Other
Scientific paper
Sep 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985esasp.239..221c&link_type=abstract
In ESA Proceedings of ESA Workshop on a Cosmic X-Ray Spectroscopy Mission p 221-228 (SEE N86-22461 12-89)
Other
Mirrors, Spectrometers, X Ray Scattering, X Ray Telescopes, Gold Coatings, Quality Control, Surface Roughness Effects, Thin Films
Scientific paper
In developing a high throughput X-ray telescope for XMM, various techniques were employed to deposit a thin film of Au on a smooth substrate. A triple axis X-ray spectrometer was employed to measure the reflectivity and surface scattering of the gold surface or the substrates. For comparison, the same kind of measurements were performed on a high quality Au-coated test flat for EXOSAT and a Pt-coated test flat for AXAF. In the triple axis spectrometer a perfect channel cut Si crystal extracts Fe K radiation from a conventional X-ray tube. The X-rays are incident on the thin film surface at grazing angles and the specularly reflected and scattered radiation from the thin film is analyzed by another perfect Si crystal. A tailless probe of the scattered X-rays is obtained when the X-rays are reflected several times through a channel in each of the perfect Si crystals. It is demonstrated that the technique provides an excellent and detailed test of the quality of the mirror surface.
Christensen Finn E.
Jensen Peter L.
Schnopper Herbert W.
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