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The concept of Universal Shower Profile is used to characterize the averagebehavior of high energy cosmic rays. The shape variables contain importantinformation about composition. They are independent of the primarycross-section by construction, but affected by other hadronic parameters, likemultiplicity. The two variables give access to the average nuclear mass of thesample and their compatibility serves as a test of hadronic models.

Sensitivity to primary composition and hadronic models from average shape of high energy cosmic ray shower profiles