Titlebook: Microphysics of Cosmic Plasmas; André Balogh,Andrei Bykov,John Raymond Book 2014 Springer Science+Business Media New York 2014 Collisionle

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Solar Surface and Atmospheric Dynamics,all the quiet sun fields is studied in some detail. Although dynamo action has been proved numerically, it is argued that current simulations are still far from achieving the complexity that might be present on the Sun. We based this statement not so much on the low magnetic Reynolds numbers used in

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Astrophysical Hydromagnetic Turbulence, and its extension to compressible magnetohydrodynamic turbulence are introduced. Implications for cosmic ray diffusion and acceleration is being discussed. Dynamo-generated magnetic fields with and without helicity are contrasted against each other. Certain turbulent transport processes are being m

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Nonclassical Transport and Particle-Field Coupling: from Laboratory Plasmas to the Solar Wind,laboratory fusion experiments, confinement of particles and energy is essential for sustaining the plasma long enough to reach burning conditions. For solar wind and magnetospheric plasmas, transport properties determine the spatial and temporal distribution of energetic particles, which can be harm

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Collisional and Radiative Processes in Optically Thin Plasmas,verview of the main collisional and radiative processes and examples of diagnostics relevant to the microphysical processes in the plasma. Many analyses assume a time-steady plasma with ion populations in equilibrium with the local temperature and Maxwellian distributions of particle velocities, but

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Notes on Magnetohydrodynamics of Magnetic Reconnection in Turbulent Media,n many astrophysical plasmas, which allows restructuring of magnetic fields and conversion of stored magnetic energy into heat and kinetic energy. Turbulence is known to dramatically change different transport processes and therefore it is not unexpected that turbulence can alter the dynamics of mag

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