Ultra heavy comsic rays: The next generation

Details Ultra heavy comsic rays: The next generation Ultra heavy comsic rays: The next generation

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995adspr..15...29b&link_type=abstract

Advances in Space Research (ISSN 0273-1177), vol. 15, no. 6, p. (6)29-(6)38

Physics

3

Abundance, Charge Distribution, Cosmic Rays, Flux (Rate), Heavy Nuclei, Particle Energy, Propagation, Actinide Series, Lead (Metal), Nuclear Fusion, Particle Acceleration, Platinum, Radiation Counters

Scientific paper

Ultra-heavy galactic cosmic rays have been of great interest for the last several decades since a knowledge of their elemental and isotopic abundances yields important information relevant to their origin, the nucleosynthesis processes in which they were created, their selection and injection into the cosmic ray beam, their acceleration and propagation to earth, their age, and to evolution of galactic matter. In this paper the current status of ultra-heavy measurements is described, an approach to taking the next experimental step is discussed, and the knowledge that can be gained from such an investigation is outlined.

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