Physics – Plasma Physics
Scientific paper
May 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ppcn.conf..279s&link_type=abstract
In ESA, Fourth International Toki Conference on Plasma Physics and Controlled Nuclear Fusion p 279-280 (SEE N94-22624 05-75)
Physics
Plasma Physics
Chemical Composition, Particle Acceleration, Relativistic Electron Beams, Solar Flares, Solar Protons, Gamma Ray Spectra, Ionization Potentials, Magnetic Field Configurations, Solar Atmosphere, Sunspots, X Ray Spectra
Scientific paper
The mechanisms by which particles are accelerated in solar flares are investigated. To perform this task it is necessary to know the chemical composition of solar flare particles and gamma ray line emissions associated with flares. High energy quanta such as gamma rays and hard x rays are emitted in association with the acceleration of high energy protons and other nuclei in solar flares. They are called solar flare particles. Radio waves covering microwave to decametric frequencies are usually emitted from relativistic electrons. These electrons are accelerated in solar flares. The efficiency for these particles to be accelerated is shown to be dependent on the ratio of particle masses to their actual charges.
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