All Figures

$\begin{figure} \par\includegraphics[width=7cm,clip]{2244fig1.eps} \end{figure}$ Figure 1: Logarithm of the Coriolis number, ${\rm Co} = 2~\Omega_\odot \alpha H_{\rm p}/v$ , in the solar convection zone.
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In the text

$\begin{figure} \par\includegraphics[width=16.5cm,clip]{2244fig2.eps} \end{figure}$ Figure 2: Correlations of u_z with respect to the reference levels $z_{\rm ref} = 0$ (solid), 0.17 (dotted), 0.26 (dashed), 0.5 (dot-dashed), 0.77 (triple dot dashed), and 0.87 (long dashed) from the run s2Co0 as function of the number of pressure scale heights, $N_{\rm p}$ , ( left) and the actual distance $\Delta z$ ( right).
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In the text

$\begin{figure} \par\includegraphics[width=6.5cm,clip]{2244fig3.eps} \end{figure}$ Figure 3: Relations between the vertical velocity and temperature fluctuations versus the superadiabatic gradient from the run s2Co1-90.
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In the text

$\begin{figure} \par\includegraphics[width=16.7cm,clip]{2244fig4.eps} \end{figure}$ Figure 4: The mixing length parameters calculated from Eqs. (12) to (15) as functions of depth and rotation.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{2244fig5.eps} \end{figure}$ Figure 5: Superadiabaticity $\nabla - \nabla _{\rm ad}$ as function of depth and rotation.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{2244fig6.eps} \end{figure}$ Figure 6: Superadiabaticity $\nabla - \nabla _{\rm ad}$ as a function of depth and rotation in the transition layer between the convectively unstable and stable regions. Note that the scale is different by roughly an order of magnitude in comparison to Fig. 5.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{2244fig7.eps} \end{figure}$ Figure 7: Superadiabaticity $\nabla - \nabla _{\rm ad}$ as function of depth and latitude.
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In the text

$\begin{figure} \par\includegraphics[width=16.7cm,clip]{2244fig8.eps} \end{figure}$ Figure 8: Mixing length parameters $\alpha _{\rm i}$ , defined via Eqs. (12) to (15), as function of Ra and resolution for the runs siCo0 from Table 1.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{2244fig9.eps} \end{figure}$ Figure 9: Temperature gradients $\nabla = d\ln T/d \ln P$ near the base of theconvection zone. The actual gradient ( heavy line) is identical tothe radiative gradient in the core, and closely follows the adiabatic in the convection zone and in the region of overshooting. A local model with no overshooting ( lower line); non-local models with mean path l/2 ( above), as assumed in local theory, and with mean path l/5 ( middle).
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In the text

$\begin{figure} \par\includegraphics[width=7cm,clip]{2244fig1.eps} \end{figure}$	Figure 1: Logarithm of the Coriolis number, ${\rm Co} = 2~\Omega_\odot \alpha H_{\rm p}/v$ , in the solar convection zone.
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$\begin{figure} \par\includegraphics[width=16.5cm,clip]{2244fig2.eps} \end{figure}$	Figure 2: Correlations of u_z with respect to the reference levels $z_{\rm ref} = 0$ (solid), 0.17 (dotted), 0.26 (dashed), 0.5 (dot-dashed), 0.77 (triple dot dashed), and 0.87 (long dashed) from the run s2Co0 as function of the number of pressure scale heights, $N_{\rm p}$ , ( left) and the actual distance $\Delta z$ ( right).
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$\begin{figure} \par\includegraphics[width=6.5cm,clip]{2244fig3.eps} \end{figure}$	Figure 3: Relations between the vertical velocity and temperature fluctuations versus the superadiabatic gradient from the run s2Co1-90.
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$\begin{figure} \par\includegraphics[width=16.7cm,clip]{2244fig4.eps} \end{figure}$	Figure 4: The mixing length parameters calculated from Eqs. (12) to (15) as functions of depth and rotation.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{2244fig5.eps} \end{figure}$	Figure 5: Superadiabaticity $\nabla - \nabla _{\rm ad}$ as function of depth and rotation.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{2244fig6.eps} \end{figure}$	Figure 6: Superadiabaticity $\nabla - \nabla _{\rm ad}$ as a function of depth and rotation in the transition layer between the convectively unstable and stable regions. Note that the scale is different by roughly an order of magnitude in comparison to Fig. 5.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{2244fig7.eps} \end{figure}$	Figure 7: Superadiabaticity $\nabla - \nabla _{\rm ad}$ as function of depth and latitude.
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$\begin{figure} \par\includegraphics[width=16.7cm,clip]{2244fig8.eps} \end{figure}$	Figure 8: Mixing length parameters $\alpha _{\rm i}$ , defined via Eqs. (12) to (15), as function of Ra and resolution for the runs siCo0 from Table 1.
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