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The sensitivity to the mass composition as well as the reconstruction of theenergy of the primary particle are explored here by leveraging the features ofthe radio lateral distribution function. For the purpose of this analysis, aset of events measured with the LOPES experiment is reproduced with the latestCoREAS radio simulation code. Based on simulation predictions, a method whichexploits the slope of the radio lateral distribution function is developed(Slope Method) and directly applied on measurements. As a result, thepossibility to reconstruct both the energy and the depth of the shower maximumof the cosmic ray air shower using radio data and achieving relatively smalluncertainties is presented.

Investigation on the energy and mass composition of cosmic rays using LOPES radio data