• Acta Photonica Sinica
  • Vol. 51, Issue 6, 0612004 (2022)
Kunyan WANG1、2, Yichun DAI1、*, and Zhenyu JIN1
Author Affiliations
  • 1Astronomical Technology Laboratory,Yunnan Observatory,Chinese Academy of Sciences,Kunming 650216,China
  • 2University of Chinese Academy of Sciences,Beijing 100049,China
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    DOI: 10.3788/gzxb20225106.0612004 Cite this Article
    Kunyan WANG, Yichun DAI, Zhenyu JIN. Attitude Alignment Method of Solar Telescope Secondary Mirror Based on Aberration Detection[J]. Acta Photonica Sinica, 2022, 51(6): 0612004 Copy Citation Text show less
    Optical system structure
    Fig. 1. Optical system structure
    The alignment process of secondary mirror
    Fig. 2. The alignment process of secondary mirror
    Comparison between the calculated value and the original value of misalignment(damped least square method)
    Fig. 3. Comparison between the calculated value and the original value of misalignment(damped least square method)
    Comparison between the calculated value and the original value of misalignment(least square method)
    Fig. 4. Comparison between the calculated value and the original value of misalignment(least square method)
    Cumulative error of misalignment after 1 day alignment(alignment based on stable 0-point position)
    Fig. 5. Cumulative error of misalignment after 1 day alignment(alignment based on stable 0-point position)
    Cumulative error of misalignment after 1 day alignment(alignment based on relative position)
    Fig. 6. Cumulative error of misalignment after 1 day alignment(alignment based on relative position)
    Comparison between the calculated value and the original value of misalignment for restricting decenter
    Fig. 7. Comparison between the calculated value and the original value of misalignment for restricting decenter
    Cumulative error of misalignment after 1 day alignment for restricting decenter
    Fig. 8. Cumulative error of misalignment after 1 day alignment for restricting decenter
    NameParameter
    ApertureOutside diameter:2 000 mm
    Internal diameter:1 300 mm
    Ring width:350 mm
    Field3'×3'
    Observation band0.39 μm~2.3 μm
    Focal ratio of primary mirrorF/1.5
    Focal ratio of telescopeF/6.53
    Focal length13 060 mm
    Table 1. Main optical parameters of 2mRST
    MisalignmentSensitivity
    Dx4.98×10-4
    Dy6.30×10-4
    Tx0.167 9
    Ty0.170 0
    Dz1
    Table 2. Order of misalignment sensitivities
    MisalignmentDx/mmDy/mmDz/mmTx/(°)Ty/(°)
    RMSE(DLSM)0.050 20.051 50.000 40.003 70.003 6
    RMSE(LSM)0.120 40.148 60.000 40.010 70.008 8
    Table 3. RMSE of misalignment solution
    MisalignmentDx/mmDy/mmDz/mmTx/(°)Ty/(°)
    RMSE0.056 70.057 90.000 40.004 20.004 0
    Table 4. RMSE of misalignment solution for restricting decenter*
    MisalignmentAlignment
    RMS of aberration(regularization)0.495 9λ0.006 2λ
    RMS of aberration(restrict decenter)0.495 9λ0.127 4λ
    Table 5. Image quality compensation effect
    Kunyan WANG, Yichun DAI, Zhenyu JIN. Attitude Alignment Method of Solar Telescope Secondary Mirror Based on Aberration Detection[J]. Acta Photonica Sinica, 2022, 51(6): 0612004
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