从近源角度解释10TV区域的光谱不均匀性

V. Yurovsky, I. Kudryashov, F. Gasratov, Vasiliy Latonov
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引用次数: 0

摘要

本文考虑了用单一近源的各向同性扩散来描述实验数据中观测到的10 TV区域宇宙射线谱的不均匀性。结果表明,这样的描述是可能的,求得了源在空间和时间上可能定位的区域,其能量。罚函数法用于解释所有粒子谱上的数据。计算了银河系磁场中感兴趣的能量范围内扩散张量的各向异性
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Interpretation of the spectral inhomogeneity in the 10TV region in terms of a close source
The description of the inhomogeneity of the cosmic ray spectrum in the region of 10 TV, which is observed in experimental data, in terms of isotropic diffusion from a single close source is considered. It is shown that such a description is possible, the area of possible localization of the source in space and time, its energy is found. The method of penalty functions is used to account for the data on the spectrum of all particles. nhe calculation of the anisotropy of the diffusion tensor for the energy range of interest in the galactic magnetic field is also shown
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