Shocks and Fermi-I Acceleration. Non-Relativistic Shocks p 1, 1, T 1 p 0, 0, T 0 vsvs p 1, 1, T 1 p 0, 0, T 0 v 0 = -v s Stationary Frame Shock Rest Frame.
Matt Hill Gang Li SHINE 2007 Session summary for Shock geometry & upstream and downstream phenomena 1-day session: Tuesday morning Tuesday afternoon.
Strong nonresonant amplification of magnetic fields in particle accelerating shocks A. E. Vladimirov, D. C. Ellison, A. M. Bykov Submitted to ApJL.
Outstanding problems in Particle Astrophysics
School of Cosmic-ray Astrophysics, Erice, July 3, 2004 Thomas K. Gaisser Outstanding problems in Particle Astrophysics Cosmic-ray propagation Acceleration.
Magnetic-Field Amplification and Cosmic-Ray Acceleration in Turbulent MHD Shocks
Particle Astrophysics
PLASMA WAKEFIELD ACCELERATION
Radiation Processes in High Energy Astrophysics
Matt Hill Gang Li
Fabrizio Tavecchio - INAF/OA Brera
