Table B.1.
Summary of the successfully acquired Solar Orbiter datasets coordinated with DKIST.
| Instrument | Wavelength channel(s) | Start-End [UT] | Pointing [″] | 1 px size [km] | FOV [Mm] | Cadence[s] | ||
|---|---|---|---|---|---|---|---|---|
| 18 October 2022 | ||||||||
| EUI/FSI | 174, 304 | 00:00 - 23:50 | (-1187″, 916″) | 1040 | 3161×3194 | 10 min; 20 min | ||
| SPICE | SW, LW | 07:55 - 23:37 | (-1256″, 748″) | x:1405, y:257 | 180×214 | 11 min 29 sec | ||
| PHI/HRT | - | 03:15 - 23:15 | (-1265″, 791″) | 117 | 240×240 | 1h | ||
| 19 October 2022 | ||||||||
| EUI/FSI | 174, 304, | 00:00 - 23:50 | (-812″, 826″) | 1071 | 3257×3291 | 10 min, 20 min | ||
| EUI/HRI | 174, Ly-α | 19:05 - 20:05 | (-1060″, 784″) | 119 | 243×243 | 5 s., 30 s. | ||
| SPICE | SW, LW | 07:40 - 22:36 | (-881″, 661″) | x:1448,y:265 | 185×220 | 11 min 29 sec | ||
| PHI/HRT | - | 00:15 - 23:15 | (-889″, 704″) | 121 | 247×247 | 1h | ||
| 20 October 2022 | ||||||||
| EUI/FSI | 174, 304 | 00:00 - 23:50 | (-388″, 789″) | 1106 | 3363x3398 | 10 min, 20 min | ||
| EUI/HRI | 174, Ly-α | 19:05 - 20:05 | (-637″, 750″) | 123 | 251×251 | 5 s., 30 s. | ||
| SPICE | SW, LW | 08:00 - 22:44 | (-456″, 620″) | x:1495, y:274 | 191×228 | 11 min 29 sec | ||
| PHI/HRT | - | 03:15 - 23:15 | (-464″, 663″) | 125 | 256×256 | 1h | ||
| 21 October 2022 | ||||||||
| EUI/FSI | 174, 304 | 00:00 - 23:50 | (21″, 730″) | 1143 | 3476×3512 | 10 min, 20 min | ||
| EUI/HRI | 174, Ly-α | 19:05 - 20:05 | (-228″, 691″) | 127 | 259×259 | 5 s., 30 s. | ||
| SPICE | SW, LW | 07:55 - 22:39 | (-46″, 567″) | x:1545, y:283 | 198×235 | 11 min 29 sec | ||
| PHI/HRT | - | 00:15 - 23:15 | (-57″, 610″) | 129 | 264×264 | 1h | ||
| 24 October 2022 | ||||||||
| EUI/FSI | 174, 304 | 00:00 - 23:50 | (1134″, 641″) | 1265 | 3846×3886 | 10 min, 20 min | ||
| EUI/HRI | 174, - | 19:05 - 19:35 | (884″, 609″) | 140 | 287×287 | 5 s | ||
| SPICE | SW, LW | 07:55 - 21:53 | (1070″, 476″) | x:1710, y:313 | 219×260 | 11 min 29 sec | ||
| PHI/HRT | - | 03:15 - 23:20 | (1069″, 521″) | 143 | 219×219 | 1h | ||
Notes. The target coordinates correspond to the centre of the FOV of the Solar Orbiter instruments in helioprojective coordinates as viewed from Solar Orbiter. The distance between the Sun and Solar Orbiter on each day are defined in the Table 1. The table presents UT measured at the Earth. Pointing information are presented in the table at 19:05 UT for each coordinated observation day (i.e. when the high-resolution coordinated observations began). SPICE provided two types of observations. The table presents details for SCI_DYN-MED_SC_SL04_5.0S_FF SPICE observations. The SPICE SCI_DYN-MED_SC_SL04_5.0S_FF observations were provided with duration of ≈3.25h, but out of DKIST observation time range (thus we do not show its details in the table). The pointing position in arcsec depends on the distance of the spacecraft to the Sun, and distance of the Solar Orbiter changed between 0.32 and 0.39 au for observations presented in this table.
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