Lateral distribution of muons in small EAS and p(t) Distribution of secondaries

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Cosmic Ray Showers, High Altitude Nuclear Detection, Muons, Radiation Distribution, Secondary Cosmic Rays, Normal Density Functions, Scaling Laws, Spectral Energy Distribution, Statistical Correlation

Scientific paper

The lateral distribution functions (LDFs) and energy spectra of muons with energy greater than 5 GeV in small EAS (Ne = 8000-200,000) at mountain level are determined from experimental observations, presented in graphs, and compared with the results of model simulations. The flatness of the LDF is reproduced by using a Gaussian secondary-p(t) distribution and taking the energy spectrum, a mixed chemical composition, an isotropic angular distribution of the primaries, and the triggering conditions into account. The muon-component energy is found to be well correlated with the total number of muons (Nmu), and the dependence of Nmu on Ne supports a model with weak scaling violation.

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