Determination of energy spectra of solar electrons under different scenarios in solar flare sources

Details Determination of energy spectra of solar electrons under different scenarios in solar flare sources Determination of energy spectra of solar electrons under different scenarios in solar flare sources

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987rmxaa..14..700g&link_type=abstract

(IAU, Reunion Regional Latinoamericana de Astronomia, 5th, Merida, Mexico, Oct. 6-10, 1986) Revista Mexicana de Astronomia y Ast

Astronomy and Astrophysics

Astronomy

Energy Spectra, Fokker-Planck Equation, Particle Acceleration, Solar Cosmic Rays, Solar Electrons, Solar Flares, Earth Surface, Energetic Particles, Energy Distribution

Scientific paper

The energy spectrum of the solar flare electrons is investigated within the frame of three different scenarios. Solutions of the Fokker-Planck equation are employed under the assumption of a short fly time of particles within the source and low density therein (thin-geometry). The obtained results are compared with observational spectra measured at the earth level. This intercomparison allows the authors to infer about the appropriate scenario in each particular solar event.

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