SBOK085 April 2024 SN54SC2T74-SEP
PRODUCTION DATA
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 shown in Heavy Ion Orbital Environment Single-Event Effects Estimations. A minimum shielding configuration of 100mils (2.54mm) of aluminum, and worst-week solar activity is assumed. (This is similar to a 99% upper bound for the environment.) Using the 95% upper-bounds for the SEL and the SET, the event rate calculation for the SEL and the SET is listed in Table 5-3 and Table 5-4, respectively. Note that this number is for reference since no SEL or SET events were observed.
Orbit Type | Onset LETEFF (MeV-cm2 / mg) | CREME96 Integral FLUX ( per day / cm2) | σSAT (cm2) | Event Rate (per day) | Event Rate (FIT) | MTBE (Years) |
---|---|---|---|---|---|---|
LEO (ISS) | 48 | 6.40 × 10-4 | 1.23 × 10-7 | 7.87 × 10-11 | 3.28 × 10-3 | 3.48 × 107 |
GEO | 2.17 × 10-3 | 2.67 × 10-10 | 1.11 × 10-2 | 1.03 × 107 |
Orbit Type | Onset LETEFF (MeV-cm2 / mg) | CREME96 Integral FLUX (per day / cm2) | σSAT (cm2) | Event Rate (per day) | Event Rate (FIT) | MTBE (Years) |
---|---|---|---|---|---|---|
LEO (ISS) | 48 | 6.40 × 10-4 | 1.94 × 10–8 | 1.24 × 10–11 | 5.16 × 10–4 | 2.21 × 108 |
GEO | 2.17 × 10-3 | 4.20 × 10–11 | 1.75 × 10–3 | 6.52 × 107 |
MTBE is the mean-time-between-events in years at the given event rates. These rates clearly demonstrate the SEE robustness of the SN54SC2T74-SEP in two harshly conservative space environments. Customers using the SN54SC2T74-SEP must only use the above estimations as a rough guide and TI recommends performing event rate calculations based on specific mission orbital and shielding parameters to determine if the product satisfies the reliability requirements for the specific mission.