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Dortmund 2006 – scientific programme

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T: Teilchenphysik

T 607: Kosmische Strahlung XI

T 607.4: Talk

Friday, March 31, 2006, 12:00–12:15, HG2-HS1

Simulation of very high-energy events for the Pierre Auger Observatory — •Viviana Scherini, Heiko Geenen, Karl-Heinz Kampert, Lorenzo Perrone, and Simon Robbins — Bergische Universität Wuppertal, Fachbereich C Physik, 42119 Wuppertal

The Pierre Auger Observatory combines two independent detection techniques, fluorescence and surface water-Cherenkov, allowing the reconstruction of extensive air showers with two complementary measurements. The hybrid detector has been designed in order to cover a large dynamic signal range extending its aperture to showers induced by very high-energy cosmic rays of energies up to 1021 eV and above. A detailed study of the fluorescence detector response to very high-energy showers is done in order to check its performances and improve the capability of the reconstruction at the highest energies.

Gefördert mit Mitteln der BMBF Verbundforschung Astroteilchenphysik.

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