在浏览器中平滑调用MICAPS系统

介绍了通过安装，配置Web服务器软件并编写CGI程序实现在浏览器中平滑调用MICAPS系统的方法，指出融合因特网技术是进行新一代MICAPS系统和天气预报业务平台设计开发的必同之路。     

基于VML的IE绘图软件的设计与实现

就当前获取VML格式数据源难的现状,采用IE内嵌的VML解析器,结合JavaScript+DOM技术,在IE的界面上成功实现了能可视化编辑VML格式的图形绘制软件,该软件实现了一般GIS绘图软件的基本功能。它的实现,使得图形数据能够及时动态的在因特网上在线绘制和发布。     

LUNARINFO: A Data Archiving and Retrieving System for the Circumlunar Explorer Based on XML/Web Services

It is essential to build a modern information management system to store and manage data of our circumlunar explorer in order to realize the scientific objectives. It is difficult for an information system based on traditional distributed technology to communicate information and work together among heterogeneous systems in order to meet the new requirement of Internet development. XML and Web Services, because of their open standards and self-containing properties, have changed the mode of information organization and data management. Now they can provide a good solution for building an open, extendable, and compatible information management system, and facilitate interchanging and transferring of data among heterogeneous systems. On the basis of the three-tiered browse/server architectures and the Oracle 9i Database as an information storage platform, we have designed and implemented a data archiving and retrieval system for the circumlunar explorer-LUNARINFO. We have also     

用VML技术构建WebGIS客户端矢量图形的方法研究

在WebGIS中显示矢量数据的关键问题是网络传输。借助VML图形技术,可以很好地解决该问题。本文首先介绍了WebGIS技术的发展现状以及VML的基本要素,然后根据矢量图形类型和VML要素的自身特点,提出基于VML图形技术的点、线和面矢量数据的浏览器端实现方法。结合背景图层,该方式可以在WebGIS中得到充分地应用。特别是对于构建专业的网络图形服务具有一定的借鉴作用。     

Effects of topographic–isostatic masses on gravitational functionals at the Earth’s surface and at airborne and satellite altitudes

Topographic–isostatic masses represent an important source of gravity field information, especially in the high-frequency band, even if the detailed mass-density distribution inside the topographic masses is unknown. If this information is used within a remove-restore procedure, then the instability problems in downward continuation of gravity observations from aircraft or satellite altitudes can be reduced. In this article, integral formulae are derived for determination of gravitational effects of topographic–isostatic masses on the first- and second-order derivatives of the gravitational potential for three topographic–isostatic models. The application of these formulas is useful for airborne gravimetry/gradiometry and satellite gravity gradiometry. The formulas are presented in spherical approximation by separating the 3D integration in an analytical integration in the radial direction and 2D integration over the mean sphere. Therefore, spherical volume elements can be considered as being approximated by mass-lines located at the centre of the discretization compartments (the mass of the tesseroid is condensed mathematically along its vertical axis). The errors of this approximation are investigated for the second-order derivatives of the topographic–isostatic gravitational potential in the vicinity of the Earth’s surface. The formulas are then applied to various scenarios of airborne gravimetry/gradiometry and satellite gradiometry. The components of the gravitational vector at aircraft altitudes of 4 and 10 km have been determined, as well as the gravitational tensor components at a satellite altitude of 250 km envisaged for the forthcoming GOCE (gravity field and steady-state ocean-circulation explorer) mission. The numerical computations are based on digital elevation models with a 5-arc-minute resolution for satellite gravity gradiometry and 1-arc-minute resolution for airborne gravity/gradiometry.     

环月卫星可见时段的计算和分析

根据"嫦娥一1"的探测任务特点,其将在绕月段运行至少1年,本文主要讨论了这个阶段内环月卫星的可见时段及地面站的布设问题。文中阐述了可见时段的计算原理,对两种不同的地面站(局域和全球)布设方式进行了仿真计算。结果表明,全球布站较局域布站对环月卫星的可见时段明显增长,便于对环月卫星进行测控。     

火星探测器着陆区地貌环境特征初释

2个火星探测器着陆区均为平原地貌, 但形态特征、物质结构和动力过程都有明显差异。勇士号着陆区主要为风蚀区,而机遇号着陆区主要为风积区;前者为板状砾质平原,后者是基岩出露的波状砂质平原。可能常年有主风向,它们属于无表水环境下极干旱的风成地貌,缺少融冻过程,风化速度远低于地球环境。地貌结构与物质都证明,火星过去曾有液态水存在。限于着陆区环境及探测器功能,如果水存在于地下深部,这两个探测器很难发现。     

我国Argo浮标的设计与研究

自沉浮式剖面探测浮标是一种海洋观测平台,首先应用在国际Argo计划,故又称之为Argo浮标,专用于海洋次表层温、盐、深剖面测量。仪器布放后自行在大海中工作2a以上,直至电源耗尽;2004年11月8日实验的Argo浮标潜入深度已达到1900m,历时两年的浮标研究工作,在下潜深度、上浮水面、剖面测量、数据处理、卫星传递数据等功能上已经达到国际Argo组织的要求。文章详细阐述了剖面浮标的设计与研制内容和各种试验项目及所得数据,不仅为浮标设计提供科学的实测数据,还为今后该仪器产品化进程提供大量可靠依据和检测方法。