REG NASA-LLIS-0310--1994 Lessons Learned Mars Observer Inertial Reference Loss.pdf
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1、Lessons Learned Entry: 0310Lesson Info:a71 Lesson Number: 0310a71 Lesson Date: 1994-03-03a71 Submitting Organization: JPLa71 Submitted by: G. T. Chien / J. O. BlosiuSubject: Mars Observer Inertial Reference Loss Abstract: Mars Observer experienced inertial reference loss on several occasions during
2、its cruise to Mars. These incidents were due to the lack of a detailed code walk-through, and to use of gyro noise values, obtained from in-house test, that were more optimistic than the manufacturers specifications. Do not depend on hardware performance being better than the manufacturers specifica
3、tion. Perform detailed code walk-through of critical software modules. Pay special attention to inherited critical software. Design the flight computer and software to permit necessary changes in flight.Description of Driving Event: Mars Observer experienced inertial reference loss on several occasi
4、ons during its cruise to Mars. Two classes of inertial reference loss have been observed:A. In early January 1993, the flight software was unable to identify any star that transited the celestial sensor assembly field of view. The unidentified stars count exceeded the “loss logic limit,“ and the fau
5、lt protection software commanded the spacecraft to the sun coning attitude contingency mode. This occurred three times before a temporary software script to widen the star identification tolerance was uplinked in order to artificially increase the attitude uncertainties, or covariances, used by the
6、software. Design flexibility of the fight computer and software allowed the software patch to be easily performed. It was suspected that the cause was due to the use of the more optimistic gyro noise parameters and values obtained from the in-house test results rather than the manufacturers specific
7、ations. Recovery time: 3 days per occurrence.B. During April and May 1993, three more incidents caused the spacecraft to declare inertial reference loss when the “sun monitor ephemeris“ test, which compares the expected new position with the measured positions, was violated. An algorithm error in th
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