Particle acceleration in solar flares

Details Particle acceleration in solar flares Particle acceleration in solar flares

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987nascp2464...47r&link_type=abstract

In its Essays in Space Science p 47-73 (SEE N87-24247 17-88)

Astronomy and Astrophysics

Astrophysics

Astrophysics, Earth Atmosphere, Earth Magnetosphere, Energetic Particles, Mathematical Models, Particle Acceleration, Solar Flares, Abundance, Anisotropy, Energy Spectra, Shock Wave Propagation, Signature Analysis, Stochastic Processes

Scientific paper

The most direct signatures of particle acceleration in flares are energetic particles detected in interplanetary space and in the Earth's atmosphere, and gamma rays, neutrons, hard X-rays, and radio emissions produced by the energetic particles in the solar atmosphere. The authors review the stochastic and shock acceleration theories in flares, and discuss the implications of observations on particle energy spectra, particle confinement and escape, multiple acceleration phases, particle anisotropies, and solar atmospheric abundances.

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