• Optics and Precision Engineering
  • Vol. 31, Issue 10, 1419 (2023)
Fenghua ZUO1, Xiuqing HU2,3,*, Xia WANG1, Chengli QI2,3, and Lu LI2,3
Author Affiliations
  • 1School of Optics and Photonics, Beijing Institute of Technology, Beijing0008, China
  • 2Key Laboratory of Radiometric Calibration and Validation for Environmental Satellites, National Satellite Meteorological Center (National Center for Space Weather), China Meteorological Administration, Beijing100081, China
  • 3Innovation Center for FengYun Meteorological Satellite (FYSIC), Beijing100081, China
  • show less
    DOI: 10.37188/OPE.20233110.1419 Cite this Article
    Fenghua ZUO, Xiuqing HU, Xia WANG, Chengli QI, Lu LI. Improvement of phase correction for FY-3D hyper-spectral infrared atmospheric sounder[J]. Optics and Precision Engineering, 2023, 31(10): 1419 Copy Citation Text show less
    Schematic diagram of the minimum spectral imaginary part method (λ is the interferogram sampling interval)
    Fig. 1. Schematic diagram of the minimum spectral imaginary part method (λ is the interferogram sampling interval)
    Original complex spectrum (LWIR) of ES, ICT and DSP
    Fig. 2. Original complex spectrum (LWIR) of ES, ICT and DSP
    Deviations of ES and DSP spectral phase relative to ICT spectral phase
    Fig. 3. Deviations of ES and DSP spectral phase relative to ICT spectral phase
    Results difference between two calculation methods
    Fig. 4. Results difference between two calculation methods
    Spectrum phase of ES, ICT and DSP
    Fig. 5. Spectrum phase of ES, ICT and DSP
    Phase correction flow chart.
    Fig. 6. Phase correction flow chart.
    δES changes with the temperature of the observed target (the left/right column shows the forward/reverse swing direction of the interferometer moving mirror)
    Fig. 7. δES changes with the temperature of the observed target (the left/right column shows the forward/reverse swing direction of the interferometer moving mirror)
    δDSP changes with Time series (the left/right column shows the forward/reverse swing direction of the interferometer moving mirror)
    Fig. 8. δDSP changes with Time series (the left/right column shows the forward/reverse swing direction of the interferometer moving mirror)
    HIRAS-CrIS spectral distribution, mean BT deviation and standard deviation of BT bias
    Fig. 9. HIRAS-CrIS spectral distribution, mean BT deviation and standard deviation of BT bias
    Mean BT deviation of HIRAS-CrIS (solid green line) and the variation of mean BT deviation after phase correction (dotted red line)
    Fig. 10. Mean BT deviation of HIRAS-CrIS (solid green line) and the variation of mean BT deviation after phase correction (dotted red line)
    Standard deviation of HIRAS-CrIS deviation (green solid line) and the variation of standard deviation after phase correction (red dotted line)
    Fig. 11. Standard deviation of HIRAS-CrIS deviation (green solid line) and the variation of standard deviation after phase correction (red dotted line)
    Scatter distribution and regression line of deviations with the mean BT of HIRAS spectrum in four independent LW spectral channels (green/ red represents before/ after correction)
    Fig. 12. Scatter distribution and regression line of deviations with the mean BT of HIRAS spectrum in four independent LW spectral channels (green/ red represents before/ after correction)
    Scatter distribution and regression line of deviations with the mean BT of HIRAS spectrum in four independent MW spectral channels (green/ red represents before/ after correction)
    Fig. 13. Scatter distribution and regression line of deviations with the mean BT of HIRAS spectrum in four independent MW spectral channels (green/ red represents before/ after correction)
    Scatter distribution and regression line of deviations with the mean BT of HIRAS spectrum in four independent SW spectral channels (green/ red represents before/ after correction)
    Fig. 14. Scatter distribution and regression line of deviations with the mean BT of HIRAS spectrum in four independent SW spectral channels (green/ red represents before/ after correction)
    ParameterMaximum scanning angle /(°)Scan period /sField of regard /(°)Field of view /(°)Focal plane detector configuration
    Value50.4103.61.12×2
    ParameterSpectral calibration accuracy /ppmDirection pointing bias /(°)Spectral range /μmSpectral resolution /(cm-1Number of channels
    Value100.2515.38-8.8 (LWIR), 8.26-5.71 (MWIR), 4.64-3.92 (SWIR)0.6252 287
    Table 1. Instrument parameter characteristics of HIRAS
    Fenghua ZUO, Xiuqing HU, Xia WANG, Chengli QI, Lu LI. Improvement of phase correction for FY-3D hyper-spectral infrared atmospheric sounder[J]. Optics and Precision Engineering, 2023, 31(10): 1419
    Download Citation