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High resolution analysis of the rotational levels of the (0 0 0), (0 1 0), (1 0 0), (0 0 1), (0 2 0), (1 1 0) and (0 1 1) vibrational states of SO2
Authors:WJ Lafferty  J-M Flaud  El Hadji Abib Ngom
Institution:a Optical Physics Laboratory, National Institutes of Standards and Technology, 100 Bureau Drive, Room B260, MS 8441, Gaithersburg, MD 20899-8441, USA
b Laboratoire Inter Universitaire des Systemes Atmosphériques, CNRS, Universités Paris-Est et Paris 7, 61 Av du General de Gaulle, 94010 Créteil Cedex, France
c Pacific Northwest National Laboratory, P.O. Box 999, Richland, WA 99352, USA
d University of Cheikh Anta Diop, Ecole Supérieure Polytechnique, BP 5085, Dakar, Senegal
Abstract:A high resolution (0.0018 cm−1) Fourier transform instrument has been used to record the spectrum of an enriched 34S (95.3%) sample of sulfur dioxide. A thorough analysis of the ν2, 2ν2 − ν2, ν1, ν1 + ν2 − ν2, ν3, ν2 + ν3 − ν2, ν1 + ν2 and ν2 + ν3 bands has been carried out leading to a large set of assigned lines. From these lines ground state combination differences were obtained and fit together with the existing microwave, millimeter, and terahertz rotational lines. An improved set of ground state rotational constants were obtained. Next, the upper state rotational levels were fit. For the (0 1 0), (1 1 0) and (0 1 1) states, a simple Watson-type Hamiltonian sufficed. However, it was necessary to include explicitly interacting terms in the Hamiltonian matrix in order to fit the rotational levels of the (0 2 0), (1 0 0) and (1 0 1) states to within their experimental accuracy. More explicitly, it was necessary to use a ΔK = 2 term to model the Fermi interaction between the (0 2 0) and (1 0 0) levels and a ΔK = 3 term to model the Coriolis interaction between the (1 0 0) and (0 0 1) levels. Precise Hamiltonian constants were derived for the (0 0 0), (0 1 0), (1 0 0), (0 0 1), (0 2 0), (1 1 0) and (0 1 1) vibrational states.
Keywords:Rovibrational energy levels  34SO2  Infrared spectra  Fermi and Coriolis resonances  Hamiltonian constants
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