论文标题
在2x10 $^{13} $ -3x10 $^{17} $ eV时，对Tien -Shan阵列数据的进一步分析的结果
Results of the further analysis of Tien-Shan array data on the energy spectrum of primary cosmic rays at 2x10$^{13}$ - 3x10$^{17}$ eV
论文作者
论文摘要
根据Tien Shan Array的数据，根据在广泛的空气淋浴器中检测到电子数量，根据Tien Shan Array的数据显示，在2x10 $^{13} $ -3x10 $ -3x10 $ -3x10 $^{17} $ eV之间的能量射线的能量光谱。在能量范围5x10 $^{15} $ -3x10 $^{17} $ eV中，通过强子阵列获得了频谱，并以单个实验的结果为基础，从2x10 $^{13} $ eV扩展到了低势能区域。在10 $^{16} $ -3x10 $^{17} $ eV的能量范围内，光谱的斜率变化以及该频谱在约1017 eV处的功能进行了详细分析并进行了详细分析并进行了描述。将所讨论的频谱与其他一些阵列获得的结果进行了比较。
The energy spectrum of primary cosmic rays at energies between at 2x10$^{13}$ - 3x10$^{17}$ eV is presented according to data from the Tien Shan array on the basis of the detection of the number of electrons in extensive air showers. In the energy range 5x10$^{15}$ - 3x10$^{17}$ eV, the spectrum was obtained by means of the HADRON array and was extended to the region of lower energies from 2x10$^{13}$ eV on the basis of the results of an individual experiment. The changes in the slope of the spectrum in the energy range of 10$^{16}$ - 3x10$^{17}$ eV and a feature of this spectrum at about 1017 eV are analyzed in detail and are described. The spectrum in question is compared with the results obtained at some other arrays.
