Design of a convex and camera mirror support system for Altair, the Gemini-North adaptive optics system

被引:1
作者
Szeto, K [1 ]
Roberts, S [1 ]
Anthony, A [1 ]
Fitzsimmons, J [1 ]
Gaunt, R [1 ]
Sebesta, J [1 ]
Véran, JP [1 ]
机构
[1] Natl Res Council, Herzberg Inst Astrophys, Victoria, BC V8X 4M6, Canada
来源
OPTICAL AND IR TELESCOPE INSTRUMENTATION AND DETECTORS, PTS 1 AND 2 | 2000年 / 4008卷
关键词
flexure; mirror mount; mirror support; error budget; adaptive optics;
D O I
10.1117/12.395416
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Convex Camera Structure (CCS) is a welded Invar structure that supports of the final two optical elements in the Altair science path. The CCS assembly holds the large camera mirror, a 295 mm diameter off-axis conic, in close relation with the smaller convex mirror, a 146 mm diameter off-axis conic. The image quality requirement imposed stringent spatial tolerance between the two mirrors: +/-45 mu m in axial separation, +/-70 mu m in decentre and +/-30 arcsecond in allowable tilt. These tolerances include contributions from initial alignment error, geometrical and dimensional changes due to gravity and temperature. This paper gives an overview of the CCS and its associated components. Flexures are integral part of the CCS assembly, they are utilized to connect the CCS to the aluminum main optical bench, the mirror to the six degree-of-freedom (6DOF) mount, and the 6DOF mount to the CCS end plate. The design considerations and engineering analyses of the CCS assembly are outlined.
引用
收藏
页码:942 / 949
页数:8
相关论文
共 3 条
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*GEM AD OPT SYST, 1997, REV E APR
[2]  
Spyrakos C., 1994, FINITE ELEMENT MODEL
[3]  
VERAN JP, 1999, UNPUB J OPT SOC AM A