Modified models of electron distribution in the magnetosphere at L = 2.3

Details Modified models of electron distribution in the magnetosphere at L = 2.3 Modified models of electron distribution in the magnetosphere at L = 2.3

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992p%26ss...40..671s&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 40, no. 5, May 1992, p. 671-679. Research supported by NERC and SERC.

Mathematics

Electron Distribution, Electron Energy, Magnetospheric Electron Density, Whistlers, Helium Ions, Hydrogen Ions, Mathematical Models, Oxygen Ions, Positive Ions

Scientific paper

The existing simple diffusive equilibrium model distributions in the magnetosphere are modified in such a way that they become as close as possible to the mathematical model distribution. The magnetospheric conditions are appropriate to the equinox and L of 2.3 for the solar minimum and solar maximum. The approximations to the model electron distribution results are used to compute the group delay of the signals from the NAA and NSS transmitters, with the perturbations due to the effects of finite electron density, ion effects, and nonzero electron temperature effects taken into account.

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