Upper limit on the fraction of the cosmic ray flux from a separable source in the energy interval (10 17 -10 19 eV), estimated using data from the Yakutsk array

Anatoly Ivanov

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Upper limit on the fraction of the cosmic ray flux from a separable source in the energy interval (10 17 -10 19 eV), estimated using data from the Yakutsk array

机译：使用Yakutsk阵列的数据估算的能量间隔中（10 17 -10 19 eV）来自可分离源的宇宙射线通量的分数的上限

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Arrival directions of ultra-high energy cosmic rays (UHECRs) in the equatorial system, detected with the Yakutsk array in the energy range (10~(17)-10~(19)eV), are re-analyzed using a new approximation for the zenith angle distribution of the event rate of extensive air showers (EAS). While the null hypothesis cannot be rejected based on the data used here, an upper limit on the fraction of cosmic rays from a separable source in the uniform background is derived as a function of declination and energy.

机译：使用雅库茨克阵列在能量范围（10〜（17）-10〜（19）eV）中探测到的赤道系统中的超高能宇宙射线（UHECR）的到达方向，使用新的近似方法重新分析大型空气淋浴（EAS）事件发生率的天顶角分布。尽管不能基于此处使用的数据拒绝零假设，但根据磁偏角和能量推导了来自统一背景中可分离源的宇宙射线份额的上限。

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《EPJ Web of Conferences》 |2019年第10期|共4页
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Anatoly Ivanov;
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中图分类物理学;
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1. Lateral Distribution Functions of Signals in Surface Scintillation Detectors of the Yakutsk Array, New Energy Estimates of Extensive Air Showers and the Energy Spectrum of the Primary Cosmic Radiation at Energies similar to 10(17)-10(19) eV [J] . Physics of atomic nuclei . 2019,第6期

机译：横梁阵列的表面闪烁探测器中的信号的横向分布函数，广泛的空气淋浴的新能量估计和初级宇宙辐射的能谱类似于10（17）-10（19）EV
2. Estimating the Fraction of Gamma Quanta in the Primary Cosmic Ray Flux with Energies of ~10~(17) eV from the MSU EAS Array Data [J] . N.N.Kalmykov, G.V.Kulikov, V.P.Sulakov, Bulletin of the Russian Academy of Sciences. Physics . 2013,第5期

机译：根据MSU EAS阵列数据估算约10〜（17）eV能量的主要宇宙射线通量中伽玛量子的分数
3. Estimate of the Fraction of Primary Photons in the Cosmic-Ray Flux at Energies ~10~(17) eV from the EAS–MSU Experiment Data~1 [J] . Yu. A. Fomina, N. N. Kalmykov, G. V. Kulikov, Journal of Experimental and Theoretical Physics . 2013,第6期

机译：从EAS-MSU实验数据〜1估算能量〜10〜（17）eV时宇宙射线通量中原光子的分数
4. Energy Spectrum of Primary Cosmic Rays in the Energy Region of 10~(17)-10~(20) eV by Yakutsk Array Data [C] . A.V.Glushkov, V.P.Egorova, A.A.Ivanov, International Cosmic Ray Conference . 2003

机译：yakutsk阵列数据的10〜（17）-10〜（20）EV中的初级宇宙射线的能谱
5. Upper limits on the ultra-high energy cosmic ray flux from unresolved sources. [D] . Burton, Ross E. 2012

机译：来自未解析源的超高能宇宙射线通量的上限。
6. Some Mineral Intakes of Koreans Estimated Using Food Composition Database and Real-time Food Analysis Data in Total Diet Study Were Comparable (P10-106-19) [O] . Jee Yeon Lee, Min Jung Seo, Sung Ok Kwon, 2019

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7. Estimate of the fraction of primary photons in the cosmic-ray flux at energies ~10^17 eV from the EAS-MSU experiment data [O] . Fomin, Yu. A., Kalmykov, N. N., Kulikov, G. V., 2013

机译：估算宇宙射线通量中初级光子的分数来自Eas-msU实验数据的能量~10 ^ 17eV

Upper limit on the fraction of the cosmic ray flux from a separable source in the energy interval (10 17 -10 19 eV), estimated using data from the Yakutsk array

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