Other
Scientific paper
Oct 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990sci...250..229c&link_type=abstract
Science (ISSN 0036-8075), vol. 250, Oct. 12, 1990, p. 229-236. Research supported by the University of New Hampshire and Max-Pla
Other
22
Charged Particles, Particle Acceleration, Solar Flares, Emission Spectra, Energy Spectra, Gamma Ray Bursts, Particle Interactions, Solar Atmosphere, Solar X-Rays
Scientific paper
Mechanisms that apply to solar flares are discussed, and their applicability to other astrophysical sites, where transient X-ray and gamma-ray bursts occur, is tested. Two different approaches are used to determine the characteristics of the charged particles, accelerated in association with solar flares: (1) measurement of the energy spectra and composition of charged particles observed in space and believed to be associated with a specific solar flare; and (2) recording of electromagnetic emissions in the visible, ultraviolet, soft X-ray, hard X-ray, and gamma-ray spectral regions, and also high-energy neutrons produced in the solar atmosphere by the particles accelerated in association with the solar flare. It is suggested that, at the present level of knowledge, regions where particle acceleration and interactions occur are unlikely to be specified.
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