Solar EUV flux variation during a solar cycle as derived from ionospheric modeling considerations

Details Solar EUV flux variation during a solar cycle as derived from ionospheric modeling considerations Solar EUV flux variation during a solar cycle as derived from ionospheric modeling considerations

Jan 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976jgr....81..265r&link_type=abstract

Journal of Geophysical Research, vol. 81, Jan. 1, 1976, p. 265-269.

Physics

6

Atmospheric Models, Electron Energy, Far Ultraviolet Radiation, Ionospheric Electron Density, Solar Cycles, Solar Flux, Contours, Diurnal Variations, Electron Density Profiles, Incoherent Scattering, Ionospheric Composition, Temperature Inversions, Vertical Distribution

Scientific paper

Calculations in modeling the general ionospheric structure observed during solar minimum and solar maximum suggest that the Hinteregger (1970) solar EUV flux values are adequate for modeling the midlatitude ionospheric structure during solar minimum. However, these flux values should be doubled for modeling solar maximum conditions. The calculations also suggest that the atomic oxygen density at 120 km was approximately a factor of 2 lower during solar cycle minimum than during solar cycle maximum.

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