Auroral N2(c prime 4 1Sigma/+/ - a1Pi g) emission, II

Details Auroral N2(c prime 4 1Sigma/+/ - a1Pi g) emission, II Auroral N2(c prime 4 1Sigma/+/ - a1Pi g) emission, II

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986p%26ss...34..399s&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 34, April 1986, p. 399-401.

Physics

9

Auroras, Emission Spectra, Nitrogen Ions, Energy Bands, Franck-Condon Principle

Scientific paper

A determination by Filippelli et al. of the branching ratio between N2(c prime 4 1Sigma u/+/) emission to the ground state and the a1Pi g state indicate that our earlier estimate of auroral N2(c prime 4 - X) emission intensities is too low, and that more than 1 MR is expected in this transition. The intensities of the bands in the N2(c prime 4 - a) O-V double prime progression follow values calculated on the basis of a transition moment invariant with internuclear separation.

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