Table 1.
Arrival times of solar wind on Earth and period covered by the magnetogram at the Sun.
| Event | Observed at the Earth | Period of magnetogram | Solar minimum | Corresponding study | ||
|---|---|---|---|---|---|---|
| or maximum | ||||||
| Start date | End date | Start date | End date | |||
| 1 | 31/05/2018 10:08 | 05/06/2018 10:21 | 16/05/2018 10:57 | 12/06/2018 05:55 | Minimum | Reiss et al. (2021) |
| 2 | 22/12/2020 17:59 | 23/12/2020 15:10 | 28/11/2020 14:46 | 25/12/2020 22:31 | Minimum | Koukras et al. (2022) |
| 3 | 04/08/2017 13:19 | 05/08/2017 10:11 | 20/07/2017 06:08 | 16/08/2017 11:27 | Minimum | Koukras et al. (2022) |
| 4 | 13/04/2012 04:07 | 13/04/2012 23:13 | 31/03/2012 21:25 | 28/04/2012 03:48 | Maximum | Koukras et al. (2022) |
Notes. These events are used to calculate the magnetic connectivity between the Earth and the surface of the Sun for a given period. The telescope used for all the events is SDO/HMI. The events are taken from two different studies, Koukras et al. (2022) and Reiss et al. (2021).
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