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Table 3.
Linear regressions for the logarithm of the SEP Proton Peak Flux per CME width type and integral energy channel. Pearson’s correlation coefficients (cc), as well as their standard error SE cc are also presented, where n is the number of pairs used for the calculation of cc.
| CME type | Energy channel (MeV) | Equation | cc ± SE cc (n) |
|---|---|---|---|
| Halo | E > 10 | log[Proton Peak Flux] = 0.001 × V CME + 0.243 | 0.60 ± 0.08 (106) |
| E > 30 | log[Proton Peak Flux] = 0.0009 × V CME − 0.350 | 0.56 ± 0.09 (89) | |
| E > 60 | log[Proton Peak Flux] = 0.00066 × V CME − 0.513 | 0.49 ± 0.11 (70) | |
| E > 100 | log[Proton Peak Flux] = 0.000564 × V CME − 0.601 | 0.45 ± 0.13 (47) | |
| Partial halo | E > 10 | log[Proton Peak Flux] = 0.000584 × V CME + 0.811 | 0.33 ± 0.16 (35) |
| E > 30 | log[Proton Peak Flux] = 0.000572 × V CME + 0.243 | 0.33 ± 0.19 (27) | |
| E > 60 | log[Proton Peak Flux] = 0.000798 × V CME − 0.222 | 0.44 ± 0.23 (17) | |
| E > 100 | log[Proton Peak Flux] = 0.00087 × V CME − 0.466 | 0.48 ± 0.29 (11) | |
| Non halo | E > 10 | log[Proton Peak Flux] = 0.00078 × V CME + 0.536 | 0.57 ± 0.21 (17) |
| E > 30 | log[Proton Peak Flux] = 0.000476 × V CME + 0.234 | 0.44 ± 0.30 (11) | |
| E > 60 | log[Proton Peak Flux] = 0.00021 × V CME + 0.160 | 0.26 ± 0.48 (6) | |
| E > 100 | log[Proton Peak Flux] = 0.000184 × V CME − 0.121 | 0.58 ± 0.57 (4) |
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