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$\begin{figure} \par\includegraphics[width=9cm,clip]{0530fig1.eps}\end{figure}$ Figure 1: Effect of the obliquity angle on the equatorial cloud-top zonal flow for a) exp. V (circles), b) exps. T (circles) and TS (squares), and c) exps. E (circles) and ES (squares). Vertical profiles of mean global atmospheric rotation rates for $\phi _{\rm INC} = {\rm0^{\circ }}$ (black), ${\rm 23.45^{\circ }}$ (blue), and ${\rm 60^{\circ }}$ (red) in exps. V d), T e), and E f).
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In the text

$\begin{figure} \par\includegraphics[width=9cm,clip]{0530fig2.eps}\end{figure}$ Figure 2: Latitude-altitude distributions of annually averaged zonal mean flow for a) $\phi _{\rm INC} = {\rm0^{\circ }}$ and b) $\phi _{\rm INC} = {\rm 60^{\circ }}$ in exps. V, T and E.
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In the text

$\begin{figure} \par\includegraphics[width=9cm,clip]{0530fig3.eps}\end{figure}$ Figure 3: Latitude-altitude distributions of annually averaged a) residual mean vertical flow and b) horizontal eddy angular-momentum fluxes for $\phi _{\rm INC} = {\rm0^{\circ }}$ in exps. V, T and E.
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In the text

$\begin{figure} \par\includegraphics[width=9cm,clip]{0530fig4.eps}\end{figure}$ Figure 4: Variations in seasonally averaged a)- c) zonal mean flow and d- f) residual mean vertical flow for $\phi _{\rm INC} = {\rm 60^{\circ }}$ in exp. E. The gray dotted rectangle in e) shows the area in which the meridional circulation stops at the equinox.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{0530fig5.eps}\end{figure}$ Figure 5: Seasonal variations in the angular-momentum transport (gray arrows) caused by meridional circulation (thick black lines) for a) $\phi _{\rm INC} = {\rm0^{\circ }}$ , b) $\phi _{\rm INC} = {\rm 23.45^{\circ }}$ and c) $\phi _{\rm INC} = {\rm 60^{\circ }}$ in exp. E. Thin solid and dashed lines are contours of the prograde and retrograde wind speeds, respectively.
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In the text

$\begin{figure} \par\includegraphics[width=9cm,clip]{0530fig1.eps}\end{figure}$	Figure 1: Effect of the obliquity angle on the equatorial cloud-top zonal flow for a) exp. V (circles), b) exps. T (circles) and TS (squares), and c) exps. E (circles) and ES (squares). Vertical profiles of mean global atmospheric rotation rates for $\phi _{\rm INC} = {\rm0^{\circ }}$ (black), ${\rm 23.45^{\circ }}$ (blue), and ${\rm 60^{\circ }}$ (red) in exps. V d), T e), and E f).
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$\begin{figure} \par\includegraphics[width=9cm,clip]{0530fig2.eps}\end{figure}$	Figure 2: Latitude-altitude distributions of annually averaged zonal mean flow for a) $\phi _{\rm INC} = {\rm0^{\circ }}$ and b) $\phi _{\rm INC} = {\rm 60^{\circ }}$ in exps. V, T and E.
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$\begin{figure} \par\includegraphics[width=9cm,clip]{0530fig3.eps}\end{figure}$	Figure 3: Latitude-altitude distributions of annually averaged a) residual mean vertical flow and b) horizontal eddy angular-momentum fluxes for $\phi _{\rm INC} = {\rm0^{\circ }}$ in exps. V, T and E.
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$\begin{figure} \par\includegraphics[width=9cm,clip]{0530fig4.eps}\end{figure}$	Figure 4: Variations in seasonally averaged a)- c) zonal mean flow and d- f) residual mean vertical flow for $\phi _{\rm INC} = {\rm 60^{\circ }}$ in exp. E. The gray dotted rectangle in e) shows the area in which the meridional circulation stops at the equinox.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{0530fig5.eps}\end{figure}$	Figure 5: Seasonal variations in the angular-momentum transport (gray arrows) caused by meridional circulation (thick black lines) for a) $\phi _{\rm INC} = {\rm0^{\circ }}$ , b) $\phi _{\rm INC} = {\rm 23.45^{\circ }}$ and c) $\phi _{\rm INC} = {\rm 60^{\circ }}$ in exp. E. Thin solid and dashed lines are contours of the prograde and retrograde wind speeds, respectively.
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