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$\begin{figure} \par\includegraphics[angle=-90,width=8.9cm,clip]{5991fig1.eps} \par\end{figure}$ Figure 1: The ${\rm O}^{++}$ density comparison between the model and the PVO experiment. The black points correspond to the PVO measurements. The thick full lines shows the result of our modelling. The thin full lines correspond to the larger divergence when varying ${\rm H}$ between $5\times 10^4$ and $2\times 10^5~{\rm cm}^{-3}$ beyond $200~{\rm km}$ . The dashed lines correspond to the model without ${\rm O}^+$ photoionisation.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8.9cm,clip]{5991fig2.eps} \par\end{figure}$ Figure 2: ${\rm O}^{++}$ , ${\rm N_2}^{++}$ , ${\rm CO_2}^{++}$ densities. Latitude: $45\hbox {$^\circ $ }$ , solar zenith angle: $45\hbox {$^\circ $ }$ ${\rm H}$ density: $5\times 10^4$ Full lines: F_10.7=200. Dashed lines: F_10.7=80.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8.9cm,clip]{5991fig2.eps} \par\end{figure}$	Figure 2: ${\rm O}^{++}$ , ${\rm N_2}^{++}$ , ${\rm CO_2}^{++}$ densities. Latitude: $45\hbox {$^\circ $ }$ , solar zenith angle: $45\hbox {$^\circ $ }$ ${\rm H}$ density: $5\times 10^4$ Full lines: F_10.7=200. Dashed lines: F_10.7=80.
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