Evidence for a large bulk ion conic heating region

Physics

Scientific paper

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Atmospheric Heating, Auroral Zones, Ion Temperature, Lines Of Force, Conics, Ion Distribution, Latitude, Monte Carlo Method, Oxygen Ions, Particle Motion, Satellite Observation

Scientific paper

The ion bowl distribution, a type of ion conic with a low energy ion cutoff and field-aligned low energy ions, can be explained by purely perpendicular heating of ions on auroral magnetic field lines. The ion bowl distribution provides evidence that there exists a bulk ion heating mechanism, as opposed to a mechanism that effects only the tail of the ion distribution, and that this heating mechanism acts along a large portion of the magnetic field line.

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