Paper
2 August 2014 New method for characterizing the state of optical and opto-mechanical systems
Babak Saif, Ritva Keski-Kuha, Lee Feinberg, David Chaney, Marcel Bluth, Perry Greenfield, Warren Hack, Scott Smith, James Sanders
Author Affiliations +
Abstract
James Webb Space Telescope Optical Telescope Element (OTE) is a three mirror anastigmat consisting of a 6.5 m primary mirror (PM), a secondary mirror (SM) and a tertiary mirror. The primary mirror is made out of 18 segments. The telescope and instruments will be assembled at Goddard Space Flight Center (GSFC) to build the Optical Telescope Element-Integrated Science Instrument Module (OTIS). The OTIS will go through environmental testing at GSFC before being transported to Johnson Space Center for testing at cryogenic temperature. The objective of the primary mirror Center of Curvature test (CoC) is to characterize the PM before and after the environmental testing for workmanship. This paper discusses the CoC test including both a surface figure test and a new method for characterizing the state of the primary mirror using high speed dynamics interferometry.
© (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Babak Saif, Ritva Keski-Kuha, Lee Feinberg, David Chaney, Marcel Bluth, Perry Greenfield, Warren Hack, Scott Smith, and James Sanders "New method for characterizing the state of optical and opto-mechanical systems", Proc. SPIE 9143, Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave, 91430C (2 August 2014); https://doi.org/10.1117/12.2055243
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KEYWORDS
Mirrors

Space telescopes

Computer generated holography

James Webb Space Telescope

Telescopes

Interferometers

Monochromatic aberrations

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