The mass composition of the primary cosmic rays in the low-TeV range derived from grjound-level muon measurements

Details The mass composition of the primary cosmic rays in the low-TeV range derived from grjound-level muon measurements The mass composition of the primary cosmic rays in the low-TeV range derived from grjound-level muon measurements

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984nciml..41..373a&link_type=abstract

Nuovo Cimento, Lettere, Serie 2, vol. 41, Nov. 10, 1984, p. 373-376. Research supported by the Deutsche Forschungsgemeinschaft,

Computer Science

9

Cosmic Ray Showers, Energetic Particles, Magnetic Spectroscopy, Mass Spectroscopy, Muons, Primary Cosmic Rays, Energy Spectra, Neutron Flux Density, Nucleons

Scientific paper

With a magnetic spectrometer the charge ratio of muons was measured at
sea-level up to an energy of 7 TeV. Using these data the primary mass
composition, i.e. the ratio of neutrons of the primary mixture of nuclei
could be determined up to about 50 TeV. The results are in agreement
with the mass composition at lower energies.

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