空间技术系统的讨论

从社会需求出发和以满足空间任务目标的角度, 依据一般系统论的原则, 提出了建立空间技术系统的新概念。将空间技术系统划分为航天器进入空间技术、空间功能运用技术、空间防护技术和空间武器技术四大分系统组成的技术系统, 这有别于以发展运载器和航天器为主要目标而建立的空间技术系统体系     

空间遥感器热光学分析的研究与应用

论述空间遥感器热光学分析与应用现状及其发展趋势;分析当前遥感器热光学分析的意义,认为这是提高长寿命遥感器可靠性的一种重要手段;针对某长寿命遥感相机,提出进行热光学分析研究的总体方案、具体实施途径、技术关键和解决方法。     

卫星磁层亚暴环境模拟试验设备的设计

卫星表面充电是七十年代初发现的严重危害同步轨道卫星的新问题。为了寻求解决卫星表面充电问题的方法,许多国家进行了广泛的研究。我们于82年开展卫星表面充电模拟试验技术研究。本文仅就我们在磁层亚暴环境模拟设备设计中考虑的一些问题作简要介绍。阐述了对模拟系统的要求,模拟系统的组成和用途,介绍了真空系统,电子枪,光源和测量系统设计中应考虑的问题。     

可重复使用空间往返运输系统的最新发展

可重复使用的空间往返运输系统具有广泛的军事用途和商业应用前景 ,因此成为各国争相发展的目标。本文简要介绍了世界主要航天国家在重复使用运输系统方面的发展情况、技术特点和发展趋势     

Space-radiation-induced photon luminescence of the Moon

We report on the results of a continuing study of the photon luminescence of the Moon induced by Galactic Cosmic Rays (GCRs) and space radiation from the Sun, using the Monte Carlo program FLUKA. Understanding the space radiation environment is critical to future exploration of the Moon, and this includes photons. The model of the lunar surface is taken to be the chemical composition of soils found at various landing sites during the Apollo and Luna programs, averaged over all such sites to define a generic regolith for the present analysis. This surface model then becomes the target that is bombarded by Galactic Cosmic Rays (GCRs) and Solar Energetic Particles (SEPs) or Solar Particle Events (SPEs) above 1 keV in FLUKA to determine the photon fluence albedo produced by the Moon’s surface when there is no sunlight and Earthshine. The result is to be distinguished from the gamma-ray spectrum produced by the radioactive decay of radiogenic constituents lying in the surface and interior of the Moon. From the photon fluence we derive the spectrum which can be utilized to examine existing lunar spectral data and to aid future orbiting instrumentation in the measurement of various components of the space-radiation-induced photon luminescence present on the Moon.     

Debris area distribution of spacecraft under hypervelocity impact

Cross-sectional area is an important parameter for spacecraft breakup debris as it is the directly measured data in space observation. It is significant for observing and analysing the spacecraft breakup event to accurately modelling the area distribution of the breakup debris. In this paper, experimental study has been performed on debris area distribution characteristics of spacecraft under hypervelocity impact. The tests are carried out at the ballistic ranges of CARDC. Aluminium projectiles are launched to normally impact the simulated spacecrafts at about 3.0 km/s. The simulated spacecrafts are made up of aluminium plates, filled with some simulated electronics boxes, each of which was installed with a circuit board. “Soft-catch” devices are used to recover the breakup fragments. The test results show that: 1) the relationship between the cross-sectional area and the characteristic length of debris, which can be obtained in the logarithmic coordinates by linear fitting, represents the debris shape characteristic in a certain extent; 2) the area-to-mass ratios of fragments show normal distributions in the logarithmic coordinates; 3) debris made of different materials can be distinguished by different peaks on the distribution curves; 4) the area-to-mass ratio distributions can be expressed by a linear superimposition of several normal functions which represent the main materials of the spacecraft.     

大气层内动能拦截弹直接力/气动力复合控制

以大气层内拦截弹气动力和力矩式侧向直接力复合控制系统为研究对象,基于参考模型变结构控制理论设计了拦截弹末制导段复合控制系统,并研究了相应的控制力分配算法、脉冲发动机组调度算法。数学仿真结果表明,该复合控制方法可以很好地实现拦截弹姿态控制。与气动力系统相比,复合控制系统具有更好的动态性能。     

弹道导弹中段监视与跟踪仿真系统设计

随着反导防御系统的发展,弹道导弹突防将受到更大的威胁,而弹道导弹中段是攻防对抗集中体现的区域。本文以美国的天基红外预警系统为参考,对弹道导弹中段监视与跟踪仿真系统进行了研究,提出了仿真系统的体系结构,并对仿真模型的具体实现进行了详细的描述。系统的建立可为弹道导弹作战模拟提供研究平台,并可对面向空间预警的信息处理算法进行评估,为中段反导作战的具体影响提供有益的参考信息。     

"十一五"规划期间中国航天发射数量预测

根据截至2006年的与中国卫星相关的中国航天发射数量的统计值,主要应用灰色系统理论预测了“十一五”规划期间(2006~2010年)中国航天器的发射数量和相关的中国航天运载火箭的发射数量。     

基于Space radiation 5.0软件平台分析典型GEO空间辐射环境

文章介绍了兰州空间技术物理研究所真空低温技术与物理国家重点实验室从美国引进的空间辐射环境及效应分析软件Space Radiation 5.0的结构功能模块,采用该软件计算分析了典型的GEO（地球同步轨道）空间辐射环境。计算表明:GEO的总剂量效应比较严重,主要是由捕获电子和太阳耀斑质子辐射引起的;GEO的带电粒子主要由质子、α粒子、碳离子、氮离子、氧离子等重核离子组成,此轨道上的单粒子效应主要由太阳宇宙射线中的高能质子和重离子以及银河宇宙射线的重离子引发。