Zobrazeno 1 - 10
of 18
pro vyhledávání: '"D. Yu. Kolobov"'
Autor:
V. E. Tomin, A. Yu. Shikhovtsev, P. G. Kovadlo, D. Yu. Kolobov, Vladimir P. Lukin, A. V. Kiselev
Publikováno v:
Atmospheric and Oceanic Optics. 33:295-301
Modern methods for altitude profiling of atmospheric turbulence are discussed. A method for estimating the altitudes of atmospheric layers characterized by strong turbulence, which is an alternative to the Slodar method, is suggested. The method is b
Autor:
A. Yu. Shikhovtsev, A. A. Selin, O. N. Emaleev, Vladimir P. Lukin, L. V. Antoshkin, N. N. Botygina, P. G. Kovadlo, E. L. Soin, P. A. Konyaev, S. A. Chuprakov, D. Yu. Kolobov, A. G. Borzilov
Publikováno v:
Atmospheric and Oceanic Optics. 32:597-606
Hardware components were created for the Large Solar Vacuum Telescope (LSVT) of the Institute of Solar-Terrestrial Physics, Siberian Branch, Russian Academy of Sciences, in 2017 for development of techniques for recording and correcting distortions o
Autor:
A. Yu. Schikhovtcev, P. A. Konyaev, A. G. Borzilov, P. G. Kovadlo, S. A. Chuprakov, D. Yu. Kolobov, N. N. Botygina, Vladimir P. Lukin, O. N. Emaleev, L. V. Antoshkin
Publikováno v:
Adaptive Optics Systems VII.
A multi-cascade adaptive optical system for imaging and image stabilization for the Large Solar Vacuum Telescope is described. This system was created in 2017 by specialists of the V.E. Zuev Institute of Atmospheric Optics SB RAS, Tomsk, with the tec
Autor:
I. V. Russkih, P. G. Kovadlo, Vladimir P. Lukin, D. Yu. Kolobov, A. V. Kiselev, A. Yu. Shikhovtsev, M. Yu. Shikhovtsev
Publikováno v:
26th International Symposium on Atmospheric and Ocean Optics, Atmospheric Physics.
We propose the concept of the new SCIDAR-based method to determine the characteristics of the atmospheric turbulent layers including its heights and strength. In this paper we discuss the possibility of the estimating of the heights of the atmospheri
Autor:
N. N. Botygina, Vladimir P. Lukin, S. A. Chuprakov, D. Yu. Kolobov, P. G. Kovadlo, A. Yu. Shikhovtsev
Publikováno v:
Atmospheric and Oceanic Optics. 31:709-717
Features of a two-mirror adaptive system for correction of atmospheric disturbances of the Large Solar Vacuum Telescope are described. The system has been developed with allowance for the correction of instrumental vibrations of the telescope in a wi
Autor:
A. Yu. Shikhovtsev, V. V. Lavrinov, Vladimir P. Lukin, S. A. Chuprakov, D. Yu. Kolobov, P. G. Kovadlo, P. A. Konyaev, L. A. Bolbasova, A. A. Selin, O. N. Emaleev, N. N. Botygina, Alexis Kudryashov, L. N. Lavrinova, E. A. Kopylov, L. V. Antoshkin
Publikováno v:
Atmospheric and Oceanic Optics. 30:291-299
New results obtained within Russian Science Foundation Project no. 15-19-20013 are presented. The project was started in the middle of 2015 and is aimed at the solution of actual problems of the development of the optoelectronic industry using adapti
Autor:
K. I. Budnikov, T. V. Lyakh, A. A. Zotov, A. S. Maksimov, S. V. Perebeinos, S. V. Vlasov, A. N. Bevzov, A. A. Lubkov, V. N. Kotov, P. G. Kovadlo, I. V. Russkikh, Yu. A. Popov, A. D. Petukhov, V. S. Peshcherov, D. Yu. Kolobov, A. V. Kurochkin, S. A. Lylov, V. E. Tomin
Publikováno v:
Optoelectronics, Instrumentation and Data Processing. 52:187-195
The architecture, composition, specific features of operation, and technical characteristics of an automated control system of the Large Solar Vacuum Telescope of the Baikal astrophysical observatory are considered. The system is used for automation
Publikováno v:
Astronomy Letters. 42:55-62
The oscillations of the half-width of the Ba II 4554 Ǻ and Ca II 8542 Ǻ spectral lines have been analyzed using observations at the base of solar coronal holes (CHs). The observed variations (~50 m Ǻ for Ca II and ~4 m Ǻ for Ba II) exceed conside
Autor:
D. E. Kukushkin, Alexey Bakholdin, Mikhail Demidov, A. R. Belan, V. N. Vasil’ev, S. A. Chuprakov, D. Yu. Kolobov
Publikováno v:
Journal of Optical Technology. 87:705
This article presents a polarization calculation for the LST-3 large solar telescope. It describes the interaction of the telescope mirrors and includes a calculation of the transmittance of the telescope’s optical system for incident radiation wit
Autor:
N. N. Botygina, S. A. Chuprakov, D. Yu. Kolobov, P. G. Kovadlo, A. Yu. Shikhovtcev, Vladimir P. Lukin
Publikováno v:
24th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics.
This paper describes the features of the two-mirror adaptive system for correcting atmospheric disturbances of the Large Solar Vacuum Telescope, developed with allowance for the correction of instrumental vibrations of telescopes in a wide amplitude-