Acta Optica Sinica, Volume. 43, Issue 8, 0822018(2023)

Design of Geostationary Full-Spectrum Wide-Swath High-Fidelity Imaging Spectrometer and Development of Its Spectrometers

Jiacheng Zhu1,2, Zhicheng Zhao1,2, Quan Liu1,2、*, Xinhua Chen1,2, Huan Li3, Shaofan Tang3, and Weimin Shen1,2、**
Author Affiliations
  • 1School of Optoelectronic Science and Engineering, Soochow University, Suzhou 215006, Jiangsu, China
  • 2Key Lab of Advanced Optical Manufacturing Technologies of Jiangsu Province & Key Lab of Modern Optical Technologies of Education Ministry of China, Soochow University, Suzhou 215006, Jiangsu, China
  • 3Beijing Institute of Space Mechanics and Electricity, Beijing 100094, China
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    Figures & Tables(27)
    Working principle diagram of GeoFWHIS. (a) Layout diagram; (b) pointing to different coverages by turning the platform
    Afocal three-mirror system. (a) Coaxial three-mirror; (b) off-axis three-mirror; (c) zigzag-axis three-mirror
    Off-axis three-mirror imaging systems. (a) Two-mirror system; (b) three-mirror system with intermediate image; (c) three-mirror system without intermediate image
    Optical path of fore-optics system. (a) 3D model of fore-optics system; (b) optical path with scanning mirror at edge position of -2.56°; (c) optical path with scanning mirror at edge position of +2.56°
    MTF curves and spot diagrams of fore-optics system in B2 band. (a)-(c) MTF curves with scanning angle of -‍2.56°, 0°, and +2.56°; (d)-(f) sport diagrams with scanning angle of -2.56°, 0°, and +2.56°
    Schematic of spectrometer splicing system
    Optical path of different spectrometers
    Optical path of spectrometers in GeoFWHIS. (a) B1 band; (b) B2 band; (c) B3 band; (d) B4 band; (e) B5 band
    SRF of optical splitting systems for each band. (a) B1 band; (b) B2 band; (c) B3 band; (d) B4 band; (e) B5 band
    Lightpath diagram of GeoFWHIS
    SNR curves for B2 band in cloudless environment when observation zenith angle is 35° and integration time is 80 ms
    Silicon long slits. (a) Slit for B1 and B2 bands with length of 61.44 mm and width of 15 μm; (b) slit for B3 and B4 bands with length of 49.16 mm and width of 24 μm; (c) slit for B5 band with length of 24.58 mm and width of 24 μm
    Micrograph of slit for B2. (a) 10× micrograph; (a) test result of slit width
    Convex blazed gratings and their groove shapes, the lower right corner shows AFM test results of groove shapes. (a) B1 band, groove density is 312.1 lp/mm and blazed angle is 3.8°; (b) B2 band, groove density is 210.1 lp/mm and blazed angle is 4.75°; (c) B3 band, groove density is 68.5 lp/mm and blazed angle is 3.1°; (d) B4 band, groove density is 19.1 lp/mm and blazed angle is 2.8°; (e) B5 band, groove density is 8.8 lp/mm and blazed angle is 2.8°
    Diffraction efficiency curves of gratings at B1-B5 bands. (a) B1 band; (b) B2 band; (c) B3 band; (d) B4 band; (e) B5 band
    Alignment of the spectrometer by utilizing a point source microscope. (a) Self-developed point source microscope; (b) alignment of two separated meniscus in B3 spectrometer with point source microscope; (c) star images of two spherical surfaces in field of view of point source microscope
    Full-spectrum spectrometer prototypes. (a) B1 band; (b) B2 band; (c) B3 band; (d) B4 band; (e) B5 band
    Test device and test results of B2 spectrometer. (a) Test device of spectral property; (b) spectral lines; (c) SRF of 546.1 nm spectral line; (d) scatter diagram of 546.1 nm spectral line and its fitting curve
    Test device and spectral lines of B5 spectrometer. (a) Test device; (b) spectral lines
    • Table 1. Specifications and system parameters of GeoFWHIS

      View table

      Table 1. Specifications and system parameters of GeoFWHIS

      Specification and parameterValue
      Orbital altitudeGeostationary orbit(~36000 km)
      Swath width /(km×km)400×400
      Field of view /[(°)×(°)]0.64×0.64
      Entrance pupil diameter /m3.2
    • Table 2. System parameters of GeoFWHIS at full-spectrum

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      Table 2. System parameters of GeoFWHIS at full-spectrum

      BandB1B2B3B4B5
      Wavelength range /μm0.3-0.560.55-1.011-2.53-58-12.5
      Spatial resolution /m25255050100
      Spectral resolution /nm451050200
      MTF0.170.170.170.120.12
      SNR250250150
      NETD /K0.30.3
      Focal length /m21.621.617.2817.288.64
      F number6.756.755.45.42.7
      Detector resolution4096×20484096×20482048×2562048×2561024×256
      Pixel size /μm15×1515×1524×3224×3224×32
      Total length of slit /mm241.3241.319319396.5
      Number of splicing spectrometers44444
      Single slit length /mm61.4461.4449.15249.15224.576
    • Table 3. Specifications of three objectives

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      Table 3. Specifications of three objectives

      SpecificationObjective ⅠObjective ⅡObjective Ⅲ
      Wavelength range /μm0.3-1.011-58-12.5
      Entrance pupil diameter /mm200200200
      Field of fiew /[(°)×(°)]10.24×0.2210.24×0.2610.24×0.53
      Focal length /mm13501080540
      F number6.755.42.7
    • Table 4. Comparison of advantages and disadvantages for different spectrometers

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      Table 4. Comparison of advantages and disadvantages for different spectrometers

      Spectrometer typeCharacteristicAdvantageDisadvantage
      Offner

      ·Convex grating;

      ·Concentric structure

      ·Long working distance;

      ·No smile and keystone

      ·Large volume with a long slit;

      ·Residual astigmatism

      Wynne-Offner·A meniscus is added near the grating of Offner type

      ·Advantages of Offner type;

      ·Anastigmatism;

      ·Compact

      ·Additional polarization;

      ·Hard to manufacture grating on meniscus

      Freeform Offner·Three freeform elements

      ·Advantages of Offner type;

      ·Compact

      ·Extremely difficulty;

      ·High cost

      Immersed Offner·Light travels in dielectric

      ·Advantages of Offner type;

      ·Ultra-compact

      ·High cost;

      ·High risk

      Dyson

      ·Concave grating;

      ·Concentric structure

      ·Large relative aperture;

      ·No smile and keystone

      ·Large volume with a long slit;

      ·Short working distance

      Wynne-Dyson·A meniscus is added behind the hemispherical lens of Dyson type

      ·Advantages of Dyson type;

      ·Ultra-compact

      ·Short working distance

      Advanced

      Dyson

      ·Several meniscus lenses added into the classic Dyson type

      ·Advantages of Dyson type;

      ·Relatively long working distance

      ·Large volume with a long slit
      R-T

      ·Double pass structure;

      ·Plane grating;

      ·Littrow mounting

      ·Compact;

      ·Small distortion

      ·High cost;

      ·Tight tolerance;

      ·Small space between slit and image

      CCVIS

      ·Catadioptric structure;

      ·Immersed grating

      ·Long working distance;

      ·Compact

      ·Residual keystone;

      ·Thermal sensitive

    • Table 5. System parameters and performance of spectrometers

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      Table 5. System parameters and performance of spectrometers

      BandB1B2B3B4B5
      Package size /(mm×mm×mm)140×110×100170×111×106160×132×89168×165×8890×92×49
      Smile /pixel0.06%0.11%0.26%0.31%0.95%
      Keystone /pixel0.33%0.47%0.79%0.42%1.00%
      MTF0.860.770.720.410.28
      Grating density /(lp·mm-13102106819.18.8
      Blazed angle of grating /(°)3.74.63.12.62.8
    • Table 6. MTF of GeoFWHIS at Nyquist frequency

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      Table 6. MTF of GeoFWHIS at Nyquist frequency

      BandSerial numberScanning angle of -2.56°Scanning angle of 0°Scanning angle of +2.56°
      B1Wavelength /μm0.300.430.560.300.430.560.300.430.56
      Diffraction limit0.880.840.800.880.840.800.880.840.80
      Spectrometer 10.800.760.750.800.790.770.600.590.57
      Spectrometer 20.820.790.760.820.800.780.770.720.66
      Spectrometer 30.810.790.770.850.790.780.750.710.63
      Spectrometer 40.730.690.670.780.740.720.610.580.53
      B2Wavelength /μm0.550.781.010.550.781.010.550.781.01
      Diffraction limit0.780.720.660.780.720.660.780.720.66
      Spectrometer 10.650.620.570.710.640.590.600.580.53
      Spectrometer 20.660.650.580.740.700.620.650.620.56
      Spectrometer 30.690.670.580.730.700.630.640.590.53
      Spectrometer 40.650.600.560.720.690.620.600.550.52
      B3Wavelength /μm1.001.752.501.001.752.501.001.752.50
      Diffraction limit0.840.740.630.840.740.630.840.740.63
      Spectrometer 10.690.630.550.720.600.540.630.550.40
      Spectrometer 20.790.700.620.810.700.650.690.620.51
      Spectrometer 30.770.700.610.800.710.650.770.690.55
      Spectrometer 40.780.710.610.790.680.630.780.660.54
      B4Wavelength /μm345345345
      Diffraction limit0.520.470.420.520.470.420.520.470.42
      Spectrometer 10.420.380.350.420.390.360.380.330.31
      Spectrometer 20.490.450.400.500.460.420.450.450.39
      Spectrometer 30.470.390.380.500.440.400.430.420.37
      Spectrometer 40.460.400.320.470.390.340.360.320.29
      B5Wavelength /μm8.010.312.58.010.312.58.010.312.5
      Diffraction limit0.350.310.270.350.310.270.350.310.27
      Spectrometer 10.280.250.220.310.260.250.290.250.23
      Spectrometer 20.310.270.230.320.270.240.310.270.24
      Spectrometer 30.300.260.230.310.270.260.300.260.22
      Spectrometer 40.290.250.240.300.260.230.300.250.22
    • Table 7. FWHM (spectral resolution) of B2 spectrometer

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      Table 7. FWHM (spectral resolution) of B2 spectrometer

      Wavelength /nmFWHM /nm
      -1 field-0.5 field0 field+0.5 field+1 fieldAverage
      546.15.025.014.994.995.015.01
      643.85.025.025.025.005.015.02
      959.85.025.005.025.025.025.02
      10175.025.025.015.015.025.02
    • Table 8. FWHM (spectral resolution) of B5 spectrometer

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      Table 8. FWHM (spectral resolution) of B5 spectrometer

      Wavelength /nmFWHM /nm
      -1 field0 field+1 fieldAverage
      8224201.3201.0200.9201.1
      8834202.4202.1201.9202.1
      9350205.9204.9204.2205.0
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    Jiacheng Zhu, Zhicheng Zhao, Quan Liu, Xinhua Chen, Huan Li, Shaofan Tang, Weimin Shen. Design of Geostationary Full-Spectrum Wide-Swath High-Fidelity Imaging Spectrometer and Development of Its Spectrometers[J]. Acta Optica Sinica, 2023, 43(8): 0822018

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    Paper Information

    Category: Optical Design and Fabrication

    Received: Oct. 26, 2022

    Accepted: Nov. 25, 2022

    Published Online: Apr. 6, 2023

    The Author Email: Liu Quan (liuquan@suda.edu.cn), Shen Weimin (swm@suda.edu.cn)

    DOI:10.3788/AOS221884

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