Presentation + Paper
29 August 2022 Manufacturing and integration status of the UH2.2 adaptive secondary mirror
Wouter Jonker, Stefan Kuiper, Fred Kamphues, Arjo Bos, Bert Dekker, Mark Chun, André Benschop, Hans Priem, Bert Monna, Manav Nair, Taavishe Gupta, Gilles Ackaert, Suman Bola, Loannis Varvaringos, Julian Schroth
Author Affiliations +
Abstract
A consortium of industrial and academic partners, coordinated by TNO, is working on the realization of a 620mm adaptive secondary mirror (ASM) for the University of Hawaii’s 2.2-meter telescope [1][2][3]. The ASM consists of a 620mm-diameter slumped convex aspherical mirror shell, manipulated by 210 variable-reluctance actuators mounted on a light-weighted support frame. The mirror shell is manufactured to the required accuracy at low cost through slumping. The actuators are driven by dedicated PWM current drivers and commanded through a real-time FPGA-based interface. After successful performance testing of several laboratory prototypes[4], this project will provide the definitive on-sky demonstration of this new technology. We report on the manufacturing and testing of the major subsystems, and on the integration status of the ASM as a whole.
Conference Presentation
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Wouter Jonker, Stefan Kuiper, Fred Kamphues, Arjo Bos, Bert Dekker, Mark Chun, André Benschop, Hans Priem, Bert Monna, Manav Nair, Taavishe Gupta, Gilles Ackaert, Suman Bola, Loannis Varvaringos, and Julian Schroth "Manufacturing and integration status of the UH2.2 adaptive secondary mirror", Proc. SPIE 12188, Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation V, 1218816 (29 August 2022); https://doi.org/10.1117/12.2629254
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KEYWORDS
Actuators

Manufacturing

Electronics

Mirrors

Amplifiers

Telescopes

Field programmable gate arrays

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