INFRARED LINE INTENSITIES OF ClO FROM HIGH RESOLUTION FOURIER TRANSFORM SPECTROSCOPY$^{\wedge}$

$^{\wedge}$This research is supported, in part, by the NASA Upper Atmosphere Program.Author Institution: Laboratory for Extraterrestrial Physics, NASA/Goddard Space Flight CenterInfrared line intensities of C10 in the fundamental rotation-vibration (1-0) band near $850 cm^{-1}$ are inferred from a (Herman-Wallis type) rotation-vibration interaction analysis of Fourier transform spectra. These data were recorded with the one-meter FTS located at the McMath solar telescope at the National Solar Observatory. The FTS was used in the double-pass mode to produce an unapodized spectral resolution of $0.0025 cm^{-1}$. We will present details of the experiment, results of the analysis, comparison with previous works, and a discussion of the intrinsic sensitivity of the technique for the determination of vibrational band intensities