All Figures

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{aa1164-fig1.ps}\end{figure}$ Figure 1: Temporal average image of MDI magnetograms; the two magnetic polarities are given in black and white. The large white rectangle shows the FOV that was covered by TRACE (cf. Fig. 5). The two small rectangles indicate the regions R1 and R2 that were used for magnetic field extrapolations (shown in Fig. 4). The colorbar gives magnetic flux values.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{aa1164-fig2.ps}\vspace*{4mm} \includegraphics[width=8.8cm,clip]{aa1164-fig3.ps}\end{figure}$ Figure 2: Spatial distribution of power for MDI intensity I. The top image shows the integrated power between 2.3-4.3 mHz (5 min range) and the bottom one between 5.5-7.5 mHz (2-3 min range). Dark areas have less power than bright ones. The large white rectangle shows the FOV that was covered by TRACE (cf. Fig. 5). The two small rectangles indicate the regions R1 and R2 that were used for magnetic field extrapolations (shown in Fig. 4). The colorbar gives arbitrary numbers.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{aa1164-fig4.ps}\vspace*{4mm} \includegraphics[width=8.8cm]{aa1164-fig5.ps}\end{figure}$ Figure 3: Spatial distribution of power for MDI Doppler velocity v. The top image shows the integrated power between 2.3-4.3 mHz (5 min range) and the bottom one between 5.5-7.5 mHz (2-3 min range). Dark areas have less power than bright ones. The large white rectangle shows the FOV that was covered by TRACE (cf. Fig. 5). The two small rectangles indicate the regions R1 and R2 that were used for magnetic field extrapolations (shown in Fig. 4). The colorbar gives arbitrary numbers.
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In the text

$\begin{figure} \par\includegraphics[width=7.1cm,clip]{aa1164-fig6.ps}\includegraphics[width=6.9cm,clip]{aa1164-fig7.ps}\end{figure}$ Figure 4: Magnetic field extrapolation of two network cells: R1 ( left) centered at x = -230 $^{\prime \prime }$ , y = 70 $^{\prime \prime }$ (in Fig. 1) which is also covered by the TRACE FOV and R2 ( right) at x = -70 $^{\prime \prime }$ , y = 160 $^{\prime \prime }$ further away from the AR. The x-y surface shows contours of equal magnetic field strength in solid and dashed lines for the two polarities. Fieldlines between h = 400-1000 km are included. The closed and open field configuration can be clearly seen.
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In the text

$\begin{figure} \par\includegraphics[width=5.5cm,clip]{aa1164-fig8.ps}\hspace*{1c... ...ps}\hspace*{1cm} \includegraphics[width=5.5cm,clip]{aa1164-fig11.ps}\end{figure}$ Figure 5: Detailed comparison of the spatial distribution of MDI velocity power ( top) and TRACE 1700 Å intensity power ( bottom). The left images show the integrated power between 2.3-4.3 mHz (5 min range) and the right ones between 5.5-7.5 mHz (2-3 min range). The white contours show the location of h = 500 km where plasma $\beta$ = 0.5 (dotted line), 1 (dashed line), 10 (solid line). Region R1 is outlined with the white rectangle, the numbers at the colorbars give arbitrary units.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{aa1164-fig1.ps}\end{figure}$	Figure 1: Temporal average image of MDI magnetograms; the two magnetic polarities are given in black and white. The large white rectangle shows the FOV that was covered by TRACE (cf. Fig. 5). The two small rectangles indicate the regions R1 and R2 that were used for magnetic field extrapolations (shown in Fig. 4). The colorbar gives magnetic flux values.
Open with DEXTER