Bolometric radiative intensity (left) and bolometric radiative flux (right) leaving the computational domain in the vertical direction through the top boundary as a function of time for both the magnetic (blue curve) and the non-magnetic (red curve) models. From top to bottom: models K8V, K2V, and F5V. The cyan and orange curves are the moving (box car) average of the magnetic and non-magnetic model, respectively, with a time window width of 5000 s.