Paper
7 September 2010 The Wide-field Infrared Survey Explorer (WISE) beamsplitter assembly
R. W. Esplin, D. O. Miles, D. K. McLain, H. M. Latvakoski, M. F. Larsen, M. Kahan, J. D. Elwell
Author Affiliations +
Abstract
The design, fabrication and testing of the BeamSplitter Assembly (BSA) of the Wide-field Infrared Survey Explorer (WISE) instrument are discussed in the paper. The BSA splits the WISE telescope optical output beam into 4 spectral wavelength bands: 2.8-3.8, 4.1-5.2, 7.5-16.5, and 20-26 μm. The BSA also provides focus adjustments to focus the WISE instrument prior to launch. The methods used to focus WISE are also discussed in this paper. Funding for and management of the WISE program were provided by the NASA Jet Propulsion Laboratory.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
R. W. Esplin, D. O. Miles, D. K. McLain, H. M. Latvakoski, M. F. Larsen, M. Kahan, and J. D. Elwell "The Wide-field Infrared Survey Explorer (WISE) beamsplitter assembly", Proc. SPIE 7796, An Optical Believe It or Not: Key Lessons Learned II, 77960B (7 September 2010); https://doi.org/10.1117/12.864349
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KEYWORDS
Beam splitters

Staring arrays

Telescopes

Infrared radiation

Solids

Collimators

Detector arrays

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