期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 358, 期 1, 页码 181-187出版社
OXFORD UNIV PRESS
DOI: 10.1111/j.1365-2966.2005.08774.x
关键词
acceleration of particles; magnetic fields; plasmas; turbulence; cosmic rays
A large flux of cosmic rays streaming through a magnetized plasma creates cavities of low plasma density and low magnetic field. The magnetic field focuses the cosmic ray trajectories into the cavities with the possible formation of filaments or beams of high-energy cosmic rays.
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