The O2/b 1Sigma g+/ - X/3Sigma g-/ system in aurora

Details The O2/b 1Sigma g+/ - X/3Sigma g-/ system in aurora The O2/b 1Sigma g+/ - X/3Sigma g-/ system in aurora

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974jgr....79.4821j&link_type=abstract

Journal of Geophysical Research, vol. 79, Nov. 1, 1974, p. 4821, 4822.

Physics

4

Auroral Spectroscopy, Energy Transfer, Infrared Spectra, Oxygen Spectra, Emission Spectra, Line Spectra, Molecular Energy Levels, Molecular Excitation, Spectral Bands

Scientific paper

Emissions from the O2 atmospheric band system with V-prime not greater than 5 have been identified in auroral spectra, contrary to the previous belief that only bands with V-prime not greater than 2 were present. The intensities of the observed bands, referred to I (5577), have been determined for medium intensity aurora. Excitation mechanisms involving energy transfer from O(1S), N(2D), and O(1D) have been considered.

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