The Cassini Grand Finale capped the 20 year Cassini mission with 22 one-week-long orbits each with periapsis inside the ring plane just above Saturn’s cloud tops. One aspect of these remarkable orbits was unprecedented measurements of Saturn’s magnetic field very close to the planet. Processing this data required precise estimates of Cassini’s orientation during these ring plane crossings. These periods coincided with planned gyro-only attitude propagation due to the enormous bright bodies in the star tracker field-of-view. This paper describes how attitude reacquisition information, when the star tracker reacquires an absolute inertial reference, can be used to correct errors introduced during gyro-only propagation. The resulting high fidelity reconstruction significantly improves the extraction of Saturn’s magnetic field from the raw data obtained during gyro-only periods when Cassini’s changing orientation makes precise attitude estimation a challenge.
High Fidelity Reconstructed Attitude Estimation Using Cassini Flight Telemetry
AIAA Science and Technology Forum and Exposition (AIAA SciTech 2018) ; 2018 ; Kissimmee, FL, United States
2018-01-01
Aufsatz (Konferenz)
Keine Angabe
Englisch
High Fidelity Reconstructed Attitude Estimation Using Cassini Flight Telemetry (AIAA 2018-2113)
British Library Conference Proceedings | 2018
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