Investigation on the Energy and Mass Composition of Cosmic Rays Using LOPES Radio Data

The sensitivity to the mass composition as well as the reconstruction of the energy of the primary particle are explored here by leveraging the features of the radio lateral distribution function. For the purpose of this analysis, a set of events measured with the LOPES experiment is reproduced with the latest CoREAS radio simulation code. Based on simulation predictions, a method which exploits the slope of the radio lateral distribution function is developed (Slope Method) and directly applied on measurements. As a result, the possibility to reconstruct both the energy and the Xmax, i.e. depth of the shower maximum, of the cosmic ray air shower using radio data and achieving relatively small uncertainties is presented.