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

Volumn 321, Issue 3, 2001, Pages 433-438

  Bell, A R ^a   Lucek, S G ^a  

^a IMPERIAL COLLEGE LONDON   (United Kingdom)

Author keywords

Acceleration of particles; Cosmic rays; Magnetic fields; Plasmas; Shock waves; Turbulence

Indexed keywords

ACCELERATION; COSMIC RAYS; COSMOLOGY; HEAVY IONS; MAGNETIC FIELDS; MAGNETOPLASMA; PARTICLE ACCELERATORS; SUPERNOVAE;

ACCELERATION OF PARTICLES; ACCELERATION RATES; HIGH VELOCITY; LINEAR AMPLIFICATION; MAGNETIC-FIELD; NON LINEAR; SHOCK FRONTS; SHOCK-WAVES; VERY HIGH ENERGIES;

SHOCK WAVES;

EID: 0000831168     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2001.04063.x     Document Type: Article

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