Scale-dependent anisotropy of the velocities for all models (panel (a)) and the intermittency of magnetic and velocity fields (panel (b)). Panel (a): The coordinates ℓ_⊥ and ℓ_∥ represent the perpendicular and parallel scales of the eddies along the local magnetic field, respectively. Panel (b): The scaling exponent ζ vs. the order of structure functions. Our numerical results, with error bars estimated from the standard deviation, are compared with theoretical predictions from intermittency models: the Kolmogorov, She-Leveque, and Müller-Biskamp. The numerical results that we analyzed, t = 20t_A, are based on SD1 listed in Table 1.