Implications of high-energy neutron observations from solar flares

Details Implications of high-energy neutron observations from solar flares Implications of high-energy neutron observations from solar flares

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...273l..41r&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 273, Oct. 1, 1983, p. L41-L45. NASA-NSF-supported r

Astronomy and Astrophysics

Astrophysics

27

Gamma Ray Spectra, High Energy Interactions, Neutron Flux Density, Particle Acceleration, Solar Corpuscular Radiation, Solar Flares, Solar Neutrons, Energetic Particles, Energy Spectra, Particle Production, Relativistic Electron Beams, Solar Protons, Solar Spectra

Scientific paper

The time-dependent flux of high-energy neutrons discovered from the solar flare of 1980 June 21 provides a new technique for determining the total number and energy spectrum of accelerated protons and nuclei at the Sun. The implications of these observations on gamma-ray emission, relativistic electron spectrum and number, proton and electron energy contents, and the location of the interaction region are also examined.

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