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- W2020148251 abstract "Abstract The chemical equilibrium of sodium in the upper atmosphere is shown to lead to a peaked distribution of sodium atoms, the peak coinciding with the transition from O 2 to O. Curves for the intensity of the twilight emission of the D -lines are calculated for three model distributions. A study of the ionization of sodium by sunlight suggests that an annual intensity variation similar to the observed one should result, and that any evening-morning intensity difference should be greatest at the equinoxes. Observations are reported in another paper." @default.
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- W2020148251 title "A study of sodium in twilight. I. Theory" @default.
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