Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/32276
Title: Space-compatible strain gauges as an integration aid for the James Webb Space Telescope Mid-Infrared Instrument
Authors: Samara-Ratna, Piyal
Sykes, Jon
Bicknell, Chris
Pye, John
Jessen, N. C.
Nøgaard-Nielsen, H. U.
First Published: 17-Dec-2014
Publisher: SAGE Publications (UK and US), Professional Engineering Publishing (Institution of Mechanical Engineers)
Citation: The Journal of Strain Analysis for Engineering February 2015 vol. 50 no. 2 92-102
Abstract: Space instruments are designed to be highly optimised, mass efficient hardware required to operate in extreme environments. Building and testing is extremely costly, and damage that appears to have no impact on performance at normal ambient conditions can have disastrous implications when in operation. The Mid-Infrared Instrument is one of four instruments to be used on the James Webb Space Telescope which is due for launch in 2018. This telescope will be successor to the Hubble Space Telescope and is the largest space-based astronomy project ever to be conceived. Critical to operation of the Mid-Infrared Instrument is its primary structure, which provides both a stable platform and thermal isolation for the scientific instruments. The primary structure contains strain-absorbing flexures and this article summarises how these have been instrumented with a novel strain gauge system designed to protect the structure from damage. Compatible with space flight requirements, the gauges have been used in both ambient and cryogenic environments and were successfully used to support various tasks including integration to the spacecraft. The article also discusses limitations to using the strain gauge instrumentation and other implications that should be considered if such a system is to be used for similar applications in future.
DOI Link: 10.1177/0309324714558149
ISSN: 0309-3247
eISSN: 2041-3130
Links: http://sdj.sagepub.com/content/50/2/92
http://hdl.handle.net/2381/32276
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: This article is distributed under the terms of the Creative Commons Attribution 3.0 License (http://www.creativecommons.org/licenses/by/3.0/) which permits any use, reproduction and distribution of the work without further permission provided the original work is attributed as specified on the SAGE and Open Access page (http://www.uk.sagepub.com/aboutus/openaccess.htm).
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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