Solar flare neutron fluxes derived from interplanetary charged particle measurements

Details Solar flare neutron fluxes derived from interplanetary charged particle measurements Solar flare neutron fluxes derived from interplanetary charged particle measurements

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....4...97e&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Conference Papers. Volume 4 (A85-2

Physics

Interplanetary Medium, Neutron Spectra, Solar Corpuscular Radiation, Solar Flares, Solar Neutrons, International Sun Earth Explorer 3, Solar Protons

Scientific paper

The first observation of interplanetary protons produced by the decay of solar neutrons made by Evenson et al. (1983) after a solar flare which occurred on June 3, 1982, is expanded, extending the measurement of the spectrum of the decay protons to higher energy. The spectrum of the decay protons for the June 21, 1980, neutron event observed by Chupp et al. (1982) is also determined. The measurements suggest that neutron emission from solar flares is isotropic and that different flares emit neutrons with similar spectra. The importance of such measurements in the study of interplanetary propagation of charged particles is discussed.

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