Nightglow emissions of OH(X²π): Comparison of theory and measurements in the (9-3) band
- 1 January 1978
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 83 (A6) , 2441
- https://doi.org/10.1029/ja083ia06p02441
Abstract
No abstract availableKeywords
This publication has 27 references indexed in Scilit:
- Ozone Abundances in the Lower Mesosphere Deduced from Backscattered Solar RadiancesJournal of the Atmospheric Sciences, 1977
- Atomic resonance fluorescence for rate constants of rapid bimolecular reactions. Part 5—Hydrogen atom reactions; H + NO2and H + O3Journal of the Chemical Society, Faraday Transactions 2: Molecular and Chemical Physics, 1977
- Contamination of the O I (³P2-¹D2) emission line by the (9-3) band of OHX²II in high-resolution measurements of the night skyJournal of Geophysical Research, 1974
- The visible‐airglow experiment on Atmosphere ExplorerRadio Science, 1973
- Atomic hydrogen concentrations in the mesosphere and the hydroxyl emissionsJournal of Geophysical Research, 1973
- Formation of Vibrationally Excited OH by the Reaction H + O_3Applied Optics, 1971
- Rocket-borne ultraviolet spectrometer measurement of OH resonance fluorescence with a diffusive transport model for mesospheric photochemistryJournal of Geophysical Research, 1971
- Interpretation of Airglow in Terms of Excitation MechanismsPublished by Springer Nature ,1971
- The airglow spectrum, 3100-10,000 AJournal of Geophysical Research, 1968
- The photochemistry of atmospheric water vaporJournal of Geophysical Research, 1950