ROTATIONAL ANALYSIS OF THE NEAR INFRARED SINGLET-TRIPLET ELECTRONIC SPECTRUM OF OZONE

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1999

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Ohio State University

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High Resolution Fourier Transform Infrared Spectrometry was used to study the rotational fine structure of the lowest energy singlet-triplet electronic spectrum of ozone, $^{16}O_{3}$ and $^{18}O_{3}$ near $9300 cm^{-1}$. With a near pure case (b) coupling model, approximately 100 lines were assigned in the spectrum of $^{16}O_{3}$. A combined least-squares/band contour analysis yielded an overall standard deviation of $0.045 cm^{-1}$. The fit to the ${^{18}}O_{3}$ spectrum used approximately 30 lines and gave a slightly higher overall standard deviation. The rotational analysis has established that the upper state is ${^{3}}A_{2}$ in agreement with recent theoretical calculations. Numerous perturbations are observed in the spectrum of both isotopomers and limited our least-squares fit to the three rotational constants, the symmetric top distortion constants, the three spin-rotation constants and the alpha spin-spin constant. The talk will feature an overview of the rotational analysis along with a brief discussion of the perturbations seen in the spectrum.

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Author Institution: Laboratoire de Spectrom\'{e}trie lonique et Mol\'{e}culaire (associ\'{e} au CNRS U.M.R. 5579), Universit\'{e} Claude Bernard Lyon; Laboratoire de Chimie-Physique, Facult\'{e} des Sciences de Reims; Department of Chemistry, University of Wisconsin-Parkside

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