$\begin{figure} \par\includegraphics[angle=90,width=8.1cm,clip]{8617fig1.ps}\end{figure}$ Figure 1: Raster images from dataset s27153r00. The vertical lines show the location of the CDS slit, corresponding to the temporal series dataset s27152r01 and the small white boxes (between $Y\approx$ -200 $\to$ -170'') mark the location of the pixels 55-59.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[angle=90,width=7.35cm,clip]{8617fig2.ps}\end{figure}$ Figure 2: Space-time behaviour of the intensity in the different temperature lines. The right panels show the summed (over time) count values.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[angle=90,width=12cm,clip]{8617fig3.ps}\end{figure}$ Figure 3: Variation with time of intensity (black lines) and velocity (grey lines) corresponding to pixel 57 of dataset s27152r01. The horizontal dashed lines indicates the Signal-to-Noise level (S/N) of 5. O III is not shown due to its low count values <S/N=5.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{8617fig4.ps}\end{figure}$ Figure 4: a) ( Left panel) Time series of the relative intensity in He I; ( right panel) the resulting power spectrum. b) Pre-whitened time series and the resulting power spectrum.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{8617fig5.ps}\end{figure}$ Figure 5: a) Time series and power spectrum for O V. b) Pre-whitened time series and resulting power spectrum.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[angle=90,width=8.1cm,clip]{8617fig1.ps}\end{figure}$	Figure 1: Raster images from dataset s27153r00. The vertical lines show the location of the CDS slit, corresponding to the temporal series dataset s27152r01 and the small white boxes (between $Y\approx$ -200 $\to$ -170'') mark the location of the pixels 55-59.
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=90,width=7.35cm,clip]{8617fig2.ps}\end{figure}$	Figure 2: Space-time behaviour of the intensity in the different temperature lines. The right panels show the summed (over time) count values.
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=90,width=12cm,clip]{8617fig3.ps}\end{figure}$	Figure 3: Variation with time of intensity (black lines) and velocity (grey lines) corresponding to pixel 57 of dataset s27152r01. The horizontal dashed lines indicates the Signal-to-Noise level (S/N) of 5. O III is not shown due to its low count values <S/N=5.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8cm,clip]{8617fig4.ps}\end{figure}$	Figure 4: a) ( Left panel) Time series of the relative intensity in He I; ( right panel) the resulting power spectrum. b) Pre-whitened time series and the resulting power spectrum.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8cm,clip]{8617fig5.ps}\end{figure}$	Figure 5: a) Time series and power spectrum for O V. b) Pre-whitened time series and resulting power spectrum.
Open with DEXTER