Mass Composition of Cosmic Rays with Energies Greater than 1017 eV, According to the Data from Surface Scintillation Detectors of the Yakutsk EAS Array

A.V. Glushkov; M. I. Pravdin; A. V. Sabourov

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Mass Composition of Cosmic Rays with Energies Greater than 1017 eV, According to the Data from Surface Scintillation Detectors of the Yakutsk EAS Array

机译：根据Yakutsk EAR阵列的表面闪烁探测器的数据，宇宙射线的质量组成大于1017eV。

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《Bulletin of the Russian Academy of Sciences. Physics》 |2019年第8期|共3页
作者
A.V. Glushkov; M. I. Pravdin; A. V. Sabourov;
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Shafer Institute of Cosmophysical Research and Aeronomy Siberian Branch Russian Academy of Sciences677980YakutskRepublic of SakhaRussia;

Shafer Institute of Cosmophysical Research and Aeronomy Siberian Branch Russian Academy of Sciences677980YakutskRepublic of SakhaRussia;

Shafer Institute of Cosmophysical Research and Aeronomy Siberian Branch Russian Academy of Sciences677980YakutskRepublic of SakhaRussia;

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中图分类物理学;
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1. Mass Composition of Cosmic Rays with Energies Greater than 1017 eV, According to the Data from Surface Scintillation Detectors of the Yakutsk EAS Array [J] . A.V. Glushkov, M. I. Pravdin, A. V. Sabourov Bulletin of the Russian Academy of Sciences. Physics . 2019,第8期

机译：根据Yakutsk EAR阵列的表面闪烁探测器的数据，宇宙射线的质量组成大于1017eV。
2. Mass Composition of Cosmic Rays with Energies above 10(17) eV According to the Data from the Muon Detectors of the Yakutsk EAS Array [J] . Glushkov A. V., Saburov A. V. JETP Letters . 2019,第9期

机译：根据Yakutsk EAS阵列的MUON探测器的数据，具有10（17）eV以上的宇宙射线的大规模组成
3. Mass Composition of Cosmic Rays with Energies E-0 >= 10(17) eV According to the Data from the Ground-Based Detectors of the Yakutsk EAS Array [J] . Glushkov A. V., Saburov A. V. JETP Letters . 2014,第11期

机译：宇宙射线的质量组成e-0> = 10（17）EV根据Yakutsk EAR阵列的地面检测器的数据
4. Spectrum and mass composition of cosmic rays in the energy range 10~(15)-10~(18) eV derived from the Yakutsk array data [C] . S.P.Knurenko, A.Sabourov Symposium on Future Directions in UHECR Physics . 2013

机译：在能量范围内的宇宙射线的光谱和质量组成10〜（15）-10〜（18）EV来自Yakutsk阵列数据
5. Galactic cosmic ray composition at TeV energies: CREAM balloon data [D] . Childers, John Taylor, III 2007

机译：TeV能量下的银河系宇宙线成分：CREAM气球数据
6. The Pandora multi-algorithm approach to automated pattern recognition of cosmic-ray muon and neutrino events in the MicroBooNE detector [O] . R. Acciarri, C. Adams, R. An, -1

机译：Pandora多算法方法可自动识别MicroBooNE检测器中的宇宙射线μ子和中微子事件
7. Mass composition of cosmic rays with energy above 10**17 eV according to surface detectors of the Yakutsk EAS array [O] . Glushkov, A. V., Sabourov, A. 2014

机译：宇宙射线的质量成分，能量超过10 ** 17 eV，根据雅库茨克Eas阵列的表面探测器

Mass Composition of Cosmic Rays with Energies Greater than 1017 eV, According to the Data from Surface Scintillation Detectors of the Yakutsk EAS Array

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