The cosmogenic Al-26 and cosmic ray intensity in the distant past

Details The cosmogenic Al-26 and cosmic ray intensity in the distant past The cosmogenic Al-26 and cosmic ray intensity in the distant past

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977izssr..41q.446b&link_type=abstract

(Mezhdunarodnyi Seminar po Aktivnym Protsessam na Solntse i Probleme Solnechnykh Neitrino, 8th, Leningrad, USSR, Sept. 25-27, 19

Computer Science

Abundance, Aluminum 26, Cosmic Rays, Lunar Rocks, Meteoritic Composition, Ablation, Cosmology, Lunar Surface, Radioactive Age Determination

Scientific paper

Studies determining concentrations of Al-26, which has a long half-life, provide information on cosmic ray activity in the distant past. Although some meteorites contain comparatively large amounts of Al-26, the amount in the sun-irradiated surface areas of meteors can not be determined owing to ablation in the atmosphere. In this paper, data on Al-26 concentrations in lunar surface and subsurface samples are used to interpret information on Al-26 concentrations in terrestrial and meteorite samples.

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