Abstract
Effects of cosmic ray pressure on space plasma dynamics and effects of kinetic stream instability of non isotropic cosmic ray fluxes on the magnetic structure of space plasma are considered. These effects are important in our Galaxy and other galaxies, in the outer heliosphere, in cosmic ray sources, in the processes of cosmic ray acceleration by shock waves and in regions of magnetic field reconnection. Here we will consider general characteristics of cosmic ray nonlinear effects and its application to the dynamic processes in the galactic halo.
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Dorman, L.I. (1995). Cosmic Ray Nonlinear Effects in Space Plasma, 1. General Characteristics and Dynamic Galactic Halo. In: Shapiro, M.M., Silberberg, R., Wefel, J.P. (eds) Currents in High-Energy Astrophysics. NATO ASI Series, vol 458. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0253-7_15
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DOI: https://doi.org/10.1007/978-94-011-0253-7_15
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