Abstract
A electrons generation spectrum in galactic sources of cosmic rays is reconstructed within the fractal diffusion model according to the energy spectrum of particles and synchrotron radiation observed in the Solar system. It is shown that a self-consistent description of the experimental data can be obtained if the exponent of the electrons generation spectrum in the sources within the range of 0.1–103 GeV varies from p = 2.6 in the low energy range to p = 2.85 at E ≥ 103 GeV.
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