SBOK061 October 2022 SN54SLC8T245-SEP
Event rates were calculated for LEO (ISS) and GEO environments by combining CREME96 orbital integral flux estimations and simplified SEE cross-sections according to methods described in Heavy Ion Orbital Environment Single-Event Effects Estimations application report. We assume a minimum shielding configuration of 100 mils (2.54 mm) of aluminum, and worst-week solar activity (this is similar to a 99% upper bound for the environment). Table 5-3 and Table 5-4 provides the event rate calculation using the 95% upper-bounds for the SEL and the SET, respectively.
Orbit Type | Onset LETEFF (MeV-cm2/mg) | CREME96 Integral FLUX (/day/cm2) | σSAT (cm2) | Event Rate (/day) | Event Rate (FIT) | MTBF (Years) |
---|---|---|---|---|---|---|
LEO (ISS) | 43 | 6.40 × 10–4 | 1.85 × 10–7 |
1.18 × 10–10 |
4.93 × 10–3 |
2.31 × 107 |
GEO | 2.17 × 10–3 | 4.01 × 10–10 |
1.67 × 10–2 |
6.82 × 106 |
Orbit Type | Onset LETEFF (MeV-cm2/mg) | CREME96 Integral FLUX (/day/cm2) | σSAT (cm2) | Event Rate (/day) | Event Rate (FIT) | MTBF (Years) |
---|---|---|---|---|---|---|
LEO (ISS) | 43 | 6.40 × 10–4 | 3.69 x 10–6 |
2.36× 10–9 |
9.84× 10–2 |
1.16 × 106 |
GEO | 2.17 × 10–3 |
8.01× 10–9 |
3.34 × 10–1 |
3.42 × 105 |