Optics and Precision Engineering, Volume. 30, Issue 4, 442(2022)

Wind disturbance simulation and optical performance prediction for large ground-based optical telescopes based on two-dimensional stochastic fields

Yuyan CAO1...2,*, Jianli WANG1,2, Zhichen WANG1,2, Hongwen Li1, Yan ZHANG1,2, Hongliang CHU1 and Yuxia LI1 |Show fewer author(s)
Author Affiliations
  • 1Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun30033, China
  • 2University of Chinese Academy of Sciences, Beijing100049, China
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    Figures & Tables(15)
    Simplified structure of 2 m telescope
    Finite element model of 2 m telescope structure
    Simplified model of wind disturbance
    Wind load acting on telescopes
    Sampling points of the primary mirror
    Wind speed for each sample point of the primary mirror
    Surface precision of the primary and secondary mirror-primary mirror loaded separately
    Optical axis perturbation of the primary and secondary mirror-primary mirror loaded separately
    Position deviation of the primary and secondary mirror-primary mirror loaded separately
    Surface precision of the primary and secondary mirror-secondary mirror and truss loaded separately
    Optical axis perturbation of the primary and secondary mirror-secondary mirror and truss loaded separately
    Position deviation of the primary and secondary mirror-secondary mirror and truss loaded separately
    Frequency spectrum of position deviation between primary and secondary mirror-secondary mirror and truss loaded separately
    • Table 1. Parameters of wind load

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      Table 1. Parameters of wind load

      ParametersMeaningValue
      vmExternal wind speed10 m/s and 15 m/s
      ρAir density1.293 kg/m3
      AsmArea for SM and baffle227 500 mm2
      AtrussArea for truss1 025 088 mm2
      AspiderArea for spider809 600 mm2
      AringArea for top ring392 370 mm2
      CD,smDrag coefficient for SM1.2
      CD,trussDrag coefficient for truss1.2
      CD,spiderDrag coefficient for spiders1.2
      CD,pmDrag coefficient for PM1.05
      LxSpatial length in x direction2 500 mm
      LySpatial length in y direction2 500 mm
      HHeight6 400 mm
    • Table 2. Discretized parameters of wind speed fields

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      Table 2. Discretized parameters of wind speed fields

      ParametersMeaningValue
      zHeight above ground10 m
      z0Ground roughness coefficient0.01
      λxDecay coefficient in x direction7
      λyDecay coefficient in y dir7
      NxWave-number in x dir128
      NyWave-number in y dir128
      NωFrequencies1 024
      M1Sample numbers in x dir256
      M2Sample numbers in y dir256
      M3Sample numbers in time domain2048
      TSimulation time length100s
      ∆κxWave-number space in x dir0.002 5 mm-1
      ∆κyWave-number space in y dir0.002 5 mm-1
      ωFrequency space0.062 8 s-1
      xSpatial step in x dir9.766 mm
      ySpatial step in y dir9.766 mm
      tTime step0.048 8 s
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    Yuyan CAO, Jianli WANG, Zhichen WANG, Hongwen Li, Yan ZHANG, Hongliang CHU, Yuxia LI. Wind disturbance simulation and optical performance prediction for large ground-based optical telescopes based on two-dimensional stochastic fields[J]. Optics and Precision Engineering, 2022, 30(4): 442

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    Paper Information

    Category: Micro/Nano Technology and Fine Mechanics

    Received: Jun. 22, 2021

    Accepted: --

    Published Online: Mar. 4, 2022

    The Author Email: CAO Yuyan (yuyan_cao@126.com)

    DOI:10.37188/OPE.20223004.0442

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