Table 1.
Detailed information on the datasets used in this work.
| Sequence | Instruments | ||||||||
|---|---|---|---|---|---|---|---|---|---|
| Dataset | Date | DSun [AU] | θ [°] | # Events | Name | Time [UTC] | Δt [s] | Comment | |
| S1 | 2022 March 30 | 0.487 | 0.8 | 8 | HRIEUV | 00:00–03:00 | 3–20 | ||
| AIA | 6 | ||||||||
| SPICE | 00:00–02:43 | 25 | Three-step raster | ||||||
| S2 | 2022 March 17 | 0.380 | 25.9 | 1 | HRIEUV | 00:18–00:48 | 3 | ||
| AIA | 6 | ||||||||
| SPICE | 25 | Three-step raster | |||||||
| S3 | 2023 April 4 | 0.326 | 27.5 | 2 | HRIEUV | 04:23–06:56 | 3 | ||
| AIA | 04:23–06:56 | 12 | |||||||
| EIS | 04:23–05:25 | 3720 | 60-step raster | ||||||
| EIS | 06:01–06:56 | 414 | 25-step raster | ||||||
Notes. DSun is the distance between Solar Orbiter and the centre of the Sun. θ is the separation angle between the Solar Orbiter view and the Earth perspective. The number of events refers to the events listed in Table 3. Δt is the observation cadence. When no time is indicated in the “time” column, this means that the observation is available during the whole HRIEUV sequence.
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