$\begin{figure} \par\includegraphics[width=8cm,clip]{8708fig1a.eps}\hspace*{0.5cm} \includegraphics[width=8cm,clip]{8708fig1b.eps} \end{figure}$ Figure 1: a) Number density profiles for the plasma-only models of all four groups, in the directions upwind (0), crosswind (90), and downwind (180) with respect to the LIC flow, respectively. b) Detail around upwind BS.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{8708fig1a.eps}\hspace*{0.5cm} \includegraphics[width=8cm,clip]{8708fig1b.eps} \end{figure}$	Figure 1: a) Number density profiles for the plasma-only models of all four groups, in the directions upwind (0), crosswind (90), and downwind (180) with respect to the LIC flow, respectively. b) Detail around upwind BS.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{8708fig2.eps}\end{figure}$	Figure 2: Upwind profiles of flux conservation n v r² in the supersonic solar wind.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{8708fig3a.eps}\hspace*{0.5cm} \includegraphics[width=8cm,clip]{8708fig3b.eps}\end{figure}$	Figure 3: Density profiles of plasma ( left), and of neutral H ( right), for three directions, for the five self-consistent plasma/neutral models.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{8708fig4a.eps}\hspace*{0.5cm} \includegraphics[width=8cm,clip]{8708fig4b.eps}\end{figure}$	Figure 4: Plasma radial velocity profiles of all models for three directions ( left), and a magnification around the upwind bow shock ( right).
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