流特征;（3）就基于数字滑坡技术而言,只能选取遥感方法可能...     

星系盘中的磁重平衡:星系贮留原初磁场的观测证据

邻近旋涡星系中观测到的磁场被理论学家解释为发电机作用的结果.而我们发现,在邻近的星系中,磁场的强度与中性氢的柱密度紧密相关.星系盘中的磁场处于磁重平衡状态.这一结果与发电机放大机制相悖,从而支持星系磁场是原初起源的假说.     

Large-Area Back-Illuminated CCD Imager Development

We describe recent work in the area of large, back-illuminated CCD imagers at M.I.T. Lincoln Laboratory as well as new technology applicable to astronomy. We completed in 1995 the development of a 2560 x 1960-pixel frame-transfer imager that filled a 100-mm wafer and several back-illuminated versions of this device were completed. More recently we have begun the development, in collaboration with the U. of Hawaii, of a three-side abuttable 2k x 4k CCD for a multi-chip focal plane. In the unused chord area of the wafer layout, we added test imagers as development vehicles for blooming control and for the demonstration of a CCD that is capable of charge transfer in all four directions. We expect the latter to find application as an electronic means of performing tip-tilt correction to compensate for atmospheric turbulence.     

A Peculiar Broad Line Radio Galaxy 1938-155： VLA Observation at 90 cm

We observed 1938-155, a broad line radio galaxy (BLRG), with the Very Large Array (VLA) at 90cm with an angular resolution of 6.8" × 4.0". The source consists of two components separated by 4 arcsec (- 20kpc, for H0 = 65km s-1 Mpc-1, q0 = 0.5) along the SE-NW direction. Both components show steep-spectra with a similar spectral index α - 0.83 ± 0.07 (Sv ∝ v-α). The bright double components are surrounded by a low-brightness cocoon. The radio properties of the two bright components are consistent with the hot spots produced by twin jets. An upper limit of - 0.0008 for the core dominance parameter (R) is inferred, suggesting there is no prominent radio core in the source. Assuming a modest viewing angle 30f77, a jet velocity is estimated - 0.07 c, based on the jet to counter-jet brightness ratio (J). The lower limit in jet speed inferred is consistent with no Doppler beaming effect on the jet. The radio galaxy 1938-155 could be an exceptional BLRG with no prominent radio core or jet.