Translationally hot O( 3P) atoms are produced in the atmosphere of Earth by photolysis of O 2 and O 3 and quenching of O( 1D). A rigorous kinetic theory analysis of this problem is developed and compared with the approach previously employed by Logan and McElroy [ Planet. Space Sci. 25, 117 (1977)]. It is shown that the kinetic theory employed by the previous workers is somewhat deficient. With the line-of-centers cross-section, the rates of reactions of the translationally hot O( 3P) atoms with other atmospheric gases are calculated and found to be in some instances many orders of magnitude larger than the equilibrium rates. Though the non-equilibrium reaction rates with O( 3P) are substantially increased, they are still not competitive with the corresponding reaction rates with O( 1D).
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