Titlebook: Cosmic Plasma Physics; Boris V. Somov Book 2000 Springer Science+Business Media Dordrecht 2000 MHD.Plasma.astronomy.magnetic field.magneto

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A Hydrodynamic Description of Cosmic Plasma,In this Chapter we are not concerned with individual particles but we will treat individual kinds of particles as continuous mediums interacting between themselves and with an electromagnetic field.

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Magnetohydrodynamics of Cosmic Plasma,Magnetohydrodynamics (MHD) is the simplest but sufficient approximation to describe many large-scale phenomena in space.

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MHD Waves in Cosmic Plasma,Magnetohydrodynamic waves create turbulence, nonlinearly cascade in a wide range of wavenumbers, accelerate particles and produce a lot of effects in cosmic plasma.

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Heterodoxy

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Particle Acceleration by Shock Waves,Sir Charles Darwin (1949) presumably thought that shock waves are responsible for accelerating cosmic rays. Nowadays shocks are widely recognized as a key to understanding particle acceleration in a variety of astrophysical environments.

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Stationary Flows in a Magnetic Field,There exist two different sorts of stationary flows depending on whether or not a medium can be considered as ideal or non-ideal.