Computer Science
Scientific paper
Jul 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987p%26ss...35..887b&link_type=abstract
Planetary and Space Science (ISSN 0032-0633), vol. 35, July 1987, p. 887-901. SERC-supported research.
Computer Science
2
Electron Energy, F Region, Ionospheric Electron Density, Diurnal Variations, Equatorial Atmosphere, Midlatitude Atmosphere
Scientific paper
A theoretical study is made of the dependence of electron temperature, Te, on electron concentration, Ne, and on solar activity F(10.7) flux in the daytime (10:00-14:00 LT) mid- to low-latitude F-layer. The set of Te, Ne, and F(10.7) values is analyzed and compared to incoherent scatter and satellite observations of these variables. The observed quasi-linear dependence of Te on Ne values less than about 500,000/cu cm is simulated in the theoretical results and is due to the nonlinear interaction of the several competing processes in the heat balance equation for the electron gas. Photoelectron heat input and electron-O(+) Coulomb heat loss tend to become dominant as Ne increases.
Bailey Graham J.
Moffett R. J.
Simmons P. A.
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