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Preliminary results of the cosmic ray study in the NUCLEON space experiment.

Leonid Tkachev,N. Gorbunov,Victor Grebenyuk,S. Porokhovoy,A. Sadovsky,A. Tkachenko,E. Atkin,V. Shumikhin,V. Bulatov,V. Dorokhov,S. Filippov,D. Polkov,D. Karmanov,I. Kovalev,I. Kudryashov,M. Merkin,A. Pakhomov,A. Panov,D. Podorozhny,L. Sveshnikova, M. Torochkov,A. Turundaevskiy,O. Vasiliev,A. Voronin

Proceedings of 38th International Conference on High Energy Physics — PoS(ICHEP2016)（2017）

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Abstract
The orbital NUCLEON detector was launched at 26 December 2014 for 5 years of data taken.The experiment is designed to measure cosmic ray energy spectrum and charge composition at 100 GeV -1000 TeV and Z = 1-30 respectively.The NUCLEON apparatus structure, methods of primary cosmic ray charge and energy measurements are described.Preliminary results of the measurements of the cosmic nuclei energy spectra and the charge composition are presented from the first year and a half of data taking from orbit.
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Cosmic Rays,Neutrino Detection,Neutrino Oscillations,Cosmology,Neutrino Interactions
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