A recovery procedure has been developed to correct instrument line-sha
pe distortions observed in Fourier transform spectroscopy. The procedu
re can be described as a phase-error collection performed in the spect
ral domain to correct for path-difference-dependent phase errors obser
ved in sharp spectral features. The technique has been applied success
fully to high-resolution atmospheric emission spectra. The inherent br
oadening of the real features has been separated accurately from instr
umental distortions. Using models for the path-difference-dependent er
ror sources and data from two narrow window regions at 50 and 118 cm(-
1), we show that the distortion has a simple dependence on the spectra
l frequency. (C) 1998 Optical Society of America.