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Results of Measurements of the Spectral Index of GCR Protons in the Energy Range 1-40 TeV

机译：1-40 TeV能量范围内GCR质子光谱指数的测量结果

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摘要

Figures summarize the measurement results shown in Tables 2-5. Figure 1 shows their distribution over the value of β_p (line segment along the abscissa axis corresponds to the energy range, within which lies about 90% of statistics of a given experiment). Figure 2 shows a histogram of this distribution. The averaged value of β_p from all experiments is < β_p > = 3.1 ± 0.05. We believe that the main cause of existing uncertainty in the discussion about the value of β_p in the proton spectrum in the range E > 1 TeV is not deficiency in the number of experiments, but the existence of two values β_p = 2.8 obtained in papers by JACEE and RUNJOB collaborations. It is unlikely that new measurements can solve existing uncertainty until the methodological causes of their large deviation from the bulk of results with β_p ≥ 3.0 are clarified.
机译：图总结了表2-5中显示的测量结果。图1显示了它们在β_p值上的分布（沿横坐标轴的线段对应于能量范围，在该范围内约占给定实验统计数据的90％）。图2显示了这种分布的直方图。来自所有实验的β_p的平均值为<β_p> = 3.1±0.05。我们认为，在讨论E> 1 TeV范围内质子谱中β_p值时存在不确定性的主要原因不是实验次数不足，而是存在通过论文获得的两个值β_p= 2.8。 JACEE和RUNJOB合作。新的测量方法不可能解决现有的不确定性，直到弄清它们与大量结果（β_p≥3.0）有很大偏差的方法学原因。

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