Global empirical models of ionospheric electron temperature in the upper F-region and plasmasphere based on in situ measurements from the Atmosphere Explorer-C, ISIS-1 and ISIS-2 satellites

Computer Science – Sound

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Atmospheric Models, Electron Energy, Electrostatic Probes, F Region, Ionospheric Electron Density, Plasmasphere, Satellite Sounding, Explorer 51 Satellite, Extreme Ultraviolet Radiation, Ionospheric Sounding, Isis Satellites, Satellite-Borne Instruments, Solar Radiation

Scientific paper

Langmuir probe measurements of electron temperature, T sub e, in the vicinity of 300, 400, 1400 and 3000 km from the Atmosphere Explorer-C and the ISIS satellites have been employed to construct empirical models of the global distribution of T sub e at each of these altitudes. Legendre polynomials are employed to describe the observations at solstice and equinox in terms of dip latitude and local time. Sources of T sub e variations, such as solar activity, magnetic activity and longitude are found to be of second order importance, although they are resolvable in some cases by comparisons of the data with the model. The behavior of T sub e at the altitudes of these models is discussed in terms of its implications for our understanding of the energy exchange between the F-region and the plasmasphere.

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