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NASA NTRS · 20020067760

Self-Consistent Magnetosphere-Ionosphere Coupling: Theoretical Studies

Abstract

A self-consistent ring current (RC) model has been developed that couples electron and ion magnetospheric dynamics with the calculation of the electric field. Two new features were taken into account in order to close the self-consistent magnetosphere- ionosphere coupling loop. First, in addition to the RC ions, we solve an electron kinetic equation in our model. Second, using the relation of Galand and Richmond [2001], we calculate the height integrated ionospheric conductances as a function of the precipitated high energy magnetospheric electrons and ions that are produced by our code. To validate the results of our model we simulate the magnetic storm of May 2, 1986, a storm that has has been comprehensively studied, and compare our results with different theoretical approaches. The self-consistent inclusion of the hot electrons and, their effect on the conductance results in deeper penetration of the magnetospheric electric field. In addition, a slight westward rotation of the potential pattern (compared to previous self-consistent results) is evident in the inner magnetosphere. This changes the hot plasma distribution, especially by allowing increased access of plasma sheet ions and electrons to low L shells.

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BibTeXRIS

Khazanov, G. V., Newman, T. S., Liemohn, M. W., Fok, M.-C., Spiro, R. W., Six, N. Frank. 2002-01-01. Self-Consistent Magnetosphere-Ionosphere Coupling: Theoretical Studies. https://ntrs.nasa.gov/citations/20020067760

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