Instrument line-shape modeling and correction for off-axis detectors in Fourier-transform spectrometry

被引:17
作者
Bowman, KW [1 ]
Worden, HM [1 ]
Beer, R [1 ]
机构
[1] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
关键词
D O I
10.1364/AO.39.003765
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
Spectra measured by off-axis detectors in a high-resolution Fourier-transform spectrometer are characterized by frequency scaling, asymmetry and broadening of their line shape, and self-apodization in the corresponding interferogram. For a narrow-band input spectrum and a specified detector geometry, a formalism is presented that accounts for these effects with separate terms. Some of the terms are used to correct the larger off-axis effects as part of the calibration. The remaining terms are used to model the residual effects with the on-axis instrument line shape. We extend this approach to the broadband case using filter banks. The technique is applied to simulated spectra for the Tropospheric Emissions Spectrometer. This approach is shown to maintain a radiometric accuracy to less than 0.1%. (C) 2000 Optical Society of America.
引用
收藏
页码:3765 / 3773
页数:9
相关论文
共 13 条
  • [1] BEER R, 1989, P SOC PHOTO-OPT INS, V1129, P42
  • [2] BEER R, UNPUB APPL OPT, P16825
  • [3] BEER R, 1996, D11294 JET PROP LAB
  • [4] Bell R.J., 1972, Introductory Fourier Transform Spectroscopy
  • [5] Chamberlain J., 1979, PRINCIPLES INTERFERO
  • [6] Instrument line shape of Fourier transform spectrometers: analytic solutions for nonuniformly illuminated off-axis detectors
    Genest, J
    Tremblay, P
    [J]. APPLIED OPTICS, 1999, 38 (25) : 5438 - 5446
  • [7] Mallat S., 2008, A wavelet tour of signal processing: The sparse way, Vthird
  • [8] MALLIARD J, 1994, P SOC PHOTO-OPT INS, V2198, P185
  • [9] Oppenheim A. V., 1989, DISCRETE TIME SIGNAL
  • [10] Imaging spectrometers for future Earth observing systems
    Puschell, JJ
    Tompkins, P
    [J]. EARTH OBSERVING SYSTEMS II, 1997, 3117 : 36 - 48