arXiv 1809.072852018-09astro-ph.HEastro-ph.IM

通过NUCLEON实验的Cosmic ray镍核谱

Cosmic ray Nickel nuclei spectrum by the NUCLEON experiment

V. Grebenyuk, D. Karmanov, I. Kovalev, I. Kudryashov, A. Kurganov, A. Panov, D. Podorozhny, A. Tkachenko, L. Tkachev, A. Turundaevskiy, O. Vasiliev, A. Voronin

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摘要：

核子实验的目的是测量宇宙射线的化学成分，电荷从Z=1到30，能量范围从5*10^11到10^15 eV。本文介绍了NUCLEON实验中Ni和Fe核的数据分析算法和能谱。

英文摘要：

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.

机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。