Further observations of protons resulting from the decay of neutrons ejected by solar flares

Details Further observations of protons resulting from the decay of neutrons ejected by solar flares Further observations of protons resulting from the decay of neutrons ejected by solar flares

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4..130e&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 4 p 130-133 (SEE N85-34729 23-92)

Physics

Gamma Rays, Neutrons, Proton Flux Density, Solar Cosmic Rays, Solar Flares, Solar Neutrons, International Sun Earth Explorers, Interplanetary Space, Neutron Spectra, Particle Emission, Protons

Scientific paper

The solar flare of 1984 April 24 produced a large γ-ray fluence with energy >2 MeV. The time profile of the interplanetary proton flux from this flare indicates the presence of decaying solar neutrons. This makes a total of three neutron flares so far observed by this method. The three flares are used to place constraints on the fluence and spectra of neutrons emitted by the sun.

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