三维数字地形图生成技术研究

在论述三维真实感数字地形图生成算法的基础上,结合数字高程模型(DTM)数据,用OpenGL在计算机上实现三维数字地形图的显示。     

Modelling the Torques Affecting the Hipparcos Satellite

Reconstructed attitude data for the Hipparcos mission as obtained in the final stages of the data analysis for the published catalogue is used to derive detailed information on the dynamics of the satellite. Most elements of the inertia tensor of the satellite could be calibrated from the observed acceleration data, which are also used to reconstruct torques due to solar radiation and gravity gradient, and the magnetic moment of the satellite and it's interaction with the magnetic field surounding the Earth. The effects of the oblateness of the Earth on the gravity gradient are evaluated and shown to be negligable. The magnetic field model includes both the `main' and the `disturbance' fields. The remaining systematic effects in residual torques are most likely attributed to variations in the magnetic field that are local and are beyond the models used to describe it. The angular momentum vector for one of the gyros was reconstructed from the torque it asserted on the satellite while it was running in redundant mode. This revised version was published online in August 2006 with corrections to the Cover Date.     

基于空中发射点的在线诸元计算方法研究

现代战争的快节奏要求弹道导弹具有快速机动发射能力,采用伪卫星组合制导的弹道导弹随机快速发射需要诸元在线计算。提出了一种基于空中发射点的在线诸元计算方法,该方法具有计算量小、制导方法误差小的特点,可用于陆基机动弹道导弹或潜射弹道导弹的快速发射。     

空间推进系统的故障推理研究

空间推进系统必须可靠地完成轨道保持、轨道修正、姿态控制的重要任务 ,要求当其某一功能模块出现故障时、能及时发现并有效隔离。文中介绍了利用有向图方法分析此推进系统故障传播机理的方法 ,并建立相应的故障推理模型。离线检测和理论分析表明 ,此方法逻辑性强 ,简单高效 ,具有空间实时应用的可能性     

A Brief Introduction and Recent Progress of the Geospace Double Star Program

The Geospace Double Star Project (DSP) consists of two small satellites operating in the near-earth equatorial and polar regions, respectively. The goals of DSP are: (1) to provide high-resolution field, particle, and wave measurements in some important near-earth active regions which have not been covered by current ISTP missions, such as the near-earth plasma sheet and its boundary layer, the ring current, the radiation belts, the dayside magnetopause boundary layer, and the polar region; (2) to investigate the trigger mechanisms of magnetic storms, magnetospheric substorms, and magnetospheric particle events,as well as the responses of geospace storms to solar activities and interplanetary disturbances; (3) to set up the models describing the spatial and temporal variations of the near-earth space environment.To realize the above goals, the equatorial satellite TC-1 and the polar satellite TC-2 will accommodate, respectively, eight instruments on board. TC-1was launched successfully in December 2003 while the polar satellite (TC-2)will be launched in July 2004. The orbit of the equatorial satellite TC-1 consists of a perigee at 550 km, an apogee at 60 000 km, and an inclination of about 28.5; while the orbit of the polar satellite will have a perigee of 700 km, an apogee of 40 000 km, and an inclination of about 90. The two satellites will take coordinated measurements with Cluster Ⅱ and will first form a "six-point exploration" in geospace.The operational status of TC-1 are introduced in this paper.     

航天发射用磁悬浮助推发射系统概念研究

针对日益增加的航天发射成本问题和安全、可靠、低成本航天发射方式的需求,阐述了磁悬浮助推发射概念及其优越性.初步分析了磁悬浮助推发射系统组成及各分系统功能.通过比较电磁悬浮(EMS)和超导电动(EDS)两种磁悬浮系统性能,结果表明EDS是更适合于磁悬浮助推发射的磁悬浮系统方案.通过助推发射能量需求初步分析,直线电机加速能量供给系统是难题之一,需要重点解决.采用飞行弹道分析方法,说明地面助推水平起飞单级入轨运载器方案的可行性及特点.与其它航天助推发射方式比较,磁悬浮助推发射在提高入轨载荷和降低发射成本方面具有优势.     

Remote sensing of natural resources : Legal and political considerations for the Third World

A state's posture on remote sensing of the Earth by orbiting satellites varies depending upon whether it is a ‘sensing’ or a ‘sensed’ state, upon its present economic status, and upon its economic and political history. This article considers the international legal questions related to remote sensing and discusses the political aspects with special emphasis upon the views of the Third World. The author concludes that, unless Third World states and others who support them alter their views somewhat, it is probable that remote sensing of natural resources will continue without specific legal guidelines.     

The infrared space observatory (ISO)

The Infrared Space Observatory (ISO), a fully approved and funded project of the European Space Agency (ESA), is an astronomical satellite, which will operate at wavelengths from 2.5–240 m. ISO will provide astronomers with a unique facility of unprecedented sensitivity for a detailed exploration of the universe ranging from objects in the solar system right out to distant extragalactic sources. The satellite essentially consists of a large cryostat containing at launch over 2000 litres of superfluid helium to maintain the Ritchey-Chrétien telescope, the scientific instruments and the optical baffles at temperatures between 2 K and 8 K. The telescope has a 60-cm diameter primary mirror and is diffraction-limited at a wavelength of 5 m. A pointing accuracy of a few arc seconds is provided by a three-axis-stabilisation system consisting of reaction wheels, gyros and optical sensors. ISO's instrument complement consists of four instruments, namely: an imaging photo-polarimeter (2.5–240 m), a camera (2.5–17 m), a short wavelength spectrometer (3–45 m) and a long wavelength spectrometer (43–196 m). These instruments are being built by international consortia of scientific institutes and have been delivered to ESA for in-orbit operations. ISO will be launched in September 1995 by an Ariane 4 into an elliptical orbit (apogee 70000 km and perigee 1000 km) and will be operational for at least 18 months. In keeping with ISO's role as an observatory, the majority of its observing time is being made available to the general astronomical community via a Call for Observing Proposals.     

一种改进的空间目标接近分析快速算法

Alfano-Negron(1993)提出的空间目标接近分析算法将最小相对距离及其对应时刻和进出误差椭球时刻的求解问题均转化为插值多项式求根问题.A-N算法在判断三次多项式根的存在性、筛选合理实根时存在缺陷,可能导致多余计算.由A-N算法提出的准则不能直接计算插值时间步长并可能导致丢根,对此根据多项式插值误差理论提出了一种自适应的插值时间步长选取方法.相比原始A-N算法,完善后的A-N算法计算结果更加可靠.与精确的逐秒比较结果相比,改善后的A-N算法计算速度远高于逐秒比较,具有较高精度,更适合于有实时计算要求的任务.     

基于内窥式PIV的回流燃烧室冷态内流场测量

为了突破传统测量光路限制,实现对航空发动机三头部全尺寸回流燃烧室模型试验件内部冷态流场精细化测量,自主搭建了一套内窥式PIV测量系统,在自模区工况下对其内部冷态流场进行了测量调试。结果表明,在壁面之上预设内窥小孔即可实现测量光路布置,采用大焦距光学适配接口能够很好的解决相机内窥镜成像圈较小的技术难题。通过缩短相机内窥镜工作距离和采取多种消光措施大幅提高了测量空间分辨率和信噪比,最终实现了模型燃烧室内部冷态流场精细化测量,获得了内部流场结构信息。