If you click on the start date, you will see a daily overview of the SUMER observations. Shown is the temporal development of the radiance, averaged across the whole slit and summed over a spectral range 1 Å around the flare line. Thus, flare events in the SUMER field of view become visible; they can be quantified and compared to other instruments' observations.
date from to # good solar X, Y expos. spectr. windows flare /UTC images coord. /" time /s around /Å line ----------- ---- ---------- ---- -------------- ------ 28.Feb.01 11:25 23:18 253 +954 -420 162.5 1115 1118 etc. Fe XIX 01.Mar.01 11:06 22:59 253 +954 -420 162.5 1115 1118 etc. Fe XIX 04.Mar.01 08:09 20:02 253 +994 +236 162.5 1115 1118 etc. Fe XIX 05.Mar.01 06:30 16:24 211 +994 +236 162.5 1115 1118 etc. Fe XIX 16:33 23:57 158 +994 +287 162.5 1115 1118 etc. Fe XIX 06.Mar.01 00:00 04:26 95 +994 +287 162.5 1115 1118 etc. Fe XIX 14:54 23:57 191 +994 +287 162.5 1115 1118 etc. Fe XIX 07.Mar.01 00:00 02:47 60 +994 +287 162.5 1115 1118 etc. Fe XIX 13:14 23:59 228 +994 +310 162.5 1115 1118 etc. Fe XIX 08.Mar.01 00:02 01:07 24 +994 +310 162.5 1115 1118 etc. Fe XIX 11:35 23:28 251 +994 +310 162.5 1115 1118 etc. Fe XIX 09.Mar.01 09:55 21:42 251 +994 +310 162.5 1115 1118 etc. Fe XIX 11.Mar.01 19:03 23:57 105 +954 +480 162.5 1115 1118 etc. Fe XIX 12.Mar.01 00:00 06:56 148 +954 +480 162.5 1115 1118 etc. Fe XIX 18.Oct.01 09:41 19:41 442 +930 -520 78.0 1108 1115 1118 Fe XIX -----------------------------------------------------------------------
Observed lines (incl. wavelength/Å and log temperature/K):
The studies of February and March 2001 transmit one full detector (1098-1138 Å) as well as five times the right and the left half of the detector, in an alternating mode. Only Ca X and Fe XIX are contained in all images. - Of the five flare watch studies of October 2001, only the last one could be used here.