Abstract
A consistent theory of energy exchange between high-energy charged cosmic-ray particles and the random inhomogeneities of a magnetic field frozen in the moving solar wind plasma is developed. It is shown that the mode of the particle energy variations at a given law of plasma velocity variation in space is determined by the specific form of the particle distribution function. The equation for the density of cosmic-ray energy is obtained. Consideration is given to the generation of a charged particle energy spectrum in the course of multiple scatterings by the random inhomogeneities of the magnetic field.
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Dorman, L.I., Katz, M.E., Fedorov, Y.I. et al. Variations of cosmic-ray energy in interplanetary space. Astrophys Space Sci 94, 43–95 (1983). https://doi.org/10.1007/BF00651760
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DOI: https://doi.org/10.1007/BF00651760