Computer Science – Performance
Scientific paper
Jul 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006spie.6267e..27e&link_type=abstract
Ground-based and Airborne Telescopes. Edited by Stepp, Larry M.. Proceedings of the SPIE, Volume 6267, pp. 62670U (2006).
Computer Science
Performance
2
Scientific paper
The 2.5 meter (m) effective diameter telescope on SOFIA - the Stratospheric Observatory for Infrared Astronomy - will operate in an open-port cavity which will be closed below operating altitudes by a cavity-door assembly. When operating, the telescope will view the sky through an aperture defined by an aperture assembly (AA) with a nearly rectangular opening extending 112 inches (2.84 m) in elevation (roll) and 129 inches (3.27 m) in cross-elevation. The aperture will be servo-controlled in roll to track the telescope elevation (EL), and the aircraft heading will be adjusted to maintain the telescope centered on the aperture in cross-elevation (XEL). An upper rigid door (URD) and lower flexible door (LFD) move with the aperture to minimize the opening into the cavity containing the telescope. This paper describes basic parameters of the door system, and estimates possible science impacts of its specification, configuration and planned operation. Topics included are the geometry, expected aerodynamic disturbances, control system, gear life, influences of radiative and diffraction effects on science instrument performance, testing, operational considerations, and development status. As designed, the door system is expected not to limit the performance of science instruments or observatory operational efficiency, but several potential concerns are considered. These include modulation of stray and diffracted radiation, reliability, and maintainability.
Brown Ted M.
Erickson Edwin F.
Haas Michael R.
Howe David A.
Perry John N.
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