Colloquium: Magnetohydrodynamic turbulence and time scales in astrophysical and space plasmas

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Anisotropy in Fast and Slow Solar Wind Fluctuations (2005, background): “Although wave and turbulence descriptions appear to be very different, it is likely that elements of each picture enter into describing the solar wind, since it is expected that MHD turbulence in its various regimes involves a balance of propagation and nonlinear effects (Zhou et al. 2004).”
Astrophysical magnetic fields and nonlinear dynamo theory (2004, unknown): “For some succinct reviews see also [291,292].”
Wave turbulence in incompressible Hall magnetohydrodynamics (2006, background): “However, note that several phenomenologies may be used to take into account the various regimes involving a non-trivial balance between propagation and nonlinear effects as for standard MHD (see, e.g., Zhou et al. 2004).”
Dissipation of Magnetohydrodynamic Waves on Energetic Particles: Impact on Interstellar Turbulence and Cosmic-Ray Transport (2005, methodology): “Comprehensive reviews of MHD turbulence have been given by Verma (2004), and by Zhou et al. (2004), Elmergreen & Scalo (2004), and Scalo & Elmergreen (2004) with application to interstellar turbulence.”