Study of Cosmic Rays with Energies above 5 EeV Using Radio Method

IF 0.3 4区 物理与天体物理 Q4 PHYSICS, NUCLEAR Physics of Atomic Nuclei Pub Date : 2024-05-26 DOI:10.1134/S1063778824020157
I. S. Petrov, S. P. Knurenko
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Abstract

Regular measurements of radio emission produced by relativistic air shower particles were started at the Yakutsk array in 1986. After monitoring of the background noise in the array area, the frequency of 30–35 MHz was chosen, because noise level is minimal in this frequency range. During this time, air showers with highest energies of 100 EeV were registered. By means of hybrid measurements of charged particles, Cherenkov light and radio emission, it was shown that signal amplitude proportional to air shower energy and shape of lateral distribution at sea level correlates with the depth of maximum development. By these characteristics, the atomic weight of primary particles that generated air shower is estimated within QGSjetII-04 framework simulation.

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利用无线电方法研究能量超过 5 EeV 的宇宙射线
摘要1986 年开始在雅库茨克阵列对相对论气流粒子产生的无线电辐射进行定期测量。在对阵列区域的背景噪声进行监测后,选择了 30-35 兆赫的频率,因为该频率范围内的噪声水平最低。在此期间,记录了最高能量为 100 EeV 的气流。通过对带电粒子、切伦科夫光和无线电发射的混合测量表明,信号振幅与气流能量成正比,海平面上的横向分布形状与最大发展深度相关。根据这些特征,在 QGSjetII-04 框架模拟中估算了产生气雨的原生粒子的原子量。
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来源期刊
Physics of Atomic Nuclei
Physics of Atomic Nuclei 物理-物理:核物理
CiteScore
0.60
自引率
25.00%
发文量
56
审稿时长
3-6 weeks
期刊介绍: Physics of Atomic Nuclei is a journal that covers experimental and theoretical studies of nuclear physics: nuclear structure, spectra, and properties; radiation, fission, and nuclear reactions induced by photons, leptons, hadrons, and nuclei; fundamental interactions and symmetries; hadrons (with light, strange, charm, and bottom quarks); particle collisions at high and superhigh energies; gauge and unified quantum field theories, quark models, supersymmetry and supergravity, astrophysics and cosmology.
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