Surface density profiles of the O VI and C IV ions in the galactic outflow (R<30 kpc) for the CRMHD (left) and MHD (right) simulations. We show the median of the surface densities as thick lines and their 20^th to 80^th percentiles using shaded areas. Both metal ions trace the warm-hot component (T∼10⁵−10⁶ K) of the CGM. The different phase structures of both galactic winds lead to differences in the abundance of both ions.