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Proceedings Paper

An Optical Test And Alignment Method For The XMM Mirror Module
Author(s): M. Schmidt; K. Beckstette; U. Dinger; P. Kaufmann
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Paper Abstract

XMM is a highly nested (58 individual shells) Wolter-I type X-ray telescope with a focal length of 7.5 m. The specified resolution (HEW) is 30 (goal 20) arcsec. In order to qualify single mirror shells and align and assemble the whole mirror module in a reasonable time it is inevitable to apply fast test and strongly converging alignment procedures. By means of two scanning laser beams intra- and extrafocal images of two mirror shells will be registered on a CCD-camera coupled to an image processing PC. One of the mirrors is already glued and serves as a reference while the second one has to be aligned yet. From the data axial and lateral focus positions as well as focus dimensions are calculated. A feed back loop then activates a set of actuators coupled to the mirror to be aligned. In an iterative way the alignment status of this mirror will be optimized. Finally, this mirror is cemented under optical control. First results from a basic test setup with only one mirror will be presented.

Paper Details

Date Published: 28 July 1989
PDF: 4 pages
Proc. SPIE 1160, X-Ray/EUV Optics for Astronomy and Microscopy, (28 July 1989); doi: 10.1117/12.962680
Show Author Affiliations
M. Schmidt, Carl Zeiss (Germany)
K. Beckstette, Carl Zeiss (Germany)
U. Dinger, Carl Zeiss (Germany)
P. Kaufmann, Carl Zeiss (Germany)

Published in SPIE Proceedings Vol. 1160:
X-Ray/EUV Optics for Astronomy and Microscopy
Richard B. Hoover, Editor(s)

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