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VOLUME 27 (1978) | ISSUE 6 | PAGE 374
Energy balance of cosmic rays in multiple scattering in a randomly inhomogeneous magnetic field
The equation for the energy density of cosmic rays is used to analyze the variation of their energy following multiple scattering by random magnetic-field inhomogeneities that move with velocity u(r). It is shown that if the radial gradient of the cosmic rays is positive the particles land in the acceleration regime.