This book explores the ponderomotive wave forces of space plasma, which have implications for a large number of cosmic plasma phenomena. Plasma is a state of matter comprising an equal amount of negative (electrons) and positive (ions) charged particles. The ionized state is the dominating state of matter in the cosmos for stars, galaxies and their corresponding intermediate regions. This book discusses the plasma state and its corresponding theoretical implications based on the analysis of space plasma data. The theory of ponderomotive forcing offers a most important tool for the analysis of “in situ” plasma data of acceleration processes in the terrestrial and Martian plasma environment. In addition, the solar wind interaction with objects in the solar system also provides a roadmap for the analysis and interpretations of other stellar and galactic objects, out of reach for direct “in-situ” measurements.

Chapter 1 briefly describes the main properties of space plasmas and primary CR. Chapter 2 considers the problem of CR propagation in space plasmas described by the kinetic equation and different types of diffusion approximations. Chapter 3 is devoted to CR non-linear effects in space plasmas caused by CR pressure and CR kinetic stream instabilities with the generation of Alfvèn turbulence. In Chapter 4 different processes of CR acceleration in space plasmas are considered. The book ends with a list providing more than 1,300 full references, a discussion on future developments and unsolved problems, as well as Object and Author indexes.

A reprint/copy of the original - free on the internet, but published here for those who prefer reading a physical copy. Magnetic fields in cosmic physics are investigated, with special attention to plasma related phenomena. A concept of Magneto-hydrodynamic waves is proposed and investigated. A special review of solar physics is provided with magnetic storms, aurorae, and cosmic radiation all covered.