Cosmic ray propagation and interactions in the Galaxy

V.N. Zirakashvili
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引用次数: 5

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.

宇宙射线在银河系中的传播和相互作用
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。
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