| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 8133041 | Astroparticle Physics | 2013 | 15 Pages |
Abstract
⺠Understanding of cosmic ray acceleration has progressed remarkably in recent years. ⺠Magnetic field amplification is necessary for acceleration to 1 PeV. ⺠There are differences between parallel, oblique and perpendicular shocks. ⺠High efficiency probably requires non-linear self-regulation. ⺠There is still much we do not know.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
A.R. Bell,