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• W2039612239 abstract "The electron continuity equation and the heat conduction equations for electrons, ions and neutral species are solved simultaneously for specified boundary conditions and values of the solar flux. These solutions have yielded a set of selfconsisterrt steady state profiles for a variety of midday solar conditions that are in agreement with observational data. To produce these profiles only the boundary conditions and solar flux are used as variable parameters of the problem. It is shown that the neutral temperature and the resulting neutral gas composition play a dominant role in determining the charged particle density and temperature profiles. This leads to a picture of the solar cycle variation where composition changes in the neutral gas (introduced at the lower boundary) must be combined with the solar flux variation to produce physically reasonable results. Of the five neutral gases used, (N2, O2, O, He, H) the atomic oxygen density variations are shown to be most effective in producing the observed trends for all the temperatures and densities in the E and F-regions." @default.
• W2039612239 created "2016-06-24" @default.
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• W2039612239 date "1969-05-01" @default.
• W2039612239 modified "2023-09-26" @default.
• W2039612239 title "The influence of varying solar flux on ionospheric temperatures and densities: A theoretical study" @default.
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• W2039612239 doi "https://doi.org/10.1016/0032-0633(69)90090-7" @default.
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