Infrared and Laser Engineering, Volume. 46, Issue 8, 818006(2017)

Tuned damping technique for large telescope

Zhao Yongzhi1、*, An Qichang1,2, and Han Xida1
Author Affiliations
  • 1[in Chinese]
  • 2[in Chinese]
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    References(11)

    [1] [1] MacMartin D G, Thompson P, Colavita M M, et al. Dynamic analysis of the active-controlled segmented mirror of the Thirty Meter Telescope[J]. IEEE Trans Control Sys Tech, 2013, 22: 58-68.

    [4] [4] Frank W Kan, Daniel W Eggers. Wind vibration analyses of Giant Magellan Telescope[C]//SPIE, 2006, 6271: 62710Q.

    [7] [7] Sébastien Poupar, Pierre Haguenauer, Jaime Alonso, et al. VLTI-UT vibrations effort and performances[C]//SPIE, 2014, 9145: 91452M.

    [8] [8] Ford V, Carter C, Delrez C. Jitter studies for the secondary and tertiary mirror systems on the thirty meter telescope[C]//SPIE, 2014, 9151(2): 1-15.

    [10] [10] Keas P, Guerra J, Brewster R, et al. SOFIA telescope modal survey test and test-model correlation[C]//SPIE, 2010, 7738: 77380K.

    [11] [11] Maly J, Glaese R, Keas P. Damping SOFIA: passive and active damping for the stratospheric observatory for infrared astronomy[C]//SPIE, 2001, 4331: 60.

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    Zhao Yongzhi, An Qichang, Han Xida. Tuned damping technique for large telescope[J]. Infrared and Laser Engineering, 2017, 46(8): 818006

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    Paper Information

    Category: 光学设计及仿真

    Received: Dec. 5, 2016

    Accepted: Jan. 5, 2017

    Published Online: Nov. 7, 2017

    The Author Email: Yongzhi Zhao (13504314756@126.com)

    DOI:10.3788/irla201746.0818006

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