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Proceedings Paper

The Current Status Of Grazing Incidence Optics
Author(s): Bernd Aschenbach
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Paper Abstract

Grazing incidence optics have been in use for quite some time for x-ray applications, including fusion research, synchrotron beam lines and x-ray astronomy. X-ray astronomy in particular has benefitted significantly from the development and performance improvements of large x-ray telescopes. Both high angular resolution and large collecting area are aimed at in the design and manufacturing. The x-ray telescope for the German ROSAT x-ray astronomy satellite mission has been finished and assembled with an unprecedented resolution of 3.3 arcsec for the half energy width of the point spread function and less than 3% scattering. A set of 3 light weight telescopes with an effective collecting area of 700 cm2 at 8 keV per telescope is being developed for the XMM mission of the European Space Agency using a nest of 58 thin wall Wolter type I systems. A review of the design, manufacturing and x-ray optical performance of both the ROSAT and XMM telescopes is presented.

Paper Details

Date Published: 27 November 1989
PDF: 7 pages
Proc. SPIE 1140, X-Ray Instrumentation in Medicine and Biology, Plasma Physics, Astrophysics, and Synchrotron Radiation, (27 November 1989); doi: 10.1117/12.961866
Show Author Affiliations
Bernd Aschenbach, Max-Planck- Institut fur Physik Astrophysik (Germany)


Published in SPIE Proceedings Vol. 1140:
X-Ray Instrumentation in Medicine and Biology, Plasma Physics, Astrophysics, and Synchrotron Radiation
Rene Benattar, Editor(s)

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