Spatial Distribution of the Magnetic Field Amplified in Young Supernova Remnants

Zirakashvili, Vladimir; Ptuskin, V. S.

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Spatial Distribution of the Magnetic Field Amplified in Young Supernova Remnants

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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). Spatial Distribution of the Magnetic Field Amplified in Young Supernova Remnants. In J. Blümer (Ed.), Contributions to the 29th International Cosmic Ray Conference (pp. 167-170). Karlsruhe: Forschungszentrum Karlsruhe.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-8773-4

Abstract

The spatial distribution of the magnetic field generated by a cosmic ray streaming instability in supernova remnants is determined. An alfvénic turbulence generated upstream supernova shock is amplified at the shock and advected downstream where its level rapidly approach to the value determined by the cosmic ray streaming downstream. Applications for an interpretation of X-ray observations are considered.