Poster + Paper
11 September 2024 Refrigerant cooling services for the Thirty Meter Telescope
John W. Miles, Brent Ellerbroek, Jamie Dodge, Hugh Thompson, Adam Densmore, Calvin Winter, Ian Welle
Author Affiliations +
Conference Poster
Abstract
The Thirty Meter Telescope (TMT) must remove waste heat generated by electronics on the telescope to prevent overheating and reduce their impact on dome seeing. Traditionally, chilled water-glycol cooling loops have been used for this purpose. However, the potential (and realization on existing telescopes) for damage and disruption due to glycol leaks at the telescope top end has prompted a shift to a refrigerant system, where any leaking refrigerant vaporizes immediately. Additionally, a refrigerant system is needed to cool adaptive optics enclosures to -30°C and cool the telescope hydrostatic bearing oil to -21°C, below the operating range of a chilled water system. This paper discusses the refrigerant services infrastructure in development for the observatory, including the cooling requirements, the trade study that led to the choice of carbon dioxide as the refrigerant, the conceptual design, and the concept of operations.
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
John W. Miles, Brent Ellerbroek, Jamie Dodge, Hugh Thompson, Adam Densmore, Calvin Winter, and Ian Welle "Refrigerant cooling services for the Thirty Meter Telescope", Proc. SPIE 13094, Ground-based and Airborne Telescopes X, 130945O (11 September 2024); https://doi.org/10.1117/12.3016313
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KEYWORDS
Liquids

Telescopes

Thirty Meter Telescope

Water

Carbon dioxide

Observatories

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