Acta Optica Sinica, Volume. 43, Issue 6, 0612008(2023)

Design of Integrated Cloud Detection Optical System from Visible to Terahertz Bands

Haiwei Jiang1,2,3 and Xinhua Niu1,3、*
Author Affiliations
  • 1Key Laboratory of Infrared System Detection and Imaging Technology, Chinese Academy of Sciences, Shanghai 200083, China
  • 2University of Chinese Academy of Sciences, Beijing 100049, China
  • 3Shanghai Institute of Technical Physics, Chinese Academy of Sciences, Shanghai 200083, China
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    Figures & Tables(12)
    Initial structure of coaxial three-mirror system
    Design results of off-axis three-mirror system. (a) Optical layout of off-axis three-mirror system; (b) visible and infrared spot diagrams; (c) THz spot diagram
    Design results of VNIR. (a) Optical layout; (b) MTF curves; (c) spot diagram
    Design results of SWIR.(a) Optical layout of SWIR system; (b) MTF curves; (c) spot diagram
    Design results of TIR. (a) Optical layout of TIR system; (b) MTF curves; (c) spot diagram
    Overall diagram of integrated optical system
    • Table 1. Channel set

      View table

      Table 1. Channel set

      BandCentral wavelength /μmResolution /mUtilization
      10.47075True color(blue)
      20.55075True color(green)
      30.65075True color(red),optical thickness
      40.86575Optical thickness
      51.600100Optical thickness,effective particle radius
      62.100100Effective particle radius
      78.000100Cloud phase
      811.000100Cloud phase,cloud top temperature,effective particle radius
      912.000100Cloud phase,cloud top temperature,effective particle radius
      10343.250(874 GHz)10000Ice water path
    • Table 2. Design parameters of system

      View table

      Table 2. Design parameters of system

      ParameterTHzVNIRSWIRTIR
      F number3222
      Wavelength /μm

      324.680-364.080

      [(874±50)GHz]

      0.470-0.8651.600-2.1008.000-12.000
      Input aperture /mm150426868
      IFOV(instantaneous field of view)/mrad22.000.170.220.22
    • Table 3. Tolerance of telescope system

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      Table 3. Tolerance of telescope system

      TolerancePMSMTM
      x/y decentered tolerance /mm0.100.050.05
      x/y tilt tolerance /(″)303030
      Radius tolerance /mm0.20.20.2
      Conical coefficient tolerance0.00100.00100.0005
      Surface tolerance(λ=632.8 nm)λ/25λ/25λ/25
    • Table 4. Tolerance of VNIR optical system

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      Table 4. Tolerance of VNIR optical system

      TolerancePM/ SM/ TM
      x/y decentered tolerance /mm0.05
      x/y tilt tolerance /(″)30
      Radius tolerance /mm0.2
      Conical coefficient tolerance0.001
      Surface tolerance(λ=632.8 nm)λ/25
    • Table 5. Tolerance of TIR and SWIR systems

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      Table 5. Tolerance of TIR and SWIR systems

      ToleranceTIRSWIR
      x/y decentered tolerance /mm0.020.02
      x/y tilt tolerance /(″)3636
      Thickness /mm0.100.02
      Radius /fringe33
    • Table 6. Monte-Carlo tolerance analysis results

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      Table 6. Monte-Carlo tolerance analysis results

      Probability /%Tolerance
      VNIRSWIRTIR
      900.7510.7260.390
      500.8600.8120.433
      100.9110.8600.454
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    Haiwei Jiang, Xinhua Niu. Design of Integrated Cloud Detection Optical System from Visible to Terahertz Bands[J]. Acta Optica Sinica, 2023, 43(6): 0612008

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    Paper Information

    Category: Instrumentation, Measurement and Metrology

    Received: Jul. 6, 2022

    Accepted: Aug. 22, 2022

    Published Online: Mar. 13, 2023

    The Author Email: Niu Xinhua (nxh@mail.sitp.ac.cn)

    DOI:10.3788/AOS221433

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