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<!-- DOI: 10.1051/0004-6361/200912059 -->

<h2 class="sec">Online Material</h2>

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<tr><td><!-- init Label --><A NAME="fig:wavelet8april_1003">&#160;</A><!-- end Label--><A NAME="818"></A><A NAME="figure701"
 HREF="img28.png"><IMG
 WIDTH="182" HEIGHT="72" SRC="Timg28.png"
 ALT="\begin{figure}
\par\mbox{\includegraphics[angle=90,width=9cm]{ban12059_f6a.eps}\includegraphics[angle=90, width=9cm]{ban12059_f6b.eps} }
\end{figure}"></A><!-- HTML Figure number: 6 --></td>
<td class="img-txt"><span class="bold">Figure 6:</span><p>
Wavelet analysis for the <IMG
 WIDTH="22" HEIGHT="26" ALIGN="MIDDLE" BORDER="0"
 SRC="img1.png"
 ALT="$8{\rm th}$">
April data at
 Solar 
<!-- MATH: $Y\sim-1003\hbox{$^{\prime\prime}$ }$ -->
<IMG
 WIDTH="77" HEIGHT="26" ALIGN="MIDDLE" BORDER="0"
 SRC="img7.png"
 ALT="$Y\sim -1003\hbox {$^{\prime \prime }$ }$">
for both Ne&nbsp; <SMALL>VIII</SMALL> 770&nbsp;&#197; (<I> left</I>) and
 Fe&nbsp; <SMALL>XII</SMALL> 195&nbsp;&#197; (<I> right</I>). Both light curves are obtained by averaging
 over 9
<!-- MATH: $\hbox{$^{\prime\prime}$ }$ -->
<IMG
 WIDTH="14" HEIGHT="14" ALIGN="BOTTOM" BORDER="0"
 SRC="img4.png"
 ALT="$\hbox {$^{\prime \prime }$ }$">
along the slit. Panels as in Fig.&nbsp;<a href="/articles/aa/full_html/2009/21/aa12059-09/aa12059-09.html#fig:wavelet8april">4</a>.</p></td>
</tr><tr><td colspan="2"><a href="http://dexter.edpsciences.org/applet.php?pdf_id=6&DOI=10.1051/0004-6361/200912059" target="DEXTER">Open with DEXTER</a></td></tr>

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<tr><td><!-- init Label --><A NAME="fig:wavelet15april_1003">&#160;</A><!-- end Label--><A NAME="820"></A><A NAME="figure713"
 HREF="img29.png"><IMG
 WIDTH="182" HEIGHT="72" SRC="Timg29.png"
 ALT="\begin{figure}
\par\mbox{\includegraphics[angle=90,width=9cm]{ban12059_f7a.eps}\includegraphics[angle=90, width=9cm]{ban12059_f7b.eps} }
\end{figure}"></A><!-- HTML Figure number: 7 --></td>
<td class="img-txt"><span class="bold">Figure 7:</span><p>
Wavelet analysis for the 
<!-- MATH: $15{\rm th}$ -->
<IMG
 WIDTH="28" HEIGHT="26" ALIGN="MIDDLE" BORDER="0"
 SRC="img2.png"
 ALT="$15{\rm th}$">
April data at
 Solar 
<!-- MATH: $Y\sim-1003\hbox{$^{\prime\prime}$ }$ -->
<IMG
 WIDTH="77" HEIGHT="26" ALIGN="MIDDLE" BORDER="0"
 SRC="img7.png"
 ALT="$Y\sim -1003\hbox {$^{\prime \prime }$ }$">
for both Ne&nbsp; <SMALL>VIII</SMALL> 770&nbsp;&#197; (<I> left</I>) and
 Fe&nbsp; <SMALL>XII</SMALL> 195&nbsp;&#197; (<I> right</I>). Both light curves are obtained by averaging
 over 9
<!-- MATH: $\hbox{$^{\prime\prime}$ }$ -->
<IMG
 WIDTH="14" HEIGHT="14" ALIGN="BOTTOM" BORDER="0"
 SRC="img4.png"
 ALT="$\hbox {$^{\prime \prime }$ }$">
along the slit. Panels as in Fig.&nbsp;<a href="/articles/aa/full_html/2009/21/aa12059-09/aa12059-09.html#fig:wavelet8april">4</a>.</p></td>
</tr><tr><td colspan="2"><a href="http://dexter.edpsciences.org/applet.php?pdf_id=7&DOI=10.1051/0004-6361/200912059" target="DEXTER">Open with DEXTER</a></td></tr>

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