Physics
Scientific paper
Oct 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986georl..13.1059t&link_type=abstract
Geophysical Research Letters (ISSN 0094-8276), vol. 13, Oct. 1986, p. 1059-1062. Research supported by the University of Califor
Physics
52
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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