Paper
31 October 1996 Status of the x-ray mirror production for the ESA XMM spacecraft
Daniel de Chambure, Robert Laine, Kees van Katwijk, Jan F. M. van Casteren, P. Glaude
Author Affiliations +
Abstract
The high throughput x-ray spectroscopy mission XMM is 'cornerstone' project in the ESA Long Term Programme for Space Science. This observatory has at its heart three heavily nested Wolter 1 grazing incidence x-ray telescopes which will provide a large collecting area (1,600 cm2 each at 1.5 keV). This optical system has a spatial resolution of 2 - 30 arcsec and when coupled with reflection grating spectrometers and x-ray CCD cameras, it will provide a major advance in astrophysics by the end of the century. In this paper, we first present the design of the telescope and then describe the manufacturing and the integration processes of the telescope with the emphasis on the production of the x-ray mirrors. We then concentrate on the technical problems and the solutions found for the production of these mirrors. Last but not least, the results achieved on the qualification model of the XMM telescope are also presented.
© (1996) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Daniel de Chambure, Robert Laine, Kees van Katwijk, Jan F. M. van Casteren, and P. Glaude "Status of the x-ray mirror production for the ESA XMM spacecraft", Proc. SPIE 2808, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy VII, (31 October 1996); https://doi.org/10.1117/12.256012
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Cited by 2 scholarly publications.
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KEYWORDS
Mirrors

X-rays

Nickel

X-ray optics

Gold

Space telescopes

Optics manufacturing

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