Gamma-ray, neutron, and hard X-ray studies and requirements for a high-energy solar physics facility

Details Gamma-ray, neutron, and hard X-ray studies and requirements for a high-energy solar physics facility Gamma-ray, neutron, and hard X-ray studies and requirements for a high-energy solar physics facility

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..118...17r&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 118, no. 1-2, 1988, p. 17-46.

Astronomy and Astrophysics

Astronomy

10

Gamma Ray Astronomy, Particle Acceleration, Solar Flares, Solar Neutrons, Solar X-Rays, Charged Particles, Energetic Particles, Solar Atmosphere, Solar Physics, Solar Spectra

Scientific paper

The requirements for future high-resolution spatial, spectral, and temporal observations of hard X-rays, gamma rays and neutrons from solar flares are discussed in the context of current high-energy flare observations. There is much promise from these observations for achieving a deep understanding of processes of energy release, particle acceleration and particle transport in a complicated environment such as the turbulent and highly magnetized atmosphere of the active Sun.

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