$\begin{figure} \par\includegraphics[width=8.4cm,clip]{3082fig1.eps} \end{figure}$ Figure 1: The variation of the relative rms contrast of the continuum intensity during the time series. The wavelength range used was centered at 4993.12 Å and the slit length used for the calculation was 65 $^{\prime \prime }$ .
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{3082fig2.eps} \end{figure}$ Figure 2: Temporal-spatial map of the continuum intensity. The horizontal stripes of lower intensity contrast are due to seeing (see Fig. 1).
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{3082fig5.eps} \end{figure}$ Figure 5: Comparison of the rms fluctuations of the continuum intensity (same as Fig. 1) with the temporal variations of correlations to determine the influence of seeing.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{3082fig6.eps} \end{figure}$ Figure 6: Temporal variation of two correlation coefficients versus the rms of the continuum fluctuations (Asterisks: $\left\langle I,r_{1}\right\rangle$ , triangles: $\left\langle I,v_{2}\right\rangle$ ).
Open with DEXTER

In the text

$\begin{figure} \resizebox{\hsize}{!}{\includegraphics{3082fg7a.eps}}\par\resizeb... ...fg7b.eps}}\par\resizebox{\hsize}{!}{\includegraphics{3082fg7c.eps}} \end{figure}$ Figure 7: The autocorrelations of the intensities I (continuum), r₁ (Fe II) and r₂ (Fe I) with increasing time difference. Each second of the first 70 spectra was taken as a starting spectrum.
Open with DEXTER

In the text

$\begin{figure} \resizebox{\hsize}{!}{\includegraphics{3082fg8a.eps}}\par\resizebox{\hsize}{!}{\includegraphics{3082fg8b.eps}} \end{figure}$ Figure 8: The autocorrelations of the velocities v₁ (Fe II) and v₂ (Fe I) with increasing time difference. Each second of the first 70 spectra was taken as a starting spectrum.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{3082fig9.eps} \end{figure}$ Figure 9: The temporal variation of the crosscorrelation between continuum and residual intensities for the Fe II line (solid) and the Fe I line (dotted) and between both residual intensities (dashed). Horizontal bars indicate times of worse seeing.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{3082fg10.eps} \end{figure}$ Figure 10: The temporal variation of the crosscorrelation of the velocity of the Fe I line with continuum intensity (solid), residual intensity of Fe II (dashed), and residual intensity of Fe I (dotted). Horizontal bars indicate times of worse seeing.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{3082fg11.eps} \end{figure}$ Figure 11: The temporal variation of the crosscorrelation between both velocities. Horizontal bars indicate times of worse seeing.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{3082fig1.eps} \end{figure}$	Figure 1: The variation of the relative rms contrast of the continuum intensity during the time series. The wavelength range used was centered at 4993.12 Å and the slit length used for the calculation was 65 $^{\prime \prime }$ .
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{3082fig2.eps} \end{figure}$	Figure 2: Temporal-spatial map of the continuum intensity. The horizontal stripes of lower intensity contrast are due to seeing (see Fig. 1).
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{3082fg3a.eps} \includegraphics[width=8.4cm,clip]{3082fg3b.eps} \end{figure}$	Figure 3: Temporal-spatial maps of the residual intensities of Fe II ( upper panel) and Fe I ( lower panel).
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{3082fg4a.eps} \includegraphics[width=8.4cm,clip]{3082fg4b.eps} \end{figure}$	Figure 4: Temporal-spatial maps of the velocities of Fe II ( upper panel) and Fe I ( lower panel).
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{3082fig5.eps} \end{figure}$	Figure 5: Comparison of the rms fluctuations of the continuum intensity (same as Fig. 1) with the temporal variations of correlations to determine the influence of seeing.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{3082fig6.eps} \end{figure}$	Figure 6: Temporal variation of two correlation coefficients versus the rms of the continuum fluctuations (Asterisks: $\left\langle I,r_{1}\right\rangle$ , triangles: $\left\langle I,v_{2}\right\rangle$ ).
Open with DEXTER

$\begin{figure} \resizebox{\hsize}{!}{\includegraphics{3082fg7a.eps}}\par\resizeb... ...fg7b.eps}}\par\resizebox{\hsize}{!}{\includegraphics{3082fg7c.eps}} \end{figure}$	Figure 7: The autocorrelations of the intensities I (continuum), r₁ (Fe II) and r₂ (Fe I) with increasing time difference. Each second of the first 70 spectra was taken as a starting spectrum.
Open with DEXTER

$\begin{figure} \resizebox{\hsize}{!}{\includegraphics{3082fg8a.eps}}\par\resizebox{\hsize}{!}{\includegraphics{3082fg8b.eps}} \end{figure}$	Figure 8: The autocorrelations of the velocities v₁ (Fe II) and v₂ (Fe I) with increasing time difference. Each second of the first 70 spectra was taken as a starting spectrum.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{3082fig9.eps} \end{figure}$	Figure 9: The temporal variation of the crosscorrelation between continuum and residual intensities for the Fe II line (solid) and the Fe I line (dotted) and between both residual intensities (dashed). Horizontal bars indicate times of worse seeing.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{3082fg10.eps} \end{figure}$	Figure 10: The temporal variation of the crosscorrelation of the velocity of the Fe I line with continuum intensity (solid), residual intensity of Fe II (dashed), and residual intensity of Fe I (dotted). Horizontal bars indicate times of worse seeing.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{3082fg11.eps} \end{figure}$	Figure 11: The temporal variation of the crosscorrelation between both velocities. Horizontal bars indicate times of worse seeing.
Open with DEXTER