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\@writefile{lof}{\contentsline {figure}{\numberline {5}{\ignorespaces Radial (left panel) and latitudinal (right panel) differential rotation from Runs\nobreakspace  {}A--E (diamonds), and Set\nobreakspace  {}D (blue dotted line with asterisks) and B (red dashed line with triangles). Adapted from \cite  {KKB14} }}{4}}
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\@writefile{lof}{\contentsline {figure}{\numberline {6}{\ignorespaces From left to right: Time-averaged Reynolds stresses $Q_{r\phi }$ and $Q_{\theta \phi }$ normalized by $\nu _{\rm  t}\Omega _\odot $, the turbulent viscosity divided by the molecular viscosity $\nu _{\rm  t}/\nu $, $\Lambda _{\rm  V}$ and $\Lambda _{\rm  H}$ normalized by $\nu _{\rm  t}$, and the anisotropy parameters $A_{\rm  V}$ and $A_{\rm  H}$. Top row: Run\nobreakspace  {}A; bottom row: Run\nobreakspace  {}D1. In the fifth column we only use data some degrees away from the equator so as to avoid the singularity associated with the division by $\mathop {\mathgroup \symoperators cos}\nolimits \theta $. The contours in the lower row are oversaturated near the $\theta $-boundaries in order to highlight the features at lower latitudes. Adapted from \cite  {KKB14} }}{5}}
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