Chinese Optics, Volume. 15, Issue 4, 747(2022)

Aberration coupling characteristics of axial and lateral misalignments of off-axis three-mirror telescopes

Xiao-quan BAI1,2,3, Liang GUO1,2,3, Hong-cai MA1,3, Bo-qian XU1,3, Guo-hao JU1,3, and Shu-yan XU1,3
Author Affiliations
  • 1Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130033, China
  • 2University of Chinese Academy of Sciences, Beijing 100049, China
  • 3CAS Key Laboratory of On-orbit Manufacturing and Integration for Space Optics system, Changchun 130033, China
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    Figures & Tables(15)
    (a) Schematic diagram and (b) experiment device of the 500 mm off-axis three-mirror system
    FFDs (full field displays) for astigmatism in different states
    FFDs for the coma in different states
    Aberration field distribution when the minimized astigmatism field change is set as the goal for compensation
    Aberration field distribution when the minimized coma field change is set as the goal for compensation
    Full-field distributions of RMS wavefront error for different states in the process of compensating the aberrations induced by lateral misalignments using axial mialignments
    Aberration field distribution in different states when the lateral misalignment compensates for the axial misalignment
    Full-field distributions of RMS wavefront error before and after compensating the aberrations induced by axial misalignments (ZDE_SM=1mm) using lateral mialignments
    Full-field distributions of RMS wavefront error before and after compensating the aberrations induced by axial misalignments (ZDE_SM=−1mm) using lateral misalignments
    Measurement results with interferometer under different conditions (remove some high frequency)
    • Table 1. Sensitivity of the wavefront aberration coefficient to the distance between primary and secondary mirrors (632.8 nm/mm)

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      Table 1. Sensitivity of the wavefront aberration coefficient to the distance between primary and secondary mirrors (632.8 nm/mm)

      像差系数像差系数对主次镜间距的敏感度
      $ {K_{040{d_1}}} $0.080
      $ {K_{222{d_1}}} $0.239
      $ {K_{131{d_1}}} $−0.119
    • Table 2. Sensitivity of the wavefront aberration coefficient to the distance between the secondary and tertiary mirrors (632.8 nm/mm)

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      Table 2. Sensitivity of the wavefront aberration coefficient to the distance between the secondary and tertiary mirrors (632.8 nm/mm)

      像差系数像差系数对次三镜间距的敏感度
      $ {K_{040{d_2}}} $−0.006
      $ {K_{222{d_2}}} $−0.016
      $ {K_{131{d_2}}} $0.028
    • Table 3. The difference in the astigmatism coefficient obtained by different methods (λ=632.8 nm)

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      Table 3. The difference in the astigmatism coefficient obtained by different methods (λ=632.8 nm)

      视场Zernike 像差系数仿真软 件获取值 公式 计算值
      (0.3°,−0.8°)$ \Delta {C_5} $−0.0038−0.0026
      $ \Delta {C_6} $−0.0495−0.0388
      (−0.3°,−0.8°)$ \Delta {C_5} $0.01090.0118
      $ \Delta {C_6} $−0.0659−0.0618
    • Table 4. The difference in the coma coefficient obtained by different methods (λ=632.8 nm)

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      Table 4. The difference in the coma coefficient obtained by different methods (λ=632.8 nm)

      视场Zernike 像差系数仿真软件获取值公式 计算值
      (0.3°,−0.8°)$ \Delta {C_7} $−0.0107−0.0108
      $ \Delta {C_8} $0.01150.0108
      (−0.3°,−0.8°)$ \Delta {C_7} $−0.0136−0.0134
      $ \Delta {C_8} $0.01130.0110
    • Table 5. Sensitivity of the aberration coefficient to misalignment (632.8 nm/mm and 632.8 nm/°)

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      Table 5. Sensitivity of the aberration coefficient to misalignment (632.8 nm/mm and 632.8 nm/°)

      C5C6C7C8
      XDE0.0531.4190.290-0.001
      YDE−1.4100.051−0.00010.276
      ZDE−0.2400.0310.01290.139
      ADE8.394−2.396−0.014−2.600
      BDE2.3518.1902.522−0.0165
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    Xiao-quan BAI, Liang GUO, Hong-cai MA, Bo-qian XU, Guo-hao JU, Shu-yan XU. Aberration coupling characteristics of axial and lateral misalignments of off-axis three-mirror telescopes[J]. Chinese Optics, 2022, 15(4): 747

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    Paper Information

    Category: Original Article

    Received: Aug. 30, 2021

    Accepted: Jan. 6, 2022

    Published Online: Sep. 6, 2022

    The Author Email:

    DOI:10.37188/CO.2021-0164

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