$\begin{figure} \par\includegraphics[width=6cm,clip]{8370fig1.eps}\par \end{figure}$ Figure 1: The observed disk-centre, Neckel intensity spectrum (solid line) is plotted over the fit (crosses) obtained using a grid of synthetic spectra based on the ${{\rm CO}^5{\rm BOLD}}$ model computed with Linfor3D.
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In the text

$\begin{figure} \includegraphics[width=7.1cm,clip]{8370fig2.eps} % \par \end{figure}$ Figure 2: Relative horizontal RMS temperature fluctuations (on surfaces of equal Rosseland optical depth) in the solar ${{\rm CO}^5{\rm BOLD}}$ model.
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In the text

$\begin{figure} \par\includegraphics[width=6cm,clip]{8370fig1.eps}\par \end{figure}$	Figure 1: The observed disk-centre, Neckel intensity spectrum (solid line) is plotted over the fit (crosses) obtained using a grid of synthetic spectra based on the ${{\rm CO}^5{\rm BOLD}}$ model computed with Linfor3D.
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$\begin{figure} \includegraphics[width=7.1cm,clip]{8370fig2.eps} % \par \end{figure}$	Figure 2: Relative horizontal RMS temperature fluctuations (on surfaces of equal Rosseland optical depth) in the solar ${{\rm CO}^5{\rm BOLD}}$ model.
Open with DEXTER