The isotopic composition of cosmic rays with 5 is less than or equal to Z which is less than or equal to 26

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Chemical Composition, Cosmic Rays, Balloon Flight, Cerenkov Counters, Heavy Nuclei, Scintillation Counters

Scientific paper

Results obtained from a high altitude balloon flight from Thompson, Canada in August, 1973 are reported. The instrument consisted of a spark chamber, a Lucite Gerenkov counter and thirteen layers of scintillators. For heavy particles the Cerenkov-range method of analysis was used to determine the mass of particles energetic enough to produce a Cerenkov signal and then stop in the layered scintillators. The data appear to be consistent with current cosmic-ray propagation models. Using a simple exponential path length propagation model this data is extrapolated to the cosmic-ray source and some implications of the data are discussed as to the nature of the source.

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