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The fluxes and energy spectra of deuterium, protons, and helium were measured on the IMP-III satellite at a time near minimum solar activity. The deuterium differential energy spectrum in the range 17-63 MeV/nucleon is ∝E⁺² and, at 60 MeV/nucleon, the relative abundance ratios are H²/He⁴=0.15 and H²/H¹=0.05. If present values of experimental cross sections for the production of H² from nucleon interactions with He⁴ are used, the observed deuterium abundance may be accounted for by the traversal of He⁴ through 4 to 6 g/cm² of matter in cosmic-ray sources and the interstellar medium.
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Fan et al. (1966) studied this question.
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