Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981plap.rept..405m&link_type=abstract
In ESA Plasma Astrophys. p 405-406 (SEE N82-20030 10-88)
Astronomy and Astrophysics
Astrophysics
Cyclotron Resonance, Ion Cyclotron Radiation, Magnetohydrodynamic Shear Heating, Solar Wind Velocity, Alpha Particles, Energy Transfer, Ion Temperature, Plasma-Electromagnetic Interaction, Radial Distribution, Solar Protons
Scientific paper
A model is presented which describes the radial evolution of solar wind ion temperatures and speeds within a fluid framework. Resonant wave-particle interactions are taken into account and the ion-wave dynamic equilibrium is calculated self-consistenly. Numerical results show that self-consistency in the calculations is of major importance for a realistic description of energy and momentum balance between waves and particles.
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