Oxygen emissions in the night airglow of the earth, Venus and Mars

Details Oxygen emissions in the night airglow of the earth, Venus and Mars Oxygen emissions in the night airglow of the earth, Venus and Mars

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986p%26ss...34..511k&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 34, June 1986, p. 511-518.

Physics

Atomic Physics

30

Earth Atmosphere, Emission Spectra, Mars Atmosphere, Nightglow, Oxygen Spectra, Venus Atmosphere, Airglow, Atomic Excitations, Atomic Recombination, Energy Transfer, Metastable State, Oxygen Recombination, Quenching (Atomic Physics), Vertical Distribution

Scientific paper

Airglow data are analyzed to obtain a set of excitation, energy transfer and quenching reactions and their rate coefficients. To reduce the number of reactions a restriction is imposed on the reactions proceeding via planar collisional complexes with all reactants and products in Σ or S states. The airglow altitude profiles measured can be explained by the excitation of five metastable O2 states and O(1S) via a common precursor having the ratio of the rate coefficient of quenching by O to that by O2 equal to 5. Only O2(2πg) satisfies all constraints imposed on this precursor.

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