New electronics for the surface detectors of the Pierre Auger Observatory

Abstract : The surface detector array of the Pierre Auger Observatory consists of 1660 water Cherenkov detectors that sample the charged particles and photons of energetic cosmic ray air showers at the ground. In the framework of the planned upgrade of the Auger Observatory, AugerPrime, new electronics has been designed for the surface detectors. The electronics upgrade includes higher sampling frequency, increased dynamic range, increased processing capability, improved timing with up-to-date GPS receivers, and a better calibration and monitoring system. It will also process the data of the additional scintillator detectors planned for the upgrade.
Type de document :
Poster
34th International Cosmic Ray Conference (ICRC), Jul 2015, The Hague, Netherlands. Proceedings of Science, ICRC2015, pp.565, 2016
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http://hal.in2p3.fr/in2p3-01357039
Contributeur : Emmanuelle Vernay <>
Soumis le : lundi 29 août 2016 - 09:19:29
Dernière modification le : mardi 22 mai 2018 - 21:48:11

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  • HAL Id : in2p3-01357039, version 1

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M. Aglietta, P.S. Allison, R. Assiro, J.J. Beatty, K-H. Becker, et al.. New electronics for the surface detectors of the Pierre Auger Observatory. 34th International Cosmic Ray Conference (ICRC), Jul 2015, The Hague, Netherlands. Proceedings of Science, ICRC2015, pp.565, 2016. 〈in2p3-01357039〉

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