Rendering of density, magnetic field strength and toroidal magnetic field of the medium resolution simulations with varying feedback schemes. The blastwave model generates hotter winds and less mass loading than the superbubble model, leading to less magnetic field advection from the central plane of the disk. This generates a more radial compact structure for the magnetic field. Increasing the injection length in superbubble makes the vertical density structure more compact, leading to more resolved vertical velocity structures. In addition, we see a clear increase in the scale of the toroidal mean-field with the feedback strength as the galaxy extends both radially and vertically.