15min:

N. MOAZZEN-AHMADI, Department of Physics and Astronomy, University of Calgary, Calgary, AB T2N 1N4, Canada; V.-H. HORNEMAN, Department of Physical Sciences, University of Oulu, PO Box 3000, Fin-90014, Oulu, Finland.

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 ₉ and ₃ fundamentals, the ₉- ₄- ₄ hot band, and the ₁₂- ₉ difference band.

Because measurements of ¹²C/¹³C 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 ¹³CH₃CH₃. We have already reported a global fit which included data from the torsional bands, and the ₁₂ and ₅ fundamentals. In this work we describe a global fit which also includes data from ₁₂+ ₆- ₆ and ₁₁- ₁₂ bands.