Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987iraj...18....1m&link_type=abstract
Irish Astronomical Journal (ISSN 0021-1052), vol. 18, March 1987, p. 1-18.
Astronomy and Astrophysics
Astronomy
Solar Flares, Solar Radiation, Gamma Ray Astronomy, Particle Acceleration, Solar Atmosphere, Solar Cosmic Rays, Solar Magnetic Field, Solar Temperature, Solar X-Rays
Scientific paper
The characteristics of three forms of energy that emerge in solar flares, hot plasma, fast particles, and bulk motion of the surrounding gas, are described. Consideration is given to thermal X-rays from flares, temperature variations during a flare, the origin of hard X-rays from flares, and gamma rays from flares. The magnetic constraints and turbulence related to bulk motion in flares are examined. Flares with energetic ions in space and flares rich in He-3 are analyzed. The distinction between fast electrons created by a flare at the flare site and in interplanetary space is investigated. Electron rich flares, solar cosmic rays, and the positive charge on solar cosmic ray ions are studied. The relation between ion cyclotron waves and the acceleration of certain particles and the release of magnetic energy in the sun are discussed.
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