论文标题
关于$ 10^{16} -10^{18} $ eV范围的宇宙射线频谱中的不规则性
On irregularities in the cosmic ray spectrum of $10^{16}-10^{18}$ eV range
论文作者
论文摘要
现有的中小型阵列用于研究超高能量的宇宙射线，旨在获取有关我们的星系和阿拉加术空间的信息，即搜索和研究产生相对主义颗粒磁通的天文对象。在星际空间中发生的这种颗粒与磁场和冲击波的漂移和相互作用引起了相同的兴趣。能量范围内宇宙光线的能量光谱的形状$ 10^{15} -10^{18} $ eV，其中观察到“膝盖”和“第二膝盖”，可以形成作为各种化学元件的部分光谱的叠加。使用最新的实验光谱数据对银河模型的验证使得可以研究宇宙射线的银河系和外乳外部成分的性质。该论文介绍了宇宙光线的能量光谱范围内的$ 10^{16} -10^{18} $ eV的测量结果是用小Cherenkov阵列获得的 - Yakutsk阵列的一部分。
Existing small, medium and large arrays for the study of cosmic rays of ultra-high energies are aimed for obtaining information about our galaxy and extragalactic space, namely to search and study astronomical objects that produce the flux of relativistic particles. The drift and interaction of such particles with magnetic fields and shock waves taking place in interstellar space causes the same interest. The shape of the energy spectrum of cosmic rays in the energy range $10^{15}-10^{18}$ eV, where the "knee" and the "second knee" are observed, can be formed as a superposition of the partial spectra of various chemical elements. Verification of galactic models, using recent experimental spectral data, makes it possible to study the nature of the galactic and extragalactic components of cosmic rays. The paper presents the result of the energy spectrum of cosmic rays in the range $10^{16}-10^{18}$ eV of measurements obtained with the Small Cherenkov array -- a part of the Yakutsk array.
