M. Aglietta et al., STUDY OF THE PRIMARY COSMIC-RAY COMPOSITION AROUND THE KNEE OF THE ENERGY-SPECTRUM, Physics letters. Section B, 337(3-4), 1994, pp. 376-382
A study of the primary cosmic ray composition in the energy range 5.10
(14)-5.10(15) eV is performed through the analysis of the deep undergr
ound muons and of the e.m. component of Extensive Air Showers detected
in coincidence by the MACRO and EAS-TOP experiments at the Gran Sasso
Laboratory. We conclude that: a) pure proton and Iron primary beams a
re excluded by the experimental data; b) a fraction of nuclei heavier
than Helium is necessary to explain the experimental data both below a
nd above the knee; c) a mixed composition, obtained a priori from extr
apolations of the spectra directly measured below 100 TeV, yields a re
asonable account of the observations up to the knee of the primary spe
ctrum.