Physics
Scientific paper
Aug 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991p%26ss...39.1163w&link_type=abstract
Planetary and Space Science (ISSN 0032-0633), vol. 39, Aug. 1991, p. 1163-1170.
Physics
8
Earth Ionosphere, Magnetic Storms, Ring Currents, Solar Terrestrial Interactions, Solar Wind, Ampte (Satellites), Atmospheric Models, Earth Magnetosphere, Hydrogen Ions, Oxygen Ions
Scientific paper
An adiabatic drift model applied to a magnetic storm development simulation reveals the significance of initial energy, initial pitch angle, and the site of ions injection for the intensity, growth time, and growth rate of a storm produced by two ion species - H(+) and O(+). The most severe storms are caused by the ring current intensified by low initial pitch angle ions injected at low radial distance in the postmidnight local time region.
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