小卫星高分辨率成像系统

对小卫星对地观测高分辨率成像系统进行了综述。介绍了国内外有极高分辨率（0．5～1．0m）、高分辨率（1．8～2．5m）和中高分辨率（4-10m）小卫星光学成像系统的性能,并与合成孔径雷达（SAR）成像系统进行了比较。给出了小卫星光学成像系统、SAR高分辨率成像系统和卫星平台的关键技术。讨论了未来小卫星及其高分辨率成像系统技术的发展趋势。     

卫星导航系统及其在空天安全中的重要作用

简要介绍了美国"全球定位系统"(GPS)、俄罗斯"全球导航卫星系统"(GLONASS)和欧洲正在建设的"伽利略"(Galileo)卫星导航系统的发展及其基本发展态势.详细介绍了中国自主建设的"北斗"(COMPASS)卫星导航系统的发展思路、系统组成和应用情况.分析总结了卫星导航系统在空天安全中的几项重要作用,如实现协同...     

平台惯导系统飞行试验性能误差分析

针对某型平台式惯导系统试飞中存在的性能超差现象,对惯导系统误差机理和飞行数据进行了分析,提出了影响飞行性能的误差因素。根据分析结果,从提高惯性元件精度和对相关误差进行标定和补偿两方面采取措施对惯导系统进行改进。改进后的惯导系统经过试飞验证,其性能满足设计指标,表明所采取的改进措施有效可行。     

基于结构不确定性的非线性鲁棒制导律设计

根据多普勒雷达导引头和红外成像导引头多模制导导弹弹道中段制导信息精度的特点,以非线性鲁棒控制理论为依据,设计了一种制导律.仿真结果表明,该制导律对弹目相对距离测量干扰有较好的鲁棒性,对目标大机动也有鲁棒性.因此,这种制导律可以作为多普勒雷达导引头和红外成像导引头多模制导导弹弹道中段的制导律使用.     

一种弹目遭遇点预测方法

为充分利用舰空导弹中制导段所获信息并减小导弹中制导段的弹道曲率,给出一种弹目预测遭遇点的解算方法,并据此设计比例导引制导律。在初始发射坐标系中,假设目标由当前位置以当前速度大小沿当前速度方向匀速运动至遭遇点,导弹由当前位置以当前速度大小按照一定的导引规律匀速运动至遭遇点。在该假设条件下,导弹到达遭遇点的总航路大小一方面...     

水下重力辅助惯性导航关键技术研究及实现

重力辅助惯性导航已渐成水下导航领域的研究热点,其实现是一项复杂的工程,涉及多项的关键技术.文章首先介绍了重力辅助导航的基本原理;之后详细阐述了在真实海洋环境下,重力辅助导航所需解决的若干关键技术问题,并给出了相应的研究成果;最后总结了我国水下重力辅助导航的发展趋势及研究的若干建议.     

Feasibility of performing space surveillance tasks with a proposed space-based optical architecture

Under ESA contract an industrial consortium including Aboa Space Research Oy (ASRO), the Astronomical Institute of the University of Bern (AIUB), and the Dutch National Aerospace Laboratory (NLR), proposed the observation concept, developed a suitable sensor architecture, and assessed the performance of a space-based optical (SBO) telescope in 2005. The goal of the SBO study was to analyse how the existing knowledge gap in the space debris population in the millimetre and centimetre regime may be closed by means of a passive optical instrument. The SBO instrument was requested to provide statistical information on the space debris population in terms of number of objects and size distribution. The SBO instrument was considered to be a cost-efficient with 20 cm aperture and 6° field-of-view and having flexible integration requirements. It should be possible to integrate the SBO instrument easily as a secondary payload on satellites launched into low-Earth orbits (LEO), or into geostationary orbit (GEO). Thus the selected mission concept only allowed for fix-mounted telescopes, and the pointing direction could be requested freely. Since 2007 ESA focuses space surveillance and tracking activities in the Space Situational Awareness (SSA) preparatory program. Ground-based radars and optical telescopes are studied for the build-up and maintenance of a catalogue of objects. In this paper we analyse how the proposed SBO architecture could contribute to the space surveillance tasks survey and tracking. We assume that the SBO instrumentation is placed into a circular sun-synchronous orbit at 800 km altitude. We discuss the observation conditions of objects at higher altitude, and select an orbit close to the terminator plane. A pointing of the sensor orthogonal to the orbital plane with optimal elevation slightly in positive direction (0° and +5°) is found optimal for accessing the entire GEO regime within one day, implying a very good coverage of controlled objects in GEO, too. Simulations using ESA’s Program for Radar and Optical Observation Forecasting (PROOF) in the version 2005 and a GEO reference population extracted from DISCOS revealed that the proposed pointing scenario provides low phase angles together with low angular velocities of the objects crossing the field-of-view. Radiometric simulations show that the optimal exposure time is 1–2 s, and that spherical objects in GEO with a diameter of below 1 m can be detected. The GEO population can be covered under proper illumination nearly completely, but seasonal drops of the coverage are possible. Subsequent observations of objects are on average at least every 1.5 days, not exceeding 3 days at maximum. A single observation arc spans 3° to 5° on average. Using a simulation environment that connects PROOF to AIUB’s program system CelMech we verify the consistency of the initial orbit determination for five selected test objects on subsequent days as a function of realistic astrometric noise levels. The initial orbit determination is possible. We define requirements for a correlator process essential for catalogue build-up and maintenance. Each single observation should provide an astrometric accuracy of at least 1”–1.5” so that the initially determined orbits are consistent within a few hundred kilometres for the semi-major axis, 0.01 for the eccentricity, and 0.1° for the inclination.     

卫星导航系统天线阵接收机波束指向误差分析

研究表明：卫星导航系统阵元几何位置误差是影响波束指向误差的主要因素,而卫星和接收机位置误差则影响甚微,其中千米级的卫星位置误差以及接收机位置误差导致的波束指向误差不超过0.1°,而毫米级的阵元几何位置随机误差可导致典型7阵元天线阵波束指向误差达到几度。该研究成果可为卫星导航系统天线阵接收机的设计提供依据。     

长焦距同轴三反空间相机光学系统研究

为了满足空间遥感不同应用的需求,完成了4种型式的长焦距同轴三反光学系统设计。根据同轴三反光学系统设计理论,介绍了同轴三反光学系统设计初始结构设计方法,以工作谱段0．45-0．9μm、F数10、焦距10m为例,对4种型式的长焦距同轴三反光学系统进行优化设计,设计视场内获得接近衍射极限的成像品质,并分析和比较了这几种光学系...     

天问一号探测器高动态着陆惯导系统设计与试验

考虑到火星探测任务着陆过程动态变化大,稀薄大气环境下开伞会对探测器产生剧烈晃动,为此天问一号探测器研制了一套高动态着陆惯导系统,从硬件产品、使用时序到导航算法方面均进行了针对性设计,以适应着陆过程中的高动态环境.此外,为验证天问一号探测器高动态着陆惯导系统的性能,设计了模拟火星开伞工况的火箭弹高空开伞试验,结果表明该高...