The longitudinal development of muons in cosmic ray air showers at energies 10(15) - 10(17) eV

Details The longitudinal development of muons in cosmic ray air showers at energies 10(15) - 10(17) eV The longitudinal development of muons in cosmic ray air showers at energies 10(15) - 10(17) eV

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....7..135.&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 7 p 135-138 (SEE N85-35968 24-93)

Computer Science

Cosmic Ray Showers, Iron, Longitude Measurement, Monte Carlo Method, Muons, Nuclear Interactions, Simulation, Particle Density (Concentration), Proton Beams

Scientific paper

The relationship between longitudinal development of muons and conventional equi-intensity cuts is carefully investigated. The development of muons in Extensive Air Showers (EAS) has been calculated using simulation with a scaling violation model at the highest energies and mixed primary composition. Profiles of equi-intensity cuts expected at observation altitudes of 550, 690 and 930/sq cm can fit the observed data very well.

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