Magnetic field amplification by cosmic rays in supernova remnants

Magnetic field amplification by cosmic rays in supernova remnants

Magnetic field amplification is needed to accelerate cosmic cays to PeV energies in supernova remants. Escaping cosmic rays trigger a return current in the plasma that drives a non-resonant hybrid instability. We run simulations in which we represent the escaping cosmic rays with the plasma return c...

书目详细资料
Main Authors:	Schure, K, Bell, A
格式:	Conference item
出版:	2012

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