Measurements of night-time 6300 Å airglow intensities at the Arecibo Observatory have been compared with dissociative recombination calculations based on electron densities derived from simultaneous incoherent backscatter measurements. The agreement indicates that the nightglow can be fully accounted for by dissociative recombination. The comparisons are examined to determine the importance of quenching, heavy ions, ionization above the F-layer peak, and the temperature parameter of the model atmosphere. Comparable fits between the observed and calculated intensities are found for several available model atmospheres (e.g. CIRA, Jacchia). The least-squares fitting process, used to make the comparisons, produces comparable fits over a wide range of combinations of neutral densities and of reaction constants. Yet, the fitting places constraints upon the possible combinations: these constraints indicate that the latest laboratory chemical constants and densities extrapolated to a base altitude are mutually consistent. However, by imposing an additional constraint, an aeronomically derived preference is given for about one O(1D) per combination. A preference is also given for the lower base densities of O2 derived from rockets rather than from models. Altitude profiles for the 6300 Å and 5577 Å emissions are deduced. In the early evening, there are no large discrepancies in the fits that might indicate an effect from elicited states of O+, vibrational excitation of O2, or both. The technique of comparing observed and calculated 6300 Å intensities has considerable potential as an aeronomical tool for examination of other possible sources of emission and for determination of relative changes in the neutral atmosphere.
The 6300Å O(1D) Airglow and Dissociative RecombinationPlanetary and Space Science
Citation InformationV.B. Wickwar, L.L. Cogger, H.C. Carlson, The 6300 Å O1D airglow and dissociative recombination, Planetary and Space Science, Volume 22, Issue 5, May 1974, Pages 709-724, ISSN 0032-0633, 10.1016/0032-0633(74)90141-X. (http://www.sciencedirect.com/science/article/pii/003206337490141X)