Share Email Print

Proceedings Paper

Qualification and performances of a highly repeatable cryogenic actuator
Author(s): Jean Christophe Barrière; Olivier Corpace; Axel Arhancet; Damien Bachet; Michel Berthé; Michael Carty; Bruno Duboué; Luc Dumaye; Gilles-Alphonse Durand; Jean Fontignie; Philippe Galdemard; Mickael Lacroix; Yannick Le Noa; Jérôme Martignac; Marin Prieur
Format Member Price Non-Member Price
PDF $14.40 $18.00
cover GOOD NEWS! Your organization subscribes to the SPIE Digital Library. You may be able to download this paper for free. Check Access

Paper Abstract

The CEA Cryo-Mechanism (CM) was created to actuate infrared instruments wheels equipped with filters, coronographs or diffractive optics. Based on an optimized integration of basic industrial components, the CM operates with a high positioning repeatability (down to ±13 arcsec) in infrared astrophysical environment (very low temperatures and under vacuum). In 2004, for the first light of the mid-infrared imager/spectrometer VISIR, 12 CM units were produced. Among them, 10 units are operating once every hour since 13 years with a very high reliability.

From 2010, the CM was improved with the goal of space missions. Today, the CM reaches the status of a flight model mechanism already delivered for the EUCLID space mission (launch expected by 2021). It is also derived into a cost optimized actuator so called ICAR that will be manufactured in approximately 20 units for the ELT-METIS ground based instrument.

This paper gives an overview of the CM design and its different configurations. The paper will describe more in details the different tests that were carried out on the Euclid-CM, covering performances, vibrations, electromagnetism, thermal cycles, exported torques and life-time tests.

Paper Details

Date Published: 10 July 2018
PDF: 10 pages
Proc. SPIE 10706, Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation III, 107061B (10 July 2018); doi: 10.1117/12.2303381
Show Author Affiliations
Jean Christophe Barrière, CEA-Paris-Saclay, IRFU-DIS (France)
Olivier Corpace, CEA-Paris-Saclay, IRFU-DIS (France)
Axel Arhancet, CEA-Paris-Saclay, IRFU-DIS (France)
Damien Bachet, CEA-Paris-Saclay, IRFU-DIS (France)
Michel Berthé, CEA-Paris-Saclay, IRFU-DAp (France)
Michael Carty, CEA-Paris-Saclay, IRFU-DIS (France)
Bruno Duboué, CEA-Paris-Saclay, IRFU-DIS (France)
Luc Dumaye, CEA-Paris-Saclay, IRFU-DAp (France)
Gilles-Alphonse Durand, CEA-Paris-Saclay, IRFU-DAp (France)
Jean Fontignie, CEA-Paris-Saclay, IRFU-DAp (France)
Philippe Galdemard, CEA-Paris-Saclay, IRFU-DIS (France)
Mickael Lacroix, CEA-Paris-Saclay, IRFU-DIS (France)
Yannick Le Noa, CEA-Paris-Saclay, IRFU-DIS (France)
Jérôme Martignac, CEA-Paris-Saclay, IRFU-DAp (France)
Marin Prieur, CEA-Paris-Saclay, IRFU-DAp (France)

Published in SPIE Proceedings Vol. 10706:
Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation III
Ramón Navarro; Roland Geyl, Editor(s)

© SPIE. Terms of Use
Back to Top