All Figures

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{4665fig1.eps} \end{figure}$ Figure 1: The adopted three-dimensional magnetic field structure: perspective view and three orthogonal projections.
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In the text

$\begin{figure} \par\includegraphics[width=7.5cm,clip]{4665fig2.eps} \end{figure}$ Figure 2: Source heliographic positions: 20 $^\circ$ S 0 $^\circ$ W (center), 20 $^\circ$ S 40 $^\circ$ W and 20 $^\circ$ S 80 $^\circ$ W (near limb). The arcs were scaled by a factor 15 larger to be visible in this figure.
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In the text

$\begin{figure} \par\includegraphics[width=7cm,clip]{4665fig3.eps} \end{figure}$ Figure 3: Center-to-limb variations of spectral parameters: a), b) spectral index $\alpha _{\rm thin}$ , c), d) peak frequency $\nu _{\rm peak}$ , and e), f) flux density at $\nu _{\rm peak}$ . The homogeneous source model results are indicated by continuous lines and our inhomogeneous models by dash-dotted lines. The left and right columns show the results for low and high ambient density profiles, respectively.
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In the text

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{4665fig4.eps} \end{figure}$ Figure 4: Calculated spectra for our source models at three solar longitudes: $\rm0^\circ W$ (continuous), $\rm 40^\circ W$ (dashed), and $\rm 80^\circ W$ (dash-dotted). a) Low ambient density source; b) high ambient density source.
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In the text

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{4665fig5.eps} \end{figure}$ Figure 5: Emitting area (at half power) as a function of frequency.
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In the text

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{4665fig6.eps} \end{figure}$ Figure 6: Flux density maps calculated for the low density source model at center ( left) and limb ( right); the top row shows 3 GHz maps and bottom row shows 10 GHz. The contour levels are 10, 30, 50, 70, and 90% of normalized flux. The 10'' $\times$ 10'' dashed lined boxes indicate the regions taken to simulate high spatial resolution spectra. In the maps presented in this work, the north is up and west is to the right.
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In the text

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{4665fig7.eps} \end{figure}$ Figure 7: Looptop (continuous lines) and footpoint (dash-dotted) spectra for the low (thin lines) and high (thick) density source models at a) center and b) limb positions.
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In the text

$\begin{figure} \par\includegraphics[width=7cm,clip]{4665fig8.eps} \end{figure}$ Figure 8: Longitudinal component of the magnetic field. Black region shows negative field and gray regions shows positive field. The dashed line indicates the QT line, where the magnetic field invert its sign.
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In the text

$\begin{figure} \par\includegraphics[width=7.7cm,clip]{4665fig9.eps} \end{figure}$ Figure 9: Circular polarization maps for 3 GHz ( top row) and 10 GHz ( bottom). The dashed contours are left-handed circular polarization (LCP), and continuous contours are right-handed circular polarization (RCP) at 10, 30, 50, 70, and 90% levels. The dashed line indicates the inversion of the circular polarization due to the inversion of the longitudinal component of the magnetic field sign.
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In the text

$\begin{figure} \par\includegraphics[width=5.5cm,clip]{4665fig10.eps} \end{figure}$ Figure 10: Polarization degree (RCP - LCP) of the whole source. The polarization for the three source positions are shown for the low ambient density model.
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In the text

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{4665fig1.eps} \end{figure}$	Figure 1: The adopted three-dimensional magnetic field structure: perspective view and three orthogonal projections.
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$\begin{figure} \par\includegraphics[width=7.5cm,clip]{4665fig2.eps} \end{figure}$	Figure 2: Source heliographic positions: 20 $^\circ$ S 0 $^\circ$ W (center), 20 $^\circ$ S 40 $^\circ$ W and 20 $^\circ$ S 80 $^\circ$ W (near limb). The arcs were scaled by a factor 15 larger to be visible in this figure.
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$\begin{figure} \par\includegraphics[width=7.8cm,clip]{4665fig4.eps} \end{figure}$	Figure 4: Calculated spectra for our source models at three solar longitudes: $\rm0^\circ W$ (continuous), $\rm 40^\circ W$ (dashed), and $\rm 80^\circ W$ (dash-dotted). a) Low ambient density source; b) high ambient density source.
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$\begin{figure} \par\includegraphics[width=7.8cm,clip]{4665fig5.eps} \end{figure}$	Figure 5: Emitting area (at half power) as a function of frequency.
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$\begin{figure} \par\includegraphics[width=7.8cm,clip]{4665fig7.eps} \end{figure}$	Figure 7: Looptop (continuous lines) and footpoint (dash-dotted) spectra for the low (thin lines) and high (thick) density source models at a) center and b) limb positions.
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$\begin{figure} \par\includegraphics[width=7cm,clip]{4665fig8.eps} \end{figure}$	Figure 8: Longitudinal component of the magnetic field. Black region shows negative field and gray regions shows positive field. The dashed line indicates the QT line, where the magnetic field invert its sign.
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$\begin{figure} \par\includegraphics[width=5.5cm,clip]{4665fig10.eps} \end{figure}$	Figure 10: Polarization degree (RCP - LCP) of the whole source. The polarization for the three source positions are shown for the low ambient density model.
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