
The Pierre Auger Observatory has been designed to investigate the origin and nature of the ultra high energy cosmic rays using a hybrid detection technique. A review of selected results is presented, with the emphasis given to the measurement of energy spectrum, mass composition and arrival directions.
Nuclear and High Energy Physics, Physics, Astronomy, Nuclear physics, Pierre Auger Observatory, Engineering (General). Civil engineering (General), Astrophysics, Cosmic ray, Quantum mechanics, Particle Dark Matter and Detection Methods, Auger, Atomic physics, Physics and Astronomy, High-Energy Astrophysics, Physical Sciences, High-Energy Astrophysics and Particle Acceleration Studies, Neutrino Flavor Transformation and Detection, Energy spectrum, Ultra-high-energy cosmic ray, TA1-2040, Observatory, Energy (signal processing)
Nuclear and High Energy Physics, Physics, Astronomy, Nuclear physics, Pierre Auger Observatory, Engineering (General). Civil engineering (General), Astrophysics, Cosmic ray, Quantum mechanics, Particle Dark Matter and Detection Methods, Auger, Atomic physics, Physics and Astronomy, High-Energy Astrophysics, Physical Sciences, High-Energy Astrophysics and Particle Acceleration Studies, Neutrino Flavor Transformation and Detection, Energy spectrum, Ultra-high-energy cosmic ray, TA1-2040, Observatory, Energy (signal processing)
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