All Figures

$\begin{figure} \par\includegraphics[width=6cm,clip]{4993fg1.eps}\end{figure}$ Figure 1: Figure illustrating the definition of separation from the neutral line (polarity inversion line) and propagation along the neutral line of the brightness following the filament/prominence eruptions.
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In the text

$\begin{figure} \par\includegraphics[width=11cm,clip]{4993fg2.eps}\end{figure}$ Figure 2: Series of absolute intensity ( top panel) and running difference ( bottom panel) images taken by EIT at 195 Å on 17-Nov.-2000. Asterisks in the top panel marks the features which were tracked in order to estimate the speed of the prominence. P1 and P2 in the bottom panel are the two end points of the prominence. (This figure is available in color in the electronic version.)
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In the text

$\begin{figure} \par\includegraphics[width=6cm,clip]{4993fg3.eps}\end{figure}$ Figure 3: Height/distance versus time plot for the erupting prominence (asterisks) and propagation of the brightening (diamonds) for the event on 17-Nov.-2000. The height of the prominence is measured from the center of the solar disk by tracking a feature marked by asterisks in Fig. 2. The relative distance is measured in solar radii. The lines are linear fits to the data points.
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In the text

$\begin{figure} \par\includegraphics[width=9cm,clip]{4993fg4a.eps}\par\includegraphics[width=9cm,clip]{4993fg4b.eps}\end{figure}$ Figure 4: Series of absolute intensity images ( top panel) and running difference ( bottom panel) images taken by EIT at 195 Å on 12-Sep.-2000. (This figure is available in color in the electronic version.)
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In the text

$\begin{figure} \par\includegraphics[width=6cm,clip]{4993fg5.eps} \end{figure}$ Figure 5: Height/distance versus time plot for the erupting prominence (asterisks) and distance time diagram for the propagating brightening (diamonds) for the event in 02-Mar.-02. The lines are linear fits to the data point.
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In the text

$\begin{figure} \par\includegraphics[width=6.15cm,clip]{4993fg6a.eps}\includegraphics[width=6.15cm,clip]{4993fg6b.eps}\end{figure}$ Figure 6: Schematic diagrams showing asymmetric ( left panel) and symmetric ( right panel) eruption of the filament/prominence. The direction of propagation along and separation away from the polarity inversion line is marked by arrows. These figures are taken from Shiota et al. (2005) and have been modified.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=6cm,clip]{4993fg1.eps}\end{figure}$	Figure 1: Figure illustrating the definition of separation from the neutral line (polarity inversion line) and propagation along the neutral line of the brightness following the filament/prominence eruptions.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=11cm,clip]{4993fg2.eps}\end{figure}$	Figure 2: Series of absolute intensity ( top panel) and running difference ( bottom panel) images taken by EIT at 195 Å on 17-Nov.-2000. Asterisks in the top panel marks the features which were tracked in order to estimate the speed of the prominence. P1 and P2 in the bottom panel are the two end points of the prominence. (This figure is available in color in the electronic version.)
Open with DEXTER

$\begin{figure} \par\includegraphics[width=6cm,clip]{4993fg3.eps}\end{figure}$	Figure 3: Height/distance versus time plot for the erupting prominence (asterisks) and propagation of the brightening (diamonds) for the event on 17-Nov.-2000. The height of the prominence is measured from the center of the solar disk by tracking a feature marked by asterisks in Fig. 2. The relative distance is measured in solar radii. The lines are linear fits to the data points.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=9cm,clip]{4993fg4a.eps}\par\includegraphics[width=9cm,clip]{4993fg4b.eps}\end{figure}$	Figure 4: Series of absolute intensity images ( top panel) and running difference ( bottom panel) images taken by EIT at 195 Å on 12-Sep.-2000. (This figure is available in color in the electronic version.)
Open with DEXTER

$\begin{figure} \par\includegraphics[width=6cm,clip]{4993fg5.eps} \end{figure}$	Figure 5: Height/distance versus time plot for the erupting prominence (asterisks) and distance time diagram for the propagating brightening (diamonds) for the event in 02-Mar.-02. The lines are linear fits to the data point.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=6.15cm,clip]{4993fg6a.eps}\includegraphics[width=6.15cm,clip]{4993fg6b.eps}\end{figure}$	Figure 6: Schematic diagrams showing asymmetric ( left panel) and symmetric ( right panel) eruption of the filament/prominence. The direction of propagation along and separation away from the polarity inversion line is marked by arrows. These figures are taken from Shiota et al. (2005) and have been modified.
Open with DEXTER