Astronomy & Astrophysics

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{5465fig1.eps} \end{figure}$ Figure 1: The time-dependent perpendicular mean free path for pure slab geometry. Shown is the QLT-result (dash-dotted line), the NLGC-result (dashed line), the ENLGC-result (solid line) and the simulations (dotted line).
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{5465fig2.eps} \end{figure}$ Figure 2: The time-dependent perpendicular mean free path for strong slab geometry ( $90\%$ slab/ $10\%$ 2D). Shown is the NLGC-result (dashed line), the ENLGC-result (solid line) and the simulations (dotted line).
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{5465fig3.eps} \end{figure}$ Figure 3: The time-dependent perpendicular mean free path for strong 2D geometry ( $20\%$ slab/ $80\%$ 2D). Shown is the NLGC-result (dashed line), the ENLGC-result (solid line) and the simulations (dotted line).
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{5465fig1.eps} \end{figure}$	Figure 1: The time-dependent perpendicular mean free path for pure slab geometry. Shown is the QLT-result (dash-dotted line), the NLGC-result (dashed line), the ENLGC-result (solid line) and the simulations (dotted line).
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{5465fig2.eps} \end{figure}$	Figure 2: The time-dependent perpendicular mean free path for strong slab geometry ( $90\%$ slab/ $10\%$ 2D). Shown is the NLGC-result (dashed line), the ENLGC-result (solid line) and the simulations (dotted line).
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{5465fig3.eps} \end{figure}$	Figure 3: The time-dependent perpendicular mean free path for strong 2D geometry ( $20\%$ slab/ $80\%$ 2D). Shown is the NLGC-result (dashed line), the ENLGC-result (solid line) and the simulations (dotted line).
Open with DEXTER