
Proceedings Paper
Predicted JWST imaging performanceFormat | Member Price | Non-Member Price |
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Paper Abstract
The James Webb Space Telescope optical telescope element mirror components, 18 individual primary mirror segment
assemblies (PMSA), the secondary mirror (SM), tertiary mirror (TM), and Fine Steering Mirror, have all been fabricated.
The performance of the optical telescope (OTE) based on the as-measured optical components is combined with
alignment tolerances and the on-orbit alignment process to predict the imaging performance of JWST. The best
estimate of the wavefront error, Strehl ratio and Encircled Energy stability is presented.
Paper Details
Date Published: 21 September 2012
PDF: 13 pages
Proc. SPIE 8442, Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave, 84422G (21 September 2012); doi: 10.1117/12.926817
Published in SPIE Proceedings Vol. 8442:
Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave
Mark C. Clampin; Giovanni G. Fazio; Howard A. MacEwen; Jacobus M. Oschmann Jr., Editor(s)
PDF: 13 pages
Proc. SPIE 8442, Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave, 84422G (21 September 2012); doi: 10.1117/12.926817
Show Author Affiliations
J. Scott Knight, Ball Aerospace & Technologies Corp. (United States)
Paul Lightsey, Ball Aerospace & Technologies Corp. (United States)
Paul Lightsey, Ball Aerospace & Technologies Corp. (United States)
Allison Barto, Ball Aerospace & Technologies Corp. (United States)
Published in SPIE Proceedings Vol. 8442:
Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave
Mark C. Clampin; Giovanni G. Fazio; Howard A. MacEwen; Jacobus M. Oschmann Jr., Editor(s)
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