Optimization method for large-aperture space mirror's gravity unload

被引:0
|
作者
Sun Y. [1 ]
Luo S. [1 ]
Gao C. [1 ]
Chen F. [1 ]
Zong X. [1 ]
Du J. [1 ]
Liu Z. [1 ]
Bai J. [1 ]
机构
[1] Beijing Institute of Space Mechanics and Electricity, Beijing
关键词
Gravity unload; Large aperture; Space mirror; Surface figure optimization;
D O I
10.3788/IRLA20200103
中图分类号
学科分类号
摘要
A Φ1550 mm aperture space mirror's surface figure RMS was required to be superior to 1/50λ (λ=632.8 nm) under the zero-gravity orbit environment. In order to simulate the state of weightlessness and reduce the influence of gravity in the mirror's surface figure test with horizontal optic axis, the mirror was actively supported by multiple forces to unload the gravity and the forces' parameters were optimized. Firstly, the principle to determine the value, the number of support points and the initial axial position of each unload force was proposed based on dividing the mirror into blocks. Secondly, with the optimization goal of the mirror's surface figure RMS be superior to 0.002λ under the function of gravity along with all unload forces, a structural FEM model was established. Taking the positions of all unload forces along the optic axis as optimal variables, influences on target were analyzed and quick optimization points were concluded to simplify the optimization. Finally, the mirror's surface figure RMS when unloaded was found minimal of 0.00145λ. Putting the parameters of the optimization result into use of the surface figure test of the mirror with horizontal optic axis, it turned out that when the mirror revolved around the optic axis 0°, 120° and 240°, the surface figure RMS were 0.0157λ, 0.0161λ and 0.0159λ respectively and the figures were consistent, which proved that the gravity impact was eliminated effectively. The optimization method for gravity unload is flexible and efficient which guarantee the large-aperture mirror's high-precision machining and space mission. Copyright ©2021 Infrared and Laser Engineering. All rights reserved.
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  • [1] Lu Gang, Gao Lei, Wang Yanmin, Evaluation and analysis on multiple fusion methods for GJ-1 satellite imagery, Remote Sensing Information, 33, 6, pp. 124-131, (2018)
  • [2] Xu Wei, Jin Guang, Wang Jiaqi, Optical imaging technology of JL-1 lightweight high resolution multispectral remote sensing satellite, Optics and Precision Engineering, 25, 8, pp. 1969-1978, (2017)
  • [3] Wang Xiaoyong, Zhang Bowen, Guo Chongling, Et al., Parameter optimization of 3 m aperture space- based mirror, Infrared and Laser Engineering, 48, S1, (2019)
  • [4] Li Shenhua, Guan Yingjun, Xin Hongwei, Et al., Lightweight design and flexible support of large diameter mirror in space camera, Laser and Infrared, 47, 11, pp. 1422-1427, (2017)
  • [5] Dong Deyi, Pang Xinyuan, Zhang Xuejun, Et al., Key technology in developing of metrology mount for large aperture monolithic space-based mirror, Optics and Precision Engineering, 27, 10, pp. 2165-2179, (2019)
  • [6] Wang Kejun, Dong Jihong, Structural design of Φ2m-level large-diameter SiC reflector used in space remote sensor, Infrared and Laser Engineering, 46, 7, (2017)
  • [7] Guo Jiang, Zhu Lei, Zhao Ji, Et al., Design and optimize of high tolerance support structure for large aperture space mirror, Optics and Precision Engineering, 27, 5, pp. 1138-1147, (2019)
  • [8] Montagino L A., Test and evaluation of the Hubble Space Telescope 2.4-meter primary mirror, 571, pp. 182-190, (1985)
  • [9] Besuner R W, Chow K P, Kendrick S E., Selective reinforcement of a 2 m-class lightweight mirror for horizontal beam optical testing, 7018, (2008)
  • [10] Takao N, Hiroshi S, Takashi O, Et al., The next-generation infrared astronomy mission SPICA under the new framework, 9143, (2014)