UID:
almahu_9947363622302882
Format:
XIII, 199 p. 49 illus.
,
online resource.
ISBN:
9783642003097
Series Statement:
Astrophysics and Space Science Library, 362
Content:
This book deals with the physics of cosmic ray diffusion theory, focusing on the physics of nonlinear transport of cosmic rays through turbulent interplanetary or interstellar plasma. The author discusses fundamental processes such as cosmic ray propagation and acceleration in the solar system or in interstellar space, the properties of such plasmas, the standard quasilinear approach to describing plasma-particle interactions as well as several more accurate nonlinear theories. Within a nonlinear treatment he revisits the mechanism of diffusive shock acceleration, which is responsible for the high cosmic ray energies. Based on new results presented in this book the author proposes future numerical, theoretical and observational research that could advance the field of cosmic ray diffusion theory.
Note:
The General scenario -- On Astrophysical Turbulence -- The Quasilinear Theory -- The Nonlinear Guiding Center Theory -- The Weakly Nonlinear Theory -- The Second-Order QLT -- The Extended Nonlinear Guiding Center Theory -- Applications -- Summary and Outlook.
In:
Springer eBooks
Additional Edition:
Printed edition: ISBN 9783642003080
Language:
English
DOI:
10.1007/978-3-642-00309-7
URL:
http://dx.doi.org/10.1007/978-3-642-00309-7
