Energetic ions in solar gamma-ray flares

Details Energetic ions in solar gamma-ray flares Energetic ions in solar gamma-ray flares

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph..100..515h&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 100, Oct. 1985, p. 515-535.

Astronomy and Astrophysics

Astronomy

17

Energetic Particles, Gamma Ray Astronomy, Neutron Emission, Solar Corpuscular Radiation, Solar Flares, Emission Spectra, Gamma Ray Spectra, High Energy Interactions, Ion Motion, Particle Acceleration, Primary Cosmic Rays, Solar Magnetic Field, Solar Spectra

Scientific paper

Solar flares emit line and continuum gamma-radiation, as well as neutrons and charged particles. These high-energy emissions require the presence of energetic ions within the magnetic structures of the flare proper. A great deal about the location and mode of particle acceleration is already known. The observations have now become extensive enough so that it is possible to begin to study the dynamics of the energetic ions within the flare structures themselves. The gamma-ray and neutron observations and the theory of their emission are reviewed, and, on this basis, the presence of energetic ions deep within the flaring atmosphere is discussed.

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