Vertical pressure profiles through the galactic disk and the inner CGM of both the CRMHD (left) and MHD (right) simulations. We show the vertical ram pressure $P_{\text{ram}}=\rho v_z^2$, vertical magnetic stress $T_{\text{mag}}=(B_x^2+B_y^2-B_z^2)/8\pi$, thermal pressure P_th, and CR pressure P_cr. The respective thick lines show the volume-weighted median values at each galactic height while the shaded regions enclose the 20^th to 80^th volume-weighted percentiles. We differentiate between three regions: the inner galactic disk R/kpc<5 (top panels), the main body of the galactic disk 5<R/kpc<10, and the outer (still star-forming) galactic disk 10<R/kpc<15. Most non-CR pressure components show similar values if we compare the CRMHD and MHD simulations at similar galactic radii. Their values show a rapid decline from the galactic disk into the CGM. The CR pressure shows larger scale heights and is the dominant pressure component inside the inner CGM.