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dc.creatorCamy-Peyret, C.en_US
dc.creatorFlaud, J.- M.en_US
dc.creatorJohns, J. W. C.en_US
dc.date.accessioned2006-06-15T14:44:41Z
dc.date.available2006-06-15T14:44:41Z
dc.date.issued1983en_US
dc.identifier1983-FA-02en_US
dc.identifier.urihttp://hdl.handle.net/1811/11765
dc.descriptionAuthor Institution: Laboratoire de Physique, Mol\'eculaire et d'optique, Atmosph\'erique C N R S; Herzberg Institute of Astrophysics N.R.C., Ottawa Ontario K 1A OR6, Canada.en_US
dc.description.abstractThe pure rotation spectrum of hydrogen Sulfide has been recorded between 50 and $300 cm^{-1}$ on a Fourier transform spectrometer with a resolution of $0.005 cm^{-1}$. This high resolution and a good signal to noise ratio has allowed a real improvement in the precision of the wavenumbers of the rotational transitions of the three isotopic species$ H_{2}^{32}S$, $H_{2}^{33}S$, and $H_{2}^{34}S$ observed in natural abundance. Lines with J as high as 22 or $K_{a}$ as high as l5 have been observed for the most abundant isotope. Then for each isotope, the far infrared rotational transitions together with the available microwave data have been introduced in a least squares fit leading to the determination of precise Watson’s rotational constants. Finally using these constants and a permanent dipole moment $^{o}\mu_{x} = 0.974$ D, the absorption of hydrogen sulfide in the far infrared region of the spectrum has been computed.en_US
dc.format.extent91537 bytes
dc.format.mimetypeimage/jpeg
dc.language.isoEnglishen_US
dc.publisherOhio State Universityen_US
dc.titleTHE PURE ROTATION SPECTRUM OF HYDROGEN SULFIDEen_US
dc.typearticleen_US


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