Time-averaged (t = 1.25 − 2.00 Gyr) vertical accelerations within a cylinder of r = 20 kpc for the four simulation setups. Accelerations are first volume averaged and then averaged in time. The pure MHD-cases do not exhibit outflows, so the gravitational force dominates. In the CRMHD simulation, the CR acceleration dominates the outward forces and is comparable to the inward gravitational acceleration up to a height of around 10 kpc. The CRMHD-low galaxy is dominated by CR acceleration at all heights.