“…Therefore, the scalar parametrization can be given by a function α(r, θ) = α 0 a(r) cos θ = α 0 α(r, θ), where the coefficient α 0 is positive and determines the highest intensity of the α-effect, α(r, θ) is a dimensionless quantity that satisfies the condition max|α(r, θ)| = 1 and the radial component a(r) = r. In accordance with the considered dynamo model, it is assumed that the action of the Archimedean (buoyancy) force with a mass density f out determines the differential rotation of the averaged flow v [14,15,21]. Thus, the MHD-equations, including the equations of the Navier-Stokes and the magnetic field induction B, taking into account the turbulent α-effect, the continuity condition of the velocity field v, the solenoidality condition of the magnetic field B and boundary conditions of adhesion, take the form [8]:…”