Table 2.
Time periods with enhanced electron flux in the E200 channel.
| Start | End | Fpeak | Emax | Long. | Lat. | r | A1 |
|---|---|---|---|---|---|---|---|
| (s cm2 sr MeV)−1 | ° | ° | AU | ||||
| 2021-10-28 15:40 | 2021-11-07 02:40 | 1430 | E5700 | 33 | −3 | 0.8 | < 1 |
| 2021-11-09 17:20 | 2021-11-11 02:20 | 9 | E800 | 47 | −2 | 0.88 | < 1 |
| 2022-01-18 17:50 | 2022-01-19 07:30 | 8 | E800 | 102 | 2 | 0.93 | < 1 |
| 2022-01-20 06:20 | 2022-01-22 22:40 | 176 | E5700 | 103 | 2 | 0.92 | < 1 |
| 2022-02-16 03:50 | 2022-02-24 04:10 | 36 | E800 | 130 | 3 | 0.72 | – |
| 2022-03-10 21:10 | 2022-03-11 18:00 | 3 | E200 | 177 | 3 | 0.45 | < 1 |
| 2022-03-14 17:40 | 2022-03-15 20:00 | 9 | E800 | −168 | 2 | 0.41 | < 1 |
| 2022-03-21 05:30 | 2022-03-22 05:30 | 42 | E2200 | −135 | 1 | 0.34 | > 1 |
| 2022-03-30 17:40 | 2022-04-06 10:50 | 10 | E800 | −75 | −2 | 0.34 | < 1 |
| 2022-04-07 18:00 | 2022-04-08 09:40 | 1 | E800 | −34 | −3 | 0.41 | < 1 |
| 2022-04-09 11:40 | 2022-04-10 05:00 | 95 | E800 | −27 | −3 | 0.43 | > 1 |
| 2022-04-13 13:10 | 2022-04-14 22:40 | 6 | E800 | −13 | −3 | 0.48 | < 1 |
| 2022-04-15 03:00 | 2022-04-18 12:00 | 51 | E2200 | −9 | −3 | 0.50 | > 1 |
| 2022-04-30 18:20 | 2022-05-02 15:10 | 4 | E200 | 22 | −2 | 0.69 | < 1 |
| 2022-05-11 04:50 | 2022-05-11 08:20 | 1 | E200 | 35 | −2 | 0.79 | < 1 |
| 2022-06-08 20:10 | 2022-06-09 03:10 | 3 | E200 | 60 | −0.23 | 0.97 | < 1 |
| 2022-06-14 01:00 | 2022-06-15 14:30 | 9 | E800 | 64 | −0.04 | 0.98 | < 1 |
| 2022-07-23 23:40 | 2022-07-25 13:50 | 116 | E200 | 91 | 1 | 0.99 | – |
| 2022-07-25 18:40 | 2022-07-28 02:30 | 5 | E200 | 93 | 1 | 0.98 | – |
| 2022-07-30 08:20 | 2022-07-31 01:00 | 3 | E200 | 96 | 2 | 0.96 | – |
| 2022-08-29 08:20 | 2022-09-04 10:30 | 126 | E800 | 123 | 3 | 0.77 | – |
Notes. The first and second columns give the start and end time of the period, respectively. In the third column, the peak flux of the time period is provided in units of (s cm2 sr MeV)−1. In addition, the highest energy channel that has observed fluxes above its individual threshold is shown in column four and Solar Orbiter’s longitude, latitude, and radial distance to the Sun are given in columns five, six, and seven, respectively. The eighth column shows if the anisotropie A1 in a time window of 30 min before the start until 30 min after the start of the time period with enhanced flux in 1 min time resolution had at least five values above 1 or less than −1 (> 1). If this is not the case, this is indicated with < 1, or a dash if insufficient or no data were available (for more detail see Sect. 4).
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