Poster + Paper
29 August 2022 In-lab calibration and testing of adaptive secondary mirrors using phase measuring deflectometry
Author Affiliations +
Conference Poster
Abstract
An adaptive secondary mirror (ASM) with novel actuator technology is being designed and built for the UH88 telescope as a demonstration of a new generation of ASMs that might be deployed at ground based observatories such as Keck, Subaru, and TMT. Before putting the ASM on the telescope, a set of calibrations and characterizations need to be made in the lab. The crucial lab characterizations of the ASM are to measure its influence functions, and its surface shape when powered and unpowered. To measure these, we develop a novel and inexpensive optical metrology approach using phase measuring deflectometry. This paper describes the simulations we wrote to model the deflectometry method, our data acquisition/analysis pipeline, and a lab prototype system we built that demonstrates its feasibility on a microelectromechanical systems (MEMS) deformable mirror. Based on the information gained through the deflectometry simulation and the setup prototype, we conclude that phase measuring deflectometry is a reasonable method for obtaining the influence functions but that the absolute surface shape of the ASM will be limited by our knowledge of the placement of components within the deflectometry setup itself. We discuss challenges with extending this approach to larger convex adaptive secondary mirrors.
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Ruihan Zhang and Mark R. Chun "In-lab calibration and testing of adaptive secondary mirrors using phase measuring deflectometry", Proc. SPIE 12185, Adaptive Optics Systems VIII, 1218569 (29 August 2022); https://doi.org/10.1117/12.2627278
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Mirrors

Cameras

Deflectometry

Actuators

Prototyping

Wavefronts

Fringe analysis

RELATED CONTENT

Performance of ChAOS on the Apache Point Observatory's 3.5 m...
Proceedings of SPIE (September 11 1998)
First light of the 6.5-m MMT adaptive optics system
Proceedings of SPIE (December 24 2003)
The GTC project: preparing the first light
Proceedings of SPIE (June 23 2006)
The Giant Magellan Telescope phasing system
Proceedings of SPIE (September 13 2012)
Real time open loop control of a 1024 actuator MEMS...
Proceedings of SPIE (July 14 2010)

Back to Top