2018
DOI: 10.1088/1748-0221/13/08/p08026
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The Extreme Energy Events experiment: an overview of the telescopes performance.

Abstract: The muon telescopes of the Extreme Energy Events (EEE) experiment are based on Multigap Resistive Plate Chambers (MRPC). The EEE network is composed, so far, of 53 telescopes, each made of three MRPC detectors; it is organized in clusters and single telescope stations distributed all over the Italian territory and installed in High Schools, covering an area larger than 3×105 km2. The study of Extensive Air Showers (EAS), that is one of the goal of the project, requires excellent performance in… Show more

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Cited by 29 publications
(28 citation statements)
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References 13 publications
(21 reference statements)
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“…The geographical area spanned by these telescopes exceeds 3×10 5 km 2 , namely the largest area in the world used for such kind of experiments. In order to operate as a real network, all collected data are sent in real time to the INFN CNAF computing center for storage and reconstruction [10].…”
Section: The Eee Project and The Polarqueeest Detectorsmentioning
confidence: 99%
“…The geographical area spanned by these telescopes exceeds 3×10 5 km 2 , namely the largest area in the world used for such kind of experiments. In order to operate as a real network, all collected data are sent in real time to the INFN CNAF computing center for storage and reconstruction [10].…”
Section: The Eee Project and The Polarqueeest Detectorsmentioning
confidence: 99%
“…Apart from that, a broad distribution is evident, which covers from approximately 20 km to more than 1200 km. The EEE network and the performance of the individual detectors have been described in many previous papers [26,27]. Here we will only briefly recall its main features and working parameters.…”
Section: The Eee Networkmentioning
confidence: 99%
“…The average time resolution is approximately 240 ps, allowing a precise measurement of the time of flight between the top and bottom chamber. An efficiency better than 90% is reached by 77% of the chambers, with possible sources of inefficiencies related to ageing effects or/and dead strips [17,18]. The trajectory of the charged particles crossing a telescope is obtained by fitting the impact points reconstructed on the 3 MRPCs, which are placed at a distance of 50 cm from each other.…”
Section: Pos(icrc2021)292mentioning
confidence: 99%
“…M. Abbrescia 1,2 , C. Avanzini 3 , L. Baldini 3,4 , R. Baldini Ferroli 5 , G. Batignani 3,4 , M. Battaglieri 6,7 , S. Boi 8,9 , E. Bossini 3,4 , F. Carnesecchi 10,11 , C. Cicalò 9 , L. Cifarelli 10,11 , F. Coccetti 12 , E. Coccia 13 , A. Corvaglia 14 , D. De Gruttola 15,16 , S. De Pasquale 15,16 , F. Fabbri 5 , L. Galante 17,18 , M. Garbini 10,12 , G. Gemme 6 , I. Gnesi 12,19 , S. Grazzi 6,20 , D. Hatzifotiadou 10,21 , P. La Rocca 22,23…”
Section: Full Authors List: Eee Collaborationunclassified