Third-order correlations and skewness in convection - I. A new approach for three-equation non-local models

Open Access

Fig. B.3.

Probing the TOM $\bar{w θ^{2}}$ $Mathematical equation: $ \overline{w\theta^2} $$ with 3D RHD solar simulation data for closed vertical boundary conditions. Details on the line style and colour coding can be found in the captions to Figs. 2 and 3. The top panel shows the full vertical depth range and the bottom one gives a zoom into the upper 40% of that range.

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