Abundances of 'secondary' elements among the ultraheavy cosmic rays - Results from HEAO-3

Details Abundances of 'secondary' elements among the ultraheavy cosmic rays - Results from HEAO-3 Abundances of 'secondary' elements among the ultraheavy cosmic rays - Results from HEAO-3

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....9..279k&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Late Papers. Volume 9 (A85-22801 0

Computer Science

Abundance, Heao 3, Heavy Nuclei, Secondary Cosmic Rays, Cosmochemistry, Solar System, Spaceborne Experiments

Scientific paper

The HEAO-3 Heavy Nuclei Experiment has measured elemental abundances of ultraheavy cosmic rays near earth. The elements with atomic number (Z) in the intervals Z = 44-48 and Z = 62-74 arriving at earth are expected to have significant secondary components. However, their source abundances are unlikely to be low enough to warrant treating them as pure secondaries. The present results are consistent with solar system abundances modified for first ionization potential with possibly some enhancement of the r to s ratio.

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