Other
Scientific paper
Feb 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ge%26ae..22...28d&link_type=abstract
Geomagnetizm i Aeronomiia, vol. 22, Jan.-Feb. 1982, p. 28-32. In Russian.
Other
Equatorial Atmosphere, Ionospheric Electron Density, Ionospheric Ion Density, Space Plasmas, Vertical Distribution, Charged Particles, Daytime, Particle Energy, Solar Activity Effects
Scientific paper
An analytic solution of the ionospheric-plasma equations is used to obtain the vertical distribution of charged-particle density and temperature above the magnetic equator at heights of 100-2000 km at midday hours for quiet geomagnetic conditions and various levels of solar activity. It is shown that the calculated vertical electron-temperature profiles have a maximum at 250 km, while the isothermal region (T sub e = T sub n) is situated in the 380-500 km region at low solar activity and in the 380-650 km region at high solar activity. The nonisothermicity of the medium does not produce changes in hmF2 and NmF2 but produces an increase in O(+) concentration above the isothermal region and a decrease in H(+) concentration in a wide range of heights.
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