Abundance Ratios for Primary Cosmic-Ray Nuclei from Be to Fe for 5 to 50 GV/c

Details Abundance Ratios for Primary Cosmic-Ray Nuclei from Be to Fe for 5 to 50 GV/c Abundance Ratios for Primary Cosmic-Ray Nuclei from Be to Fe for 5 to 50 GV/c

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975icrc....1..280o&link_type=gif

Proceedings from the 14th International Cosmic Ray Conference, held in München, Germany, 15-29 August, 1975. Volume 1 (OG Sessi

Physics

4

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