Transport of aurorally produced N(2D) by winds in the high latitude thermosphere
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference37 articles.
1. The energy spectrum of primary auroral electrons determined from auroral luminosity profiles;Belon;Planet. Space Sci.,1966
2. Vacuum-ultraviolet photolysis of N2, d, deactivation of N(2D);Black;J. chem. Phys.,1969
3. The quenching of N(2d) by O(3P);Davenport;J. geophys. Res.,1976
4. Rocket measurements of oxygen and nitrogen emissions in the aurora;Deans;Planet. Space Sci.,1978
5. A three-dimensional general circulation model of the thermosphere;Dickinson;J. geophys. Res.,1980
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2. Observation and analysis of NI 520.0 nm auroral emissions;Journal of Atmospheric and Terrestrial Physics;1996-04
3. Interpretation of satellite airglow observations during the March 22, 1979, magnetic storm, using the coupled ionosphere-thermosphere model developed at University College London;Journal of Geophysical Research;1994
4. N(2D) + O2: A source of thermospheric 6300 Å emission?;Planetary and Space Science;1992-05
5. A theoretical study of thermospheric composition perturbations during an impulsive geomagnetic storm;Journal of Geophysical Research: Space Physics;1991-08-01
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