Solar neutron decay proton observations in cycle 21

Astronomy and Astrophysics – Astrophysics

Scientific paper

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17

Radioactive Decay, Solar Cycles, Solar Flares, Solar Neutrons, Solar Protons, Emission Spectra, Energy Spectra, Interplanetary Magnetic Fields, Solar System

Scientific paper

Measurement of the flux and energy spectrum of the protons resulting from the decay of solar flare neutrons gives unique information on the spectrum of neutrons from 5 to 200 MeV. Neutrons from three flares have been observed in this manner during solar cycle 21. The use of the decay protons to determine neutron energy spectra is reviewed, and new and definitive energy spectra are presented for the two large flares on June 3, 1982 and April 25, 1984.

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