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Table 1

Time-line of the solar phenomena and energetic electron onset times associated with the 26 Dec 2013 SEP event.

Time (UT) Properties Observer
2:10 Filament eruption (region #1) associated to CME1 STA, STB/EUVI
2:30 CME1 at 1 RS STA, STB
2:35 CME1 first appearance STA/COR1
2:41–4:45 Main flare (region #2) STA, STB
2:47–2:55 1st (faint) type II burst STB/SWAVES
2:47 Filament eruption (region #3) and interaction with northern CH STB/EUVI
2:50 Impulsive phase of main flare STA, STB/EUVI
2:53 Partly occulted type III burst STA, STB, Wind
2:55 Partly occulted type III burst STA, STB, Wind
3:02–3:12 2nd (main) type II burst STB, (STA)
3:02–3:09 Main type III bursts STA, STB, (Wind/WAVES)
3:05 CME2 first appearance at 2.7 RS STA/COR1
3:15–4:17 Frifting type II-like structure (see Fig. 4) STB/SWAVES
4:00–4:30 Flare in region #4 STB/EUVI
3:25 Latest possible 55–105 keV electron injection (according to
Onset time assuming a nominal travel time along the Parker spiral)
3:45 ± 1 min 55–105 keV electron onset STA/SEPT
3:53 ± 5 min 55–105 keV electron onset STB/SEPT
4:10 ± 15 min 62–103 keV electron onset ACE/EPAM
4:07 ± 15 min 0.7–2.8 MeV electron onset STA/HET
4:22 ± 15 min 0.7–2.8 MeV electron onset STB/HET
4:30 ± 20 min 0.7–3.0 MeV electron onset SOHO/EPHIN
6:45 Type III burst Wind/WAVES
6:53 C2.2 flare at W28 GOES, SDO
7:05 CME3 first appearance STA/COR1
7:15–8:30 SEP onsets of the second component STA, STB/HET, SOHO/EPHIN, ERNE

Notes. Observers of radio features in brackets denote a high-frequency occultation for that viewpoint.

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