Behaviour of the lateral shower age of cosmic ray extensive air showers

Abstract Some simple arguments are introduced for a possible explanation of the behavior lateral shower age proton-initiated showers. The corresponding analytical treatment based on proposed argument is then illustrated. Using Monte Carlo simulation (MC) code CORSIKA, we have validated how different characteristics associated with predicted in present parametrization, can be understood. and its correlations ages electron- neutral pion-initiated showers supports idea that result superposition several electromagnetic sub-showers initiated by pions might produce density distribution electrons proton shower. It also noticed simulated data stated feature still persists even local representation.