|
|
|
|
| LEADER |
02323nmm a2200397 u 4500 |
| 001 |
EB000381842 |
| 003 |
EBX01000000000000000234894 |
| 005 |
00000000000000.0 |
| 007 |
cr||||||||||||||||||||| |
| 008 |
130626 ||| eng |
| 020 |
|
|
|a 9783642003097
|
| 100 |
1 |
|
|a Shalchi, Andreas
|
| 245 |
0 |
0 |
|a Nonlinear Cosmic Ray Diffusion Theories
|h Elektronische Ressource
|c by Andreas Shalchi
|
| 250 |
|
|
|a 1st ed. 2009
|
| 260 |
|
|
|a Berlin, Heidelberg
|b Springer Berlin Heidelberg
|c 2009, 2009
|
| 300 |
|
|
|a XIII, 199 p. 49 illus
|b online resource
|
| 505 |
0 |
|
|a 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
|
| 653 |
|
|
|a Atoms
|
| 653 |
|
|
|a Nuclear physics
|
| 653 |
|
|
|a Plasma Physics
|
| 653 |
|
|
|a Nuclear and Particle Physics
|
| 653 |
|
|
|a Space Physics
|
| 653 |
|
|
|a Atoms and molecules in external fields
|
| 653 |
|
|
|a Particle accelerators
|
| 653 |
|
|
|a Plasma (Ionized gases)
|
| 653 |
|
|
|a Astrophysics
|
| 653 |
|
|
|a Accelerator Physics
|
| 653 |
|
|
|a Molecules
|
| 653 |
|
|
|a Solar system
|
| 041 |
0 |
7 |
|a eng
|2 ISO 639-2
|
| 989 |
|
|
|b Springer
|a Springer eBooks 2005-
|
| 490 |
0 |
|
|a Astrophysics and Space Science Library
|
| 028 |
5 |
0 |
|a 10.1007/978-3-642-00309-7
|
| 856 |
4 |
0 |
|u https://doi.org/10.1007/978-3-642-00309-7?nosfx=y
|x Verlag
|3 Volltext
|
| 082 |
0 |
|
|a 523.01
|
| 520 |
|
|
|a 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
|