Nitrogen I 3F (2P-2D) emissions in the aurora

Details Nitrogen I 3F (2P-2D) emissions in the aurora Nitrogen I 3F (2P-2D) emissions in the aurora

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989jgr....94.2595p&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 94, March 1, 1989, p. 2595-2604.

Physics

3

Auroral Spectroscopy, Gas Spectroscopy, Infrared Spectroscopy, Near Infrared Radiation, Nitrogen, Fourier Transformation, Molecular Collisions, Night Sky, Spectral Bands

Scientific paper

FT IR spectroscopy with a field-widened Michelson interferometer has been used to obtain improved forbidden N I 3F (2P-2D) multiplet observations. Reliable component emission rates were extracted from the spectrally blended data by fitting a set of critically evaluated, high-quality synthetic spectral components to the data. These improved observations have yielded an intramultiplet intensity ratio that is in agreement with the theoretical statistical equilibrium ratio for a wide range of auroral heights. A strong correlation is also established between the forbidden N I 3F emission rate and that of the forbidden O I 1F multiplet.

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