Paper
15 July 2008 Technology development for nickel x-ray optics enhancement
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Abstract
We are developing grazing-incidence x-ray optics for high-energy astrophysics using an electroform-nickel process in which mirror shells are formed by replication off super-polished cylindrical mandrels. The optics so fabricated have a demonstrated performance at the level of 11-12 arc seconds resolution (HPD) for 30 keV x rays. Future missions, however, demand ever higher angular resolutions and this places stringent requirements on all aspects of the process -- the mandrels, the shell fabrication, and the mounting and alignment of the resulting mirrors in their housings. A progress report on recent technology developments in these areas is given, including a discussion on possible post fabrication improvements in the x-ray mirrors' quality.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Mikhail Gubarev, Brian Ramsey, Darell Engelhaupt, and William Arnold "Technology development for nickel x-ray optics enhancement", Proc. SPIE 7011, Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray, 701133 (15 July 2008); https://doi.org/10.1117/12.789190
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Cited by 4 scholarly publications.
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KEYWORDS
Mirrors

Polishing

Surface finishing

X-ray optics

Nickel

Sensors

Tolerancing

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