Damping of Alfvén Waves in MHD Turbulence and Implications for Cosmic Ray Streaming Instability and Galactic Winds

Damping of Alfvén Waves in MHD Turbulence and Implications for Cosmic Ray Streaming Instability and Galactic Winds

Alfvénic component of MHD turbulence damps Alfvénic waves. The consequences of this effect are important for many processes, from cosmic ray (CR) propagation to launching outflows and winds in galaxies and other magnetized systems. We discuss the differences in the damping of the streaming instabili...

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Bibliografski detalji
Glavni autori: Alex Lazarian, Siyao Xu
Format: Članak
Jezik:English
Izdano: Frontiers Media S.A. 2022-05-01
Serija:Frontiers in Physics
Teme:
cosmic rays
magnetic fields
turbulence
interstellar medium
galactic winds
Online pristup:https://www.frontiersin.org/articles/10.3389/fphy.2022.702799/full

Internet

https://www.frontiersin.org/articles/10.3389/fphy.2022.702799/full

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