16163. Main Astronomical Observatory, National Academy of Sciences of Ukraine, ul. Academika Zabolotnogo 27, Kyiv, 03680, Ukraine 26163. Institute of Experimental Physics, Slovak Academy of Sciences, Watsonova 47, Ko?ice, 04001, Slovakia
Abstract:
Statistical acceleration of cosmic rays in a turbulent medium is considered. Charged particles are assumed to acquire energy in a bounded region of space and leave the acceleration region due to spatial diffusion caused by the scattering of cosmic rays in turbulent magnetic fields. Analytical solutions of the cosmic ray transport equation are obtained and equilibrium space-energy distributions of high-energy particles are studied in the acceleration region and beyond.