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          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



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ID: 421773.0, MPI für Astronomie / Publikationen_mpia
Development approach and first infrared test results of JWST/Mid Infra Red Imager Optical Bench
Authors:Amiaux, J.; Alouadi, F.; Augueres, J. L.; Bouchet, P.; Bouzat, M.; Cavarroc, C.; Cloue, C.; De Antoni, P.; Desforges, D.; Donati, A.; Dubreuil, D.; Eppelle, D.; Gougnaud, F.; Hervieu, B.; Lagage, P. O.; Leboeuf, D.; Le Mer, I.; Lussignol, Y.; Mattei, P.; Meigner, F.; Moreau, V.; Pantin, E.; Perrin, P.; Ronayette, S.; Tauzin, G.; Poupar, S.; Wright, D.; Glasse, A.; Wright, G.; Mazy, E.; Plesseria, J. Y.; Renotte, E.; Ray, T.; Abergel, A.; Guillard, P.; Longval, Y.; Ressler, M.; Reess, J. M.; Hofferbert, R.; Krause, O.; Justtanont, K.; Olofsson, G.
Language:English
Publisher:SPIE
Date of Publication (YYYY-MM-DD):2008
Title of Proceedings:Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter
Start Page:70100U-70100U
End Page:12
Title of Series:SPIE
Volume (in Series):7010
Review Status:not specified
Audience:Experts Only
Abstract / Description:The present paper describes the different steps leading to the Flight Model integration of the Mid-Infra Red IMager Optical Bench MIRIM-OB which is part of the scientific payload of the JWST. In order to demonstrate a space instrument capability to survive the challenging space environment and deliver the expected scientific data, a specific development approach is applied in order to reduce the high level of risks. The global approach for MIRIM-OB, and the principal results associated to the two main models, the Structural Qualification Model for vibration and the Engineering and Test Model for optical performance measured in the infra red at cryogenic temperature will be described in this paper.
Comment of the Author/Creator:Date: 2008, August 1, 2008
External Publication Status:published
Document Type:Conference-Paper
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:URL:http://adsabs.harvard.edu/abs/2008SPIE.7010E..28A [ID No:1]
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