Active Damping of the SOFIA Telescope Assembly

被引:6
|
作者
Keas, Paul J. [1 ]
Dunham, Edward [1 ]
Lampater, Ulrich [1 ]
Pfueller, Enrico [1 ]
Teufel, Stefan [1 ]
Roeser, Hans-Peter [1 ]
Wiedemann, Manuel [1 ]
Wolf, Juergen [1 ]
机构
[1] Moog CSA Engn, 2565 Leghorn St, Mountain View, CA 94043 USA
来源
GROUND-BASED AND AIRBORNE TELESCOPES IV | 2012年 / 8444卷
基金
美国国家航空航天局;
关键词
SOFIA; Active Damping; Reaction Mass Actuator; Modal Coordinates; Vibration Control; Jitter Control; Airborne Astronomy; Image Stability;
D O I
10.1117/12.924791
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The NASA/DLR Stratospheric Observatory for Infrared Astronomy (SOFIA) employs a 2.5-meter reflector telescope in a Boeing 747SP. The telescope is housed in an open cavity and is subjected to aeroacoustic and inertial disturbances in flight. To meet pointing requirements, SOFIA must achieve a pointing stability of approximately 0.5 arcseconds RMS. An active damping control system is being developed for SOFIA to reduce image jitter and image degradation due to resonance of the telescope assembly. Our paper discusses the history of the active damping design for SOFIA, from early concepts to the current implementation which has recently completed a ground and flight testing for proof-of-concept. We describe some milestones in the analysis and testing of the telescope assembly which guided the development of the vibration control system. The control synthesis approach and current implementation of the active damping control system is presented. Finally, we summarize the performance observed in early flight tests and the steps that are currently foreseen to completing the development of this system.
引用
收藏
页数:15
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