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$\begin{figure} \par\includegraphics[width=7cm]{9002f1.ps}\end{figure}$ Figure 1: Continuum intensity map at 630 nm of the limb-side of AR 10953. The umbra has been removed to increase the image contrast. This sunspot was observed using Hinode's spectropolarimeter on the 3rd of May, 2007 at an heliocentric angle of $\theta = 19^{\circ }$ . The black arrow points towards the center of the solar disk. The pair of dashed lines indicated by Y^* lie near the line of symmetry of the sunpot. Results along these two slices are discussed in Sect. 4.
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In the text

$\begin{figure} \par\begin{tabular}{cc} \includegraphics[width=6.6cm]{9002f2a.ps}... ...9002f2c.ps} & \includegraphics[width=6.6cm]{9002f2d.ps}\end{tabular}\end{figure}$ Figure 2: Two dimensional cut across the leftmost Y^* slice in Fig. 1 showing the depth-dependence of the line of sight velocity ( upper-left panel), magnetic field strength ( upper-right panel), magnetic field inclination in the local reference frame $\zeta$ ( lower-left panel) and magnetic field azimuth in the local reference frame $\Psi$ ( lower-right panel). The magnetic field vector at different locations in the $Y^{*} \tau$ plane is indicated by the arrows.
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In the text

$\begin{figure} \par\begin{tabular}{cc} \includegraphics[width=6.6cm]{9002f3a.ps}... ...9002f3c.ps} & \includegraphics[width=6.6cm]{9002f3d.ps}\end{tabular}\end{figure}$ Figure 3: Same as in Fig. 2 but for the rightmost slice across Y^* in Fig. 1.
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In the text

$\begin{figure} \par\begin{tabular}{cc} \includegraphics[width=6.6cm]{9002f3a.ps}... ...9002f3c.ps} & \includegraphics[width=6.6cm]{9002f3d.ps}\end{tabular}\end{figure}$	Figure 3: Same as in Fig. 2 but for the rightmost slice across Y^* in Fig. 1.
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