Cosmic Ray Acceleration at the Galactic Wind Termination Shock with 
Self-Excited Alfvén Waves

Zirakashvili, Vladimir; Ptuskin, V. S.

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Cosmic Ray Acceleration at the Galactic Wind Termination Shock with Self-Excited Alfvén Waves

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Zirakashvili, Vladimir
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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Citation

Zirakashvili, V., & Ptuskin, V. S. (2005). Cosmic Ray Acceleration at the Galactic Wind Termination Shock with Self-Excited Alfvén Waves. In J. Blümer (Ed.), Contributions to the 29th International Cosmic Ray Conference, Pune, India, 2005 (pp. 237-240). Karlsruhe: Forschungszentrum Karlsruhe.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-8775-F

Abstract

Cosmic ray acceleration at the Galactic wind termination shock is considered. The generation of Alfvén waves by cosmic ray streaming is taken into account. The spectrum of Alfvén waves determines the cosmic ray diffusion. Applications are given for an explanation of the cosmic ray spectrum in the "knee" region.