15min:
HIGH-RESOLUTION INFRARED AND RAMAN SPECTROSCOPY OF SF6: THE STATE-OF-THE-ART IN JUNE 2006.

V. BOUDON, LPUB -- CNRS UMR 5027, 9 Av. A. Savary, BP 47870, F-21078 Dijon Cedex, France; J. L. DOMÉNECH AND D. BERMEJO, Instituto de Estructura de la Materia, CSIC Serrano 123, E-28006 Madrid, Spain; E. B. MKADMI, H. BÜRGER, H. WILLNER, Fachbereich C -- Anorganische Chemie, Bergische Universität Wuppertal, D-42097 Wuppertal, Germany; N. LACOME, LADIR -- CNRS UMR 7075, Case Courrier 49, 4 Place Jussieu, F-75252 Paris Cedex 05, France.

Sulfur hexafluoride is recognized by the Kyoto Protocol as a powerful greenhouse gas whose emissions should be monitored and reduced. Although its abundance is still relatively small (3.8× 10-6 ppmv), it is increasing rapidly (8 %/year) while the lifetime of SF6 in the atmosphere is extremely long (3200 years) with a Global Warming Potential equal to 23900 compared to CO2,. It is thus necessary to correctly model the atmospheric absorption of SF6, especially in the strongly absorbing nu3 region (near 939 cm-1). Until recently, however, respective spectra were not very well known. In particular, the knowledge of hot bands is very important for atmospheric applications, but this implies to study various vibrational levels, some being only accessible through Raman scattering. During the past decade, we have analyzed different fundamental, harmonic and combination bands for both 32SF6 and 34SF6 using high-resolution infrared and Raman spectra\footnoteSee for instance V. Boudon and N. Lacome, J. Mol. Spectrocsc.\/ 222, 291--295 (2003), V. Boudon, J. L. Doménech, D. Bermejo and H. Willner, J. Mol. Spectrosc.\/ 228, 392--400 (2004) and references therein.. In this talk, we will discuss the present status and prospects of SF6 spectroscopy. In particular, new spectra and analyses of 34SF6 will be reported and discussed. We will also show that a correct modelling of absorption intensities is still a pending question.