Flare physics at high energies

Details Flare physics at high energies Flare physics at high energies

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990aipc..207..122r&link_type=abstract

IN: Astrophysics from the moon; Proceedings of the Workshop, Annapolis, MD, Feb. 5-7, 1990 (A91-56576 24-89). New York, American

Astronomy and Astrophysics

Astrophysics

High Energy Interactions, Particle Acceleration, Solar Atmosphere, Solar Flares, Abundance, Gamma Ray Spectra, Interplanetary Medium, Solar Magnetic Field, Solar X-Rays

Scientific paper

High-energy processes, involving a rich variety of accelerated particle phenomena, lie at the core of the solar flare problem. The most direct manifestation of these processes are high-energy radiations, gamma rays, hard X-rays and neutrons, as well as the accelerated particles themselves, which can be detected in interplanetary space. In the study of astrophysics from the moon, the understanding of these processes should have great importance. The inner solar system environment is strongly influenced by activity on the sun; the physics of solar flares is of great intrinsic interest; and much high-energy astrophysics can be learned from investigations of flare physics at high energies.

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