Energy spectra of cosmic ray nuclei to above 100 GeV/nucleon

Details Energy spectra of cosmic ray nuclei to above 100 GeV/nucleon Energy spectra of cosmic ray nuclei to above 100 GeV/nucleon

Oct 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979stin...8017011s&link_type=abstract

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Physics

Nuclear Physics

Boron, Cosmic Rays, Energy Spectra, Iron, Nuclei (Nuclear Physics), Balloon-Borne Instruments, Chemical Composition, Spectral Energy Distribution, Spectrometers

Scientific paper

The chemical composition cosmic rays as a function of energy in the range of a few GeV/nucleon to some hundreds of GeV/nucleon for boron through iron are presented. The experiment combined an ionization spectrometer and a gas Cherenkov counter, which was flown on a balloon, to perform two different and independent energy measurements. The experimental apparatus is described in detail. The energy dependence of the cosmic ray escape length for boron and iron is reported and predicted changes in the energy dependence of the ratios of primary nuclei 0/C and iron/C+0 are discussed.

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