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Cosmic ray acceleration to very high energy through the non-linear amplification by cosmic rays of the seed magnetic field

Publication status:: Published

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APA Style

Bell, A., & Lucek, S. (2001). Cosmic ray acceleration to very high energy through the non-linear amplification by cosmic rays of the seed magnetic field. Monthly Notices of the Royal Astronomical Society, 321(3), 433–438.

MLA Style

Bell, A., and S. Lucek. “Cosmic Ray Acceleration to Very High Energy through the Non-Linear Amplification by Cosmic Rays of the Seed Magnetic Field.” Monthly Notices of the Royal Astronomical Society, vol. 321, no. 3, 2001, pp. 433–38.

Chicago Style

Bell, A, and S Lucek. 2001. “Cosmic Ray Acceleration to Very High Energy through the Non-Linear Amplification by Cosmic Rays of the Seed Magnetic Field.” Monthly Notices of the Royal Astronomical Society 321 (3): 433–38.
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Publisher copy:: 10.1046/j.1365-8711.2001.04063.x

Authors

+ Bell, A More by this author

Institution:

University of Oxford

Division:

MPLS

Department:

Physics

Sub department:

Atomic & Laser Physics

Role:

Author

+ Lucek, S More by this author

Role:

Author

Bibliographic Details

Journal:: Monthly Notices of the Royal Astronomical Society
Volume:: 321
Issue:: 3
Pages:: 433-438
Publication date:: 2001-03-01
DOI:: 10.1046/j.1365-8711.2001.04063.x
EISSN:: 1365-2966
ISSN:: 0035-8711

Item Description

Keywords:: cosmic rays

magnetic fields

shock waves

turbulence

acceleration of particles

plasmas
Pubs id:: pubs:16969
UUID:: uuid:ab8943be-4658-4392-a924-89fb01dac7b9
Local pid:: pubs:16969
Source identifiers:: 16969
Deposit date:: 2012-12-19

Terms of use

Copyright date:: 2001

Licence:: Terms and Conditions of Use for Oxford University Research Archive

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