Muon signals of cosmic ray interactions.

Details Muon signals of cosmic ray interactions. Muon signals of cosmic ray interactions.

Feb 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998acppb..29..339b&link_type=abstract

Acta Phys. Pol., B, Vol. 29, No. 1 - 2, p. 339 - 348

Physics

Cosmic Rays: Muons

Scientific paper

Muons originate from the decay of hadrons, produced in interactions of the primary cosmic particles with the nuclei of the atmosphere. The observation of the features of the muonic component, arising from the cascading processes induced by the primary particle, a phenomenon called extensive air showers (EAS), provides interesting information about the nature of the primary and its interactions. The authors illustrate this information potential by: (i) studies of the longitudinal development of EAS by measurements of the relative arrival time distributions of muons in the KASCADE experiment, (ii) studies with the Bucharest electromagnetic calorimeter WILLI for energy estimates of TeV muons and for determination of the charge ratio of the atmospheric muon flux.

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