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A measurement of the momentum spectra of cosmic-ray muons at sea level was completed using a large rotatable magnetic spectrometer. The muon flux at zenith angles of 30 and 75° and for energies from 50 GeV to beyond 1000 GeV is presented. The results are compared with calculations based on the conventional production of muons from the decay of .pi. and K mesons. It is concluded that both the charge ratio of the muons and the variation of the muon flux with zenith angle indicate the presence of a much larger fraction of heavy nuclei in the primary radiation than expected. The ratio of bound nucleons to free protons is found to be approximately unity at energies in excess of 5 TeV per nucleon.
Papers for each conference issued in several volumes. Volumes distributed to conference registrants have title "Conference papers"; other volumes of papers published after the conference are identified as "Late papers", "Invited papers", or other similar titles. Most conferences also have a general index volume.