Summary of EIS data-sets (ISFM)The dates below were identified by the ISFM team as good
possibilities for making the connection between the solar wind and
corona. The links go through to the relevant EIS mapper webpage. 29-30 July 2007The study 'PRY_footpoints_v2' was run from 01:10 to 23:45 UT
on 29 July. The pointing was disk center (with tracking), and it
covered part of an active region outflow region. Note that the study
was run repeatedly (61 rasters in all) over the observing period. On 30 July approximately the same region was observed, but with SYNOP002 (05:02 UT) and SYNOP003 (08:49 UT). 1-3 & 5 November 2007The Sun was very quiet and the target of interest was the north coronal hole. Over the four days the study 'GDZ_PLUME1_2_300_50s' was run several times. The raster is large and covers part of the coronal hole. 8,9 December 2008Sun
again very quiet. A small, low-lattitude coronal hole in
the north. A single 'dhb_polar_scan_Q90' raster at 10:00 on the 8th,
and a second at 11:00 on the 9th. The EIS images show a weak active
region to the left of the coronal hole. There was a filament eruption
associated with this AR on 12-Dec at about 7 UT (seen with STEREO-A). 17 May 2010[17-May] A low-latitude coronal hole in the south. Two runs of Atlas_60 at 12:19 and 13:57 UT in the center of the hole; two runs of 'dhb_polar_scan_Q90'at 19:06 and 22:42 UT that are partly in hole and partly in quiet Sun. 3 Dec 2013[3-Dec] Small equatorial coronal hole, and the SYNOP006 study (spectral atlas) is
placed on the right-hand boundary. 16 April 2016[16-Apr] Very large 'DHB_006_v2' raster at 00:20 UT covering coronal hole and active region outflow region. 21 April 2016[21-Apr] Very large 'DHB_006_v2' raster at 1835 UT covering coronal hole extension around an active region. Two 'HPW021' rasters on opposite side of the AR. 21-23 Nov 2016Low-latitude coronal hole to the south of an active region,
plus very large north coronal hole. On the 21st and 22nd the AR and
LLCH were observed simultaneously with one of the HPW021 studies. On
the 23nd three very large DHB_006_v2 scans were run from the north pole
to the equator. Page maintained by Dr Peter R Young. |