2024/11/06 by Batrakov, P. K., Yurovsky, V. O., Kudryashov, I.
#FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE)
paper · doi:10.48550/arxiv.2411.03868
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.