THE $^{18}O_{3}$ ABSOPTION SPECTRUM $3.3 \mu m$.

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1989

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Ohio State University

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Spectra of ozone generated from a 99.98% pure oxygen sample were recorded covering the 2800−3500cm−1 at 0.010cm−1 resolution with the McMath Fourier transform interferometer at the National Solar Observatory on Kitt Peak. The first extensive analysis of the 4 bands 3ν3,2ν3+ν1,2ν1+ν3 and 3ν1 absorbing in this spectral region has been performed leading to a precise set of rotational energy levels for the 4 vibrational interacting states ((003), (201), (102), (300)). These experimental levels were then reproduced with the aid of a Hamiltonian taking into account the various resonances (Coriolis, Darling-Dennison) affecting the levels. Moreover, using the equivalent width method, intensities of lines belonging to the four bands were measured with a relative uncertainty of about 10% and used to determine the corresponding transition moment constants. Finally, from the vibrational energies, rotational and coupling constants as well as transition moment constants a complete and precise list of the line positions and intensities of the 3ν3,2ν3+ν1,ν3+2ν1 and 3ν1 bands of 16O3 has been generated.

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Author Institution: Laboratoire de Physique Mol'eculaire et Atmosph'erique, Tour 13. Universit'e Pierre et Marie Curie et CNRS; Atmospheric Sciences Division, MS 401A, NASA Langley Research Center; Department of Physics, College of William and Mary; Groupe de Spectrom'etrie Mol'eculaire et Atmosph'erique, Facult'e des Sciences

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