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The HERO project for the study of high-energy primary cosmic radiation
Authors:D. M. Podorozhnyi  E. V. Atkin  L. S. Burylov  A. G. Voronin  N. V. Kuznetsov  M. M. Merkin  R. A. Mukhamedshin  A. Yu. Pavlov  A. V. Romanov  L. G. Sveshnikova  L. G. Tkachev  A. N. Turundaevskii  A. P. Chubenko
Affiliation:1. Skobel’tsyn Institute of Nuclear Physics, Moscow State University, Moscow, 119992, Russia
2. Moscow Engineering Physics Institute (State University), Kashirskoe sh. 31, Moscow, 115409, Russia
3. Arsenal Design Bureau, ul. Komsomola 1-3, St. Petersburg, 195009, Russia
4. Institute for Nuclear Research, Russian Academy of Sciences, pr. Shestidesyatiletiya Oktyabrya 7a, Moscow, 117312, Russia
5. Joint Institute for Nuclear Research, Dubna, Moscow oblast, 141980, Russia
6. Lebedev Physical Institute, Russian Academy of Sciences, Leninskii pr. 53, Moscow, 119991, Russia
Abstract:Proposals for the High-Energy Ray Observatory (HERO) comprising scientific equipment with increased power availability are presented. Under the long exposure (>7 years), it is proposed to investigate the spectrum and charge composition of cosmic-ray nuclei up to E 0 ~ 1016 eV and to determine the behavior of the energy spectrum in the energy regions >100 GeV for cosmic-ray electrons and >50 GeV for γ radiation. The geometrical factor of the apparatus is 6.0–9.0 m2 sr depending on the type of particles.
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