All Figures

$\begin{figure} \par\mbox{\includegraphics[width=5cm,clip]{9349fig1a.ps} \hspace*... ...ps} \hspace*{4mm} \includegraphics[width=5cm,clip]{9349fig1c.ps} } \end{figure}$ Figure 1: Colour table reversed TRACE $\lambda$ 171 Å ( left) and TRACE $\lambda$ 1600 Å ( middle) images and MDI high-resolution magnetogram scaled from -200 to 200 G ( right) of the active region NOAA 08558 observed on 1999 June 2 with the SUMER slit position over-plotted.
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In the text

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{9349fig2a.ps}\hspace*{4mm}... ...c.ps}\hspace*{4mm} \includegraphics[width=7.3cm,clip]{9349fig2d.ps} \end{figure}$ Figure 2: For all cases a)- d): left: TRACE $\lambda$ 171 Å colour table reversed image showing the analysed feature. The vertical line corresponds to the position of the SUMER slit, while the two horizontal lines outline the part of the slit which was analysed in the SUMER data. right: profiles of all observed spectral lines taken closest in time to the shown TRACE image. The dotted line profile corresponds to the reference spectrum. An animation of the TRACE $\lambda$ 171 Å images can be seen online.
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In the text

$\begin{figure} \par\includegraphics[width=16.5cm,clip]{9349fig3a.ps}\par\vspace*{2mm} \includegraphics[width=16.5cm,clip]{9349fig3b.ps} \end{figure}$ Figure 3: TRACE $\lambda$ 171 Å colour table reversed image sequences of events (c) (above) and (d) (below). The black contour shows the brightening (here seen as the darkest feature) in the loop at a given time. The over-plotted white contour outlines the event at 10:43:31 UTC. The black contour traces the brightenings at the given time. The vertical line corresponds to the position of the SUMER slit.
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In the text

$\begin{figure} \par\includegraphics[width=12.5cm,clip]{9349fig4a.ps}\par\vspace*{2mm} \includegraphics[width=12.5cm,clip]{9349fig4b.ps} \end{figure}$ Figure 4: Normalised O V and N V line profiles of the four events shown in Fig. 2. The dashed line is the reference spectrum.
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In the text

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{9349fig5.ps} \end{figure}$ Figure 5: Left: TRACE $\lambda$ 171 Å colour table reversed image showing the flow in a pre-existing coronal loop. The vertical line corresponds to the position of the SUMER slit, while the two horizontal lines outline the part of the slit which was analysed in the SUMER data. Right: a reference spectrum is shown with the dotted line. The dashed line corresponds to the spectrum registered at 09:22:17 UTC averaged over the area denoted by the two horizontal lines on the TRACE image. The continuous line is the spectrum around 09:37 UTC.
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In the text

$\begin{figure} \par\includegraphics[width=6.8cm,clip]{9349fig6.ps} \end{figure}$ Figure 6: The peak radiance averaged along the SUMER slit as shown in Fig. 5 obtained from a single Gauss fit. The solid line corresponds to the Mg X $\lambda$ 624.85 Å line, dotted - O V $\lambda$ 629 Å, dashed - N V $\lambda$ 1238 Å, solid thick - Si II $\lambda$ 1251.16 Å and C I $\lambda$ 1251.17 Å. The grey area marks the time period during which the jet-like events were observed (see Madjarska et al. 2007).
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In the text

$\begin{figure} \par\mbox{\includegraphics[width=5cm,clip]{9349fig1a.ps} \hspace... ...ps} \hspace{4mm} \includegraphics[width=5cm,clip]{9349fig1c.ps} } \end{figure}$	Figure 1: Colour table reversed TRACE $\lambda$ 171 Å ( left) and TRACE $\lambda$ 1600 Å ( middle) images and MDI high-resolution magnetogram scaled from -200 to 200 G ( right) of the active region NOAA 08558 observed on 1999 June 2 with the SUMER slit position over-plotted.
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$\begin{figure} \par\includegraphics[width=12.5cm,clip]{9349fig4a.ps}\par\vspace*{2mm} \includegraphics[width=12.5cm,clip]{9349fig4b.ps} \end{figure}$	Figure 4: Normalised O V and N V line profiles of the four events shown in Fig. 2. The dashed line is the reference spectrum.
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