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AbstractAbstract
[en] Angular distributions of single hadrons and electromagnetic particles measured at the Pamir experiment (4370 m a.s.l.) are compared with distributions obtained by EAS simulations with the CORSIKA code including different primaries and different high interaction models. Additionally, the measured optical density spectrum of the e/γ particles is compared with simulated spectra, including a detector simulation based on the GEANT code
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10. international symposium on very high energy cosmic ray interactions; Assergi (Italy); 12-17 Jul 1998; S0920563299002303; Copyright (c) 1999 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.; Country of input: International Atomic Energy Agency (IAEA)
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Journal Article
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