One more explanation of superluminal motion

The occurrence of superluminal motion in extragalactic radio sources is believed to be quite common. Among others, the geometrical scattering of radio radiation can also cause superluminal expansion and or motion and halo formation, In this paper, the effectiveness of the stimulated Raman scattering in producing these features is investigated. The scattering medium is a plasma whose position, density and temperature decide the rate and angle of scattering. When the radiation from a stationary and constant source gets scattered from a stationary plasma, a halo is formed around the source. However, the scattering of a rotating radiation beam does produce superluminal motion of the virtual source. It is found that the plasma should have the characteristics of the emission-line regions and the intercloud medium in order to Raman scatter the radiation. Since the scattering is polarization dependent, it is possible to estimate the rotation of the electric vector along the direction of the apparent motion of a radio source.     

The Ensemble Kalman Filter: theoretical formulation and practical implementation

The purpose of this paper is to provide a comprehensive presentation and interpretation of the Ensemble Kalman Filter (EnKF) and its numerical implementation. The EnKF has a large user group, and numerous publications have discussed applications and theoretical aspects of it. This paper reviews the important results from these studies and also presents new ideas and alternative interpretations which further explain the success of the EnKF. In addition to providing the theoretical framework needed for using the EnKF, there is also a focus on the algorithmic formulation and optimal numerical implementation. A program listing is given for some of the key subroutines. The paper also touches upon specific issues such as the use of nonlinear measurements, in situ profiles of temperature and salinity, and data which are available with high frequency in time. An ensemble based optimal interpolation (EnOI) scheme is presented as a cost-effective approach which may serve as an alternative to the EnKF in some applications. A fairly extensive discussion is devoted to the use of time correlated model errors and the estimation of model bias.Responsible Editor: Jörg-Olaf Wolff     

全国天气雷达数据处理系统

根据《全国天气雷达终端更新》和《全国天气雷达定标》项目的技术规定,研制了一套完整的雷达业务数据处理系统,实现了全国布网天气雷达数据格式统一、产品生成、产品分发和图像回显的全自动化业务,提高了我国天气雷达网的业务质量、以及数据处理和产品应用水平,收效显著。在研发过程中,充分考虑了业务条件、实际要求和探测技术的发展,系统功能丰富,算法先进,接口开放,设计精美,投入业务两年来系统运行稳定。该系统放弃了传统对话框和工具栏的设计方式,创新设计了操作面板控制。文中的研发思路,设计方法,系统特点对我国业务软件的研制具有很好的借鉴作用。     

X-ray emission from accretion disks in active galactic nuclei

We constructed a grid of relativistic models for standard high-relative-luminosity accretion α-disks around supermassive Kerr black holes (BHs) and computed X-ray spectra for their hot, effectively optically thin inner parts by taking into account general-relativity effects. They are known to be heated to high (～10⁶–10⁹ K) temperatures and to cool down through the Comptonization of intrinsic thermal radiation. Their spectra are power laws with an exponential cutoff at high energies; i.e., they have the same shape as those observed in active galactic nuclei (AGNs). Fitting the observed X-ray spectra of AGNs with computed spectra allowed us to estimate the fundamental parameters of BHs (their mass and Kerr parameter) and accretion disks (luminosity and inclination to the line of sight) in 28 AGNs. We show that the Kerr parameter for BHs in AGNs is close to unity and that the disk inclination correlates with the Seyfert type of AGN, in accordance with the unification model of activity. The estimated BH masses M_x are compared with the masses M_rev determined by the reverberation mapping technique. For AGNs with luminosities close to the Eddington limit, these masses agree and the model under consideration may be valid for them. For low-relative-luminosity AGNs, the differences in masses increase with decreasing relative luminosity and their X-ray emission cannot be explained by this model.     

矿山地理信息元数据系统设计

分析了在矿山地理信息系统中引入元数据的重要性和可行性,然后采用建模技术,设计并实现了矿山地理信息元数据标准原型,并给出了矿山地理信息元数据系统的基本架构。     

Excel在约旦18号死海海堤沉降监测中的应用

通过死海南端约旦18号海堤的沉降监测实例,总结了用Microsoft Excel在国外进行沉降监测资料整理的方法和体会,并较为全面地介绍了各类图表的意义,这些方法可在类似的监测工作中予以借鉴。     

基于AutoCAD二次开发的矢量地形数据检查

基于CAD的矢量地形数据是一类基本的重要的基础地理数据，其应用十分广泛，同时也是各类地理信息系统重要的数据源，其属性精度、逻辑一致性是其重要质量元素，本文论述了基于AuotoCAD二次开发实现矢量地形数据计算机自动化高效检查的技术方法。     

关于建设省级地理空间数据交换中心的思考

省级地理空间数据交换中心是国家空间信息基础设施建设的核心内容之一。本文针对现阶段在我国建设省级地理空间数据交换中心的问题，分析了其基本建设内容，提出了需解决和应用的关键技术。     

利用IRS-P6卫星数据制作遥感影像地图

本文介绍了以IRS-P6卫星数据作为信息源完成大兴安岭林区的遥感影像地图制作的方法, 通过试验初步认识到:利用IRS-P6卫星数据制作遥感影像地图,可以满足1:50000、 1:25000比例尺的平面制图精度要求,在一些专业和专题应用中可以放大到1:15000比例尺使用。