• CN:11-2187/TH
  • ISSN:0577-6686

机械工程学报 ›› 2020, Vol. 56 ›› Issue (11): 151-160.doi: 10.3901/JME.2020.11.151

• 机械动力学 • 上一篇    下一篇

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飞轮扰动下大口径长焦距光学成像系统的视轴误差的分析与试验

刘瑞婧1,2, 金光1, 郭金生3, 李叶文1,2, 李宗轩1   

  1. 1. 中国科学院大学长春光学精密机械与物理研究所 长春 130033;
    2. 中国科学院大学 北京 100039;
    3. 哈尔滨工业大学卫星技术研究所 哈尔滨 150001
  • 收稿日期:2019-07-09 修回日期:2019-09-29 出版日期:2020-06-05 发布日期:2020-06-12
  • 通讯作者: 李宗轩(通信作者),男,1986年出生,博士,副研究员。主要研究方向为空间光学仪器设计与集成分析。E-mail:lizongx@126.com
  • 作者简介:刘瑞婧,女,1994年出生,博士研究生。主要研究方向为微振动的光机集成分析。E-mail:1418444530@qq.com
  • 基金资助:
    国家科技重大专项(2016YFB0501202)和吉林省科技发展计划(20180414066GH)资助项目。

Analysis and Test of Line-of-sight Error of Large-aperture Long Focal Length Optical Imaging System under Reaction wheel Disturbance

LIU Ruijing1,2, JIN Guang1, GUO Jinsheng3, LI Yewen1,2, LI Zongxuan1   

  1. 1. Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130033;
    2. University of Chinese Academy of Sciences, Beijing 100039;
    3. Research Center of Satellite Technology, Harbin Institute of Tech, Harbin 150001
  • Received:2019-07-09 Revised:2019-09-29 Online:2020-06-05 Published:2020-06-12

摘要: 为了分析飞轮产生的微振动对高分辨率卫星成像质量的影响,建立了某高分辨率卫星的结构动力学模型,测量飞轮在轨工作时产生的微振动,并基于整星层次计算卫星在飞轮扰动下视轴误差。计算结果表明该高分辨率卫星光学成像系统的视轴误差的关键模态为第8与9阶模态,主镜与次镜对视轴误差贡献最大,可以优化主镜与次镜相关结构参数提高光学卫星的成像质量。为验证整星结构设计与微振动分析优化的准确性与合理性,针对整星初样开展地面微振动试验,该卫星在轨姿控系统为偏置动量轮设计,通过星上Z/Y轴动量轮模拟在轨实际工作转速,分别在卫星悬吊状态以及固支状态下测量了卫星颤振情况。分析与试验结果表明:整星微振动时角位移的仿真计算结果与试验结果相比,其相对误差α为11.13%,绝对值为0.009 94″,小于0.01″,初步认为在轨遥感图像质量不会受微振动影响而退化,并为光学遥感卫星的微振动设计提供了参考。

关键词: 微振动, 飞轮, 遥感卫星, 结构动力学, 视轴误差

Abstract: In order to analyze the influence of the jitter on the high resolution satellites’ imaging quality, which is generated by the reaction wheel, a structural dynamic model is established to simulate the jitter effect of a high-resolution satellite on orbit. In addition, the line-of-sight (LOS) error of the optical imaging system is calculated under disturbance. The calculation results show that the critical modes of the LOS error are the 8th and 9th mode, respectively. Besides, the LOS error is deteriorated by the primary and second mirror to the largest extent, whose structural parameters can be optimized to improve the imaging quality of the satellite. To verify the accuracy and rationality of the structural design of the satellite as well as the optimization process of the jittering, an on-ground jitter simulation is performed on the prototype of the satellite, whose attitude control system is designed with the offset momentum. The actual on-orbit speed is simulated by the Z/Y axis reaction wheel on the satellite, and then the jitter is obtained when the prototype is under suspended and fixed boundary conditions, respectively. Finally, we can make a comparison between the calculation and simulation results of the angular displacement of the satellite’s jitter, and it indicates that the relative error α is 11.13%, and the absolute value is 0.009 94 arcsecond. With a value less than 0.01 arcsecond, we can safely draw a conclusion that the imaging quality of the remote sensing camera is not degraded by jitter. This paper provides a reference for the jitter design of the optical remote sensing satellites.

Key words: jitter, reaction wheel, remote sensing satellite, structural dynamics, line-of-sight error

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