HIGH RESOLUTION INFRARED SPECTRA AND VIB-ROTATIONAL ANALYSIS OF THE $\nu_{3}$ AND $\nu_{4}$ REGIONS OF CHLORINE NITRATE IN THE TEMPERATURE RANGE 190 TO 297 K

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2002

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Ohio State University

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Chlorine nitrate plays an important role in upper atmospheric chemistry. It was first detected in the stratosphere by Rinsland etal.a by observation of the ν4 band a-type Q-branch. There have been a number of laboratory infrared spectroscopic studies on the ν4 band since that ime.b Among them is the work of Bell, DuxburyandStuartc who used a tunable diode laser to study and model the a-type Q-branches of the two chlorine isotopic species 35Cl and 37Cl as well as that of the ν4+ν9ν9 hot band. At room temperature, even at the high resolution of a diode laser, the bands are only partially resolved due to the overlapping of lines of the two main isotopic species and of lines from several strong hot bands. A beautifully resolved spectrum of the ν4 region over a limited range of J and Ka was obtained later by Xu,BlakeandSharped from diode laser spectra of a molecular jet at about 7 K. In this work, 29 spectra of the region 750 to 900cm−1 at temperatures ranging from 190 to 297 K and air pressures ranging from zero to 156 hPa were recorded at DLR with resolutions of 0.00094 to 0.0083cm−1. Using the ground-state constants of M\""ulleretal.e a vib-rotational analysis of the ν4 and ν3 fundamental bands as well the hot band, ν4+ν9ν9, of the most abundant 35Cl isotopomer was carried out using the spectrum recorded at 191 K with the highest resolution and a zero air pressure. The corresponding cold bands for the lesser abundant isotope were partially assigned. Upper state rotational Hamiltonian constants were determined allowing precise modeling of the contours of the ν4 fundamental Q-branches over the temperature and pressure ranges studied as shown by comparisons with the other spectra.

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aC. P. Rinsland et al., J. Geophys. Res. D 90, 7931 (1985). bA. Goldman, C. P. Rinsland, J.-M. Flaud, and J. Orphal, J. Quant. Spectrosc. Rad. Transf. 60, 875 (1998). cW. Bell, G. Duxbury, and D. D. Stuart, J. Mol. Spectrosc. 152, 283 (1992). dS. Xu, T. A. Blake, and S. W. Sharpe, J. Mol. Spectrosc. 183, 228 (1996). eH. S. P. M""uller, P. Helminger, and S. H. Young, J. Mol. Spectrosc. 181, 363 (1997).


Author Institution: CNRS, Laboratoire de Photophysique Mol'{e}culaire; Optical Technology Division, NIST Gaithersburg; Optical Technology Division, Institute for Optoelectronics

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