Optical performance of an infrared astronomical telescope with a 5-axis secondary mirror

Eli Ettedgui-Atad; Colin M. Humphries

doi:10.1117/12.48269

1 December 1991 Optical performance of an infrared astronomical telescope with a 5-axis secondary mirror

Eli Ettedgui-Atad, Colin M. Humphries

Author Affiliations +

Proceedings Volume 1532, Analysis of Optical Structures; (1991) https://doi.org/10.1117/12.48269
Event: San Diego, '91, 1991, San Diego, CA, United States

Abstract

The optical characteristics of a 5-axis secondary mirror are discussed, stressing the infrared sky chopping and adaptive tip/tilt control capabilities. Sources of image degradation such as misalignments and manufacturing errors are considered. Different modes of operation for active, chopping, and adaptive control are described and examples of the required speed, range, and precision of these modes are presented.

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Eli Ettedgui-Atad and Colin M. Humphries "Optical performance of an infrared astronomical telescope with a 5-axis secondary mirror", Proc. SPIE 1532, Analysis of Optical Structures, (1 December 1991); https://doi.org/10.1117/12.48269

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