Cosmic ray physics with the OPERA Detector

被引：0

作者：

Brugiere, T. ^{[1
]}

机构：

[1] Univ Claude Bernard Lyon I, Inst Phys Nucl Lyon, Lyon, France

来源：

ASTROPARTICLE, PARTICLE AND SPACE PHYSICS, DETECTORS AND MEDICAL PHYSICS APPLICATIONS | 2010年 / 5卷

关键词：

long baseline experiments; neutrino oscillations; atmospheric muons;

D O I：

10.1142/9789814307529_0030

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

OPERA is a long-baseline neutrino experiment located in the Hall C of the underground Gran Sasso Laboratory at an average depth of 3.8 km.w.e., corresponding to muon energies at surface higher than 1.5 TeV. In this paper we focus on the potentialities of OPERA used as a cosmic ray detector. We report on the measurement of the atmospheric muon charge ratio, on the analysis of upgoing muons induced by atmospheric neutrinos and on the large cosmics showers inducing coincidences between different experiments in Gran Sasso.

引用

页码：180 / 184

页数：5

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