Sources of the ultraheavy cosmic rays

Details Sources of the ultraheavy cosmic rays Sources of the ultraheavy cosmic rays

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....3...21m&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 3 p 21-24 (SEE N85-34862 23-93)

Computer Science

Cosmic Rays, Heavy Nuclei, Particle Acceleration, Abundance, Atomic Weights, Bismuth, Heao 3, Ionization Potentials, Iron, Isotopes, Lead (Metal), Nuclear Fusion

Scientific paper

The suggestions that the source abundances of cosmic ray nuclei heavier then Fe differ significantly from Solar System abundances are not well supported by the data without assuming preferential acceleration. The Solar System abundances of Pb and Bi are split into r-, standard s-, and cyclic 8-process components; the apprarent deficiency of Pb seen in the HEAO-3 Heavy Nuclei Experiment data might indicate an absence of Pb from the recycling 8-process.

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