  This chapter reviews the recent progress made mainly during the last two
decades on wave turbulence in magnetized plasmas (MHD, Hall MHD and electron
MHD) in the incompressible and compressible cases. The emphasis is made on
homogeneous and anisotropic turbulence which usually provides the best
theoretical framework to investigate space and laboratory plasmas. The
interplanetary medium and the solar atmosphere are presented as two examples of
media where anisotropic wave turbulence is relevant. The most important results
of wave turbulence are reported and discussed in the context of space and
simulated magnetized plasmas. Important issues and possible spurious
interpretations are eventually discussed.
