THE $\nu_{2}$ BAND OF HOBr

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1986

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Ohio State University

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The $\nu_{2}$ band of HOBr has been observed at $0.0056cm^{-1}$ resolution using the McMath Solar Telescope Fourier transform spectrometer at Kitt Peak National Observatory. Although some difficulty was encountered generating the sample, transitions were assignable for $Ka<5$ and $J<42$. Coriolis resonances have been observed between the $Ka=2$ levels of $v_{2}$ and the otherwise unobservable $Ka=1$ levels of $2\nu_{3}$. The spectrum will be described and molecular parameters for $\nu_{2}, 2\nu_{3}$ and their interaction will be presented.

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Address of Cohen and McRae: Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109, USA
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