| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1845615 | Nuclear Physics B - Proceedings Supplements | 2014 | 6 Pages |
Abstract
Cosmic ray propagation in the Galaxy is shortly reviewed. In particular we consider the self-consistent models of CR propagation. In these models CR streaming instability driven by CR anisotropy results in the Alfvénic turbulence which in turn determines the scattering and diffusion of particles.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
