What does the magnetic storm development depend on?

Physics

Scientific paper

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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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