Propagating waves in polar coronal holes as seen by SUMER & EIS

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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