Testing the surface detector simulation for the Pierre Auger Observatory

Piera L. Ghia

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arXiv · 0706.1212

Testing the surface detector simulation for the Pierre Auger Observatory

Piera L. Ghia

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Abstract

The building block of the surface detector of the Pierre Auger Observatory is a water Cherenkov tank. The response to shower particles is simulated using a dedicated program based on GEANT4. To check the simulation chain, we compare the simulated signals produced by cosmic muons at various zenith angles with experimental data from a special Cherenkov detector equipped with a muon hodoscope. The signals from muon-decay electrons and the evolution of the charge with water level are also studied.

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Piera L. Ghia. 2007-06-12. Testing the surface detector simulation for the Pierre Auger Observatory. https://arxiv.org/abs/0706.1212

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