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Table 1
Sequence of first detection times by different instruments for the three studied events.
| Waveband or Instrument | 2013 Oct. 11 | 2014 6 Jan. | 2014 Sep. 01 | |
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| EM emission: | ||||
| Radio type II | 07:10 | 07:45 | 11:00 | |
| Radio type III | 07:15 | 07:45 | 11:00 | |
| Soft X-ray | 07:01 | 07:42 | 10:54 | |
| Hard X-ray | 06:58 | 10:57 | ||
| Fermi LAT γ-ray (>100 MeV) | 07:15 | Too weak | 11:04 | |
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| Shock connectivity to vis. disk | 07:10 | 07:45 | 11:05 | |
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| SEP electrons (1 AU): | ||||
| STEREO-A; HET (0.7–4 MeV) | 07:29 | 09:30 | 11:11 | |
| STEREO-B; HET (0.7–4 MeV) | 07:40 | Too weak | 11:25 | |
| L1; EPHIN (0.25–10 MeV) | 13:00 ± 30 | Data gap | 14:22 | |
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| SEP protons (1 AU): | ||||
| STEREO-A; HET (29.5–100 MeV) | 07:58 | 09:30 | Data gap | |
| STEREO-B; HET (29.5–100 MeV) | 08:19 | 18:45 | 11:48 | |
| L1; EPACT (28–72 MeV) | 22:30 (+1 day) | 08:25 | 00:15 (+1 day) | |
| GOES 13 (>100 MeV) | 18:00 ± 01:00 | |||
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| SEP on Mars: | 07:45 | 09:00 | 12:00 | |
Notes. First observation times in radio type II and III, soft and hard X-ray, and high-energy γ-ray observations are presented. Energetic particle (high-energy protons and electrons at 1 AU and at Mars) onset times are given as well.
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