Recent evidence has shown that the mesospheric sodium nightglow, a chemiluminescent process which produces atomic sodium D-line radiation in the Earth's upper atmosphere, proceeds through the first excited (A 2 Σ + ) electronic state of NaO. The rate of D-line radiation production is proportional to the rate constant for the reaction of NaO(A 2 Σ + ) + O( 3 P) and its branching ratio to produce excited Na( 2 P) rather than ground-state Na( 2 S). The only previously published measurement of the NaO + O( 3 P) reaction rate and branching ratio was performed under slow flow conditions and almost certainly primarily represents the reaction of ground-state NaO (X 2 Π). We present low-pressure measurements of the NaO + O reaction kinetics using an NaO source reaction known to produce NaO in the (A 2 Σ + ) state and determine the 290 K reaction rate constant to be (5.1 ± 1.8) × 10 -10 cm 3 s -1 and the branching ratio to produce Na( 2 P) to be 0.14 ± 0.04. New data on the termolecular rate coefficient for the reaction Na + O 2 + He → NaO 2 + He at 290 K are also presented.
No takes yet. Share an insight, caveat, or question.
Griffin et al. (2000) studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: