Physics – Nuclear Physics
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....6...35d&link_type=abstract
In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 6 p 35-38 (SEE N85-35848 24-93)
Physics
Nuclear Physics
Cosmic Ray Showers, High Energy Interactions, Inelastic Scattering, Protons, Scattering Cross Sections, Hadrons, Heat Measurement, Muons, Nuclei (Nuclear Physics), Radiation Distribution
Scientific paper
Proton initiated showers could be reliably separated from showers initiated by cosmic ray nuclei by means of arrays with large calorimetric area, using distributions of energy fractions for EAS electromagnetic muon and hadron components. Proton initiated showers penetrate deeper into the atmosphere and have relatively lower energy fraction in muons. Distribution of that energy fraction is sensitive to the value of the proton inelastic cross-section. It is shown that the analysis of this distribution let one distinguish between log2 S -rise and log S -rise of the cross-section at energies above 10 to the 15th power eV.
Danilova T. V.
Erlykin Anatoly D.
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