Upper limits to the quiet-time solar neutron flux from 10 to 100 MeV

Details Upper limits to the quiet-time solar neutron flux from 10 to 100 MeV Upper limits to the quiet-time solar neutron flux from 10 to 100 MeV

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975stin...7619038m&link_type=abstract

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Physics

Neutron Flux Density, Solar Neutrons, Solar Radiation, Balloon Flight, Neutron Counters, Neutron Scattering, Solar Energy

Scientific paper

The UCR large area solid-angle double scatter neutron telescope was flown to search for solar neutrons on 3 balloon flights on September 26, 1971, May 14, 1972 and September 19, 1972. The first two flights were launched from Palestine, Texas and the third from Cape Girardeau, Missouri. The float altitude on each flight was at about 5 g/sq cm residual atmosphere. Neutrons from 10 to 100 MeV were measured. No solar flares occurred during the flights. Upper limits to the quiet time solar neutron fluxes at the 95% confidence level are .00028, .00046, .00096 and .00090 neutrons/sq cm-sec in the energy intervals of 10-30, 30-50, 50-100 and 10-100 MeV, respectively.

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