Origin and propagation of galactic cosmic rays (Klaudia Herbst and Bernd Heber)

1. Particle propagation in turbulent magnetic fields

a. Parker's transport equation
a1: The diffusion tensor
a2: Convection
a3: Adiabatic energy exchange
a4: Drift effects
b. Diffusion convection approximation
c. Force-Field solution

2. Origin of GCRs

a Sources
a1: Supernova remnent
a2: acceleration by the Fermi processes
a3: some thoughts about galactic propagation



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