Composite image showing the density-weighted projection of the magnetic field strength (blue) and the temperature (orange) for the inner 25 kpc of our high-resolution MHD run at t = 1025 Myr. Mock Hα and X-ray images are also shown in the lower right of the image. The top Hα image is untouched, while the centre right one has been smoothed with a Gaussian filter to match the angular resolution of the Muse instrument, assuming our cluster is at the same distance as the Perseus cluster, and is comparable to Fig. 2 in Olivares et al. (2019). The X-ray image is a superposition of three filters; namely, the 0.3–1.2 keV (red), 1.2–keV (green), and 2–7 keV (blue) bands, and is comparable to Fig. 1 from Fabian et al. (2006). The dashed white line is a contour map from the temperature field, showing the position of the outflowing bubbles.