""\\"Very High Energy (VHE) γ-astronomy and cosmic ray physics are. the main goals of the ARGO-YBJ experiment. The detector is located in Tibet. (People’s Republic of China) and is a full-coverage Extensive Air Shower array consisting. of a carpet of Resistive Plate Chambers (RPCs). Altitude and full coverage. ensure an unprecedented reconstruction of showers close to their maximum size.. The performances of the detector and the present results concerning TeV cosmic. ray physics will be presented.\\"""

Aielli, G., Bacci, C., Bartoli, B., Bernardini, P., Bi, X.j., Bleve, C., et al. (2012). Cosmic rays in the TeV region with the ARGO-YBJ detector. IL NUOVO CIMENTO C, 35(1), 75-82 [10.1393/ncc/i2012-11125-9].

Cosmic rays in the TeV region with the ARGO-YBJ detector

BUSSINO, Severino Angelo Maria;DE VINCENZI, Mario;MARI, Stefano Maria;Montini P;Ruggieri F;
2012

Abstract

""\\"Very High Energy (VHE) γ-astronomy and cosmic ray physics are. the main goals of the ARGO-YBJ experiment. The detector is located in Tibet. (People’s Republic of China) and is a full-coverage Extensive Air Shower array consisting. of a carpet of Resistive Plate Chambers (RPCs). Altitude and full coverage. ensure an unprecedented reconstruction of showers close to their maximum size.. The performances of the detector and the present results concerning TeV cosmic. ray physics will be presented.\\"""
Aielli, G., Bacci, C., Bartoli, B., Bernardini, P., Bi, X.j., Bleve, C., et al. (2012). Cosmic rays in the TeV region with the ARGO-YBJ detector. IL NUOVO CIMENTO C, 35(1), 75-82 [10.1393/ncc/i2012-11125-9].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11590/278653
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