REG NASA-LLIS-1778-2007 Lessons Learned - Anomalous Flight Conditions May Trigger Common-Mode Failures in Highly Redundant Systems.pdf
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1、Lessons Learned Entry: 1778Lesson Info:a71 Lesson Number: 1778a71 Lesson Date: 2007-03-6a71 Submitting Organization: JPLa71 Submitted by: Martin Ratliffa71 POC Name: John Waters, Henry Stonea71 POC Email: John.J.Watersjpl.nasa.gov, Henry.W.Stonejpl.nasa.gova71 POC Phone: 818-354-1709 (John Waters),
2、818-354-9051 (Henry Stone)Subject: Anomalous Flight Conditions May Trigger Common-Mode Failures in Highly Redundant Systems Abstract: After launch, MRO was found to be susceptible to a solar flare event during the critical aerobraking phase of the mission that could corrupt the multiply redundant id
3、entical file systems in the Command if that image is also found to be corrupted, the spacecraft switches to the redundant string CMIC in search of a pristine FS image. Figure 1 is a color diagram that illustrates the architecture described in the Figure 1 caption by means of a block diagram. It show
4、s 2 major blocks positioned side by side and connected by a line labeled Figure 1. Each MRO C&DH string has a single CMIC, which in turn has a single 2 MB SRAM piece part that is logically partitioned into 8 segments. The redundant File Systems are stored in SRAM Segments 2 and 4 on each CMIC. Realt
5、ime checkpoint and fault protection data are stored in Segments 3 and 6. The RAD750 flight computer accesses its CMIC via a cPCI bus and accesses the other computers CMIC via a synchronous serial interface (SSI) cable. After MRO launch, spacecraft telemetry revealed some correctable CMIC memory erro
6、rs (Reference (1) that prompted analysis of MRO radiation exposure. This post-launch analysis identified a significant risk that solar energetic particle (SEP) events associated with a solar flare later in the mission could corrupt all four FS images (Reference (2). That is, given the high likelihoo
7、d under nominal conditions of particle strikes causing SEUs in a certain block of memory, there is a high likelihood during large solar flares of many more strikes damaging multiple blocks of memory. Since the radiation flux would also increase the likelihood of a computer reboot, FS corruption duri
8、ng the Mars aerobraking maneuver could have posed an unacceptable risk to the mission. Radiation analysis (Reference (3) also revealed a 7 percent probability that a large flare will occur and that the resulting SEUs will impact all four FS data images during the 2-year MRO primary mission. In addit
9、ion, the analysis showed a 14 percent probability of data corruption (due to entry into a period of increased solar activity) during an extended mission. This analysis showed that for large solar flares, the probability of SEUs is so high that even an increase in redundancy to 16 FSs Provided by IHS
10、Not for ResaleNo reproduction or networking permitted without license from IHS-,-,-would not bring a significant risk reduction during the primary mission. This is because the probability of all images being corrupted is driven mainly by the probability of encountering a large flare. Shielding is so
11、mewhat effective against solar protons, and the proton flux decreases with distance from the sun, but shielding does little to block high energy particles, and they pose an SEU risk throughout a planetary mission. The MRO mission risk has been mitigated by uplinked changes to flight software, and by
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