Physics
Scientific paper
Feb 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.188..271s&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 188, no. 2, Feb. 1992, p. 271-278. Research supported by UGCI.
Physics
Atmospheric Physics, E Region, Electron Energy, Ionospheric Electron Density, Solar Activity Effects, Solar Terrestrial Interactions, Atmospheric Models, Photoionization, Recombination Coefficient, Solar Flares
Scientific paper
Presuming the total life-time for recombination of molecular ions with electrons remains constant at each altitude under different solar flare conditions, the mean dissociative recombination coefficient and the electron temperatures can be calculated with a knowledge of the quiet time recombination coefficient and the production rate profiles under these conditions. To estimate the electron temperatures, the temperature dependence of the form (300/Te) exp 1/2 for the electron loss coefficient has been assumed. The computations show very high electron temperatures below about 130 km for the representative solar events considered.
No associations
LandOfFree
E-region effective electron loss rates and electron temperatures under different solar flare conditions 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 E-region effective electron loss rates and electron temperatures under different solar flare conditions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and E-region effective electron loss rates and electron temperatures under different solar flare conditions will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1046212