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Table 2

Cases selected in the southern hemisphere, with nadir viewing at large heliocentric distances.

Case Date Start time [UTC] Integration time [s] Cometocentric distance [km] Heliocentric distance [au] Spacecraft latitude [°] Spacecraft longitude [°] Total column density [1015 cm−2]
1 14/01/2015 11:38:40 3629 28.4 2.55 −23.4 −82.9 0.58
2 29/01/2015 18:40:49 6048 27.8 2.44 −63.8 5.4 0.27
3 30/01/2015 04:25:44 2419 27.8 2.43 −64.6 56.6 0.22
4 30/01/2015 06:34:42 2419 27.8 2.43 −64.2 −11.4 0.51
5 30/01/2015 07:17:41 1763 27.8 2.43 −64.0 −34.0 0.48
6 30/01/2015 11:32:18 2419 27.9 2.43 −62.5 −167.4 0.18
7 30/01/2015 15:25:50 2419 27.9 2.43 −60.5 71.35 0.28
8 26/04/2016 06:06:12 4452 21.2 2.9 −33.1 −107 1.88

9 29/01/2015 07:51:27 3629 27.8 2.44 −58.4 −17.1 0.75
10 21/04/2016 23:01:00 3398 30.9 2.85 −24.6 −57.7 1.24
11 21/03/2016 00:05:00 2603 12.2 2.62 −24.2 −36.8 1.43
12 14/05/2016 14:39:34 4613 9.8 3.0 −53.1 −111.7 1.13
13 27/05/2016 08:43:00 5592 7.0 3.09 −56.2 −42.3 1.32

Notes. The horizontal lines separate nadir cases with high (Cases 1–8) and low (Cases 9–13) electron fluxes.

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