System on chip architecture for AugerPrime surface detector electronics upgrade of the pierre auger observatory

Abstract : The Pierre Auger Observatory, located near the town of Malargüe, Argentina, is the world's largest cosmic ray observatory. It has for objectives to probe the origin and characteristics of ultrahigh-energy cosmic rays (UHECRs). The results obtained by the Pierre Auger Collaboration provide important information on key aspects of the UHECR field, leading to new questions and open challenges which call for an upgrade of the Observatory. In the upgrade program, called AugerPrime, the 1660 surface detector stations will be improved in particular by implementing new electronics with higher performance. The new electronics aims to increase the number of analog channels and their dynamic range, to get a higher sampling rate and better timing accuracy. It is designed with a new generation of component, called SOC for System On Chip. A Linux system must be integrated for higher access development. First prototypes of the new electronics have been built and deployed at the Pierre Auger Observatory.
Type de document :
Communication dans un congrès
IEEE Nuclear Science Symposium & Medical Imaging Conference (2016 IEEE NSS/MIC), Oct 2016, Strasbourg, France. 2016 IEEE Nuclear Science Symposium, Medical Imaging Conference and Room-Temperature Semiconductor Detector Workshop (NSS/MIC/RTSD), pp.1-3, 〈http://2016.nss-mic.org/index.php〉. 〈10.1109/NSSMIC.2016.8069731〉
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http://hal.in2p3.fr/in2p3-01438327
Contributeur : Emmanuelle Vernay <>
Soumis le : mardi 17 janvier 2017 - 15:59:57
Dernière modification le : jeudi 2 août 2018 - 10:06:17

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IN2P3 | LPSC | UGA

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E. Lagorio. System on chip architecture for AugerPrime surface detector electronics upgrade of the pierre auger observatory. IEEE Nuclear Science Symposium & Medical Imaging Conference (2016 IEEE NSS/MIC), Oct 2016, Strasbourg, France. 2016 IEEE Nuclear Science Symposium, Medical Imaging Conference and Room-Temperature Semiconductor Detector Workshop (NSS/MIC/RTSD), pp.1-3, 〈http://2016.nss-mic.org/index.php〉. 〈10.1109/NSSMIC.2016.8069731〉. 〈in2p3-01438327〉

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