Turbulence transport and shock acceleration in solar corona
R. Vainio, T. Laitinen
Recent efforts on modeling coronal turbulence transport and shock acceleration self-consistently are reviewed. The considered models are based on the assumption that the turbulence responsible for the scattering of energetic ions consists of slab-mode Alfv\'en waves. A short discussion of the applied wave transport equation and particle transport coefficients is followed by a more extensive review of analytical and numerical modeling results of coupled evolution of energetic particle fluxes and wave intensities.
Turbulence and Nonlinear Processes in Astrophysical Plasmas, 932, 350-355, 2007