Charge composition and energy spectra of cosmic-ray nuclei at energies above 5 GeV per nucleon

Physics – Nuclear Physics

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Abundance, Cerenkov Counters, Chemical Composition, Cosmic Rays, Energy Spectra, Nuclei (Nuclear Physics), Balloon Flight, Oxygen, Particle Energy, Particle Flux Density

Scientific paper

A scintillation-Cerenkov counter telescope, with three gas Cerenkov counters for energy determination between 5 and 90 GeV per nucleon, has been exposed for a net total of 4.5 sq m sr hr in two balloon flights in 1974. The measurement yields the chemical composition and energy spectra of cosmic-ray nuclei in the charge range 5-28. The differential spectral indices of oxygen and of the iron group are measured to be 2.67 plus or minus 0.04 and 2.5 plus or minus 0.08 above 5.4 GeV per nucleon, respectively. The results are interpreted in the context of the 'leaky-box' model of cosmic-ray confinement and propagation.

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