A Research on the Gravity Deformation of Delingha 13.7m Telescope

Based on digital photogrammetric measurements, the antenna panels of the Delingha 13.7m radio telescope are adjusted to make the main dish have an optimal paraboloidal surface at the elevation of 52°, thus the overall antenna efficiency is optimized for different observing elevations. Observations indicate that the aperture efficiency of the telescope has been improved approximately twice in comparison with the antenna panels adjusted on the basis of theodolite measurements. According to the results of the measurements at different elevations, the models of antenna gravity deformation are built, including the displacement and tilt angle of the subreflector, as well as the focal length and surface error of the main reflector, as functions of elevation angle. In the process of modeling the gravity deformation of the main dish, instead of the direct calculation method, the least square fitting on the measured surface errors at different elevation angles is adopted, in order to reduce the effect of measurement errors on the accuracy of the model.     

The effect of an optically thin region on stability of an accretion disk around a supermassive black hole

We analyse conditions of the innermost portion of an accretion disk and establish a set of equations for this region. A stable innermost region may exist, which can probably explain the observed UV and X-ray spectra, avoiding the unstable emission. We then discuss the detailed radial structure of a disk around a black hole for typical AGN parameters and obtain different kinds of- relationships for different regions of a disk. On the basis of this, we discuss the stability. A new type of cycle is present, which we call a double S shaped cycle. In this cycle, the extent of accretion rate variability is much larger than that in dwarf nova cycles. This probably solves the problem of violent variability of AGN. In the meantime, the very high accretion rate at the hottest state in limit cycles in the unstable region may provide continuous injection of matter to the jet and power the relativistic motion of the jet.     

分子外流源L1211中近红外HH天体的发现

报告分子外流源Ｌ１２１１ 中新发现的１２ 个近红外ＨＨ 天体．在Ｌ１２１１ 的～４’区域,取得了ＪＨＫ’宽带和Ｈ２ 　ｖ ＝ １０ 　Ｓ（１） 发射线窄带的近红外图像．分析表明,新探测到的许多红外源与浓密分子云物理成协,其中有２０ 多个源表现出典型的Ｔ Ｔａｕｒｉ 星、Ｈｅｒｂｉｇ Ａｅ／Ｂｅ星和原恒星的红外超．Ｌ１２１１ 中的ＩＲＡＳ点源没有被观测到,可能是更深地埋于分子云中．对红外观测和分子线观测消光估计的比较显示,小于２μｍ 的近红外观测还不足以揭示深埋于分子云的整个年轻星团．根据近红外ＨＨ 天体的形态分布和红外源性质,能进一步证认这些ＨＨ 天体的激发源．其结果表明,Ｌ１２１１ 分子云中具有多个红外源驱动的多个外流活动     

Stellar SiO 86GHz Maser Observations of IRAS Point Sources

1　ＩｎｔｒｏｄｕｃｔｉｏｎＳｉＯ ,Ｈ2 ＯａｎｄＯＨｍａｓｅｒｅｍｉｓｓｉｏｎｓａｒｅｃｏｍｍｏｎｐｈｅｎｏｍｅｎａａｓｓｏｃｉａｔｅｄｗｉｔｈｔｈｅｃｉｒｃｕｍｓｔｅｌｌａｒｓｈｅｌｌｓｏｆｌａｔｅｔｙｐｅｓｔａｒｓ .ＳｉＯｍａｓｅｒｅｍｉｓｓｉｏｎｓｈａｖｅｂｅｅｎｄｅｔｅｃｔｅｄｆｒｏｍｓｅｖｅｒａｌｈｕｎｄｒｅｄｓｏｆｌａｔｅｔｙｐｅｓｔａｒｓｏｆｓｐｅｃｔｒａｌｔｙｐｅＭ 4ｏｒｌａｔｅｒ.ＳｉＯｍａｓｅｒｉｓｃｏｎｓｉｄｅｒｅｄｔｈｅｍｏｓｔｐｒｅｖａｌｅｎｔｍａｓｅｒｉｎｌａｔｅｔｙｐ…     

Zircon U-Pb geochronology and geochemistry of syenogranites in western Niubiziliang,northwestern Qaidam,Qinghai

The study presents the results of U-Pb dating of zircons and whole-rock geochemical analyses of a syenogranite located in the western Niubiziliang area,China with the aim of determining its formation time,petrogenesis and the regional tectonic setting. Zircons within the syenogranite are euhedral-subhedral and display rhythmic growth zoning,indicating a magmatic origin. Zircon U-Pb data obtained by LA-ICP-MS indicate the syenogranite formed in the Late Permian (260.7±1.5 Ma). The w(SiO_2) of syenogranites is 70.82%--73.59%,w(Al_2O_3) is 13.49%--14.82%,and w(Na_2O + K_2O) is 7.85%--8.52%,and yield K_2O/Na_2O ratios of 1.06--1.26. Therefore,the syenogranites belong to the high-K calc-alkaline and metaluminous (A/CNK 1,A/NK 1) series which display I-type granites similarly. The syenogranites also show the geochemical characteristics of volcanic arc rocks,being enriched in large-ion lithophile elements (LILEs; K,Rb) and light rare-earth elements (LREEs; La,Ce,Sm,Nd),but depleted in high field strength elements( HFSEs; Ta,Nb,P,Ti). On the whole,trace element ratios are close to the mean of the Earth's crust,indicating a lowercrust magma source. The low Sr (161--214) ×10~(-6) and Yb (1.08--1.80)×10~(-6) concentrations indicate that plagioclase and hornblende are residual mineral phases in the source. The regional geology and whole-rock geochemistry suggest that the formation of the syenogranites was related to subduction of the Zongwulong Ocean crust,and the north margin of Qaidam Block during the Late Permian was in an active continental margin tectonic setting.     

WebGIS应用服务器数据调度优化策略研究

应用服务器的数据调度是影响WebGIS系统性能的主要因素之一。本文在分析WebGIS体系结构的基础上,探讨了可以在服务器端数据调度中应用的若干优化技术,包括对象化包装、连接池、线程池、扩展SQL、多步传输协议和代理服务机制。经在实验中验证,采用这些技术的WebGIS系统在同等网络环境下,可以显著提高整体性能。     

北京市强降雨分区及重现期研究

利用北京观象台1841—2008年年降水量资料及近50年北京市20个气象站和82个雨量站资料分析了北京地区降水量的时间和空间变化规律,对北京地区的降雨进行分区研究,并结合观象台站逐分钟降雨资料应用广义偏态分布（GPD）方法分析了北京地区不同历时降雨量重现期。结果表明：近168年来,北京地区有两个多雨时段和两个少雨时段,目前北京处于20世纪90年代至今的少雨时段内。70至80年代,北京地区强降雨主要为全市区域性降雨,90年代之后北京的短历时强降雨呈现出局地性的特征,降水分布不均,强降水中心大致成东北一西南向带状分布。根据北京市降雨EOF分析,将北京市划分为4个降雨分区,分别是山后区、城市中心区、东北部山区和东南部平原区。其中城区代表站观象台站多个历时不同重现期降雨量分析结果经过与现行排水规范对比表明,重现期模拟结果可靠。     

西太平洋地球动力学问题与未来大洋钻探目标

西太平洋区域是全球地质构造和海陆相互作用最活动的区域,经过50多年的大洋钻探研究,人们对西太平洋弧后海底扩张成因、俯冲工厂的动力学机制、地幔演化过程、发震带、热点岩浆活动、沉积古环境等都有了深入研究和分析,但是西太平洋边缘海盆具有很大的构造多样性和复杂性,仍然有很多的科学目标和科学问题有待进一步开展研究.本文详细分析了...