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  Spatial Distribution of the Magnetic Field Amplified in Young Supernova Remnants

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.

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 Creators:
Zirakashvili, Vladimir1, Author           
Ptuskin, V. S.2, Author
Affiliations:
1Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society, ou_904550              
2Institute for Terrestrial Magnetism, Ionosphere and Radiowave Propagation, 142190 Troitsk, Moscow Region, Russia, ou_persistent22              

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Free keywords: Supernova Remnants
 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.

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Language(s): eng - English
 Dates: 2005-12
 Publication Status: Issued
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: eDoc: 277795
URI: http://icrc2005.tifr.res.in/
 Degree: -

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Title: 29th International Cosmic Ray Conference
Place of Event: Pune, Mumbai
Start-/End Date: 2005-08-03 - 2005-08-10

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Title: Contributions to the 29th International Cosmic Ray Conference
Source Genre: Proceedings
 Creator(s):
Blümer, Johannes, Editor
Affiliations:
-
Publ. Info: Karlsruhe : Forschungszentrum Karlsruhe
Pages: - Volume / Issue: - Sequence Number: - Start / End Page: 167 - 170 Identifier: -