LINE POSITIONS AND INTENSITIES OF PHOSPHINE IN THE $3\mu$m REGION FOR PLANETARY APPLICATIONS

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2004

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Ohio State University

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Seven absorption bands of PH3 at 3μm, i.e 3ν2,2ν2+ν4, 2ν4+ν2,ν1+ν2,ν3+ν2, ν3+ν4 and ν1+ν4 were simultaneously analysed from spectra recorded at a resolution of 0.012cm−1 using the Fourier transform spectrometer located at the Kitt Peak Observatorya. A theoretical model suited to the strong vibro-rotational couplings among the seven bands was used. Using ground state combination differences, several hundred transitions have been assigned for these seven bands in the range 2750−3600cm−1. At present a set of 33 energy parameters was required to reproduce the experimental wavenumbers for six bands with an overall standard deviation of 0.1cm−1 up to J = 9. 1355 lines were also measured and their analysis is underway. The final objective is to provide a complete prediction of line positions and intensities of Phosphine at 3μm for remote sensing of Saturn.

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a Part of the research reported in this paper was performed at the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.


Author Institution: Laboratoire de Photophysique Mol'{e}culaire, Universit'{e} Paris Sud; Jet Propulsion Laboratory, California Institute of Technology

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