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Fig. 3


Time-averaged vertical profiles of the radiative, advective, and total flux for different runs. Top panel: run 442P during a highly convective episode. Middle panel: same run but averaging over convective and non convective episodes. Bottom panel: run 434P where there is no convection. The vertical line indicates the height above which magnetic pressure becomes larger than thermal pressure. The dashed line shows N2/ Ω2 where N is the Brunt-Väisälä frequency.

This figure is made of several images, please see below:

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