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Mid Infrared Instrument (MIRI) cooler subsystem prototype demonstration

Mid Infrared Instrument (MIRI) cooler subsystem prototype demonstration

Publication date: 16 March 2008

Authors: Durand, D. et al.

Journal: AIP Conference Proceedings
Volume: 985

Copyright: American Institute of Physics

In "Advances in Cryogenic Engineering: Transactions of the Cryogenic Engineering Conference - CEC, Vol. 53", edited by J. G. Weisend et al., AIP Conf. Proc. Volume 985, pp. 807-814, 2008, doi:10.1063/1.2908674

The Cooler Subsystem for the Mid InfRared Instrument (MIRI) of the James Webb Space Telescope (JWST) features a 6 Kelvin Joule-Thomson (JT) cooler pre-cooled by a three-stage Pulse Tube (PT) cryocooler to provide 65 mW of cooling at the instrument. MIRI's 6 Kelvin cooling load, directly behind the primary mirror of JWST, is remote from the location of the compressors and pre-cooler. This distance, and the parasitic heat load on the refrigerant lines spanning it, is accommodated by the design. The effort during 2006 and the first part of 2007 has focused on the demonstration of a MIRI Cooler prototype in the relevant environment, required to achieve Technology Readiness Level 6 (TRL 6) as defined by NASA. The tests that have been used to successfully demonstrate TRL 6: launch vibration and cooler performance in the relevant thermal-vacuum environment, will be discussed.

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Last Update: Sep 1, 2019 9:01:47 AM
19-Sep-2020 03:41 UT

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