dc.creator Moazzen-Ahmadi, N. en_US dc.creator Horneman, V.-H. en_US dc.date.accessioned 2012-07-09T18:50:50Z dc.date.available 2012-07-09T18:50:50Z dc.date.issued 2012 en_US dc.identifier 2012-FA-10 en_US dc.identifier.uri http://hdl.handle.net/1811/52170 dc.description Author Institution: Department of Physics and Astronomy, University of Calgary, Calgary, AB T2N; 1N4, Canada; Department of Physical Sciences, University of Oulu, PO Box 3000, Fin-90014, Oulu, Finland en_US dc.description.abstract Accuracy of the retrieved abundances for ethane from planetary atmospheres is directly linked to the quality of the spectroscopic parameters which are obtained from laboratory studies. For this reason, we have made several detailed studies of the lowest four vibrational states of ethane. We have previously reported global fits including data from the torsional bands in the ground vibrational state, the $\nu_9$ and $\nu_3$ fundamentals, the $\nu_9-\nu_4-\nu_4$ hot band, and the $\nu_{12}-\nu_9$ difference band. Because measurements of $^{12}$C/$^{13}$C and other isotope ratios are used to study the fractionation processes and to make inferences regarding the evolution of the planetary atmospheres, it is desirable to also have high quality spectroscopic parameters for the lowest four vibrational states of $^{13}$CH$_3$CH$_3$. We have already reported a global fit which included data from the torsional bands, and the $\nu_{12}$ and $\nu_{5}$ fundamentals. In this work we describe a global fit which also includes data from $\nu_{12}+\nu_6-\nu_6$ and $\nu_{11}-\nu_{12}$ bands. en_US dc.language.iso en en_US dc.publisher Ohio State University en_US dc.title A GLOBAL FREQUENCY ANALYSIS OF $^{13}$CH$_3$CH$_3$ INCLUDING DATA FROM THE LOWEST FOUR VIBATIONAL STATES en_US dc.type Article en_US dc.type Image en_US dc.type Presentation en_US
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