Variations, with peak emission altitude, in auroral O-2 atmospheric (1,1)/(0,1) ratio and its relation to other auroral emissions

Spectral distributions of auroral optical emissions, peaked at distinctly d ifferent heights in the thermosphere, show significant variations, with alt itude, in the O-2 atmospheric (1, 1)/(0, 1) band ratio. The latter increase s with height in auroras peaked between 110 and 150 km and then gradually d ecreases at higher altitudes. To minimize ambiguities associated with auror al height determination needed for investigating this effect, four independ ent height-assessment methods are employed. The first one is based on the i ncoherent scatter radar (ISR) soundings of the auroral ionization profile f rom which the height, where precipitating particles dissipate most of their energy, can be determined. Concurrent spectroscopic observations of the th ermalized rotational distributions of auroral band emissions yield the ambi ent air temperature, and hence an independent assessment of the height, of the thermospheric region where these emissions peak. Changes in O/O-2 and O /N-2 ratios with height lead to changes in the ratios of auroral emissions, from these species, peaked at different heights. Finally, changes in colli sion frequency with height lead to changes in the brightness of the auroral emissions, resulting from radiatively allowed transitions relative to thos e produced from radiatively forbidden transitions. The four methods yield c omparable values for the height of the thermospheric region where emissions , from each auroral event, peak. The observed variations in O-2 atmospheric (1, 1)/(0, 1) with auroral height is compared with that expected from O (D -1) + O-2 excitation source and quenching by O-2 and O. The effects of elec tron impact excitation of O-2 (b(1)Sigma(g)(+), v') and high rotational lev els of the P branch of O-2 atmospheric (0, 0) band on O-2 atmospheric (1, 1 )/(0, 1) ratio are discussed. Quantitative ratios of various auroral emissi ons, from O, N-2, and N-2(+), peaked at different heights, that can provide an assessment of auroral heights where these emissions peak, are listed.