A modeling of the magnetospheric substorm

Details A modeling of the magnetospheric substorm A modeling of the magnetospheric substorm

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975p%26ss...23..575y&link_type=abstract

Planetary and Space Science, vol. 23, Apr. 1975, p. 575-578.

Physics

2

Atmospheric Models, Auroral Electrojets, Magnetic Field Configurations, Magnetospheric Instability, Polar Substorms, Auroral Arcs, Current Sheets, Geomagnetism, Magnetic Disturbances

Scientific paper

The model adopted for the quiet-time magnetosphere is a modified version of Hones' model (1963). The existence of a three-dimensional current system in the day-side magnetosphere is assumed. The magnetic field lines in the noon-midnight meridian are shown for both the quiet-time magnetosphere and the substorm-time magnetosphere. It is found that two current systems can reproduce the two major features of the auroral substorm in the noon-midnight meridian.

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