Level of magnetic turbulence, evaluated across various length scales (defined by the length of the cubic neighborhood used to estimate local magnetic fluctuations) for all seven simulations. The figure notably illustrates that beyond a certain characteristic size (∼1 kpc), the turbulence amplitude reaches a plateau, indicating the physical scales below which magnetic inhomogeneities manifest and evolve (for the present simulations). The stabilizing effect of stronger magnetic fields on turbulence is particularly evident here. The calculations were performed only once each simulations reached their late evolutionary stage, i.e., when the jets approached the domain boundary (Figs. 6 and 7).