Charge composition of medium energy cosmic-ray nuclei from neon to iron

Details Charge composition of medium energy cosmic-ray nuclei from neon to iron Charge composition of medium energy cosmic-ray nuclei from neon to iron

May 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ap%26ss..62..465s&link_type=abstract

Astrophysics and Space Science, vol. 62, no. 2, May 1979, p. 465-475. Research supported by the Department of Atomic Energy and

Physics

Nuclear Physics

3

Cosmic Rays, Energy Spectra, Nuclei (Nuclear Physics), Radiant Flux Density, Abundance, Balloon-Borne Instruments, Optimization, Particle Tracks, Radiation Counters

Scientific paper

The charge composition of cosmic-ray nuclei from neon to iron has been studied in a stack of cellulose nitrate plastic detectors exposed in a balloon flight over Fort Churchill. Some 401 cosmic-ray nuclei with Z between 10 to 26 and stopped in the detector system have been analyzed. Fluxes of individual nuclei have been extrapolated to the top of the atmosphere. Relative abundances, obtained from these fluxes, have been compared with those obtained by other investigators.

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