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Fig. 12

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2D histograms relating the temperature (vertical axes) to swirling strength (upper panels) and velocity divergence (lower panels) in the upper photosphere. Results for the non-magnetic case are shown on the left panels and those for the magnetic case on the right panels. The dashed red lines indicate the mean temperature at a given value of the quantity on the horizontal axis. Each histogram is normalized by its 2D integral.

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