Typical magnetic butterfly diagrams (i.e., time–latitude diagram of the axisymmetric toroidal magnetic field) achieved in the simulations published in Brun et al. (2022). On the top panel, the butterfly diagram is shown as a colour contour plot in Gauss for the rapidly rotating cases (low Rossby numbers), in the middle panel for intermediate value (Sun-like) and in the bottom panel for statistically steady solutions for slowly rotating stars with large Rossby numbers.