$\begin{figure} \par\includegraphics[width=8.4cm,clip]{0120fig2.ps}\end{figure}$ Figure 2: Scatter plot of East-West diameter vs brightness temperature of the quiet Sun at 34.5 MHz.
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In the text

$\begin{figure} \par\includegraphics[width=7.6cm,clip]{0120fig3.ps}\end{figure}$ Figure 3: Variation of optical depth at 34.5 MHz with density enhancement factor. The solid curve is for density gradient 3.32, the dotted one for 4.32 and the dashed one for 5.32.
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In the text

$\begin{figure} \par\includegraphics[width=7.6cm,clip]{0120fig4.ps}\end{figure}$ Figure 4: Variation of turning point in solar radii at 34.5 MHz with the density enhancement factor. The solid curve is for density gradient 3.32 and the dotted one for 4.32 and the dashed one for 5.32.
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In the text

$\begin{figure} \par\includegraphics[width=7.4cm,clip]{0120fig1.ps}\end{figure}$	Figure 1: One dimensional scan of the quiet Sun obtained on June 6th, 1986 at 34.5 MHz.
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$\begin{figure} \par\includegraphics[width=8.4cm,clip]{0120fig2.ps}\end{figure}$	Figure 2: Scatter plot of East-West diameter vs brightness temperature of the quiet Sun at 34.5 MHz.
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$\begin{figure} \par\includegraphics[width=7.6cm,clip]{0120fig3.ps}\end{figure}$	Figure 3: Variation of optical depth at 34.5 MHz with density enhancement factor. The solid curve is for density gradient 3.32, the dotted one for 4.32 and the dashed one for 5.32.
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$\begin{figure} \par\includegraphics[width=7.6cm,clip]{0120fig4.ps}\end{figure}$	Figure 4: Variation of turning point in solar radii at 34.5 MHz with the density enhancement factor. The solid curve is for density gradient 3.32 and the dotted one for 4.32 and the dashed one for 5.32.
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