• Acta Optica Sinica
  • Vol. 40, Issue 8, 0830003 (2020)
Lingling Guo*, Qichang Zhao, Yong Yang, Shaolin Wang, and Rui Shu
Author Affiliations
  • Shanghai Institute of Satellite Engineering, Shanghai 201109, China
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    DOI: 10.3788/AOS202040.0830003 Cite this Article Set citation alerts
    Lingling Guo, Qichang Zhao, Yong Yang, Shaolin Wang, Rui Shu. Method for Suppression of Impulse Noise in Spaceborne Fourier Transform Infrared Spectrometer[J]. Acta Optica Sinica, 2020, 40(8): 0830003 Copy Citation Text show less
    Interferograms with impulse noise. (a) Interferogram recorded when the drive circuit of scanning motor is disabled; (b) interferogram recorded when the drive circuit of scanning motor is enabled; (c) stretched display corresponding to Fig. 1(a); (d) stretched display corresponding to Fig. 1(b)
    Fig. 1. Interferograms with impulse noise. (a) Interferogram recorded when the drive circuit of scanning motor is disabled; (b) interferogram recorded when the drive circuit of scanning motor is enabled; (c) stretched display corresponding to Fig. 1(a); (d) stretched display corresponding to Fig. 1(b)
    Noise of interferograms. (a) When the drive circuit of scanning motor is disabled; (b) when the drive circuit of scanning motor is enabled
    Fig. 2. Noise of interferograms. (a) When the drive circuit of scanning motor is disabled; (b) when the drive circuit of scanning motor is enabled
    Noise of interferograms after the low-frequency fixed noise is filtered. (a) When the drive circuit of scanning motor is disabled; (b) when the drive circuit of scanning motor is enabled
    Fig. 3. Noise of interferograms after the low-frequency fixed noise is filtered. (a) When the drive circuit of scanning motor is disabled; (b) when the drive circuit of scanning motor is enabled
    Noise histograms of interferograms without impulse noise
    Fig. 4. Noise histograms of interferograms without impulse noise
    Noise histograms of interferograms with impulse noise
    Fig. 5. Noise histograms of interferograms with impulse noise
    Comparison of standard deviationin uncalibrated spectra
    Fig. 6. Comparison of standard deviationin uncalibrated spectra
    Frequency spectra of low-frequency fixed noise and Gaussian noise
    Fig. 7. Frequency spectra of low-frequency fixed noise and Gaussian noise
    Predefined mask of interferogram
    Fig. 8. Predefined mask of interferogram
    Result of different impulse noise suppressing methods
    Fig. 9. Result of different impulse noise suppressing methods
    Spectral relative deviation of different impulse noise suppressing methods
    Fig. 10. Spectral relative deviation of different impulse noise suppressing methods
    Results of impulse noise suppression. (a) Amax=30, R=0.01; (b) Amax =60, R=0.01; (c) Amax =60, R=0.1; (d) Amax =60, R=0.05
    Fig. 11. Results of impulse noise suppression. (a) Amax=30, R=0.01; (b) Amax =60, R=0.01; (c) Amax =60, R=0.1; (d) Amax =60, R=0.05
    Interferogram comparison before and after impulse noise suppression
    Fig. 12. Interferogram comparison before and after impulse noise suppression
    NEdN comparison before and after impulse noise suppression
    Fig. 13. NEdN comparison before and after impulse noise suppression
    AmaxRRelative deviation of noisy interferogram /%Relative deviation of denoised interferogram /%
    2000.010.430.15
    300.010.180.14
    600.010.240.17
    600.050.430.17
    600.100.570.19
    Table 1. Comparison of relative deviation after impulse noise suppression
    Lingling Guo, Qichang Zhao, Yong Yang, Shaolin Wang, Rui Shu. Method for Suppression of Impulse Noise in Spaceborne Fourier Transform Infrared Spectrometer[J]. Acta Optica Sinica, 2020, 40(8): 0830003
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