Table A.1
Spectral parameters for GLE fluences of SCs 23 and 24.
| GLE | Date | J0 [cm-2] | γ1 | γ2 | R0 [GV] |
|
|
|||||
| 55 | 1997-Nov.-06 | (8.15 ± 0.85) × 108 | 0.28 ± 0.09 | 5.38 ± 0.09 | 0.116 ± 0.004 |
| 56 | 1998-May-02 | (8.98 ± 0.76) × 106 | 1.31 ± 0.07 | 6.51 ± 0.55 | 0.196 ± 0.008 |
| 57 | 1998-May-06 | (1.64 ± 0.04) × 106 | 1.92 ± 0.02 | 7.46 ± 0.41 | 0.202 ± 0.003 |
| 58 | 1998-Aug.-24 | (2.10 ± 0.05) × 105 | 2.98 ± 0.02 | 5.27 ± 0.34 | 0.677 ± 0.034 |
| 58 esp | 1998-Aug.-24 | (1.63 ± 0.04) × 104 | 5.26 ± 0.03 | 7.74 ± 0.34 | 0.983 ± 0.060 |
| 59 | 2000-Jul.-14 | (2.94 ± 0.30) × 109 | 0.51 ± 0.10 | 7.46 ± 0.14 | 0.123 ± 0.003 |
| 59 esp | 2000-Jul.-14 | (6.01 ± 0.18) × 107 | 3.24 ± 0.05 | 7.85 ± 0.29 | 0.226 ± 0.005 |
| 60 | 2001-Apr.-15 | (5.22 ± 0.54) × 107 | 1.39 ± 0.09 | 5.69 ± 0.08 | 0.260 ± 0.012 |
| 61 | 2001-Apr.-18 | (8.39 ± 0.75) × 106 | 1.85 ± 0.07 | 5.02 ± 0.14 | 0.237 ± 0.012 |
| 62 | 2001-Nov.-04 | (2.14 ± 0.19) × 109 | 0.24 ± 0.07 | 6.67 ± 0.31 | 0.093 ± 0.003 |
| 62 esp | 2001-Nov.-04 | (4.78 ± 0.11) × 108 | 2.36 ± 0.04 | 11.2 ± 0.3 | 0.129 ± 0.002 |
| 63 | 2001-Dec.-26 | (2.17 ± 0.19) × 107 | 1.81 ± 0.07 | 7.86 ± 0.34 | 0.180 ± 0.006 |
| 64 | 2002-Aug.-24 | (5.06 ± 0.46) × 106 | 2.36 ± 0.08 | 6.70 ± 0.33 | 0.225 ± 0.010 |
| 65 | 2003-Oct.-28 | (8.44 ± 0.78) × 109 | 0.01 ± 0.08 | 6.48 ± 0.25 | 0.089 ± 0.003 |
| 65 esp | 2003-Oct.-28 | (1.12 ± 0.04) × 108 | 2.81 ± 0.05 | 8.92 ± 0.10 | 0.171 ± 0.003 |
| 66 | 2003-Oct.-29 | (7.62 ± 0.18) × 107 | 2.04 ± 0.02 | 6.86 ± 0.30 | 0.206 ± 0.004 |
| 67 | 2003-Nov.-02 | (2.27 ± 0.20) × 106 | 3.50 ± 0.07 | 7.01 ± 0.52 | 0.321 ± 0.017 |
| 68 | 2005-Jan.-17 | (3.51 ± 0.11) × 107 | 2.65 ± 0.05 | 8.29 ± 0.11 | 0.162 ± 0.003 |
| 69 | 2005-Jan.-20 | (3.81 ± 0.29) × 108 | 0.72 ± 0.07 | 5.78 ± 0.06 | 0.204 ± 0.007 |
| 70 | 2006-Dec.-13 | (1.33 ± 0.14) × 108 | 1.05 ± 0.09 | 5.80 ± 0.09 | 0.177 ± 0.007 |
| 71 | 2012-May-17 | (1.03 ± 0.11) × 107 | 1.36 ± 0.09 | 6.96 ± 0.97 | 0.219 ± 0.008 |
Notes. Events labeled with numbers are the official GLEs and the ones below appended with “esp” are the energetic storm particle components related to these GLEs. The uncertainties are estimated by varying the parameter of interest while holding the others at their best-fit value.
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