Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.251..147d&link_type=abstract
In ESA Proceedings of the Joint Varenna-Abastumani International School and Workshop on Plasma Astrophysics p 147-150 (SEE N87-
Astronomy and Astrophysics
Astrophysics
F Region, Gravity Waves, Nightglow, Oxygen Spectra, Solitary Waves, Electron Density Profiles, Ionospheric Electron Density, Wind Effects
Scientific paper
The behavior of electron density at night F-region of the Earth ionosphere and the influence of atmospheric gravity wave solitons (SAGW) are investigated. The horizontal wind is taken into account. It turns out that the height of the electron density maximum changes depending on directions of the soliton drift velocity and wind. The electron density peak falls when SAGW drifts from north to south and it rises when the drift direction is from south to north. The results are used to explain the airglow oxygen red line 6300A intensity progression.
Didebulidze G. G.
Fishkova L. M.
Pataraya D.
No associations
LandOfFree
Investigation on the intensity progression of F-region nightglow emission of the oxygen red line by means of atmospheric gravity waves soliton does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Investigation on the intensity progression of F-region nightglow emission of the oxygen red line by means of atmospheric gravity waves soliton, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Investigation on the intensity progression of F-region nightglow emission of the oxygen red line by means of atmospheric gravity waves soliton will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-892348