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THE PRIMARY COSMIC RAY MASS COMPOSITION AROUND THE KNEE OF THE ENERGY SPECTRUM

机译:能量谱拐角附近的主要宇宙射线质量组成

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Experimental muon number distributions in EAS obtained at Moscow State University are analysed to estimate the primary mass composition at energies before and after knee. The mass composition before the knee corresponds to the normal one (as at E(0) similar to 10(12) eV), while experimental data after the knee are in agreement with the assumption that normal composition becomes enriched slowly by heavy nuclei, as also supported by contemporary diffusion models. [References: 21]
机译:分析在莫斯科国立大学获得的EAS中的实验性μ子数分布,以估计膝盖前后能量的主要质量组成。膝盖前的质量成分与正常成分相对应(在E(0)处类似于10(12)eV),而膝盖后的实验数据与正常成分逐渐被重核缓慢富集的假设相符。也得到了当代扩散模型的支持。 [参考:21]

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