Abstract:Abstract. The possibility for a self-consistent description of all the basic features of the observed cosmic ray spectra and primary composition variations in the energy range of 10 15 ÷ 10 20 eV within the Galactic origin scenario is examined.We assume the existence of Galactic sources that accelerate particles up to ∼ 3 · 10 18 Z eV and take into account a highly inhomogeneous (fractal-like) distribution of matter and magnetic fields in the Galaxy that leads to extremely large free paths of particles ("Lévy … Show more
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