• Acta Optica Sinica
  • Vol. 42, Issue 2, 0212002 (2022)
Si Xiao1、2, Liping Fu1、2、*, Xiuqing Hu3, Yanting Pi1、2, Nan Jia1、2, Xuesong Bai1、2, and Tianfang Wang1、2
Author Affiliations
  • 1National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China
  • 2Beijing Key Laboratory of Space Environment Exploration, Beijing 100190, China
  • 3National Satellite Meteorological Centre, China Meteorological Administration, Beijing 100081, China
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    DOI: 10.3788/AOS202242.0212002 Cite this Article Set citation alerts
    Si Xiao, Liping Fu, Xiuqing Hu, Yanting Pi, Nan Jia, Xuesong Bai, Tianfang Wang. Radiometric Calibration Technology Based on Far Ultraviolet Hyperspectral Imaging Instrument[J]. Acta Optica Sinica, 2022, 42(2): 0212002 Copy Citation Text show less
    Light path diagram of far ultraviolet hyperspectral imaging instrument
    Fig. 1. Light path diagram of far ultraviolet hyperspectral imaging instrument
    Star image
    Fig. 2. Star image
    Schematic diagram of calibration
    Fig. 3. Schematic diagram of calibration
    Image of actual calibration
    Fig. 4. Image of actual calibration
    Response images at different incident angles. (a) 0.05°; (b) 0.15°; (c) 0.25°; (d) 0.35°; (e) 0.45°; (f) 0.55°; (g) 0.65°; (h) 0.75°; (i) 0.85°
    Fig. 5. Response images at different incident angles. (a) 0.05°; (b) 0.15°; (c) 0.25°; (d) 0.35°; (e) 0.45°; (f) 0.55°; (g) 0.65°; (h) 0.75°; (i) 0.85°
    Noise curve of single pixel
    Fig. 6. Noise curve of single pixel
    Pixel response curves at different positions. (a) (90,347); (b) (90,349); (c) (90,351); (d) (90,353); (e) (90,355)
    Fig. 7. Pixel response curves at different positions. (a) (90,347); (b) (90,349); (c) (90,351); (d) (90,353); (e) (90,355)
    Pixel response curves at different positions after noise removal. (a) (90,347); (b) (90,349); (c) (90,351); (d) (90,353); (e) (90,355)
    Fig. 8. Pixel response curves at different positions after noise removal. (a) (90,347); (b) (90,349); (c) (90,351); (d) (90,353); (e) (90,355)
    Average pixel response curve
    Fig. 9. Average pixel response curve
    Average pixel response curve after normalization
    Fig. 10. Average pixel response curve after normalization
    ItemDescription of performance indicators
    Wavelength: 120--180 nm;
    field of view: 4°;
    Optical systemF-number: 6.3;
    entrance pupil diameter: 30 mm;
    spectral resolution: 4 nm;
    space resolution: 0.1°
    DetectorPixel size: 20 μm;
    pixel number: 720×576
    WorkingPressure: better than 10-3 Pa (vacuum);
    environmenttemperature stability: better than ±2 K
    Table 1. Design parameters
    EquipmentParameter
    Vacuum chamberPressure: better than 10-3 Pa
    Deuterium lampWavelength: 120--200 nm;stability: 0.05%
    MonochromatorWavelength: 30--550 nm;spectral resolution: 0.1 nm
    DartDiameter: 0.5 mm
    Collimating systemWavelength: 120--780 nm
    Vacuum turntablePrecision: 0.05°
    Table 2. Test equipments
    Si Xiao, Liping Fu, Xiuqing Hu, Yanting Pi, Nan Jia, Xuesong Bai, Tianfang Wang. Radiometric Calibration Technology Based on Far Ultraviolet Hyperspectral Imaging Instrument[J]. Acta Optica Sinica, 2022, 42(2): 0212002
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