Paper
9 August 1988 X-Ray Mirror Assessment With Optical Light
Hideyo Kunieda, Peter J. Serlemitsos
Author Affiliations +
Abstract
The imaging capability of a thin foil x-ray mirror has been examined with optical light, using a laser beam and a wide optical parallel beam. These measurements reveal that (1) image broadening due to millimeter scale waviness (orange peel) of the aluminum substrate, partly intrinsic to the foil and partly caused during the foil treatment, is 1.2-min of arc half-power diameter (HPD) in two reflections; (2) slope errors due to foil shaping and misalignment cause broadening of 1.6-2.0-min of arc HPD; (3) total broadening is ~3-min of arc HPD, which is consistent with the broadening of 2.6-min of arc HPD measured with x rays.
© (1988) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Hideyo Kunieda and Peter J. Serlemitsos "X-Ray Mirror Assessment With Optical Light", Proc. SPIE 0830, Grazing Incidence Optics for Astronomical and Laboratory Applications, (9 August 1988); https://doi.org/10.1117/12.942155
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Cited by 1 scholarly publication.
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KEYWORDS
Mirrors

X-rays

X-ray optics

Aluminum

Astronomical imaging

Diffraction

Grazing incidence

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