Estimating primary energy of cosmic rays by calculating secondary particles density in optimum distance from shower core

Abstract

Optimum distance (R opt ) is a distance from the shower core in which the density calculated by lateral distribution function, has its minimum uncertainty. In this paper, Using CORSIKA code, proton, carbon and iron primary in the energy range between 10 13 -3×10 15 eV are simulated to find R opt for Alborz-I array located at an altitude of 1200 m above sea level. It is shown that R opt is approximately independent of characteristics of primary particle and it is only dependent to array configuration. Dependency of R opt on layout and detector spacing for 20 Alborz-I array detectors, are studied. It is shown that the Alborz-I array layout and its detector spacing result into the best (minimum uncertainty) R opt for its number of detectors. In this work R opt for Alborz-I array is obtained about 9±1 m. In addition, it is shown that, by finding dependency of primary energy to density in optimum distance, energy of primary particle can be estimated well. An energy estimation function is suggested and the function is examined by another set of simulated showers.