Abstract
The FIRS-2 is a far- to mid-infrared Fourier transform spectrometer, designed and built at the Smithsonian Astrophysical Observatory for the purpose of measuring stratospheric emission spectra. The instrument and data reduction system have been described elsewhere [Johnson et al., 1994]. We present here the method we have developed for phase recovery from highly asymmetric interferograms in the presence of an out-of-phase background signal.
© 1995 Optical Society of America
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