Turbulent heating in solar cosmic ray theory

Details Turbulent heating in solar cosmic ray theory Turbulent heating in solar cosmic ray theory

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983stin...8416108w&link_type=abstract

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Computer Science

Solar Cosmic Rays, Solar Flares, Turbulent Heat Transfer, Distribution Functions, Heating Equipment, Heavy Elements

Scientific paper

The heating of minor ions in solar flares by wave-wave-particle interaction with Langmuir waves, or ion acoustic waves, can be described by a diffusion equation in velocity-space for the particle distribution function. The dependence of the heating on the ion charge and mass, and on the composition of the plasma, is examined in detail. It is found that the heating mechanisms proposed by Ibragimov and Kocharov cannot account for the enhanced abundances of heavy elements in the solar cosmic rays.

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