HIGH RESOLUTION IR SPECTRA AND ANALYSIS OF THE $\nu_{9}$ BAND OF ETHANE
Stephen J. Daunt, W. E. Blass, George W. Halsey, Kenneth R. Fox, R. J. Lovell, Herbert Flicker, John A. King
Abstract
Stephen J. Daunt, W. E. Blass, George W. Halsey, Kenneth R. Fox, R. J. Lovell, Herbert Flicker, John A. King
Abstract
The fundamental band of $C_{2}H_{6}$ at $822\\;cm^{-1}$ has been analyzed using new spectra taken with the UT grating Instrument $(\\Delta \\nu = 0.04 - 0.05\\;cm^{-1})$, and the UT and LASL interferometric instruments $(\\Delta \\nu = 0.125 - 0.500\\;cm^{-1}$ and $\\Delta \\nu = 0.040\\;cm^{-1}$, respectively). We have obtained the following preliminary values of excited state constants: \\begin{eqnarray*} \\nu_{0}&=&821.738\\;cm^{-1}\\\\ \\alpha_{9}^{B}&=&(B^{\\prime\\prime}-B^{\\prime})=+1.29\\times 10^{-3}\\;cm^{-1}\\\\ \\alpha_{9}^{A}&=&(A^{\\prime\\prime}-A^{\\prime})=-7.5\\times 10^{-3}\\;cm^{-1}\\\\ \\zeta_{9}^{Z}&=&+0.259\\\\ q_{9}{^{(+)}}&=&-1.8\\times 10^{-3}\\;cm^{-1}\\\\ \\end{eqnarray*} In this analysis we used improved ground state parameters obtained from GSCD fits of the $\\nu_{9} + \\nu_{12}$ band by Blass and Lin, These constants will be presented in another paper at this meeting.
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The fundamental band of $C_{2}H_{6}$ at $822\\;cm^{-1}$ has been analyzed using new spectra taken with the UT grating Instrument $(\\Delta \\nu = 0.04 - 0.05\\;cm^{-1})$, and the UT and LASL interferometric instruments $(\\Delta \\nu = 0.125 - 0.500\\;cm^{-1}$ and $\\Delta \\nu = 0.040\\;cm^{-1}$, respectively). We have obtained the following preliminary values of excited state constants: \\begin{eqnarray*} \\nu_{0}&=&821.738\\;cm^{-1}\\\\ \\alpha_{9}^{B}&=&(B^{\\prime\\prime}-B^{\\prime})=+1.29\\times 10^{-3}\\;cm^{-1}\\\\ \\alpha_{9}^{A}&=&(A^{\\prime\\prime}-A^{\\prime})=-7.5\\times 10^{-3}\\;cm^{-1}\\\\ \\zeta_{9}^{Z}&=&+0.259\\\\ q_{9}{^{(+)}}&=&-1.8\\times 10^{-3}\\;cm^{-1}\\\\ \\end{eqnarray*} In this analysis we used improved ground state parameters obtained from GSCD fits of the $\\nu_{9} + \\nu_{12}$ band by Blass and Lin, These constants will be presented in another paper at this meeting.
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