A note on the revised galactic neutron spectrum of the AMES collaborative study

Details A note on the revised galactic neutron spectrum of the AMES collaborative study A note on the revised galactic neutron spectrum of the AMES collaborative study

Mar 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980uwfp.rept.....s&link_type=abstract

Final Report University of West Florida, Pensacola.

Computer Science

Flux (Rate), Galactic Radiation, Neutron Spectra, Scattering Cross Sections, Spectral Energy Distribution, Cosmic Rays, Dosimeters, Elastic Scattering, Neutron Flux Density, Radiation Shielding, Recoil Protons

Scientific paper

Energy distributions of the neutron dose equivalents in the 0.1 to 300 Mev interval for the Ames and Hess spectra are compared. The Ames spectrum shows no evaporation peak, moves the bulk of the flux away from the region of elastic collision and spreads it more evenly over higher energies. The neutron spectrum in space does not seem to hear out the Ames model. Emulsion findings on all manned missions of the past consistently indicate that evaporation events are a prolific source of neutrons in space.

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