Structural, thermal, and optical performance (STOP) modeling and results for the James Webb Space Telescope integrated science instrument module
Author(s) -
Renee Gracey,
Andrew Bartoszyk,
Emmanuel Cofie,
Brian Comber,
G. Hartig,
Joseph Howard,
Derek Sabatke,
Greg Wenzel,
Raymond G. Ohl
Publication year - 2016
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 - 10.1117/12.2233641
Subject(s) - james webb space telescope , telescope , computer science , space (punctuation) , optics , spitzer space telescope , thermal , orbital mechanics , aerospace engineering , physics , astronomy , satellite , engineering , meteorology , operating system
The James Webb Space Telescope includes the Integrated Science Instrument Module (ISIM) element that contains four science instruments (SI) including a Guider. We performed extensive structural, thermal, and optical performance (STOP) modeling in support of all phases of ISIM development. In this paper, we focus on modeling and results associated with test and verification. ISIM’s test program is bound by ground environments, mostly notably the 1g and test chamber thermal environments. This paper describes STOP modeling used to predict ISIM system performance in 0g and at various on-orbit temperature environments. The predictions are used to project results obtained during testing to on-orbit performance.
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