""The ARGO-YBJ experiment is in stable data taking since November 2007 at the YangBaJing Cosmic Ray. Laboratory (Tibet, P.R.China, 4300 m a.s.l.). It exploits a full coverage and high altitude approach to the. small air showers detection. The detector is made of a single layer of RPCs operated in streamer mode, fully. instrumenting a central carpet of about 5700 m2, then a guard ring extends the partially instrumented area to. about 11,000 m2. The large field of view (∼ 2 sr) and the high duty cycle (≥ 85%) allow a continuous monitoring. of the sky in the declination band from -10. ◦. to 70. ◦. ; the detector operates with an energy threshold of a few. hundred GeV. Recent achieved results will be reported""

Aielli, G., Bacci, C., Bartoli, B., Bernardini, P., Bi, X.j., Bleve, C., et al. (2011). The ARGO-YBJ contribution to the cosmic ray physics. NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS, 212-213, 59-67 [10.1016/j.nuclphysbps.2011.03.008].

The ARGO-YBJ contribution to the cosmic ray physics

BUSSINO, Severino Angelo Maria;DE VINCENZI, Mario;MARI, Stefano Maria;Montini P;Ruggieri F;
2011-01-01

Abstract

""The ARGO-YBJ experiment is in stable data taking since November 2007 at the YangBaJing Cosmic Ray. Laboratory (Tibet, P.R.China, 4300 m a.s.l.). It exploits a full coverage and high altitude approach to the. small air showers detection. The detector is made of a single layer of RPCs operated in streamer mode, fully. instrumenting a central carpet of about 5700 m2, then a guard ring extends the partially instrumented area to. about 11,000 m2. The large field of view (∼ 2 sr) and the high duty cycle (≥ 85%) allow a continuous monitoring. of the sky in the declination band from -10. ◦. to 70. ◦. ; the detector operates with an energy threshold of a few. hundred GeV. Recent achieved results will be reported""
Aielli, G., Bacci, C., Bartoli, B., Bernardini, P., Bi, X.j., Bleve, C., et al. (2011). The ARGO-YBJ contribution to the cosmic ray physics. NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS, 212-213, 59-67 [10.1016/j.nuclphysbps.2011.03.008].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11590/278752
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