Cosmic ray Nickel nuclei spectrum by the NUCLEON experiment

1 (2); 14-b Metrolohichna Str.; 2); (2) oint Institute for Nuclear Research; (3) Skobeltsyn Institute of Nuclear Physics; 4); (4) Bogolyubov Institute for Theoretical Physics; 6; A.Kurganov (3); A. Panov (3)

arxiv: 1809.07285 · v2 · pith:OIF5FYF6new · submitted 2018-09-19 · 🌌 astro-ph.HE · astro-ph.IM

Cosmic ray Nickel nuclei spectrum by the NUCLEON experiment

V. Grebenyuk (1 , 2) , D. Karmanov (3) , I. Kovalev (3) , I. Kudryashov (3) , A.Kurganov (3) , A. Panov (3) , D. Podorozhny (3)

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A. Tkachenko (2 4) L. Tkachev (1 A.Turundaevskiy (3) O. Vasiliev (3) A. Voronin (3) ((1) "DUBNA" University Universitetskaya str. Dubna Moscow region Russia (2) oint Institute for Nuclear Research Joliot-Curie 6 (3) Skobeltsyn Institute of Nuclear Physics Moscow State University 1 (2) Leninskie gory GSP-1 Moscow (4) Bogolyubov Institute for Theoretical Physics 14-b Metrolohichna Str. Kiev Ukraine)

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keywords experimentnucleoncosmicnucleialgorithmanalysisarticlecharges

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The NUCLEON experiment is designed to measure chemical composition of cosmic rays with charges from Z=1 to 30 in an energy region from 5*10^11 to 10^15 eV. In this article the data analysis algorithm and spectra of Ni and Fe nuclei, measured in the NUCLEON experiment, are presented.

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Cosmic ray Nickel nuclei spectrum by the NUCLEON experiment

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