Cryogenic thermal distortion performance characterization for the JWST ISIM structure
Author(s) -
John D. Johnston,
Emmanuel Cofie,
Jason E. Hylan,
Raymond G. Ohl,
Maria Nowak,
Douglas B. McGuffey,
James Pontius,
Eric L. Johnson
Publication year - 2011
Publication title -
proceedings of spie, the international society for optical engineering/proceedings of spie
Language(s) - English
Resource type - Conference proceedings
SCImago Journal Rank - 0.192
H-Index - 176
eISSN - 1996-756X
pISSN - 0277-786X
DOI - 10.1117/12.893932
Subject(s) - james webb space telescope , metrology , distortion (music) , thermal , aerospace engineering , computer science , cryogenics , remote sensing , optics , environmental science , telescope , physics , meteorology , optoelectronics , amplifier , engineering , cmos , quantum mechanics , geology
The James Webb Space Telescope (JWST) Integrated Science Instrument Module (ISIM) Structure is a precision optical metering structure for the JWST science instruments. Optomechanical performance requirements place stringent limits on the allowable thermal distortion of the metering structure between ambient and cryogenic operating temperature (~35 K). This paper focuses on thermal distortion testing and successful verification of performance requirements for the flight ISIM Structure. The ISIM Structure Cryoset Test was completed in Spring 2010 at NASA Goddard Space Flight Center in the Space Environment Simulator Chamber. During the test, the ISIM Structure was thermal cycled twice between ambient and cryogenic (~35 K) temperatures. Photogrammetry was used to measure the Structure in the ambient and cryogenic states for each cycle to assess both cooldown thermal distortion and repeatability. This paper will provide details on the post-processing of the metrology datasets completed to compare measurements with performance requirements.
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