![\begin{figure}
\par\includegraphics[width=8.cm,angle=0]{H9033f1.eps}\end{figure}](/articles/aa/full/2008/13/aa9033-07/img1.gif) |
Figure 1: X-ray flux light curve from GOES (1-8 Å) showing the B2-class flare observed by EIS. |
| Open with DEXTER | |
In the text
![\begin{figure}
{\includegraphics[width=17.cm]{H9033f2a.eps} }
{\includegraphics[width=17.cm]{H9033f2b.eps} }
\end{figure}](/articles/aa/full/2008/13/aa9033-07/img2.gif) |
Figure 2: Monochromatic images (negative) of a selection of EIS lines, starting with a few lines from the transition region (O VI) up to Fe XXIV, the hottest ion observed. |
| Open with DEXTER | |
In the text
![\begin{figure}
\par\includegraphics[width=8.5cm]{H9033f3.eps}
\end{figure}](/articles/aa/full/2008/13/aa9033-07/img5.gif) |
Figure 3: A portion of the averaged spectrum (units are counts) over an area where Fe XVII was brightest. |
| Open with DEXTER | |
In the text