Cosmic Plasma Physics / by Boris V. Somov.

The scope of this book is not typical of the majority of texts in cosmic plasma physics. The consecutive consideration of physical principles, starting from the most general ones, and simplifying assumptions allows students interested in astronomy to find the answers to two key questions: (1) what a...

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Bibliographic Details
Online Access: Full Text (via Springer)
Main Author: Somov, B. V. (Boris V.)
Format: eBook
Language:English
Published: Dordrecht : Springer Netherlands, 2000.
Series:Astrophysics and space science library ; 251.
Subjects:

MARC

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505 0 |a 1 Particles and Fields: Exact Self-Consistent Description -- 2 A Statistical Description of Cosmic Plasma -- 3 Propagation of Accelerated Particles in Cosmic Plasma -- 4 The Motion of a Particle in Given Fields -- 5 Wave-Particle Interactions in Cosmic Plasma -- 6 Coulomb Collisions of Particles in Cosmic Plasma -- 7 A Hydrodynamic Description of Cosmic Plasma -- 8 Magnetohydrodynamics of Cosmic Plasma -- 9 Cosmic Plasma Flows in a Strong Magnetic Field -- 10 MHD Waves in Cosmic Plasma -- 11 Discontinuous Flows in a MHD Medium -- 12 Evolutionarity of MHD Discontinuities -- 13 Particle Acceleration by Shock Waves -- 14 Cosmic Plasma Equilibrium in Magnetic Field -- 15 Stationary Flows in a Magnetic Field -- 16 Magnetic Reconnection in Current Sheets -- 17 Stationary Models of Reconnecting Current Sheets -- 18 Particle Acceleration in Current Sheets -- 19 Structural Instability of Reconnecting Current Sheets -- 20 The Tearing Instability of a Reconnecting Current Sheet -- 21 Selected Trends in Cosmic Plasma Physics -- 22 Magnetic Reconnection of Electric Currents -- Epilogue -- Appendix 1. Notation -- Appendix 2. Useful Expressions -- Appendix 3. Constants. 
520 |a The scope of this book is not typical of the majority of texts in cosmic plasma physics. The consecutive consideration of physical principles, starting from the most general ones, and simplifying assumptions allows students interested in astronomy to find the answers to two key questions: (1) what approximation is the simplest, but still sufficient for the description of a phenomenon in cosmic plasmas, and (2) how to build an adequate model of this phenomenon. Astronomers of the future will need such tools. Astronomy of the future will become an increasingly more precise science, similar to physics or plasma physics. This is what the book aims to teach. 
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