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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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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Atomic & Laser Physics
Role:
Author
Journal:
Monthly Notices of the Royal Astronomical Society More from this journal
Volume:
321
Issue:
3
Pages:
433-438
Publication date:
2001-03-01
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
Keywords:
Pubs id:
pubs:16969
UUID:
uuid:ab8943be-4658-4392-a924-89fb01dac7b9
Local pid:
pubs:16969
Source identifiers:
16969
Deposit date:
2012-12-19

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