Physics
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....7..351v&link_type=abstract
In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 7 p 351-354 (SEE N85-35968 24-93)
Physics
Cosmic Ray Showers, Muons, Particle Collisions, Particle Flux Density, Radial Distribution, Radiation Detectors, Shock Fronts, Spectral Energy Distribution, Time Dependence, Charged Particles, Particle Density (Concentration), Particle Interactions, Statistical Analysis, Stochastic Processes
Scientific paper
Most investigations of the muon arrival time distribution in EAS during the past decade made use of parameters which can collectively be called rise time parameters. The rise time parameter TA/B is defined as the time taken for the integrated pulse from a detector to rise from A% to B% of its full amplitude. The use of these parameters are usually restricted to the determination of the radial dependence thereof. This radial dependence of the rise time parameters are usually taken as a signature of the particle interaction characteristics in the shower. As these parameters have a stochastic nature, it seems reasonable that one should also take notice of this aspect of the rise time parameters. A statistical approach to rise time parameters is presented.
Devilliers E. J.
Vanderwalt D. J.
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