The course intends to give a broad overview and recent developments in cosmic ray physics and
high-energy radiative processes. We will cover some interesting applications ranging from small
scales in solar physics, over the inter-stellar medium in galaxies to the largest scales with
clusters of galaxies. Marks will be based on four weekly assignments. Topics include:
Feb 25 | Quasilinear theory of cosmic rays | [pdf] |
Feb 28 | Diffusive shock acceleration - Fermi I process | [pdf] |
Mar 3 | Large scale MHD turbulence in CR transport | [pdf] |
Mar 6 | Nonlinear CR transport and Fermi II acceleration | [pdf] |
Mar 10 | Turbulence and cross field tranport of Cosmic Rays | [pdf] |
Mar 13 | Small scale turbulence and instability in Fermi I and CR transport | [pdf] |
Mar 17 | Cosmic ray interactions and radiative processes | [pdf] |
Mar 20 | Confronting theory with observations | [pdf][slides] |