Astronomy & Astrophysics

$\begin{figure} \par\includegraphics[width=4.1cm,clip]{3129f1a.eps}\hspace*{2mm} \includegraphics[width=4.1cm,clip]{3129f1b.eps} \end{figure}$ Figure 1: Left: the processed H $\alpha$ image taken at 17:53:45 UT. The brightness of the off-disk region is enhanced in order to clearly show both the features on- and off-disk (see Sect. 4.1). Right: the partially calibrated EIT 30.4 nm image at 17:53:57 UT (see Sect. 4.2). Only the subfield which is selected to be transformed is shown.
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In the text

$\begin{figure} \par\includegraphics[width=4.1cm,clip]{3129f2a.eps}\hspace*{2mm} \includegraphics[width=4.1cm,clip]{3129f2b.eps} \end{figure}$ Figure 2: Left: the BBSO selection showing the marked points in this image, together with their counterparts which are marked in EIT and transformed to the BBSO coordinate system. Right: the EIT 30.4 nm selection after transformation, showing the same field of view as the BBSO image on the left.
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In the text

$\begin{figure} \par\includegraphics[width=4.2cm,clip]{3129f3a.eps}\hspace*{2mm} \includegraphics[width=4.2cm,clip]{3129f3b.eps} \end{figure}$ Figure 3: Left: H $\alpha$ image of the north-eastern quarter disk at 16:33:15 UT. The brightness of the off-disk region is enhanced in order to clearly show both the features on- and off-disk. Right: calibrated EIT 30.4 nm image of the off-disk-loop region at 16:33:18 UT.
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In the text

$\begin{figure} \par\includegraphics[width=4cm,height=6.8cm,clip]{3129f4a.eps}\hspace*{2mm} \includegraphics[width=4cm,height=6.8cm,clip]{3129f4b.eps} \end{figure}$ Figure 4: Left: H $\alpha$ image of the off-disk-loop region at 17:54:45, overplotted by the contours of EIT 30.4 nm at 17:55:05. The contour north of the flaring loop corresponds with the downward motion in EIT. Right: Idem but overplotted in colour coding.
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In the text

$\begin{figure} \par\includegraphics[width=6cm,height=6cm,clip]{3129f5a.eps}\hspace*{3mm} \includegraphics[width=8.5cm,height=9.2cm,clip]{3129f5b.eps} \end{figure}$ Figure 5: Left: the track of the intensity variations, outlined in one frame of the H $\alpha$ -sequence (at 17:49). Right: location-time plot of the outlined track. The location numbers in the left figure correspond to the numbered horizontal solid lines on the right. The horizontal dashed lines correspond to the locations where velocities were measured in the EIT images. The slopes of the blue lines correspond with these velocities. The inset shows a less bright close-up of the base of blob 5.
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In the text

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{3129f6.eps} \end{figure}$ Figure 6: The measured speeds of each "blob'' at several locations along the loop. The arrows point to measurements done in H $\alpha$ .
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In the text

$\begin{figure} \par\mbox{\epsfig{file=3129f7a.eps, height=4.4cm, clip=} \epsfig{... ....4cm, clip=} \epsfig{file=3129f7l.eps, height=4.4cm, clip=} } \par\end{figure}$ Figure 7: Touchdown of blob 5 in the BBSO H $\alpha$ images ( top) and in the EIT 30.4 nm images ( middle). The white circle in each EIT 30.4 nm image points to the part which is related to this particular blob. The bottom row shows the overplotted images in colour coding.
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In the text

$\begin{figure} \par\includegraphics[width=3.7cm,clip]{3129f8a.eps}\hspace*{3mm} \includegraphics[width=3cm,clip]{3129f8b.eps} \end{figure}$ Figure 8: Left: He II emission in a loop of 300 Mm (apex at z=150 Mm, only the left half of the loop is shown). Right: line profiles of He II in a 300 Mm loop during the fall of the condensation region (Müller et al. 2005).
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In the text

eitoverbb_col1.gif

eitoverbb_col2z.gif

eitoverbb_contour.gif

$\begin{figure} \par\includegraphics[width=4.1cm,clip]{3129f1a.eps}\hspace*{2mm} \includegraphics[width=4.1cm,clip]{3129f1b.eps} \end{figure}$	Figure 1: Left: the processed H $\alpha$ image taken at 17:53:45 UT. The brightness of the off-disk region is enhanced in order to clearly show both the features on- and off-disk (see Sect. 4.1). Right: the partially calibrated EIT 30.4 nm image at 17:53:57 UT (see Sect. 4.2). Only the subfield which is selected to be transformed is shown.
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$\begin{figure} \par\includegraphics[width=4.1cm,clip]{3129f2a.eps}\hspace*{2mm} \includegraphics[width=4.1cm,clip]{3129f2b.eps} \end{figure}$	Figure 2: Left: the BBSO selection showing the marked points in this image, together with their counterparts which are marked in EIT and transformed to the BBSO coordinate system. Right: the EIT 30.4 nm selection after transformation, showing the same field of view as the BBSO image on the left.
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$\begin{figure} \par\includegraphics[width=4.2cm,clip]{3129f3a.eps}\hspace*{2mm} \includegraphics[width=4.2cm,clip]{3129f3b.eps} \end{figure}$	Figure 3: Left: H $\alpha$ image of the north-eastern quarter disk at 16:33:15 UT. The brightness of the off-disk region is enhanced in order to clearly show both the features on- and off-disk. Right: calibrated EIT 30.4 nm image of the off-disk-loop region at 16:33:18 UT.
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$\begin{figure} \par\includegraphics[width=4cm,height=6.8cm,clip]{3129f4a.eps}\hspace*{2mm} \includegraphics[width=4cm,height=6.8cm,clip]{3129f4b.eps} \end{figure}$	Figure 4: Left: H $\alpha$ image of the off-disk-loop region at 17:54:45, overplotted by the contours of EIT 30.4 nm at 17:55:05. The contour north of the flaring loop corresponds with the downward motion in EIT. Right: Idem but overplotted in colour coding.
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$\begin{figure} \par\includegraphics[width=8.5cm,clip]{3129f6.eps} \end{figure}$	Figure 6: The measured speeds of each "blob'' at several locations along the loop. The arrows point to measurements done in H $\alpha$ .
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$\begin{figure} \par\mbox{\epsfig{file=3129f7a.eps, height=4.4cm, clip=} \epsfig{... ....4cm, clip=} \epsfig{file=3129f7l.eps, height=4.4cm, clip=} } \par\end{figure}$	Figure 7: Touchdown of blob 5 in the BBSO H $\alpha$ images ( top) and in the EIT 30.4 nm images ( middle). The white circle in each EIT 30.4 nm image points to the part which is related to this particular blob. The bottom row shows the overplotted images in colour coding.
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$\begin{figure} \par\includegraphics[width=3.7cm,clip]{3129f8a.eps}\hspace*{3mm} \includegraphics[width=3cm,clip]{3129f8b.eps} \end{figure}$	Figure 8: Left: He II emission in a loop of 300 Mm (apex at z=150 Mm, only the left half of the loop is shown). Right: line profiles of He II in a 300 Mm loop during the fall of the condensation region (Müller et al. 2005).
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