Acta Photonica Sinica, Volume. 54, Issue 4, 0422001(2025)

Design of a Wide-field Multispectral Imaging Optical System for Martian Dust Storm Detection

Hao GUO1,2, Jianfeng YANG1、*, Xiaolong MA1, and Juan LÜ1
Author Affiliations
  • 1Laboratory of Lunar and Deep Space Exploration Technology,Xi'an Institute of Optics and Precision Mechanics of Chinese Academy of Science,Xi'an 710119,China
  • 2University of Chinese Academy of Sciences,Beijing 100049,China
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    Figures & Tables(29)
    Schematic diagram of orbiting satellites
    Characterization of optical materials in the designed spectral band
    Schematic diagram of the main ray transmission of a negative meniscus lens
    Initial system optical path diagram
    Initial system magnification chromatic aberration
    Initial system field curvature
    Diagram of the final system optical path
    Spot diagram of the final system
    MTF of the final system
    Lateral color of the initial structure of the final system
    The distribution curves of the theoretical and actual values of ground element resolution
    Field curvature of the final system
    Relative Illumination of the final system
    System ditoortion grid
    750 nm monochrome MTF
    260 nm monochrome MTF
    Simulation of e light propagation when the system point series diagram
    Cumulative distribution of MTF probabilities in the system
    MTF at -40 ℃
    MTF at +50 ℃
    • Table 1. Design specifications of the optical system

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      Table 1. Design specifications of the optical system

      SampleValue
      Wavelength band/nm260 nm~750 nm
      Number of spectra≥6
      Spectral channel center wavelength720 nm,650 nm,550 nm,425 nm,340 nm,290 nm
      F number≤11
      Full field of view angle/(°)≥130°×30°
      Effective focal length/mm13
      Spatial resolution of the center field of view≤500 m@400 km
      Modulation Transfer Function(MTF)≥46 lp/mm@0.2
      Total track length/mm≤200 mm
      Field curve value(550 nm)-0.13 mm~+0.13 mm
      Relative illumination≥0.7
      Working temperature/℃-40 ℃~+50 ℃
    • Table 2. Initial optical system structure parameters

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      Table 2. Initial optical system structure parameters

      SurfaceY radius/mmThickness/mmGlass
      ObjectInfinityInfinityAir
      179.259 83.073 4Fused silica
      224.194 014.224 7Air
      3123.668 12.848 8Sapphire
      424.254 139.420 2Air
      549.275 44.766 4Calcium fluoride
      6-197.778 020.198 8Air
      StopInfinity4.670 4Air
      825.089 517.071 9Calcium fluoride
      9-12.506 20.747 0Air
      10-12.138 82.844 9Fused silica
      11-31.966 037.751 2Air
      ImageInfinity0.000 0Air
    • Table 3. Final optical system structure parameters

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      Table 3. Final optical system structure parameters

      SurfaceY radius/mmThickness/mmGlass
      ObjectInfinityInfinityAir
      154.987 33.500 0Fused silica
      223.585 920.481 9Air
      3-65.881 62.500 0Sapphire
      431.149 812.863 5Air
      5-31.291 515.816 8Sapphire
      6-41.301 91.500 0Air
      7378.582 06.351 8Sapphire
      8-119.589 41.500 0Air
      954.095 810.240 6Fused silica
      10-158.648 052.771 6Air
      StopInfinity9.461 0Air
      1224.502 54.656 3Calcium fluoride
      13-12.206 71.747 9Air
      14-10.883 517.657 1Potassium bromide
      15-25.413 41.500 0Air
      16-57.755 22.951 4Potassium bromide
      17-31.819 516.000 0Air
      18Infinity3.000 0Fused silica
      19Infinity0.500 0Air
      ImageInfinity0.000 0Air
    • Table 4. Composite filter partial parameters

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      Table 4. Composite filter partial parameters

      Center wavelength/nmFWHM/nm

      720±5

      650±5

      550±5

      425±5

      340±5

      290±5

      25±5

      20±5

      20±5

      25±5

      35±5

      30±5

    • Table 5. Main ray offset at 750 nm

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      Table 5. Main ray offset at 750 nm

      Field of view/(°)Δy /mm

      0

      24

      30

      45

      60

      65

      0.000 00

      0.004 58

      0.005 49

      0.008 40

      0.012 96

      0.013 93

    • Table 6. Main ray offset at 260 nm

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      Table 6. Main ray offset at 260 nm

      Field of view/(°)Δy /mm

      0

      24

      30

      45

      60

      65

      0.000 00

      -0.000 94

      -0.001 11

      0.000 03

      0.004 31

      0.005 49

    • Table 7. Tolerance allocation

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      Table 7. Tolerance allocation

      Tolerance itemsValue
      Radius/mm±0.05
      Thickness/mm±0.05
      Decenter X/mm±0.01
      Decenter Y/mm±0.01
      Tilt X/(°)±0.05
      Tilt Y/(°)±0.05
      Abbe number1%
      Refractive index0.001
    • Table 8. Material data sheet

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      Table 8. Material data sheet

      MaterialThermal expansion coefficient/(×10-6

      SILICA

      SAPPHIRE

      CAF2

      KBR

      TC4

      0.55

      6.7

      24

      39

      8.5

    • Table 9. The amount of change in the image plane position of the optical system at different operating temperatures

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      Table 9. The amount of change in the image plane position of the optical system at different operating temperatures

      Temperature/℃-40 ℃-20 ℃0 ℃20 ℃50 ℃
      Change amount of image plane position/mm-0.015 8-0.010 6-0.005 3-0.000 3+0.007 9
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    Hao GUO, Jianfeng YANG, Xiaolong MA, Juan LÜ. Design of a Wide-field Multispectral Imaging Optical System for Martian Dust Storm Detection[J]. Acta Photonica Sinica, 2025, 54(4): 0422001

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    Paper Information

    Category: Optical Design and Fabrication

    Received: Sep. 26, 2024

    Accepted: Nov. 11, 2024

    Published Online: May. 15, 2025

    The Author Email: Jianfeng YANG (yangjf@opt.ac.cn)

    DOI:10.3788/gzxb20255404.0422001

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