A measurement of abundances of VVH nuclei above 0.6 GeV per nucleon

Details A measurement of abundances of VVH nuclei above 0.6 GeV per nucleon A measurement of abundances of VVH nuclei above 0.6 GeV per nucleon

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...201...76j&link_type=abstract

Astrophysical Journal, vol. 201, Oct. 1, 1975, pt. 1, p. 76-81.

Astronomy and Astrophysics

Astrophysics

7

Abundance, Balloon-Borne Instruments, Cosmic Rays, Heavy Nuclei, Charge Distribution, Electron Counters, Nucleons, Solar System

Scientific paper

The abundance distribution of very very heavy (VVH) nuclei just beyond the iron group has been measured with a balloon-borne counter telescope flown in 1971 and 1972. While the statistical accuracy of these observations is limited, they are of considerable interest since very little work has so far been done to determine the abundance of nuclei with charge between 27 and 36. It is found that the element distribution in the cosmic rays arriving at the top of the atmosphere is quite similar to the solar-system abundance distribution in this interval.

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