Table 1

24 flares observed to cause a noticeable effect at Rosetta, as well as 3 flares that did not show any effect.

Date and time (UT) GOES class Location ΔEUV (mW m−2) ΔEUV (mW m−2) ΔIph0 (nA)
on Sun FISM v.1 FISM-M LAP
24 Aug 2014 12:00 M5.7 S09E76 0.08 1.2
17 Oct 2014 15:35 C6.7 S15E79 0.03 1.5
19 Oct 2014 15:20 X1.1 S14E64 0.05 0.03
20 Oct 2014 09:01 M3.9 S14E42 0.06 0.02 1.8
22 Oct 2014 01:17 M8.7 S13E21 0.09 0.03
05 Nov 2014 09:26 M7.9 N20E68 0.08 1.5
07 Nov 2014 16:53 X1.6 N14E36 0.15
14 Jun 2015 00:52 M2.0 N14W73 0.29 0.03 3.0
21 Jun 2015 09:26 M3.8 S21W57 0.45 10
25 Jun 2015 08:03 M7.9 N09W42 0.35 21
28 Jun 2015 02:43 C8.0 S13W59 0.09 11
28 Jun 2015 13:05 M2.2 S14W65 0.17 11
28 Jun 2015 19:00 M2.1 S13W70 0.26 10
29 Sep 2015 03:11 M1.2 S08W78 0.22 0.05 1.1
29 Sep 2015 05:05 M2.9 S21W37 0.25 0.1 2.0
29 Sep 2015 06:35 M1.4 S20W34 0.16 0.02 2.0
29 Sep 2015 11:09 M1.6 S20W39 0.25 0.04 2.3
29 Sep 2015 19:30 M1.1 S20W36 0.21 2.2
30 Sep 2015 13:15 M1.1 S23W59 0.15 0.03 2.5
02 Oct 2015 00:06 M5.5 S19W67 0.30 3.7
04 Nov 2015 03:20 M1.9 N15W64 0.15 2.0
27 Dec 2015 18:59 C2.8 N01W01 0.04 1.6
28 Dec 2015 11:22 M1.8 S23W11 0.07 6.0
30 Dec 2015 19:05 C1.1 S22W50 0.03 1.2
30 Dec 2015 22:42 C4.3 S24W39 0.06 0.02 1.0
13 Feb 2016 15:16 M1.8 N13W25 0.12 0.02 9.0
14 Feb 2016 19:19 M1.0 N15W47 0.07 0.02 5.0

Notes. The information on the GOES class and the location on the Sun are taken from the Hinode flare catalog. The flares that were harder to separate from the ambient plasma variability are written in italics. The dashes indicate that no information is available (e.g. not seen at Mars in the FISM-M model, or that no effect was seen). The time information refers to the observations at the GOES satellite.

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