Table 1.
Quantities of GLEs presented in Fig. 4.
| E > MeV | GLE55 | GLE56 | GLE59 | GLE60 | GLE62 | GLE63 | GLE64 | GLE65 | GLE66 | GLE67 | GLE69 | GLE70 | GLE71 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| F [cm−2] | F [cm−2] | F [cm−2] | F [cm−2] | F [cm−2] | F [cm−2] | F [cm−2] | F [cm−2] | F [cm−2] | F [cm−2] | F [cm−2] | F [cm−2] | F [cm−2] | |
| 29 | 1.22E+08 | 1.61E+07 | 1.89E+09 | 1.24E+08 | 6.98E+08 | 8.02E+07 | 4.01E+07 | 2.51E+09 | 2.77E+08 | 1.31E+08 | 3.46E+08 | 1.55E+08 | 2.32E+07 |
| 60 | 4.95E+07 | 5.65E+06 | 4.68E+08 | 5.98E+07 | 1.30E+08 | 2.15E+07 | 1.29E+07 | 2.91E+08 | 9.00E+07 | 2.90E+07 | 1.59E+08 | 5.79E+07 | 7.79E+06 |
| 103 | 2.06E+07 | 2.22E+06 | 1.44E+08 | 3.08E+07 | 3.27E+07 | 6.95E+06 | 4.89E+06 | 5.92E+07 | 3.25E+07 | 8.66E+06 | 7.95E+07 | 2.10E+07 | 3.12E+06 |
| 196 | 5.09E+06 | 5.48E+05 | 2.75E+07 | 1.13E+07 | 4.92E+06 | 1.37E+06 | 1.21E+06 | 8.87E+06 | 6.92E+06 | 1.73E+06 | 2.80E+07 | 4.96E+06 | 8.65E+05 |
| 294 | 1.93E+06 | 1.93E+05 | 8.50E+06 | 5.27E+06 | 1.33E+06 | 4.45E+05 | 4.40E+05 | 2.91E+06 | 2.15E+06 | 5.91E+05 | 1.28E+07 | 1.96E+06 | 3.50E+05 |
| 407 | 8.24E+05 | 7.52E+04 | 2.76E+06 | 2.46E+06 | 3.92E+05 | 1.61E+05 | 1.65E+05 | 1.18E+06 | 6.65E+05 | 2.20E+05 | 5.88E+06 | 8.62E+05 | 1.48E+05 |
| 602 | 2.79E+05 | 2.30E+04 | 6.14E+05 | 8.04E+05 | 8.17E+04 | 4.14E+04 | 4.02E+04 | 4.14E+05 | 1.32E+05 | 6.14E+04 | 1.87E+06 | 2.96E+05 | 4.36E+04 |
| 1000 | 5.96E+04 | 4.44E+03 | 7.25E+04 | 1.56E+05 | 9.27E+03 | 5.31E+03 | 4.18E+03 | 1.19E+05 | 1.39E+04 | 1.04E+04 | 3.24E+05 | 6.18E+04 | 5.85E+03 |
| FSXR [W/m2] | 9.40E-04 | 1.10E-04 | 5.70E-04 | 1.44E-03 | 1.00E-04 | 7.10E-05 | 3.10E-04 | 1.70E-03 | 1.00E-03 | 8.30E-04 | 7.10E-04 | 3.40E-04 | 5.10E-05 |
| FSXRrec [W/m2] | 1.34E-03 | 1.57E-04 | 8.14E-04 | 2.11E-03 | 1.43E-04 | 1.01E-04 | 4.43E-04 | 2.57E-03 | 1.55E-03 | 1.33E-03 | 1.02E-03 | 4.86E-04 | 7.29E-05 |
Notes. The integral fluence per F(> E) [cm−2] for a set of eight integral energies for 12 GLEs, as published by Koldobskiy et al. (2021). Associated solar flare flux FXSR [W/m2] followed by FXSRrec [W/m2], which are the currently accurate SXR fluxes. For these values, proper scaling was applied (using a multiplicative factor of 1/0.7 for the GOES 1–8 channel). The saturated strong X-class event values for GLE60, GLE65, GLE66, GLE67, GLE69, and GLE72 also need further attention; their re-scaled SXR classes are taken from Hudson et al. (2024).
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