Comparison of the vertical structure and CGM properties of our galaxies at t = 1.5 Gyr. From top to bottom, we show slices through the midplane of the vertical velocity, gas temperature, gas density, magnetic-to-thermal energy ratio, and the CR-to-thermal pressure ratio. Without CRs, we would have a turbulent, hot CGM with a mix of inflow and outflow. CRs help launch hot, thermally dominated outflows from the center and mix colder gas into the CGM.