Physics
Scientific paper
Jan 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..107..173o&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 107, no. 1, 1987, p. 173-181.
Physics
1
Ion Cyclotron Radiation, Magnetohydrodynamic Waves, Particle Interactions, Solar Protons, Solitary Waves, Born Approximation, Plasma Turbulence, Power Spectra, Solar Wind
Scientific paper
Nonresonant particle (proton) interactions with a turbulent state consisting of Alfven solitons are considered. Parallel and perpendicular velocities are computed and their phase averaged values are used to find corresponding energy changes. While the protons heat in the perpendicular direction, associated with this is a cooling in the parallel direction.
Ovendon C. R.
Schwartz Steve J.
Shah Arvind H.
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