Table 3.
Upper limit peak proton fluxes (IP, [pfu]) and fluences (FP, [cm−2]) for the SEP event on AD774/775 and GLE05 derived in this work, for each integral proton energy.
| AD774/775 | GLE05 | |
|---|---|---|
| Integral energy | Peak proton flux – IP | |
| (MeV) | (pfu) | (pfu) |
| E > 10 | 2.16E+06 |
2.36E+05 |
| E > 30 | 6.38E+05 |
6.96E+04 |
| E > 60 | 1.72E+05 |
1.87E+04 |
| E > 100 | 5.07E+04 |
5.53E+03 |
| Integral energy | Fluence – FP | |
| (MeV) | (cm−2) | (cm−2) |
| E > 10 | 4.25E+12 |
3.48E+11 |
| E > 30 | 1.05E+12 |
8.56E+10 |
| E > 60 | 1.46E+11 |
1.33E+10 |
| E > 100 | 2.13E+10 |
2.23E+09 |
Notes. Peak proton fluxes were calculated via Eq. (2) and fluence via Eq. (3) for a given SXR flux. The upper and lower limits listed here are driven by the FSXR range of the associated solar flare per event, and are from Cliver et al. (2022).
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