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Table 8
FLUKA-LEI Monte Carlo estimates of λΝΕΤ and λEFF for different species of GCR particles.
| Solar minimum | Solar maximum | |||
|---|---|---|---|---|
| Particle | λΝΕΤ | λEFF | λΝΕΤ | λEFF |
| (s−1) | (s−1) | (s−1) | (s−1) | |
| Protons | 48.7 | 672.1 | 14.1 | 255.9 |
| Helium | 15.0 | 289.8 | 4.1 | 183.1 |
| Carbon | 1.4 | 93.9 | 0.8 | 57.5 |
| Nitrogen | 0.4 | 26.9 | 0.2 | 21.1 |
| Oxygen | 1.7 | 123.9 | 0.9 | 64.6 |
| Iron | 0.4 | 72.8 | 0.3 | 63.3 |
| Electrons | –3.2 | 216.7 | –0.1 | 91.1 |
| Total | 64.4 | 1496.1 | 20.3 | 737.6 |
Notes. λΝΕΤ and λEFF are estimated by assuming ϕ = 200 MV/c and ϕ = 1200 MV/c at solar minimum and maximum conditions, respectively (Villani et al. 2024a).
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