Table 2
Path lengths and release times using RPM.
| 1 | 2 | 3 | 4 | 5 | |||
| # GLE | Interplanetary length | Solar release time | |||||
| − NM, rise | +NM, rise | − NM, rise | +NM, rise | ||||
|
|
|||||||
| 60 | 1.50 ± 0.16 | 1.55 ± 0.10 | 13:45 ± 05 | 13:43 ± 03 | |||
| 61 | 1.61 ± 0.12 | 1.63 ± 0.09 | 02:23 ± 04 | 02:23 ± 03 | |||
| 63 | 1.27 ± 0.06 | 1.39 ± 0.07 | 05:35 ± 02 | 05:31 ± 02 | |||
| 64 | 1.31 ± 0.09 | 1.32 ± 0.06 | 01:12 ± 03 | 01:12 ± 02 | |||
| 65 | 1.59 ± 0.16 | 1.89 ± 0.17 | 11:15 ± 05 | 11:05 ± 05 | |||
| 67 | 2.67 ± 0.15 | 2.55 ± 0.09 | 17:02 ± 05 | 17:07 ± 03 | |||
| 70 | 2.87 ± 0.13 | 2.56 ± 0.16 | 02:11 ± 04 | 02:20 ± 05 | |||
Notes. Effective interplanetary length (AU) traveled by protons and the associated solar release time (UT). The error bars correspond to the standard deviation of the linear fit. Column 1: the label of the GLEs. Column 2: length computed from the rise times and the mean energy of ERNE channels – without the NM data. Column 3: as Col. 2 but with the NM point. Column 4: the solar release time of energetic protons from the RPM applied to only to ERNE data (as Col. 2, see Fig. 4). Column 5: as Col. 4 but with the NM point.
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