This article reviews recent studies of scale interactions in magnetohydrodynamic turbulence.
The present-day increase of computing power, which allows for the exploration of different …

A discussion of the advantages and limitations of the concept of critical balance (CB), as
employed in turbulence phenomenologies, is presented. The incompressible …

The variable magnetic field of the solar photosphere exhibits periodic reversals as a result of
dynamo activity occurring within the solar interior. We decompose the surface field as …

The description of the local turbulent energy transfer and the high-resolution ion distributions
measured by the Magnetospheric Multiscale mission together provide a formidable tool to …

During common envelope evolution, an initially weak magnetic field may undergo
amplification by interacting with spiral density waves and turbulence generated in the stellar …

Analysis of the Vlasov-Maxwell equations from the perspective of turbulence cascade
clarifies the role of electromagnetic work, and reveals the importance of the pressure-strain …

The effect of rotation is considered to become important when the Rossby number is
sufficiently small, as is the case in many geophysical and astrophysical flows. Here we …

We formulate a coarse-graining approach to the dynamics of magnetohydrodynamic (MHD)
fluids at a continuum of length-scales ℓ. In this methodology, effective equations are derived …

Plasma turbulence at scales of the order of the ion inertial length is mediated by several
mechanisms, including linear wave dam**, magnetic reconnection, the formation and …

Using computations of three-dimensional magnetohydrodynamic (MHD) turbulence with a
Taylor-Green flow, whose inherent time-independent symmetries are implemented …