1 August 1990 Test facility for astronomical x-ray optics
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Optical Engineering, 29(8), (1990). doi:10.1117/12.55680
Abstract
Grazing incidence x-ray optics for x-ray astronomical applications are used outside the earth's atmosphere. These devices require a large collection aperture and the imaging of an x-ray source that is essentially placed at infinity. The ideal testing system for these optical elements has to approximate that encountered under working conditions; however, the testing of these optical elements is notoriously difficult with conventional x-ray generators. Synchrotron radiation (SR) sources are sufficiently brilliant to produce a nearly perfect parallel beam over a large area while still retaining a flux considerably higher than that available from conventional x-ray generators. A facility designed for the testing of x-ray optics, particularly in connection with x-ray telescopes, is described. It is proposed that this facility will be accommodated at the Synchrotron Radiation Source at the Daresbury Laboratory in the United Kingdom.
Robert A. Lewis, J. Bordas, Finn Erland Christensen, "Test facility for astronomical x-ray optics," Optical Engineering 29(8), (1 August 1990). http://dx.doi.org/10.1117/12.55680
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KEYWORDS
X-ray optics

X-rays

Synchrotron radiation

Sensors

Astronomy

Optical testing

Optical components

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