Modelling the VUV emission spectrum of N2:  preliminary results on the effects of rotational interactions on line intensities.
A theoretical model of the excited singlet ungerade electronic states of the nitrogen molecule is presented.  This work is an extension of a previous study (D. Stahel, M. Leoni and K. Dressler, J. Chem. Phys. 79, 2541-2558, 1983) with the addition of rotational interactions between states of different symmetry.  These rotational interactions together with the homogeneous couplings frequently lead to extreme mixing of the states.  This model is being used to analyse the high resolution vacuum ultraviolet emission spectrum which is currently being recorded photoelectrically.  The ultimate goal of this work is the reliable interpretation of the low resolution emission spectra observed from planetary atmospheres, notably that of Titan, and the transitions assigned as being important in the Voyager 1 spectra of Titan are discussed in detail.
Edwards
S A
SA
Observatoire de Paris-Meudon, Meudon, France.
Tchang-Brillet
W U
WU
Roncin
J Y
JY
Launay
F
F
Rostas
F
F
D001272:Atmosphere; D004735:Energy Transfer; D018559:Exobiology; D005118:Extraterrestrial Environment; D008958:Models, Molecular; D009584:Nitrogen / Q000032:analysis*; D018539:Saturn; D013056:Spectrophotometry, Ultraviolet / Q000379:methods*
D009584:Nitrogen