• Acta Photonica Sinica
  • Vol. 45, Issue 9, 912006 (2016)
AN Qi-Chang1、2、*, ZHANG Jing-xu1, and YANG Fei1
Author Affiliations
  • 1[in Chinese]
  • 2[in Chinese]
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    DOI: 10.3788/gzxb20164509.0912006 Cite this Article
    AN Qi-Chang, ZHANG Jing-xu, YANG Fei. Influence on the 30 m Telescope Tertiary Mirror Performance by the Internal Vibration[J]. Acta Photonica Sinica, 2016, 45(9): 912006 Copy Citation Text show less
    References

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    [2] SU Yan-qin, ZHANG Jing-xu, WANG Fu-guo, et al. Seismic analysis of TMT M3 cell assembly based on spectral response[J]. Optics and Precision Engineering, 2014, 22(4): 996-1003.

    [3] BYOUN G, NISSL Y, GEORG E, et al. Analysis of normalized point source sensitivity as a performance metric for the thirty meter telescope[C]. SPIE, 2010, 7738: 77380G.

    [4] PAZDER J S, VOGIATZIS K, ANGELIi G Z. Dome and mirror seeing estimates for the thirty meter telescope[C]. SPIE, 2008, 7017(0R): 1-9.

    [5] RUDOLER A S, HSDAR O, FISHER M, et al. Image resolution limits resulting from mechanical vibrations[C]. SPIE, 1985, 26(6): 529-533.

    [6] HADAR O, DROR I, KOPEIKA N. Image resolution limits resulting from mechanical vibrations. Part IV: real-time numerical calculation of optical transfer functions and experimental verification[J]. Optics Engineering, 1994, 33(2): 566-578.

    [7] KOPEIKA N, WULICH D. Image resolution limits resulting from mechanical vibrations[J]. Journal of Modern Optics, 2008, 55(3): 401-407.

    [8] SU Yan-qin, WANG Fu-guo, ZHANG Jing-xu, et al. TMT M3 system seismic analysis based on time history method[J]. Acta Optica Sinica, 2013, 33(11): 1112002.

    [9] SHAO Liang, WU Xiao-xia, CHEN Bao-gang, et al. Passive support system of light-weighted SiC primary mirror[J]. Optics and Precision Engineering, 2015, 23(5): 1380-1386.

    [10] LIU Xiang-yi, ZHANG Jing-xu, WU Xiao-xia, et al. Affect of environment on mirror seeing of large-aperture SiC lightweight primary mirror[J]. Optics and Precision Engineering, 2015, 23(3): 776-783.

    [11] YANG Xiao-xia, MENG Hao-ran, YIN Yu-mei, et al. Jitter measurement for large opto-electronic telescope using accelerometers[J]. Journal of Electronic Measurement and Instrument, 2013, 27(9): 823-830.

    [12] BYOUNG J, CARL N, GEORGE A, et al. Analysis of normalized point source sensitivity as a performance metric for the thirty meter telescope[C]. SPIE, 2008: 70170T.

    [13] DENG Yong-ting, LI Hong-wen, WANG Jian-li. Overview of AC servo control system for the large telescope[J]. Chinese Optics, 2015, 8(6): 895-908.

    [14] WANG Fu-guo, AN Qi-chang. Evaluation of mirror surface figures for TMT based on slope Rms[J]. Optics and Precision Engineering, 2014, 22(5): 1171-1175.

    [15] MACMYNOWSKI D, COLAVITA M, SKIDMORE W, et al. Primary mirror dynamic disturbance models for TMT: Vibration and wind[C]. SPIE, 2010: 7738E.

    [16] MACMARTIN D,THOMPSON P,COLAVITA M, et al. Dynamic analysis of the active-controlled segmented mirror of the Thirty Meter Telescope[J]. IEEE Transactions on Control Systems Technology, 2013, 22: 58-68.

    AN Qi-Chang, ZHANG Jing-xu, YANG Fei. Influence on the 30 m Telescope Tertiary Mirror Performance by the Internal Vibration[J]. Acta Photonica Sinica, 2016, 45(9): 912006
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