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Proceedings Paper

Surface scatter effects in grazing incidence x-ray telescopes
Author(s): James E. Harvey; Patrick L. Thompson; Cynthia L. Vernold
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Paper Abstract

Non-intuitive surface scatter effects resulting from practical optical fabrication tolerances frequently dominate both diffraction effects and geometrical aberrations in high resolution grazing incidence x-ray telescopes. The resulting reduction optical performance due to scattering is a strong function of x-ray energy, residual surface characteristics, incident angle, and the optical performance criterion appropriate to the application. A simple Fourier treatment of surface scatter phenomena, based upon a non-paraxial scalar diffraction theory, is referenced and utilized to produce parametric performance predictions that provide physical insight and understanding into the surface scatter phenomenon and its effect upon image quality. The optical prescription for the Solar X-ray Imager will be used as an example.

Paper Details

Date Published: 19 November 1998
PDF: 8 pages
Proc. SPIE 3444, X-Ray Optics, Instruments, and Missions, (19 November 1998); doi: 10.1117/12.331272
Show Author Affiliations
James E. Harvey, CREOL/Univ. of Central Florida (United States)
Patrick L. Thompson, CREOL/Univ. of Central Florida (United States)
Cynthia L. Vernold, CREOL/Univ. of Central Florida (United States)

Published in SPIE Proceedings Vol. 3444:
X-Ray Optics, Instruments, and Missions
Richard B. Hoover; Arthur B. C. Walker II, Editor(s)

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