宇宙射线在银河系中的传播和相互作用

V.N. Zirakashvili
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引用次数: 5

摘要

宇宙射线在银河系中的传播将很快被回顾。我们特别考虑了CR传播的自洽模型。在这些模型中,由CR各向异性驱动的CR流不稳定性导致了alfv湍流,而后者又决定了粒子的散射和扩散。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Cosmic ray propagation and interactions in the Galaxy

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.

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