12-20 July 2017
BEXCO
Asia/Seoul timezone
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Contribution

BEXCO - Room A(101/102)

[CRD021] Energy spectra of protons and helium nuclei measured by the cosmic ray NUCLEON experiment

Speakers

  • Andrey TURUNDAEVSKIY

Primary authors

Co-authors

  • Viktor GREBENYUK (Joint Institute for Nuclear Research,Russia,Dubna State University)
  • Nikolai GORBUNOV (SDB Automatika,Russia)
  • Eduard ATKIN (National Research Nuclear University, "MEPhI'',Russia)
  • D. Karmanov SKOBELTSYN (Skobeltsyn Institute of Nuclear Physics of Moscow State University,Russia)
  • Igor KOVALEV (Skobeltsyn Institute of Nuclear Physics of Moscow State University,Russia)
  • Ilya KUDRYASHOV (Skobeltsyn Institute of Nuclear Physics of Moscow State University,Russia)
  • Aleksandr KURGANOV (Skobeltsyn Institute of Nuclear Physics of Moscow State University,Russia)
  • Alexander PANOV (Skobeltsyn Institute of Nuclear Physics of Moscow State University,Russia)
  • Mikhail MERKIN (Skobeltsyn Institute of Nuclear Physics of Moscow State University,Russia)
  • Sergei POROKHOVOY (Joint Institute for Nuclear Research,Russia)
  • Vitaly SHUMIKHIN (National Research Nuclear University, "MEPhI'',Russia)
  • Dmitry PODOROZHNY (Skobeltsyn Institute of Nuclear Physics of Moscow State University,Russia)
  • Artur TKACHENKO (Joint Institute for Nuclear Research,Russia, Bogolubov Institute for Theoretical Physics,Ukraine)
  • Leonid TKACHEV (Joint Institute for Nuclear Research,Russia, Dubna State University)
  • Aleksandr VORONIN (Skobeltsyn Institute of Nuclear Physics of Moscow State University,Russia)
  • Oleg VASILIEV (Skobeltsyn Institute of Nuclear Physics of Moscow State University,Russia)

Description

The NUCLEON satellite experiment is designed for direct measurements of the energy spectra of cosmic-ray nuclei and the chemical composition (Z=1−30) at an energy range up to 1000 TeV. The energy spectra of protons and helium nuclei are presented. Some spectral peculiarities were found. The differences of protons and helium spectra are investigated.