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6 October 2011 Development of a EUV test facility at the Marshall Space Flight Center
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Abstract
This paper will describe a new Extreme Ultraviolet (EUV) test facility that is being developed at the Marshall Space Flight Center (MSFC) to test EUV telescopes. Two flight programs, Hi-C, the high resolution coronal imager (a sounding rocket program), and SUVI, the Solar Ultraviolet Imager (GOES-R), set the requirements for this new facility. This paper will discuss those requirements, the EUV source characteristics, the wavelength resolution that is expected and the vacuum chambers (Stray Light Facility, Xray Calibration Facility and the NSSTC EUV test chamber) where this facility will be used.
© (2011) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Edward West, Steve Pavelitz, Ken Kobayashi, Brian Robinson, Jonathan Cirtain, Jessica Gaskin, Amy Winebarger, Linda Krause, Michael McGuirk, and Jonathan Darnel "Development of a EUV test facility at the Marshall Space Flight Center", Proc. SPIE 8147, Optics for EUV, X-Ray, and Gamma-Ray Astronomy V, 81471A (6 October 2011); https://doi.org/10.1117/12.904922
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