A discussion of the energy transfer from N2(A3Σu+) to O(1S) in pulsating aurora

Details A discussion of the energy transfer from N2(A3Σu+) to O(1S) in pulsating aurora A discussion of the energy transfer from N2(A3Σu+) to O(1S) in pulsating aurora

Apr 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973p%26ss...21..698b&link_type=abstract

Planetary and Space Science, Volume 21, Issue 4, p. 698-702.

Physics

Scientific paper

In a recent paper, Brekke and Pettersen (1972) have introduced a method for estimating any indirect process in the production of the O(1S) atoms in pulsating aurora; for 38 per cent of their data they found that the decay time for the indirect mechanism was shorter than the effective lifetime of the 1S state. These data are related to the energy transfer from the N2(A3Σ) molecules to the O(1S) state, and evidence is found for this process to contribute in the altitude range below 125 km. Present address: University of California, San Diego, Department of Applied Physics and Information Science, La Jolla, California 92037, U.S.A.

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