On UHECR energy estimation algorithms based on the measurement of electromagnetic component parameters in EAS

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dc.creatorIvanov, A. A.
dc.date2007-04-26
dc.date.accessioned2026-07-07T09:27:46Z
dc.date.available2026-07-07T09:27:46Z
dc.descriptionModel calculations are performed of extensive air shower (EAS) component energies using a variety of hadronic interaction parameters. A conversion factor from electromagnetic component energy to the energy of ultra-high energy cosmic rays (UHECRs) and its model and primary mass dependence is studied. It is shown that model dependence of the factor minimizes under the necessary condition of the same maximum position and muon content of simulated showers.
dc.descriptioncontracted version is accepted for publication in Doklady Physics
dc.identifierhttps://arxiv.org/abs/0704.3475
dc.identifierhttp://arxiv.org/abs/0704.3475
dc.identifierDoklady Physics, vol. 52, no.10, p.523-526 (2007)
dc.identifierdoi:10.1134/S1028335807100035
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/157225
dc.subjectAstrophysics
dc.titleOn UHECR energy estimation algorithms based on the measurement of electromagnetic component parameters in EAS
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