Enviar artigo por via de e-mail Stabilization of Astronomic Images Using a Controlled Flat Mirror
- Autores: Bokalo S.Y.1, Bokashov I.M.1, Lyakhov D.M.1, Pikulev S.V.1, Chernykh A.V.1
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Afiliações:
- Research Institute of the Luch Research and Production Association
- Edição: Volume 54, Nº 1 (2018)
- Páginas: 46-51
- Seção: Optical Information Technologies
- URL: https://journals.rcsi.science/8756-6990/article/view/212338
- DOI: https://doi.org/10.3103/S8756699018010089
- ID: 212338
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Resumo
A prototype of a key element of adaptive-optics systems — a controlled flat mirror used to correct light beam tilts — was designed. An algorithm for correcting atmospheric distortions of low-intensity light waves and real-time software were developed. In laboratory experiments, a value of 100 Hz was achieved for the bandwidth of a closed-loop system. The efficiency of the developed software was confirmed by daytime observations of stars.
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Sobre autores
S. Bokalo
Research Institute of the Luch Research and Production Association
Email: svpikulev@luch.podolsk.ru
Rússia, ul. Zheleznodorozhnaya 24, Podolsk 142100 Moscow Region
I. Bokashov
Research Institute of the Luch Research and Production Association
Email: svpikulev@luch.podolsk.ru
Rússia, ul. Zheleznodorozhnaya 24, Podolsk 142100 Moscow Region
D. Lyakhov
Research Institute of the Luch Research and Production Association
Email: svpikulev@luch.podolsk.ru
Rússia, ul. Zheleznodorozhnaya 24, Podolsk 142100 Moscow Region
S. Pikulev
Research Institute of the Luch Research and Production Association
Autor responsável pela correspondência
Email: svpikulev@luch.podolsk.ru
Rússia, ul. Zheleznodorozhnaya 24, Podolsk 142100 Moscow Region
A. Chernykh
Research Institute of the Luch Research and Production Association
Email: svpikulev@luch.podolsk.ru
Rússia, ul. Zheleznodorozhnaya 24, Podolsk 142100 Moscow Region
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