Reference : New process for X-ray mirror image quality improvement
Scientific congresses and symposiums : Paper published in a book
Engineering, computing & technology : Multidisciplinary, general & others
http://hdl.handle.net/2268/93474
New process for X-ray mirror image quality improvement
English
Gailly, Patrick mailto [Université de Liège - ULg > > CSL (Centre Spatial de Liège) >]
de Chambure, Daniel [ > > ]
Collette, Jean-Paul [ > > ]
Jamar, Claude [ > > ]
Lainé, Robert [ > > ]
Mazy, Emmanuel mailto [Université de Liège - ULg > > CSL (Centre Spatial de Liège) >]
Médart, Pierre [ > > ]
Stockman, Yvan mailto [Université de Liège - ULg > > CSL (Centre Spatial de Liège) >]
24-Dec-2002
X-Ray Mirrors, Crystals, and Multilayers II (Proceedings Volume)
Freund, Andreas K.
SPIE
Proceedings of SPIE Volume: 4782
46-57
No
International
9780819445490
SPIEs 47th annual meeting on Optical Science, Engineering, and Instrumentation
July 2002
SPIE
Seattle
USA
[en] ion beam figuring ; IBF ; X-ray optics ; telescope ; metrology
[en] A new technique to improve the image quality of Ni replicated X-ray mirror is presented. During the manufacturing of XMM Mirror Module between 1994 to 1999, the classical manufacturing process showed its limits. In 1995, the XMM Mirror Module Qualification Model HEW was around 20 arcsec. In 1998, the fifth Flight Model Mirror Module reached 11 arcsec HEW, with a single mirror shell achieving 8 arcsec HEW. The performance of this technology is namely limited by the integration process of the shells.
The new technique is based on the following philosophy :
• Firstly, an accurate measurement of each mirror shell after integration. A dedicated metrology system has been built and allows a precise metrology of the actual surface.
• Secondly, a modification of the mirror shell and of the support to transfer the stress to a non optical active area.
• Finally, an ion figuring run to correct the residual shape error of the mirror.
The control and evaluation of the process is assured by EUV PSF assessment achieved in the FOCAL X facility developed for XMM.
The advantages of this new process are to shape the mirrors in their final hardware configuration and the versality of the process enabling improvement of other kinds of high accuracy mirrors.
Région wallonne : Direction générale des Technologies, de la Recherche et de l'Energie - DGTRE ; Agence spatiale européenne - ESA
NGXF (RW contract number 9914034, ESA contract number 11734/95/NL/BS)
http://hdl.handle.net/2268/93474

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