Paper
29 July 2016 Performance of a cryogenic test facility for 4 K interferometer delay line investigations
Ian Veenendaal, David Naylor, Brad Gom, Sudhakar Gunuganti, Calvin Winter, Martyn Jones, David Walker
Author Affiliations +
Abstract
The next generation of space-borne instruments for far infrared astronomical spectroscopy will utilize large diameter, cryogenically cooled telescopes in order to achieve unprecedented sensitivities. Low background, ground-based cryogenic facilities are required for the cryogenic testing of materials, components and subsystems. The University of Lethbridge Test Facility Cryostat (TFC) is a large volume, closed cycle, 4 K cryogenic facility, developed for this purpose. This paper discusses the design and performance of the facility and associated metrology instrumentation, both internal and external to the TFC. Additionally, an apparatus for measuring the thermal and mechanical properties of carbon-fiber-reinforced polymers is presented.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Ian Veenendaal, David Naylor, Brad Gom, Sudhakar Gunuganti, Calvin Winter, Martyn Jones, and David Walker "Performance of a cryogenic test facility for 4 K interferometer delay line investigations", Proc. SPIE 9904, Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave, 99045E (29 July 2016); https://doi.org/10.1117/12.2233609
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CITATIONS
Cited by 4 scholarly publications.
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KEYWORDS
Cryogenics

Copper

Interferometers

Temperature metrology

Head

Mirrors

Space telescopes

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