Physics
Scientific paper
Oct 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ge%26ae..30..782k&link_type=abstract
Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 30, Sept.-Oct. 1990, p. 782-787. In Russian.
Physics
Airglow, Auroral Arcs, Ion Cyclotron Radiation, Plasmasphere, Red Arcs, Atmospheric Attenuation, Spectral Energy Distribution
Scientific paper
The characteristics of atmospheric glow at 630 nm in a subauroral red arc region is investigated, assuming the glow energy source to be electromagnetic ion-cyclotron waves generated in the topside plasmasphere. Profiles of the volume emission rate of the atmosphere in the 140-1000 km height range are calculated. It is shown that, in contrast to nighttime conditions, two peaks can form on these profiles in the daytime; the lower peak is due to photoelectrons while the upper peak is due to thermal electrons heated to high temperature as a result of wave-dissipation energy coming from the plasmasphere.
Konikov Iu. V.
Pavlov A. V.
No associations
LandOfFree
Atmospheric glow at a wavelength of 630 nm in a region of subauroral red arcs 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 Atmospheric glow at a wavelength of 630 nm in a region of subauroral red arcs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Atmospheric glow at a wavelength of 630 nm in a region of subauroral red arcs will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1303652