Cosmic ray acceleration
Cosmic ray acceleration
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DOI：
10.1016/j.astropartphys.2012.05.022
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发表时间：
2013-03-01
影响因子：
3.5
通讯作者：
Bell, A. R.
中科院分区：
文献类型：
--
作者：
Bell, A. R.
本文综述了激波加速宇宙线的基本理论，包括激波附近等离子体不稳定性对宇宙线的限制、磁场方向的影响、宇宙线的最大能量和宇宙线谱的形状。注意力主要集中在超新星遗迹加速的银河宇宙射线上。(C)2012 Elsevier B.V.保留所有权利。
This review describes the basic theory of cosmic ray acceleration by shocks including the plasma instabilities confining cosmic rays near the shock, the effect of the magnetic field orientation, the maximum cosmic ray energy and the shape of the cosmic ray spectrum. Attention is directed mainly towards Galactic cosmic rays accelerated by supernova remnants. (C) 2012 Elsevier B.V. All rights reserved.