Confining the high-energy cosmic rays
Diffusive shock acceleration is the prime candidate for efficient acceleration of cosmic rays. Galactic cosmic rays are believed to originate predominantly from this process in supernova remnant shock waves. Confinement of the cosmic rays in the shock region is key in making the mechanism effective....
Main Authors: | Schure, K, Bell, A |
---|---|
Format: | Journal article |
Published: |
2011
|
Similar Items
-
Confining the high-energy cosmic rays
by: Schure, K, et al.
Published: (2011) -
From cosmic ray source to the Galactic pool
by: Schure, K, et al.
Published: (2013) -
Cosmic ray acceleration in young supernova remnants
by: Schure, K, et al.
Published: (2013) -
Cosmic ray acceleration at oblique shocks
by: Bell, A, et al.
Published: (2011) -
Cosmic ray acceleration at oblique shocks
by: Bell, A, et al.
Published: (2011)