Abstract The aim of the NUCLEON space was to measure spectra of high-energy cosmic rays. The cosmic ray acceleration and propagation processes are determined by the magnetic rigidities of the particles. Thus the magnetic rigidity spectra of cosmic ray carbon and oxygen nuclei obtained by the NUCLEON experiment are analyzed and compared to some other experimental results. The spectral indices calculated for different thresholds with regard to magnetic rigidity are presented. The carbon and oxygen nuclei spectra are steeper than helium nuclei spectra in the 400-10000 GV area. The spectra of carbon and oxygen nuclei are similar to the proton spectrum before the “knee”.

中文翻译：

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根据 NUCLEON 实验得到的宇宙射线碳和氧核的光谱

摘要 NUCLEON 空间的目标是测量高能宇宙射线的光谱。宇宙射线加速和传播过程由粒子的磁刚度决定。从而分析了通过 NUCLEON 实验获得的宇宙射线碳和氧核的磁刚度谱，并与其他一些实验结果进行了比较。介绍了针对磁刚度的不同阈值计算的频谱指数。在 400-10000 GV 区域，碳和氧原子核光谱比氦原子核光谱更陡峭。碳和氧原子核的光谱类似于“膝盖”之前的质子光谱。