Development of the OSO-6 high-energy neutron detector and correlation of measured solar neutron fluxes to solar flares
Description:
Thesis. The development of a directional high energy (20 to 160 MeV) neutron detector which was flown to satellite altitudes (500 km; circular equatorial orbit) in the NASA Orbiting Solar Observatory (OSO-6) in August 1969 is described. Both the angle of incidence and the energy of the neutron are determined by a proton-recoil telescope (Pilot B scintillation plastic) which provides the source for proton-recoils and defines the dE/dX versus E method for particle identification and energy determ…
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Date:
February 1, 1974
Creator:
Young, F.
Partner:
UNT Libraries Government Documents Department