Table D.1.
Statistics on timing delays between SEP release times and their associated solar phenomena.
| Δ | N | Short | Long | ||
|---|---|---|---|---|---|
| > 0 | < 0 | > 0 | < 0 | ||
| tSEP − tCME | 151 | 103 (68%) | 48 (32%) | 69 (46%) | 82 (54%) |
| tSEP − tSXR, onset | 121 | 119 (99%) | 2 (1%) | 79 (65%) | 42 (35%) |
| tSEP − tSXR, peak | 121 | 94 (78%) | 27 (22%) | 56 (46%) | 65 (54%) |
| tSEP − tHXR, onset | 87 | 76 (87%) | 11 (13%) | 53 (61%) | 34 (39%) |
| tSEP − tHXR, peak | 87 | 72 (83%) | 15 (17%) | 40 (46%) | 47 (54%) |
| tSEP − ttII | 126 | 91 (72%) | 35 (28%) | 60 (48%) | 66 (52%) |
| tSEP − ttIII | 155 | 144 (93%) | 11 (7%) | 99 (64%) | 56 (36%) |
| tSEP − ttIV | 40 | 25 (63%) | 15 (37%) | 17 (43%) | 23 (57%) |
| tSEP − tγ | 57 | 51 (89%) | 6 (11%) | 37 (65%) | 20 (35%) |
Notes. The first column indicates the delay considered, the second column gives the number of events in the statistics. In the third and fourth columns, we consider the short and long travel times for the particles (see Sect. 4 for details), and display the number of events with positive or negative delays. Percentages are relative to the total number of SEP events with an identified solar association.
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