Cosmic ray acceleration by shocks: spectral steepening due to turbulent magnetic field amplification (2019)
Attributed to:
Astrophysics at Oxford 2016-2019
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1906.12240
Publication URI: https://arxiv.org/abs/1906.12240
Type: Other