Proceedings Paper
Numerical simulation of observational telescope with the dynamic holographic correction| Format | Member Price | Non-Member Price |
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Paper Abstract
Described are the methods of numerical design and simulation of observational telescope, using the thin dynamic hologram as the corrector for image distortions, imposed by the primary mirror surface defects.
Paper Details
Date Published: 11 September 1998
PDF: 5 pages
Proc. SPIE 3353, Adaptive Optical System Technologies, (11 September 1998); doi: 10.1117/12.321748
Published in SPIE Proceedings Vol. 3353:
Adaptive Optical System Technologies
Domenico Bonaccini; Robert K. Tyson, Editor(s)
PDF: 5 pages
Proc. SPIE 3353, Adaptive Optical System Technologies, (11 September 1998); doi: 10.1117/12.321748
Show Author Affiliations
Nataly A. Bezina, S.I. Vavilov State Optical Institute (Russia)
Alexey Leshchev, S.I. Vavilov State Optical Institute (Russia)
Alexey Leshchev, S.I. Vavilov State Optical Institute (Russia)
Michael V. Vasil'ev, S.I. Vavilov State Optical Institute (United States)
Vladimir Yu. Venediktov, S.I. Vavilov State Optical Institute (Russia)
Vladimir Yu. Venediktov, S.I. Vavilov State Optical Institute (Russia)
Published in SPIE Proceedings Vol. 3353:
Adaptive Optical System Technologies
Domenico Bonaccini; Robert K. Tyson, Editor(s)
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