Sodium Nightglow. Chemically Independent of Sodium Content

摘要

The process Na + M yields NaO2 + M apparently is the first in a sequence of reactions which chemically controls the sodium content of the mesosphere. The effectiveness of this reaction is reduced by NaO2 + O yields NaO + O2, which generates only one tenth as much as NaO does the Chapman process Na + O3 yields NAO +O2, using current rate coefficients. Hence Chapman's mechanism, which requires the formation of some Na(superscript 2 p) when NaO reacts with O, remains the principal source of the sodium D-lines at night. However, the net loss of sodium by Na + O3 yields NaO + O2 is small since the reaction between NaO and O is fast and since (O)>>(O3) in the mesosphere. The chemistry of the nightglow, a catalytic cycle with sodium as the catalyst, is shown to be virtually uncoupled from that of the sodium content. It follows that seasonal variations of the content and the nightglow can be fairly independent of each other, as has been observed. Observations that both mesospheric ozone and the sodium nightglow attain maxima during the equinoxes as the dominant source of the sodium nightglow at 5893 A. Keywords: Meteor metals.