Observation of O+(2P0-2D0)λ7,319Å emissions in the twilight and night airglow

Details Observation of O+(2P0-2D0)λ7,319Å emissions in the twilight and night airglow Observation of O+(2P0-2D0)λ7,319Å emissions in the twilight and night airglow

Mar 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974natur.248..400c&link_type=abstract

Nature, Volume 248, Issue 5447, pp. 400-401 (1974).

Physics

1

Scientific paper

TEN years ago Dalgarno and McElroy1 suggested that the
2P0 --> 2D0 transition of
the atomic oxygen ion would be produced in the upper atmosphere through
the simultaneous photoionisation and excitation of atomic oxygen atoms
by solar ultraviolet radiation.

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