$\begin{figure} \resizebox{8.8cm}{!}{\includegraphics{0146fig1.eps}}\end{figure}$ Figure 1: MDI magnetogram of the studied region taken at 03:04 UTC on June 14 in 1998. The white contours correspond to bright lanes seen in the averaged image of the 1216 Å passband.
Open with DEXTER

In the text

$\begin{figure} \resizebox{18cm}{!}{\includegraphics{0146fig2.eps}}\end{figure}$ Figure 2: Panels A-D: The average intensity image of the 1216 Å passband, and maps of Fourier power in period ranges of 4-16 min, 20-40 min, and 42-75 min. Panels E-H: similar to panels A-D, but for the 195 Å passband. The regions outlined in yellow are analyzed with a wavelet transform.
Open with DEXTER

In the text

$\begin{figure} \par\mbox{\includegraphics[width=8.8cm]{146fig3a.eps}\includegrap... ...h=8.8cm]{146fig3e.eps}\includegraphics[width=8.8cm]{146fig3f.eps} } \end{figure}$ Figure 3: Wavelet power spectra of the 1216 Å ( left side) and 195 Å ( right side) passbands for the three selected regions (corresponding to the three double-rows). a) The running difference light curve. b) Time/period variation of the wavelet power spectrum. Cross-hatched regions indicate the ``cone of influence''. The darker parts represent higher power, and the contours correspond to the 99% confidence level. c) Global wavelet.
Open with DEXTER

In the text

$\begin{figure} \resizebox{8.8cm}{!}{\includegraphics{0146fig1.eps}}\end{figure}$	Figure 1: MDI magnetogram of the studied region taken at 03:04 UTC on June 14 in 1998. The white contours correspond to bright lanes seen in the averaged image of the 1216 Å passband.
Open with DEXTER

$\begin{figure} \resizebox{18cm}{!}{\includegraphics{0146fig2.eps}}\end{figure}$	Figure 2: Panels A-D: The average intensity image of the 1216 Å passband, and maps of Fourier power in period ranges of 4-16 min, 20-40 min, and 42-75 min. Panels E-H: similar to panels A-D, but for the 195 Å passband. The regions outlined in yellow are analyzed with a wavelet transform.
Open with DEXTER