Paper
12 July 2008 Architecting a revised optical test approach for JWST
Author Affiliations +
Abstract
It is imperative that we have high confidence that the optical performance capability of JWST is well-understood before launch. With the telescope operating at cryogenic temperatures and sporting a 6.6 meter primary mirror diameter, the optical metrology equipment required to measure the optical performance can be quite complex. The JWST Test team undertook an effort to greatly simplify the optical metrology approach, while retaining the key measurements and verification methodology. The result is a cryogenic optical test configuration and implementation using Chamber A at NASA's Johnson Space Center that uses the science instruments to help understand JWST's optical performance.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Charlie Atkinson, Jonathan Arenberg, Gary Matthews, Mark Waldman, Alan Wertheimer, Tony Whitman, and Jim Oschmann "Architecting a revised optical test approach for JWST", Proc. SPIE 7010, Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter, 70100Q (12 July 2008); https://doi.org/10.1117/12.788021
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Cited by 7 scholarly publications.
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KEYWORDS
Mirrors

Optical alignment

Adaptive optics

James Webb Space Telescope

Cryogenics

Optical testing

Metrology

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