Energetic particles in solar flares. Chapter 4 in the proceedings of the 2nd SKYLAB Workshop on Solar Flares

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Energetic Particles, Particle Acceleration, Solar Flares, Skylab Program, Solar Cosmic Rays, Solar Electrons, Solar Magnetic Field, Solar Radio Emission, Solar X-Rays

Scientific paper

The recent direct observational evidence for the acceleration of particles in solar flares, i.e. radio emission, bremsstrahlung X-ray emission, gamma-ray line and continuum emission, as well as direct observations of energetic electrons and ions, are discussed and intercorrelated. At least two distinct phases of acceleration of solar particles exist that can be distinguished in terms of temporal behavior, type and energy of particles accelerated and the acceleration mechanism. Bulk energization seems the likely acceleration mechanism for the first phase while Fermi mechanism is a viable candidate for the second one.

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