  We review the current status of research in MHD turbulence theory and
numerical experiments and their applications to astrophysics and solar science.
We introduce general tools for studying turbulence, basic turbulence models,
MHD equations and their wave modes. Subsequently, we cover the theories and
numerics of Alfvenic turbulence, imbalanced turbulence, small-scale dynamos and
models and numerics for supersonic MHD turbulence.
