Volume 48 Issue 5
May  2019
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Liu Xiangyi, Wang Fuguo, Zhang Jingxu, Fan Lei, Wang Wenpan. Study on moment correction method of primary mirror semi-active support[J]. Infrared and Laser Engineering, 2019, 48(5): 518003-0518003(8). doi: 10.3788/IRLA201948.0518003
Citation: Liu Xiangyi, Wang Fuguo, Zhang Jingxu, Fan Lei, Wang Wenpan. Study on moment correction method of primary mirror semi-active support[J]. Infrared and Laser Engineering, 2019, 48(5): 518003-0518003(8). doi: 10.3788/IRLA201948.0518003

Study on moment correction method of primary mirror semi-active support

doi: 10.3788/IRLA201948.0518003
  • Received Date: 2018-12-09
  • Rev Recd Date: 2019-01-20
  • Publish Date: 2019-05-25
  • In the development of large ground-based telescope technology, the primary mirror support technology is always a key technology. In this paper, a semi-active support method was researched based on a 2 m SiC lightweight primary mirror, which was used to correct some unpredictable low-order wavefront aberration caused by machining error, assembly error and other factors. Firstly, the finite element simulation model was established, and the finite element simulation was carried out. An unit correction moment (1 Nmm) of Mx or My, which were two orthogonal moments, was separately applied to the 6 Tripod soft hinge, so the primary mirror deformations under a total of 12 cases of the situation were respectively analyzed. And then with the linear superposition principle of small deformation, the correction ability of the moment correction method for low order wavefront aberration was analyzed and calculated. It could be seen from the analysis that the moment correction method could correct the tilt and astigmatism very well. The initial mirror RMS value of the tilt and initial astigmatism which were normalized to 1/10(=632.8 nm), could be respectively corrected to 0.687 nm and 2.97 nm, the correction abilities were respectively 98.9% and 95.3%, and the required maximum correction moments were respectively 6.3 Nmm and 19.9 Nmm. Then, according to the whiffletree support structure of the primary mirror, a structure of the moment correction was designed with the leaf spring at the Tripod soft hinge. Finally, the feasibility of the leaf spring correction structure was verified through experiments, and the feasibility of the semi-active support scheme of moment correction was verified further. And a certain degree of engineering experience for the implementation of the moment correction method has been accumulated with high guiding significance.
  • [1] Bely P. The Design and Construction of Large Optical Telescopes[M]. New York:Springer, 2003.
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    [3] Cheng Jingquan. Principles of Astronomical telescope Design[M]. Beijing:China Science Technology Press, 2003. (in Chinese)程景全. 天文望远镜原理和设计[M]. 北京:中国科学技术出版社, 2003.
    [4] Wang Fuguo, Wu Xiaoxia, Shao Liang, et al. Review of foreign ground-based telescope primary mirror support[J]. Laser Infrared, 2012, 42(3):237-243. (in Chinese)王富国, 吴小霞, 邵亮,等. 国外大型地基望远镜主镜支撑综述[J]. 激光与红外, 2012, 42(3):237-243.
    [5] Shao Liang, Wu Xiaoxia, Chen Baogang, et al. Passive support system of light-weighted SiC primary mirror[J]. Opt Precision Eng, 2015, 23(5):1380-1386. (in Chinese)邵亮, 吴小霞, 陈宝刚,等. SiC轻量化主镜的被动支撑系统[J]. 光学精密工程, 2015, 23(5):1380-1386.
    [6] Neufeld C, Sarnik A, Sebring T A, et al. Development of an active optical system for the SOAR telescope[C]//SPIE, 2004, 5489:1052-1060.
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    [8] Kimbrell J E, Greenwald D. AEOS 3.67 m telescope primary mirror active control system[C]//SPIE, 1998, 3352(4):506-507.
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Study on moment correction method of primary mirror semi-active support

doi: 10.3788/IRLA201948.0518003
  • 1. Changchun Institute of Optics,Fine Mechanics and Physics,Chinese Academy of Sciences,Changchun 130033,China

Abstract: In the development of large ground-based telescope technology, the primary mirror support technology is always a key technology. In this paper, a semi-active support method was researched based on a 2 m SiC lightweight primary mirror, which was used to correct some unpredictable low-order wavefront aberration caused by machining error, assembly error and other factors. Firstly, the finite element simulation model was established, and the finite element simulation was carried out. An unit correction moment (1 Nmm) of Mx or My, which were two orthogonal moments, was separately applied to the 6 Tripod soft hinge, so the primary mirror deformations under a total of 12 cases of the situation were respectively analyzed. And then with the linear superposition principle of small deformation, the correction ability of the moment correction method for low order wavefront aberration was analyzed and calculated. It could be seen from the analysis that the moment correction method could correct the tilt and astigmatism very well. The initial mirror RMS value of the tilt and initial astigmatism which were normalized to 1/10(=632.8 nm), could be respectively corrected to 0.687 nm and 2.97 nm, the correction abilities were respectively 98.9% and 95.3%, and the required maximum correction moments were respectively 6.3 Nmm and 19.9 Nmm. Then, according to the whiffletree support structure of the primary mirror, a structure of the moment correction was designed with the leaf spring at the Tripod soft hinge. Finally, the feasibility of the leaf spring correction structure was verified through experiments, and the feasibility of the semi-active support scheme of moment correction was verified further. And a certain degree of engineering experience for the implementation of the moment correction method has been accumulated with high guiding significance.

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