Top, from left to right: TRACE 171 Å image taken at 03:27 UT, XRT image at 03:27 UT, XRT image at 01:01 UT, EIS raster image in Fe xii 195.12 Å obtained between 00:40 UT and 01:21 UT. The TRACE  171 Å, the XRT image at 03:27 UT and the EIS image have the TRACE 171 Å contour overplotted. The XRT image is overplotted with the −100, −50, 50 and 100 G contours of the magnetogram taken at 00:01:01 UT. Bottom, from left to right: TRACE 1550 Å image taken at 03:28 UT, SUMER O v 629.73 Å and S i 1256.49 Å raster images taken between 02:43 UT and 02:56 UT, EIS O v 192.90 Å raster taken from 00:40 to 01:21 UT. The SUMER Si i image is overplotted with the −100, −50, 50 and 100 G contours of the magnetogram taken at 00:01:01 UT. The rest of the images have the TRACE 1550 Å contour superimposed. All the images (top and bottom) are overplotted with the SUMER slit position. The positive polarity ais shown in white and the negative in black colours.

Top: XRT image with superposition of the SUMER slit position, EUVI A and B images during the jet-like phenomenon. Bottom (from left to right): EIS He ii 256.32 Å and Fe xii 195.12 Å spectra along the EIS slit at 01:01:42 UT; SUMER O v and N v spectra along the SUMER slit; and a spectral window comprising C i 1248.0 Å, C i 1249.0 Å, Mg x 624.9 Å taken in second order, Si ii 1250.41 Å and S ii 1250.58 Å (for details on blends and formation temperatures consult Table 1) at 01:01:19 UT. The temporal evolution of as seen in the to three panels is shown in the on-line movie.

The same as Fig. 11 with EIS at 01:03:46 UT and SUMER at 01:03:26 UT.

The same as Fig. 11 with EIS at 01:04:48 UT and SUMER at 01:04:26 UT.

The same as Fig. 11 with EIS at 01:05:50 UT and SUMER at 01:05:32 UT.

The same as Fig. 11 with EIS at 01:06:52 UT and SUMER at 01:06:32 UT.

The same as Fig. 11. with EIS at 01:07:54 UT and SUMER at 01:07:40 UT.