Ring current simulation in connection with interplanetary space conditions

Details Ring current simulation in connection with interplanetary space conditions Ring current simulation in connection with interplanetary space conditions

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984p%26ss...32..975f&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 32, Aug. 1984, p. 975-984.

Physics

34

Geomagnetism, Interplanetary Medium, Magnetic Storms, Magnetospheric Instability, Ring Currents, Solar Terrestrial Interactions, Electric Field Strength, Interplanetary Magnetic Fields, Ion Injection, Quasi-Steady States, Solar Wind

Scientific paper

Attention is given to the novel concept of a quasi-steady state quiet ring current, which is observable under relatively quiet geomagnetic conditions when the ring current decay is compensated for by a certain injection level. Such a quasi-steady injection, which may vary during a storm, gives rise to a change in the value of a constant which precludes difficulties faced by Burton et al. (1975) in giving a physical interpretation of the constant C. The ring current model proposed takes the form of an ordinary differential equation with a set of factors permitting magnetic storms having an explicitly expressed expansion phase to be described with 2.5-min resolution.

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