Vertical profiles of the hydrogen number density and gas temperature measured above the galactic disk inside a cylinder with radius R<30 kpc. We show the median as a thick line and the shaded area spans from the 20^th to 80^th percentile of the volume-weighted quantity. Both, the CRMHD and MHD galaxies show similar profiles near the galactic disk. Above 2–3 kpc, their profiles start to differ and the MHD simulation shows a clear phase transition with hotter and more dilute gas at larger galactic heights.