Measurement of the fluxes of galactic cosmic ray H-2 and He-3 in 1972 - 1973

Details Measurement of the fluxes of galactic cosmic ray H-2 and He-3 in 1972 - 1973 Measurement of the fluxes of galactic cosmic ray H-2 and He-3 in 1972 - 1973

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975mfgc.book.....t&link_type=abstract

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Physics

Cosmic Rays, Galactic Radiation, Helium Isotopes, Hydrogen Isotopes, Energy Distribution, Flux (Rate), Radiation Measurement

Scientific paper

If a nearby source of low-energy helium is present, which has traversed
a relatively small amount of matter and thus has not caused the
production of a significant amount of H-2 or He-3, then these abundance
ratios will be suppressed, particularly at low energies. This seems to
be the most likely explanation for low ratios.

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