Charge and energy spectra of heavy cosmic rays

Details Charge and energy spectra of heavy cosmic rays Charge and energy spectra of heavy cosmic rays

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975icrc....1..251b&link_type=abstract

In: International Cosmic Ray Conference, 14th, Munich, West Germany, August 15-29, 1975, Conference Papers. Volume 1. (A76-26851

Physics

17

Abundance, Cosmic Rays, Energy Spectra, Heavy Nuclei, Particle Energy, Balloon Flight, Data Reduction, High Altitude Nuclear Detection, Nucleons

Scientific paper

Relative abundances of elements with Z values between 14 and 28 in the energy range from 870 to 1400 MeV/nucleon are reported, including Ni/Fe 0.050 + or - 0.004 and Co/Fe below 0.012 + or - 0.006. The Si/Fe ratio shows no major energy dependence, but the ratio of Fe-secondaries (Z values between 21 and 25) to Fe shows some variation, approximately consistent with the energy dependence of the fragmentation cross-sections.

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