arXiv · 2411.03868
Study of spatial inhomogeneities of cosmic rays in a synthetic turbulent magnetic field
Abstract
The paper presents a theoretical model describing the full power spectra of synchrotron radiation generated by relativistic electrons in a turbulent magnetic field. Using the theoretical model, numerical calculations of the complete power spectra of synchrotron radiation were performed for a turbulent field generated by the harmonic method. Additionally, a model sky map was constructed, demonstrating the structure of the spatial inhomogeneity of the synchrotron radiation power distribution as seen by an observer.
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P. K. Batrakov, V. O. Yurovsky, I. Kudryashov. 2024-11-06. Study of spatial inhomogeneities of cosmic rays in a synthetic turbulent magnetic field. https://arxiv.org/abs/2411.03868
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