Composition of Cosmic-Ray Nuclei at High Energies

Details Composition of Cosmic-Ray Nuclei at High Energies Composition of Cosmic-Ray Nuclei at High Energies

Aug 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972phrvl..29..445j&link_type=abstract

Physical Review Letters, vol. 29, Issue 7, pp. 445-448

Physics

62

Scientific paper

We have measured the charge composition of cosmic-ray nuclei from Li to Fe with energies up to about 100 GeV/nucleon. A balloon-borne counter telescope with gas Cherenkov counters for energy determination was used for this experiment. Our first results show that, in contrast to low-energy observations, the relative abundances change as a function of energy. We find that the ratio of the galactic secondary nuclei to primary-source nuclei decreases at energies above about 30 GeV/nucleon.

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