卫星AIT阶段的静电防护

随着空间技术的不断发展,静电对产品的危害越来越严重。文章在分析了静电和静电放电的产生及其危害的基础上,提出了卫星AIT（Assembly, Integration and Test,装配、总装及试验）阶段的静电防护措施,并据此制订了卫星AIT阶段静电防护具体方案,为卫星AIT阶段的静电防护提供了参考。     

一种卫星机械转动定向天线的研制

机械转动定向天线对提高卫星天线增益和传输速率大有益处。文章介绍了我国嫦娥一号月球探测卫星采用的机械转动定向天线的技术特点、任务要求、系统组成和研制成果。     

软件可靠性的量化问题讨论

在航天器中,随着软件数量的增多,软件可靠性问题日趋尖锐。软件可靠性不能只停留在定性分析阶段,要建立明确的可靠性指标,要通过全任务剖面建立起来的测试用例,对给定软件作长时间的测试和可靠性评价,以便展现软件可靠性不断增长的过程。本文介绍软件可靠性量化的方法,供软件研制者参考。     

卫星流体回路技术的动态热模型与仿真

文章通过合理的分析与简化,建立了一个包括各热组件模型、受控对象模型以及控制系统模型的系统动态热模型,并建立了仿真程序,仿真结果表明:应用这一模型可以十分简便地计算卫星内部热源及空间外热流变化时的单相流体回路系统的温度变化趋势。该动态热模型还可用于对新型控制策略做进一步的研究,指导工程设计。     

基于Lyapunov最小-最大方法的卫星编队飞行队形保持

提出一种卫星编队飞行队形保持的鲁棒控制方法.将环境摄动、推力误差等因素作为干扰项加到相对动力学方程中.然后对于该不确定系统,采用Lyapunov最小一最大方法设计相应的控制律,在存在干扰的情况下,采用该控制律仍然能保证系统渐近稳定.同时针对经典的Lyapunov最小一最大方法导致的控制颤振问题,进行了改进,证明了改进后的控制律能够实现系统的一致终极有界,同时消除颤振.通过仿真,验证了采用Lyapunov最小-最大方法在系统存在干扰的情况下,比一般控制方法具有更强的鲁棒性.     

基于消隐算法的空间结构有效辐射面判断方法研究

空间环境中若投入能量是均匀的,则到达空间结构表面的外热流只与空间结构在投入能量方向上的有效投影面积有关.据此,对空间结构外热流的求解问题将转化为空间结构有效投影面积的求解问题.文章参考图形学的相关算法,提出了一种快速的、具备较高精度的重叠投影区域判断方法,用于辅助空间结构有效投影面积计算.以大型复杂卫星为例,采用该算法...     

MEO卫星太阳电池在轨衰降特性分析

通过MEO卫星在轨遥测数据的统计,从太阳电池阵输出总功率、输出总电流,太阳电池的短路电流、开路电压等方面,对我国发射入轨的第一颗MEO卫星的硅太阳电池阵在轨衰降特性进行了分析,结果表明:输出总功率、总电流与短路电流在第一个周期衰降率较大,开路电压衰降呈线性趋势。文章的分析结果可为后续MEO卫星太阳电池阵设计提供参考。     

一种直接入轨卫星变轨阶段的供电方案

相比传统的卫星自身变轨方式,直接入轨方式下卫星的主动段时间将延长到4～5h。为解决卫星直接入轨过程中由于主动段时间大大加长,导致卫星电能需求的增加,以及电源系统配置不必要的质量增加的问题,文章提出了一种在发射和变轨阶段通过运载火箭上面级向卫星供电的方案,即在上面级上增加了一套独立的一次性电源系统。该系统与卫星自身电源系统相结合,在发射和变轨期间优先使用,卫星自身电源根据负载用电情况自主介入,能很好地解决卫星直接入轨方式下主动段的电能需求问题。     

Robust attitude coordinated control for spacecraft formation with communication delays

In this paper,attitude coordinated tracking control algorithms for multiple spacecraft formation are investigated with consideration of parametric uncertainties,external disturbances,communication delays and actuator saturation.Initially,a sliding mode delay-dependent attitude coordinated controller is proposed under bounded external disturbances.However,neither inertia uncertainty nor actuator constraint has been taken into account.Then,a robust saturated delay dependent attitude coordinated control law is further derived,where uncertainties and external disturbances are handled by Chebyshev neural networks (CNN).In addition,command filter technique is introduced to facilitate the backstepping design procedure,through which actuator saturation problem is solved.Thus the spacecraft in the formation are able to track the reference attitude trajectory even in the presence of time-varying communication delays.Rigorous analysis is presented by using Lyapunov-Krasovskii approach to demonstrate the stability of the closed-loop system under both control algorithms.Finally,the numerical examples are carried out to illustrate the efficiency of the theoretical results.     

The SAX mission

SAX denotes the X-Ray Astronomy Satellite selected by the Italian National Space Plan for inclusion in the Science Programme. The purpose of SAX is to perform spectroscopic, spectral and time variability studies of celestial X-Ray sources in the energy band from 1 to 200 KeV. It is intended to continue and expand upon previous observations of such sources. The instrumentation consists of four X-Ray imaging concentrators sensitive from 1 to 10 KeV (one of them extending down to 0.1 KeV), one Gas Scintillation Proportional Counter sensitive from 3 to 120 KeV, a Sodium Iodide Scintillator Crystal in Phoswich configuration operating from 15 KeV to 200 KeV; these detectors are coaligned to a common pointing axis. Three Wide Field Cameras (2–30 KeV) with axis at 90° to that of the narrow field instruments complete the payload.The Satellite launch is foreseen for 1988, in a low altitude (500 Km), low inclination (12°) orbit.The SAX scientific programme is carried out by a Consortium of Italian Institutes, in cooperation with Institutes from Holland; a partecipation of the Space Science Department of ESA is also foreseen.