PERSONAL Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.
The telescope structure of the Stratospheric Observatory for Infrared Astronomy (SOFIA) was subject to vibration excitation due to aircraft motions and airflow. To contribute to the efforts to meet pointing requirements and improve image stability, an active mass damping system for the primary mirror suspension has been designed and implemented during the early years of observatory operation phase. Various reasons had prevented further development for some time, but we were able to reactivate and operate the damping system for a set of selected missions before the premature decommissioning of the observatory. We present analyses from gathered engineering data and from astronomical observations about the effectiveness of the system during those missions and offer a projection on how future SOFIA campaigns would have benefited.
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
PERSONAL Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.
The alert did not successfully save. Please try again later.
Benjamin Greiner, Sonja Hofmann, Jörg F. Wagner, "SOFIA performance improvements through active mass damping," Proc. SPIE 13094, Ground-based and Airborne Telescopes X, 1309444 (11 September 2024); https://doi.org/10.1117/12.3019062