$\begin{figure} \par\includegraphics[width=7.4cm,height=5.5cm,clip]{9688fg06.eps}... ...{4mm} \includegraphics[width=7.4cm,height=5.5cm,clip]{9688fg09.eps} \end{figure}$ Figure 2: Samples of the observed, synthesized, and subtracted spectra for the $\mbox{He~{\sc i}}$ D₃, $\mbox{Na~{\sc i}}$ D₁, D₂, and $\mbox{Ca~{\sc ii}}$ IRT lines. The dotted lines represent the synthesized spectra and the upper spectra are the subtracted spectra. Vertical arrows mark the telluric lines that appeared in the spectral region.
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In the text

$\begin{figure} \par\includegraphics[width=5.2cm,height=4.2cm,clip]{9688fg10.eps}... ...{4mm} \includegraphics[width=5.2cm,height=4.2cm,clip]{9688fg21.eps} \end{figure}$ Figure 3: Samples of the profiles of the H $_{\alpha }$ lines. The dotted lines represent the synthesized spectra. The upper spectra are the subtracted spectra. The number indicates that the absorption events appeared in the excess emission profiles.
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In the text

$\begin{figure} \par\includegraphics[width=7.8cm,height=6cm,clip]{9688fg22.eps} \end{figure}$ Figure 4: The EWs of the excess emissions vs. orbital phase for $\mbox{Na~{\sc i}}$ D and $\mbox{Ca~{\sc ii}}$ IRT lines. The solid line refers to a polynomial fit to the data.
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In the text

$\begin{figure} \par\includegraphics[width=3cm,height=10.5cm,clip]{9688fg01.eps}\... ...{4mm} \includegraphics[width=3cm,height=10.5cm,clip]{9688fg05.eps} \end{figure}$	Figure 1: The $\mbox{He~{\sc i}}$ D₃, $\mbox{Na~{\sc i}}$ D₁, D₂, H $_{\alpha }$ , and $\mbox{Ca~{\sc ii}}$ IRT line profiles of SZ Psc.
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$\begin{figure} \par\includegraphics[width=7.4cm,height=5.5cm,clip]{9688fg06.eps}... ...{4mm} \includegraphics[width=7.4cm,height=5.5cm,clip]{9688fg09.eps} \end{figure}$	Figure 2: Samples of the observed, synthesized, and subtracted spectra for the $\mbox{He~{\sc i}}$ D₃, $\mbox{Na~{\sc i}}$ D₁, D₂, and $\mbox{Ca~{\sc ii}}$ IRT lines. The dotted lines represent the synthesized spectra and the upper spectra are the subtracted spectra. Vertical arrows mark the telluric lines that appeared in the spectral region.
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$\begin{figure} \par\includegraphics[width=5.2cm,height=4.2cm,clip]{9688fg10.eps}... ...{4mm} \includegraphics[width=5.2cm,height=4.2cm,clip]{9688fg21.eps} \end{figure}$	Figure 3: Samples of the profiles of the H $_{\alpha }$ lines. The dotted lines represent the synthesized spectra. The upper spectra are the subtracted spectra. The number indicates that the absorption events appeared in the excess emission profiles.
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$\begin{figure} \par\includegraphics[width=7.8cm,height=6cm,clip]{9688fg22.eps} \end{figure}$	Figure 4: The EWs of the excess emissions vs. orbital phase for $\mbox{Na~{\sc i}}$ D and $\mbox{Ca~{\sc ii}}$ IRT lines. The solid line refers to a polynomial fit to the data.
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$\begin{figure} \par\includegraphics[width=7.8cm,height=6cm,clip]{9688fg23.eps} \end{figure}$	Figure 5: As Fig. 4, but for the EWs of H $_{\alpha }$ line.
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