Table 1.

Characteristics of the 3He-rich period.

Ion injection Type III STEREO-A EUVI event
Separation Elec. injection 3He/4He (c) Fe/O (c)
time (UT) start (UT) Type (a) Location angle (b)(°) time (UT)
1 322.42 Nov-17 10:05 09:49 [41] B E90S22 20 09:20 0.61 ± 0.08 2.00 ± 0.37
2 322.62 Nov-17 14:53 15:28 [20] B E90S18 20 ... 0.22 ± 0.03 0.63 ± 0.06
3 322.74 Nov-17 17:46 18:20 [12] J E90S18 20 18:20 0.90 ± 0.03 0.91 ± 0.01
18:24 [16] ... E90S18 20 ... ... ...
4 323.54 Nov-18 12:58 13:08 [00] B E85S23 25 13:10 0.56 ± 0.01 1.35 ± 0.01
14:09 [01] B E85S23 25 14:07 ... ...
5 325.87 Nov-20 20:53 19:34 [26] B E48S19 62 19:30 0.32 ± 0.03 0.76 ± 0.03
20:33 [25] J E52S17 58 ... ... ...
21:00 [52] B E48S19 62 ... ... ...

Notes.

(a)

See text for more details. B: brightening; J: jet.

(b)

Between the Solar Orbiter magnetic footpoint longitude on the Sun and the longitude of the EUVI event.

(c)

0.2–2.0 MeV nucleon−1.

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