Cosmic ray physics with the OPERA Detector

Details Cosmic ray physics with the OPERA Detector Cosmic ray physics with the OPERA Detector

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010apsp.conf..180b&link_type=abstract

ASTROPARTICLE, PARTICLE AND SPACE PHYSICS, DETECTORS AND MEDICAL PHYSICS APPLICATIONS. Proceedings of the 11th Conference. Held

Physics

Medical Physics

Long Baseline Experiments, Neutrino Oscillations, Atmospheric Muons

Scientific paper

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.

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