Lateral distribution of high energy muons in EAS of sizes NE approximately equals 10(5) and NE approximately equals 10(6)

Details Lateral distribution of high energy muons in EAS of sizes NE approximately equals 10(5) and NE approximately equals 10(6) Lateral distribution of high energy muons in EAS of sizes NE approximately equals 10(5) and NE approximately equals 10(6)

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....7..151b&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 7 p 151-154 (SEE N85-35968 24-93)

Mathematics

Charge Distribution, Cosmic Ray Showers, Energy Spectra, Muons, Flux Density, Magnetic Spectroscopy, Mathematical Models, Particle Interactions, Primary Cosmic Rays

Scientific paper

Muon energy spectra and muon lateral distribution in EAS were investigated with the underground magnetic spectrometer working as a part of the extensive air showers (EAS) array. For every registered muon the data on EAS are analyzed and the following EAS parameters are obtained, size Ne, distance r from the shower axis to muon, age parameter s. The number of muons with energy over some threshold E associated to EAS of fixed parameters are measured, Ireg. To obtain traditional characteristics, muon flux densities as a function of the distance r and muon energy E, muon lateral distribution and energy spectra are discussed for hadron-nucleus interaction model and composition of primary cosmic rays.

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