A search for solar neutrons during solar flares

Details A search for solar neutrons during solar flares A search for solar neutrons during solar flares

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974soph...39..233i&link_type=abstract

Solar Physics, vol. 39, Nov. 1974, p. 233-241.

Physics

2

Neutron Flux Density, Satellite Observation, Solar Corpuscular Radiation, Solar Flares, Solar Neutrons, Astronomical Models, Extremum Values, Neutron Counters, Neutron Emission, Ogo-6, Particle Production, Solar Physics

Scientific paper

A new upper limit to the 1-20 MeV neutrons produced at the sun during large solar flares was obtained as a result of measurements made by a neutron detector on board the OGO-6 satellite. It was found that the 1-20 MeV solar neutron flux for the Nov. 2, June 13, June 15, Sept. 25, and Dec. 19, 1969, solar flare events cannot be greater than 0.05 n per sq cm per sec at the 95% confidence level. These measurements are consistent with the models proposed by Lingenfelter (1969) and Lingenfelter and Ramaty (1967) for solar neutron production during solar flares.

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