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Table B.1.

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.

VCME, upper | Eq.(1) VCME, upper | Eq.(6) VCME | Eq.(5)

AD774/775 GLE05 AD774/775 GLE05 AD774/775 GLE05
Integral
Energy Peak Proton Flux - IP Peak Proton Flux - IP Peak Proton Flux - IP
(MeV) (pfu) (pfu) (pfu) (pfu) (pfu) (pfu)

E>10 2.26E+07 1.27 E + 07 3.17 E + 07 $ _{1.27\rm E+07}^{3.17\rm E+07} $ 2.47E+06 1.39 E + 06 3.46 E + 06 $ _{1.39\rm E+06}^{3.46\rm E+06} $ 6.16E+06 4.01 E + 06 7.92 E + 06 $ _{4.01\rm E+06}^{7.92\rm E+06} $ 1.18E+06 7.71 E + 05 1.52 E + 06 $ _{7.71\rm E+05}^{1.52\rm E+06} $ 6.23E+05 3.60 E + 05 8.58 E + 05 $ _{3.60\rm E+05}^{8.58\rm E+05} $ 7.63E+04 4.41 E + 04 1.05 E + 05 $ _{4.41\rm E+04}^{1.05\rm E+05} $
E>30 7.16E+06 4.02 E + 06 1.00 E + 07 $ _{4.02\rm E+06}^{1.00\rm E+07} $ 7.80E+05 4.38 E + 05 1.09 E + 06 $ _{4.38\rm E+05}^{1.09\rm E+06} $ 1.95E+06 1.27 E + 06 2.50 E + 06 $ _{1.27\rm E+06}^{2.50\rm E+06} $ 3.75E+05 2.44 E + 05 4.82 E + 05 $ _{2.44\rm E+05}^{4.82\rm E+05} $ 1.97E+05 1.14 E + 05 2.71 E + 05 $ _{1.14\rm E+05}^{2.71\rm E+05} $ 2.41E+04 1.40 E + 04 3.32 E + 04 $ _{1.40\rm E+04}^{3.32\rm E+04} $
E>60 1.84E+06 1.03 E + 06 2.58 E + 06 $ _{1.03\rm E+06}^{2.58\rm E+06} $ 2.01E+05 1.13 E + 05 2.81 E + 05 $ _{1.13\rm E+05}^{2.81\rm E+05} $ 5.01E+05 3.26 E + 05 6.44 E + 05 $ _{3.26\rm E+05}^{6.44\rm E+05} $ 9.63E+04 6.27 E + 04 1.24 E + 05 $ _{6.27\rm E+04}^{1.24\rm E+05} $ 5.06E+04 2.93 E + 04 6.98 E + 04 $ _{2.93\rm E+04}^{6.98\rm E+04} $ 6.20E+03 3.59 E + 03 8.54 E + 03 $ _{3.59\rm E+03}^{8.54\rm E+03} $
E>100 5.69E+05 3.19 E + 05 7.97 E + 05 $ _{3.19\rm E+05}^{7.97\rm E+05} $ 6.20E+04 3.48 E + 04 8.69 E + 04 $ _{3.48\rm E+04}^{8.69\rm E+04} $ 1.55E+05 1.01 E + 05 1.99 E + 05 $ _{1.01\rm E+05}^{1.99\rm E+05} $ 2.98E+04 1.94 E + 04 3.83 E + 04 $ _{1.94\rm E+04}^{3.83\rm E+04} $ 1.57E+04 9.05 E + 03 2.16 E + 04 $ _{9.05\rm E+03}^{2.16\rm E+04} $ 1.92E+03 1.11 E + 03 2.64 E + 03 $ _{1.11\rm E+03}^{2.64\rm E+03} $

Integral
Energy Fluence - FP Fluence - FP Fluence - FP
(MeV) (cm−2) (cm−2) (cm−2) (cm−2) (cm−2) (cm−2)

E>10 6.18E+13 3.22 E + 13 9.05 E + 13 $ _{3.22\rm E+13}^{9.05\rm E+13} $ 5.05E+12 2.63 E + 12 7.40 E + 12 $ _{2.63\rm E+12}^{7.40\rm E+12} $ 1.42E+13 8.73 E + 12 1.89 E + 13 $ _{8.73\rm E+12}^{1.89\rm E+13} $ 2.20E+12 1.36 E + 12 2.93 E + 12 $ _{1.36\rm E+12}^{2.93\rm E+12} $ 1.07E+12 5.74 E + 11 1.53 E + 12 $ _{5.74\rm E+11}^{1.53\rm E+12} $ 9.93E+10 5.35 E + 10 1.43 E + 11 $ _{5.35\rm E+10}^{1.43\rm E+11} $
E>30 1.37E+13 7.18 E + 12 2.00 E + 13 $ _{7.18\rm E+12}^{2.00\rm E+13} $ 1.15E+12 6.00 E + 11 1.67 E + 12 $ _{6.00\rm E+11}^{1.67\rm E+12} $ 3.19E+12 1.97 E + 12 4.23 E + 12 $ _{1.97\rm E+12}^{4.23\rm E+12} $ 5.04E+11 3.11 E + 11 6.68 E + 11 $ _{3.11\rm E+11}^{6.68\rm E+11} $ 2.45E+11 1.33 E + 11 3.51 E + 11 $ _{1.33\rm E+11}^{3.51\rm E+11} $ 2.34E+10 1.26 E + 10 3.34 E + 10 $ _{1.26\rm E+10}^{3.34\rm E+10} $
E>60 1.89E+12 1.01 E + 12 2.72 E + 12 $ _{1.01\rm E+12}^{2.72\rm E+12} $ 1.72E+11 9.24 E + 10 2.48 E + 11 $ _{9.24\rm E+10}^{2.48\rm E+11} $ 4.63E+11 2.91 E + 11 6.07 E + 11 $ _{2.91\rm E+11}^{6.07\rm E+11} $ 7.80E+10 4.91 E + 10 1.02 E + 11 $ _{4.91\rm E+10}^{1.02\rm E+11} $ 3.90E+10 2.16 E + 10 5.51 E + 10 $ _{2.16\rm E+10}^{5.51\rm E+10} $ 4.03E+09 2.23 E + 09 5.70 E + 09 $ _{2.23\rm E+09}^{5.70\rm E+09} $
E>100 2.93E+11 1.62 E + 11 4.15 E + 11 $ _{1.62\rm E+11}^{4.15\rm E+11} $ 2.99E+10 1.65 E + 10 4.24 E + 10 $ _{1.65\rm E+10}^{4.24\rm E+10} $ 7.68E+10 4.93 E + 10 9.95 E + 10 $ _{4.93\rm E+10}^{9.95\rm E+10} $ 1.41E+10 9.03 E + 09 1.82 E + 10 $ _{9.03\rm E+09}^{1.82\rm E+10} $ 7.25E+09 4.13 E + 09 1.01 E + 10 $ _{4.13\rm E+09}^{1.01\rm E+10} $ 8.83E+08 4.74 E + 08 1.16 E + 09 $ _{4.74\rm E+08}^{1.16\rm E+09} $

Notes. Peak proton fluxes were calculated via the I P V CME 5 $ I_{P} \propto V_{CME}^{5} $ relations (provided in Figs. 1 & A.1) and Fluence via Eq. 7 for a given VCME, upper. The upper and lower limits included in the Table are driven by the VCME range of the associated solar flare per event. The second and third columns provide outputs based on VCME, upper from Eq. (1). The fourth and fifth columns provide the same results based on VCME, upper from Eq. (6) and the sixth and seventh columns provide the same results based on VCME from Eq. (5).

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