Rayleigh Laser Guide Star for the Zeiss-2000 Telescope at the Terskol Peak Observatory

In this paper, the design and technical features of the Rayleigh laser guide star (LGS) system as a reference source of an adaptive optical system developed for use on the Zeiss-2000 telescope at the Terskol Peak Astronomical Observatory (coordinates 43°16'34'', 42°29'57'') have been described. Experiments have been performed using the Zeiss-2000 telescope to test the developed system. As a result, a signal from the LGS sufficient for the operation of the wavefront sensor has been received. The presented numerical estimates of the effectiveness of adaptive correction from the Rayleigh LGS have shown that in the future, the use of an adaptive optical system on this telescope will significantly improve the quality of the generated image by increasing the Strehl ratio by at least ten times.

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Publication Details

Journal
Astronomy Reports
Published
2025-04-01
DOI
https://doi.org/10.1134/s1063772925701719
Primary Topic
Adaptive optics and wavefront sensing
Type
article
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article

Rayleigh Laser Guide Star for the Zeiss-2000 Telescope at the Terskol Peak Observatory

E. A. Kopylov, Mikhail Sachkov, L. А. Bolbasova, N. G. Iroshnikov et al.
Astronomy Reports
Adaptive optics and wavefront sensing
article

Rayleigh Laser Guide Star for the Zeiss-2000 Telescope at the Terskol Peak Observatory

E. A. Kopylov, Mikhail Sachkov, L. А. Bolbasova, N. G. Iroshnikov, A. V. Larichev
article en

Abstract

In this paper, the design and technical features of the Rayleigh laser guide star (LGS) system as a reference source of an adaptive optical system developed for use on the Zeiss-2000 telescope at the Terskol Peak Astronomical Observatory (coordinates 43°16'34'', 42°29'57'') have been described. Experiments have been performed using the Zeiss-2000 telescope to test the developed system. As a result, a signal from the LGS sufficient for the operation of the wavefront sensor has been received. The presented numerical estimates of the effectiveness of adaptive correction from the Rayleigh LGS have shown that in the future, the use of an adaptive optical system on this telescope will significantly improve the quality of the generated image by increasing the Strehl ratio by at least ten times.

Astronomy ReportsVol. 69(4)
Lomonosov Moscow State University (RU), Institute of Astronomy (RU), Institute of Applied Astronomy (RU), V.E. Zuev Institute of Atmospheric Optics (RU)
Openalex Percentile: Top 89%
Adaptive optics and wavefront sensing
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