10.1063/1.3068964
Crossref journal-article
AIP Publishing
Physics Today (317)
Abstract

Ultraheavy cosmic-ray nuclei, those with atomic number over thirty, constitute less than about one in 107 of the relativistic particles that stream through our solar system, yet they promise to lead to a major contribution in our understanding of the complex phenomena of the cosmic-ray gas that pervades interstellar space. The study of these nuclei should advance our understanding of the sources of cosmic rays as well as of the nature of the physical processes that influence the particles after their acceleration. This work is greatly accelerating with the advent of satellite experiments, such as the Skylab mission pictured in figure 1.

Bibliography

Israel, M. H., Price, P. B., & Waddington, C. J. (1975). Ultraheavy cosmic rays. Physics Today, 28(5), 23–31.

Authors 3
  1. Martin H. Israel (first)
  2. P. Buford Price (additional)
  3. C. Jake Waddington (additional)
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Dates
Type When
Created 16 years, 4 months ago (April 13, 2009, 1:36 p.m.)
Deposited 2 years, 1 month ago (July 8, 2023, 12:05 a.m.)
Indexed 2 years, 1 month ago (July 8, 2023, 12:42 a.m.)
Issued 50 years, 4 months ago (May 1, 1975)
Published 50 years, 4 months ago (May 1, 1975)
Published Online 16 years, 8 months ago (Dec. 30, 2008)
Published Print 50 years, 4 months ago (May 1, 1975)
Funders 0

None

@article{Israel_1975, title={Ultraheavy cosmic rays}, volume={28}, ISSN={1945-0699}, url={http://dx.doi.org/10.1063/1.3068964}, DOI={10.1063/1.3068964}, number={5}, journal={Physics Today}, publisher={AIP Publishing}, author={Israel, Martin H. and Price, P. Buford and Waddington, C. Jake}, year={1975}, month=may, pages={23–31} }