All Figures

$\begin{figure} {\includegraphics[width=8.3cm,clip]{2080f1.eps} }\end{figure}$ Figure 1: The time-evolution of the height z, radius a and mass m of a dust grain in the simple one-particle model, for three different initial dust radii. The specific weight of the dust is 3.6 g/cm³.
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In the text

$\begin{figure} {\includegraphics[width=8.5cm,clip]{2080f2.eps} }\end{figure}$ Figure 2: As Fig. 1, but now for different porosities of the grains.
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In the text

$\begin{figure} {\includegraphics[width=15cm,clip]{2080f3.eps} }\end{figure}$ Figure 3: The time-evolution of the distribution function for models S1 $\cdots$ S6 (see Table 1 for the model definitions).
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In the text

$\begin{figure} {\includegraphics[width=15cm,clip]{2080f4.eps} }\end{figure}$ Figure 4: Like Fig. 3, but in a 2d view.
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In the text

$\begin{figure} {\includegraphics[width=8cm,clip]{2080f5.eps} }\end{figure}$ Figure 5: The vertical optical depth in the UV at 1 AU (i.e. the integrated projected surface of the dust particles) as a function of time for the vertical slice models S1...S6.
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In the text

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{2080f6a.eps}\hspace*{2mm} ... ...c.eps}\hspace*{2mm} \includegraphics[width=8.5cm,clip]{2080f6d.eps} \end{figure}$ Figure 6: The SEDs ( left column) and surface heights ( right column) of the full disk models. The two top panels show the result for model F1, the calculation without turbulence. The bottom panel results are for model F2, including turbulence. Different lines indicate the results after different times, as shown in the legends.
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In the text

$\begin{figure} {\includegraphics[width=8.5cm,clip]{2080f7.eps} }\end{figure}$ Figure 7: The time-evolution of the distribution function for model SD1 (including all growth processes and aggregate fragmentation). This slice has only been evolved up to $8\times 10^5$ years (darkest curve).
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In the text

$\begin{figure} {\includegraphics[width=8.5cm,clip]{2080f8.eps} }\end{figure}$ Figure C.1: A snapshot of the distribution function of test 1 at dimensionless time $\tau =9$ , for various values of the grid resolution and time step. The symbol $\Delta t$ is the time step ( $\Delta t_{{\rm max}}\equiv {\rm max}(f(m)/S(m))$ ) and N is the number of grid points in m (N=100 corresponds to $m_{i+1}/m_{i}=\sqrt {2}$ , i.e. the highest resolution used by Ohtsuki; N=1000 corresponds to m_i+1/m_i=1.03517). The solid line is the analytic solution of Safronov.

In the text

$\begin{figure} {\includegraphics[width=8.5cm,clip]{2080f9.eps} }\end{figure}$ Figure C.2: The time evolution of the distribution function in test 2 for the model (solid line) compared to the analytic solution of Smoluchowski (dotted line). The snapshots are at dimensionless time $\tau =1,10,10^2,10^3,10^4,10^5$ from left to right. Due to different initial conditions the agreement is not good at $\tau =1$ but becomes better as time progresses because the initial conditions are "forgotten'' by the system. The tiny wiggle in the solid curve around m=4 is a remainder of the initial conditions that apparently the algorithm does not "forget''.

In the text

$\begin{figure} {\includegraphics[width=8.3cm,clip]{2080f1.eps} }\end{figure}$	Figure 1: The time-evolution of the height z, radius a and mass m of a dust grain in the simple one-particle model, for three different initial dust radii. The specific weight of the dust is 3.6 g/cm³.
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$\begin{figure} {\includegraphics[width=8.5cm,clip]{2080f2.eps} }\end{figure}$	Figure 2: As Fig. 1, but now for different porosities of the grains.
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$\begin{figure} {\includegraphics[width=15cm,clip]{2080f3.eps} }\end{figure}$	Figure 3: The time-evolution of the distribution function for models S1 $\cdots$ S6 (see Table 1 for the model definitions).
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$\begin{figure} {\includegraphics[width=15cm,clip]{2080f4.eps} }\end{figure}$	Figure 4: Like Fig. 3, but in a 2d view.
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$\begin{figure} {\includegraphics[width=8cm,clip]{2080f5.eps} }\end{figure}$	Figure 5: The vertical optical depth in the UV at 1 AU (i.e. the integrated projected surface of the dust particles) as a function of time for the vertical slice models S1...S6.
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$\begin{figure} \par\includegraphics[width=8.5cm,clip]{2080f6a.eps}\hspace{2mm} ... ...c.eps}\hspace{2mm} \includegraphics[width=8.5cm,clip]{2080f6d.eps} \end{figure}$	Figure 6: The SEDs ( left column) and surface heights ( right column) of the full disk models. The two top panels show the result for model F1, the calculation without turbulence. The bottom panel results are for model F2, including turbulence. Different lines indicate the results after different times, as shown in the legends.
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$\begin{figure} {\includegraphics[width=8.5cm,clip]{2080f7.eps} }\end{figure}$	Figure 7: The time-evolution of the distribution function for model SD1 (including all growth processes and aggregate fragmentation). This slice has only been evolved up to $8\times 10^5$ years (darkest curve).
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