Computer Science – Sound
Scientific paper
May 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980jgr....85.2043s&link_type=abstract
Journal of Geophysical Research, vol. 85, May 1, 1980, p. 2043-2056. Research supported by the Centre National de la Recherche
Computer Science
Sound
23
Energetic Particles, Geosynchronous Orbits, Magnetic Storms, Magnetospheric Instability, Plasma Dynamics, Satellite Sounding, Electric Fields, Electron Flux Density, Geophysics, Night, Proton Flux Density
Scientific paper
Two phases of substorm-associated magnetospheric dynamics are discussed in terms of particles and fields at synchronous orbit. The first phase corresponds to the 'decreases' of energetic particle flux. The second phase is the conventional expansion phase that begins with the 'onset', characterized in the study by (1) a sudden decrease in the tail current and a return of the inflated magnetosphere to a dipolelike configuration, (2) a sudden shift of trapped high-energy particles toward the tail again following contours of constant B, and at the same time (3) a surge of tail plasma toward the earth as the induced electric field now increases the total convection field.
Sauvaud Jean-Andre
Winckler John R.
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