Ultra-High Energy Cosmic Ray Study Results by Radio Emission Technique at Yakutsk Array
- 作者: Petrov I.S.1, Knurenko S.P.1, Petrov Z.E.1
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隶属关系:
- Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch
- 期: 卷 82, 编号 6 (2019)
- 页面: 795-799
- 栏目: Elementary Particles and Fields
- URL: https://journals.rcsi.science/1063-7788/article/view/194957
- DOI: https://doi.org/10.1134/S106377881966044X
- ID: 194957
如何引用文章
详细
The Yakutsk array is designed to study cosmic rays at energy 1015–1020 eV. The array detects charged particles, muons, Cherenkov light and radio emission. Radio-emission method is capable to study air shower physics independently of other shower components, including energy estimation of primary particle, longitudinal development of the particle cascade in the atmosphere (in the case of the Yakutsk array the depth of maximum development Xmax). For the showers with energy E ⩾ 1019 eV arrival directions were tracked and reconstructed in galactic and equatorial coordinate system to search for cosmic ray sources with such energies.
作者简介
I. Petrov
Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch
编辑信件的主要联系方式.
Email: igor.petrov@ikfia.ysn.ru
俄罗斯联邦, Yakutsk
S. Knurenko
Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Email: igor.petrov@ikfia.ysn.ru
俄罗斯联邦, Yakutsk
Z. Petrov
Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Email: igor.petrov@ikfia.ysn.ru
俄罗斯联邦, Yakutsk
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