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Fig. 1

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Snapshots of the emergent white light intensity during the temporal evolution (ordered upper-left to lower-right) of the hydrodynamical red giant model atmosphere. Bright granules where the matter is rising are surrounded by darker and significantly narrower intergranular lanes associated with down-flows. The spatial size of each frame is 15.6  ×  15.6 Gm2, and the time interval between frames 300 ks. The relative rms intensity contrast is given in the upper left corner of each frame.

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