Rendering of density, magnetic field strength of the Low resolution simulations with varying feedback scheme at t = 2 Gyr. Strong field growth can be seen for both the blastwave model and the high coupling superbubble model (N_FB = 200). Both the blastwave model and the physical superbubble model (N_FB = 1) leads to small feedback bubbles which pushes material far away from the disk. The mass loading in the superbubble model (N_FB = 1) is however much larger as the blastwave model mainly generate hot low-density outflows, this means that there is less transfer of magnetic fields from the central region in the blastwave model. Increasing the injection length (N_FB = 200) leads to more mass loading, larger feedback bubbles and a more concentrated vertical structure, which in turn lead to more amplification of the magnetic field within the central disk.