A Model of the Response of Surface Detectors to Extensive Air Showers Based on Shower Universality
arXiv:2405.03494 · doi:10.1103/PhysRevD.110.023030
Abstract
We present a full model of surface-detector responses to extensive air showers. The model is motivated by the principles of air-shower universality and can be applied to different types of surface detectors. Here we describe a parametrization for both water-Cerenkov detectors and scintillator surface detectors, as for instance employed by the upgraded detector array of the Pierre Auger Observatory. Using surface detector data, the model can be used to reconstruct with reasonable precision shower observables such as the depth of the shower maximum and the number of muons .
15 pages, 10 figures, prepared for submission to Phys.Rev.D
References in corpus (6)
- Depth of Maximum of Air-Shower Profiles at the Pierre Auger Observatory: Measurements at Energies above 10^17.8 eV
- The Offline Software Framework of the Pierre Auger Observatory
- Features of the energy spectrum of cosmic rays above eV using the Pierre Auger Observatory
- Measurement of the fluctuations in the number of muons in extensive air showers with the Pierre Auger Observatory
- The Concepts of "Age" and "Universality" in Cosmic Ray Showers
- Deep-Learning based Reconstruction of the Shower Maximum using the Water-Cherenkov Detectors of the Pierre Auger Observatory