“…When the Lie transformations are found, they can be used to build particular solutions of the system under consideration, to reduce the order and to obtain invariants. Considering a symmetry classification problem, the symmetry properties of the MHD equations [19], [20], [21] have general peculiarities equivalent to the symmetries of the Navier-Stokes equations, namely, scale invariance under any contraction of the time-space x → x/λ, t → t/λ 1−h and velocity υ → λ −h υ , of scale ratios l, and other symmetries, see, e.g., [20], [21], [22]. Such similarity is originated from the fact that generalized equations of motion for the Weber-Clebsh potentials (in the Eulerian-Lagrangian formulation) describes both the Navier-Stockes and MHD dynamics [23].…”