Proceedings Paper
X-ray adaptive mirror: principle and state of the art| Format | Member Price | Non-Member Price |
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Paper Abstract
Adaptive optics systems have proven their efficiency for obtaining high resolution images in the field of large astronomical telescopes. The same techniques can be applied to correct x-ray mirror shapes. The paper describes the principle of an adaptive x-ray mirror system (mirror architecture, measurement subassembly, control unit). In the second part, first results obtained during the design study of the ESRF adaptive x-ray mirror are given. The possibility of achieving cylindrical or elliptical mirror surfaces using adaptive optics techniques are suggested.
Paper Details
Date Published: 25 February 1993
PDF: 15 pages
Proc. SPIE 1739, High Heat Flux Engineering, (25 February 1993); doi: 10.1117/12.140513
Published in SPIE Proceedings Vol. 1739:
High Heat Flux Engineering
Ali M. Khounsary, Editor(s)
PDF: 15 pages
Proc. SPIE 1739, High Heat Flux Engineering, (25 February 1993); doi: 10.1117/12.140513
Show Author Affiliations
Jean-Paul Gaffard, Laserdot Aerospatiale Groupe (France)
R. Ravelet, Laserdot Aerospatiale Groupe (France)
R. Ravelet, Laserdot Aerospatiale Groupe (France)
Corinne Boyer, Laserdot Aerospatiale Groupe (France)
Published in SPIE Proceedings Vol. 1739:
High Heat Flux Engineering
Ali M. Khounsary, Editor(s)
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