Development of the Automatic Seeing Monitor for the Site Testing of Dome A

The Antarctic site-testing campaigns have shown that Dome C is an excellent astronomical site on the earth, it is better than any of existing mid-latitude astronomical sites in the world, because of its cold and dry weather, low infrared background radiation, continuously observable time as long as 3–4 months, clear and highly transparent atmosphere, low wind speed, and the absence of dust and light pollution. And in the international astronomical community it is generally believed that Dome A with a higher altitude may be better than Dome C as a potential excellent astronomical site. In the past 3 years, although held by the Center for Antarctic Astronomy of Chinese Academy of Sciences, the site testing at Dome A has preliminarily con?rmed the many advantages of Dome A as an excellent astronomical site, but the data about the atmospheric seeing, which is an important parameter for assessing the site quality for optical observations, have not been obtained until now. Hence, on the basis of a commercial telescope with the diameter of 35 cm, we have made the hardware reformation and software development to have it operate as a DIMM (Differential Image Motion Monitor), which can simultaneously monitor both the seeing and isoplanatic angle at Dome A automatically. At present this instrument has been shipped to Antarctica by the “Xuelong” exploration ship, and will be installed at Dome A, and begin to work in early 2011. Before the shipment, by through the comparative measurements together with an existing seeing monitor at the Xinglong astronomical station, the software, hardware, as well as the installation and adjustment of the instrument, are further veri?ed by testing.     

Research on the Application of Fast-steering Mirror in Stellar Interferometers

In stellar interferometers, the fast-steering mirror (FSM) is widely utilized to correct the wavefront tilt caused by the atmospheric turbulence and internal instrumental vibration, because of its high resolution and fast response frequency. In this study, the non-coplanar error between the FSM and the actuator deflection axis introduced by the manufacturing, assembly, and adjustment is analyzed systematically. Via a numerical method, the additional optical path difference (OPD) caused by the above factors is studied, and its effect on the fringe tracking accuracy of a stellar interferometer is also discussed. On the other hand, the starlight parallelism between the beams of two arms is one of the main factors for the loss of fringe visibility. By analyzing the influence of wavefront tilt caused by the atmospheric turbulence on fringe visibility, a simple and efficient real-time correction scheme of starlight parallelism is proposed based on a single array detector. The feasibility of this scheme is demonstrated by a laboratory experiment. The results show that after the correction of fast-steering mirror, the starlight parallelism meets preliminarily the requirement of a stellar interferometer on the wavefront tilt.     

初轨的稳健估计算法

讨论单测角资料(数据中包含异常值)初轨的稳健估计算法．该算法既可用于提供可靠的初轨,又可用作资料预处理,剔除异常值．稳健估计算法的崩溃点为16％至25％,可剔除6σ以上的异常值．     

The first World Atlas of the artificial night sky brightness

We present the first World Atlas of the zenith artificial night sky brightness at sea level. Based on radiance-calibrated high-resolution DMSP satellite data and on accurate modelling of light propagation in the atmosphere, it provides a nearly global picture of how mankind is proceeding to envelop itself in a luminous fog. Comparing the Atlas with the United States Department of Energy (DOE) population density data base, we determined the fraction of population who are living under a sky of given brightness. About two-thirds of the World population and 99 per cent of the population in the United States (excluding Alaska and Hawaii) and European Union live in areas where the night sky is above the threshold set for polluted status. Assuming average eye functionality, about one-fifth of the World population, more than two-thirds of the United States population and more than one half of the European Union population have already lost naked eye visibility of the Milky Way. Finally, about one-tenth of the World population, more than 40 per cent of the United States population and one sixth of the European Union population no longer view the heavens with the eye adapted to night vision, because of the sky brightness.     

登陆我国热带气旋活动的年代际变化分析

本文利用1950－1999年西北太平洋热带气旋资料，对50年来登陆我国热带气旋的月际、年际和年代际变化及异常情况进行了统计分析，指出了登陆我国的热带气旋频数存在明显的年代际差异，并对比分析了同期的副热带高压等海洋大气环流指数的统计特征。     

Millimetre and submillimetre τ relations

Relations are presented between the optical depth of the atmosphere  (τ)  in the millimetre and submillimetre windows at 350, 450, 850 and 1250 μm. These relations are derived by an analysis of 849 skydips at 850 μm performed with the submillimetre camera SCUBA at the James Clerk Maxwell Telescope (JCMT) and polynomial fits to over 19 000 measurements of a tipping radiometer operating at 350 μm. The relations allow for an improved calibration of millimetre and submillimetre observations on Mauna Kea, Hawai'i, and for better monitoring of atmospheric conditions.     

阴山陆块武川石榴基性麻粒岩P-T条件及其变质时代:来自相平衡模拟与锆石U-Pb定年的约束

武川高级片麻岩地体中石榴基性麻粒岩的变质用与同位素年代学研究对于揭示阴山陆块新太古代构造演化过程具有十分重要的研究意义。它们主要以不规则透镜体或变形岩墙/岩脉群的形式赋存于新太古代晚期英云闪长质片麻岩或变质表壳岩系之中,并切割近南-北向的区域性片麻理。岩相学观察、矿物相转变分析与矿物化学研究表明,武川石榴基性麻粒岩保留了十分典型的高压麻粒岩相矿物:石榴石+单斜辉石+斜长石+角闪石+石英+铁-钛氧化物。其中,粗粒石榴石边部常发育微弱的扩散环带,表现为从幔部至边部,镁铝榴石组分不断减少,相应地铁铝榴石组分不断增加,而钙铝榴石与锰铝榴石组分基本不变,指示晚期冷却降温作用对石榴石成分产生一定影响。斜长石具有细粒包体型与粗粒基质型两种不同的类型,它们具有十分相似化学成分,均为An=35~45的中长石。在NCFMASHTO(Na_2O-CaO-FeO-MgO-Al_2O_3-SiO_2-H_2O-TiO_2-Fe_2O_3)体系下,利用THERM OCA LC 3.33软件,对两件石榴基性麻粒岩样品进行了相平衡模拟,模拟的峰期矿物组合为:石榴石+单斜辉石+斜长石+角闪石+石英+铁-钛氧化物,与岩相学观察十分一致。采用石榴石中最小x(g)Fe~(2 +)/(Fe~(2 +)+Mg))与斜长石是中最小ca(pl)(Ca/(Ca+Na))等值线,将本区石榴基性麻粒岩峰期高压麻粒岩相的温压条件限定在P=1.31~1.40GPa,T=770~840℃的范围内。LA-ICP-MS锆石U-Pb定年结果表明,两件石榴基性麻粒岩麻粒岩中发育的变质锆石分别记录了2517±6Ma(BT58-1,MSWD=0.66,n=21)与2512±16Ma(LH66-1,MSWD=0.26,n=42)的加权平均年龄,与阴山陆块其它新太古代岩石记录的约2500Ma变质年龄一致,被解释为本区石榴基性麻粒岩遭受高压麻粒岩相变质时代。结合本区其它新的研究资料,本文认为武川石榴基性麻粒岩形成可能与区内新太古代晚期造山作用有关。     

从《徐霞客游记》看明末南方的社会经济生活——纪念徐霞客逝世350周年

本文以《徐霞客游记》为依据,对明末南方的社会经济生活状况进行了初步归纳和分析,以揭示徐霞客对我国人文地理学的突出贡献。     

近海水体悬浮物HJ-1 号小卫星CCD 定量反演研究

基于H J-1号小卫星CCD数据,开展近海水体悬浮物含量监测研究.采用邻近清洁水体和同日MODIS气溶胶产品的方法对CCD辐亮度数据进行较精准的大气校正;利用得到的水体遥感反射率,结合地面准同步实测悬浮物含量数据建立悬浮物反演模型,获得研究区悬浮物的空间分布.模型的相关系数R2为0.849,平均误差为33.0％,反演结果较为理想.结果表明,HJ-1号小卫星作为中国首个灾害监测小卫星星座,能够实现定量反演近海水体的悬浮物含量,对中国近海水体水质的监测和治理具有重要意义.     

藏南色如朗金红石矿床地质特征及控矿条件

藏南色如朗金红石矿床位于米拉山口断裂带东段北缘,矿床的赋矿岩石主要为绿片岩。由北向南圈定了3个矿体,矿体沿北东方向延伸,呈层状、似层状产出。矿石矿物以金红石为主,其他金属矿物有磁铁矿、赤铁矿、黄铁矿、黄铜矿、磁黄铁矿等。金红石主要为红褐色,少数为暗红褐色,呈自形-半自形柱状和他形粒状,粒径多为0.01~0.2mm,大者可达1~2mm。该矿床的形成主要受地层和变质作用控制,后期构造对矿床形态有一定的破坏作用。通过与中国典型金红石矿床地质特征对比,初步认为色如朗金红石矿床的成因类型为中低压变质型。