Abstract
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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Ramaty, R., Dennis, B.R. & Emslie, A.G. Gamma-ray, neutron, and hard X-ray studies and requirements for a high-energy solar physics facility. Sol Phys 118, 17–46 (1988). https://doi.org/10.1007/BF00148587
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DOI: https://doi.org/10.1007/BF00148587