Nitric oxide excited under auroral conditions: Excited state densities and band emissions

Electron impact excitation of vibrational levels in the ground electronic state and nine excited electronic states in NO has been simulated for an IBC II aurora (i.e., similar to 10 kR in 3914 Angstrom radiation) in ol der to predict NO excited state number densities and band emission intensities. New integral electron impact excitation cross sections for NO were combined with a measured IBC II auroral secondary electron distribution, and the vibrational populations of 10 NO electronic states were determined under conditions of statistical equilibrium. This model predicts an extended vibrational distribution in the NO ground electronic state produced by radiative cascade from the seven higher-lying doublet excited electronic states populated by electron impact. In addition to significant energy storage in vibrational excitation of the ground electronic state, both the a (4)Pi L(2)Phi excited electronic states are predicted to have relatively high number densities because they are only weakly connected to lower electronic stales by radiative decay. Fundamental mode radiative transitions involving the lowest nine excited vibrational levels in the ground electronic state are predicted to produce infrared (IR) radiation from 5.33 to 6.05 mu m with greater intensity than any single NO electronic emission band. Fundamental mode radiative transitions within the a (4)Pi, electronic state, in the 10.08-11.37 mu m region, are predicted to have IR intensities comparable to individual electronic emission bands in the Heath and epsilon band systems. Results from this model quantitatively predict the vibrational quantum number dependence of the NO IR measurements of Espy et al. [1988].