Abstract—
The work is aimed at the improvement of the model of a turbulent atmosphere at the Large Solar Vacuum Telescope site using the analysis of the energy turbulence spectrum in a wide range of frequencies and deformations of the vertical profile of the structure parameter of the refractive index of air in the atmospheric boundary layer (up to 1 km), depending on the energy of the surface turbulence.
Similar content being viewed by others
REFERENCES
A. S. Gurvich, A. I. Kon, V. L. Mironov, and S. S. Khmelevtsov, Laser Radiation in the Atmosphere (Nauka, Moscow, 1976) [in Russian].
B. P. Mul’tanovskii, Main Principles of the Synoptic Method for Long-Term Weather Forecast (TsUEGMS, Moscow, 1933) [in Russian].
A. Yu. Shikhovtsev, Candidate’s Dissertation in Mathematics and Physics (Institute of Solar-Terrestrial Physics, Siberian Branch, Russian Academy of Sciences, Irkutsk, 2016).
A. Kellerer and A. Tokovinin, “Atmospheric coherence time in interferometry: Definition and measurement,” Astron. Astrophys. 461 (2), 775–781 (2006).
P. G. Kovadlo and A. Yu. Shikhovtsev, “Optical turbulence and different parameters of airflow,” Proc. SPIE—Int. Soc. Opt. Eng. 9292, 6 (2014).
M. Sarazin and A. Tokovinin, “The statistics of isoplanatic angle and adaptive optics time constant derived from DIMM data,” in Beyond Conventional Adaptive Optics: A Conference Devoted to the Development of Adaptive Optics for Extremely Large Telescopes (Venice, Italy, 2001), p. 321–328.
A. S. Zverev, Synoptic Meteorology (Gidrometeoizdat, Leningrad, 1977) [in Russian].
G. D. Nastrom and K. S. Gage, “A climatology of atmospheric wavenumber spectra of wind and temperature observed by commercial aircraft,” J. Atmos. Sci. 42 (9), 950–960 (1985).
D. L. Fried, “Statistics of geometric representation of wavefront distortion,” J. Opt. Soc. Am. 55, 1427–1435 (1965).
B. Garcia-Lorenzo, A. Eff-Darwich, J. J. Fuensalida, and J. Castro-Almazan, “Adaptive optics parameters connection to wind speed at the Teide observatory,” Mon. Not. R. Astron. Soc. 397, 1633–1646 (2009).
K. K. Tung and W. W. Orlando, “The k –3 and k –5/3 energy spectrum of atmospheric turbulence: Quasigeostrophic two-level model simulation,” J. Atmos. Sci. 60, 824–835 (2003).
ACKNOWLEDGMENTS
Some results were obtained using the Large Solar Vacuum Telescope (http://ckp-rf.ru/usu/200615/) with funding of Basic Research program II.16. The analysis of the structural features of optical turbulence was supported by the Russian Foundation for Basic Research (project no. 18-35-00033). Optical and acoustic measurements were financially supported by the Russian Science Foundation (grant no. 17-79-20 077).
Author information
Authors and Affiliations
Corresponding authors
Additional information
Translated by O. Ponomareva
Rights and permissions
About this article
Cite this article
Kovadlo, P.G., Lukin, V.P. & Shikhovtsev, A.Y. Development of the Model of Turbulent Atmosphere at the Large Solar Vacuum Telescope Site as Applied to Image Adaptation. Atmos Ocean Opt 32, 202–206 (2019). https://doi.org/10.1134/S1024856019020076
Received:
Revised:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1134/S1024856019020076