EDP Sciences
Free Access
Issue
A&A
Volume 499, Number 3, June I 2009
Page(s) L29 - L32
Section Letters
DOI https://doi.org/10.1051/0004-6361/200912059
Published online 29 April 2009

Online Material

 \begin{figure}
\par\mbox{\includegraphics[angle=90,width=9cm]{ban12059_f6a.eps}\includegraphics[angle=90, width=9cm]{ban12059_f6b.eps} }
\end{figure} Figure 6:

Wavelet analysis for the $8{\rm th}$ April data at Solar $Y\sim -1003\hbox {$^{\prime \prime }$ }$ for both Ne  VIII 770 Å ( left) and Fe  XII 195 Å ( right). Both light curves are obtained by averaging over 9 $\hbox {$^{\prime \prime }$ }$ along the slit. Panels as in Fig. 4.

Open with DEXTER

 \begin{figure}
\par\mbox{\includegraphics[angle=90,width=9cm]{ban12059_f7a.eps}\includegraphics[angle=90, width=9cm]{ban12059_f7b.eps} }
\end{figure} Figure 7:

Wavelet analysis for the $15{\rm th}$ April data at Solar $Y\sim -1003\hbox {$^{\prime \prime }$ }$ for both Ne  VIII 770 Å ( left) and Fe  XII 195 Å ( right). Both light curves are obtained by averaging over 9 $\hbox {$^{\prime \prime }$ }$ along the slit. Panels as in Fig. 4.

Open with DEXTER


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