The abundances of H-3 and C-14 in the solar wind

Details The abundances of H-3 and C-14 in the solar wind The abundances of H-3 and C-14 in the solar wind

Oct 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976e%26psl..32..185f&link_type=abstract

Earth and Planetary Science Letters, vol. 32, no. 2, Oct. 1976, p. 185-190.

Physics

5

Abundance, Carbon 14, Lunar Soil, Solar Wind, Tritium, Hydrogen, Lunar Rocks, Nitrogen 15, Proportional Counters, Surveyor 3 Lunar Probe, Vertical Distribution

Scientific paper

Tritium is measured as a function of depth in a Surveyor 3 sample. The upper limit for solar-wind-implanted tritium gives a H-3/H-1 limit for the solar wind of 1 part in one hundred billion. The temperature release patterns of C-14 from lunar soils are measured. The C-14 release patterns from surface soils differ from a trench-bottom soil and give evidence for the presence of C-14 in the solar wind with a C-14/H-1 ratio of approximately 4 parts in one hundred billion. The implications of these radionuclide abundances in the solar wind are discussed.

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