Translator Disclaimer
15 July 2008 Adaptive optics system application for solar telescope
Author Affiliations +
Abstract
The possibility of applying adaptive correction to ground-based solar astronomy is considered. Several experimental systems for image stabilization are described along with the results of their tests. Using our work along several years and world experience in solar adaptive optics (AO) we are assuming to obtain first light to the end of 2008 for the first Russian low order ANGARA solar AO system on the Big Solar Vacuum Telescope (BSVT) with 37 subapertures Shack-Hartmann wavefront sensor based of our modified correlation tracker algorithm, DALSTAR video camera, 37 elements deformable bimorph mirror, home made fast tip-tip mirror with separate correlation tracker. Too strong daytime turbulence is on the BSVT site and we are planning to obtain a partial correction for part of Sun surface image.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
V. P. Lukin, V. M. Grigor'ev, L. V. Antoshkin, N. N. Botugina, O. N. Emaleev, P. A. Konyaev, P. G. Kovadlo, N. P. Krivolutskiy, L. N. Lavrionova, and V. I Skomorovski "Adaptive optics system application for solar telescope", Proc. SPIE 7015, Adaptive Optics Systems, 70156T (15 July 2008); https://doi.org/10.1117/12.787565
PROCEEDINGS
12 PAGES


SHARE
Advertisement
Advertisement
RELATED CONTENT

GREGOR MCAO looking at the Sun
Proceedings of SPIE (July 20 2014)
From Clear to DKIST advancing solar MCAO from 1.6...
Proceedings of SPIE (July 16 2018)
"The first light" for the system of inputting the elements...
Proceedings of SPIE (December 12 2018)
A review of solar adaptive optics
Proceedings of SPIE (August 03 2016)

Back to Top