Time averaged radial profiles of latitudinally averaged for θ < 70° (upper panel) and θ > 70° (lower panel). The blue (red) lines refer to kinetic (magnetic) contributions, and the black lines denote the turbulent viscous contribution. Positive (negative) values are shown as solid (dotted) lines. The kinetic contributions from different times are shown as gray lines. The gray background on the left indicates the location of the stellar envelope.