Intensity of cosmic-ray muons and of primary nucleons according to data from the Baksan underground scintillation telescope.

Details Intensity of cosmic-ray muons and of primary nucleons according to data from the Baksan underground scintillation telescope. Intensity of cosmic-ray muons and of primary nucleons according to data from the Baksan underground scintillation telescope.

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992svjnp..55.1169b&link_type=abstract

Sov. J. Nucl. Phys., Vol. 55, No. 8, p. 1169 - 1174

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Scientific paper

Data have been obtained on the energy spectrum of cosmic-ray muons at
energies 1 - 30 TeV. The data are compared with the results of other
experiments. Under the assumption that a superposition model is valid,
these data are used to calculate the spectrum of all nucleons of the
primary cosmic rays over the energy range 10 - 200 TeV/nucleon.

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