SEASON VARIATIONS OF ASTROCLIMATE PARAMETERS FOR THE TERSKOL OBSERVATORY

Cover Page

Cite item

Full Text

Open Access Open Access
Restricted Access Access granted
Restricted Access Subscription Access

Abstract

We present results of the study of seasonal variations of the astroclimate parameters for the Terskol Observatory: wind speed at the level of 200 mbar as a measure of the adaptive optics (AO) applicability, the wind speed altitude distribution, determining the requirements for the AO performance, moisture content to assess the possibility of AO operation in the IR range, the parameters of the mesospheric sodium layer, determining the brightness of the laser reference star for AO systems, in connection with the task of designing adaptive optics for the Zeiss-2000 telescope. Data on surface wind speed and total cloud cover are also analyzed to assess the available observation time. The data of atmospheric reanalysis were used, with the help of which the parameters under consideration have been studied in large astronomical observatories, as well as satellite data of measurements of mesospheric sodium and full-scale changes in surface wind velocity.

About the authors

L. A. Bolbasova

V.E. Zuev Institute of Atmospheric Optics of the Siberian Branch of the Russian Academy of Science

Email: kopylov@inasan.ru
Russia, Tomsk

E. A. Kopylov

Insitute of Astronomy of the Russian Academy of Sciences

Author for correspondence.
Email: kopylov@inasan.ru
Russia, Moscow

References

  1. J. W. Hardy Adaptive Optics for Astronomical Telescopes (Oxford: Oxford University Press, 1998), 448 p.
  2. B. García-Lorenzo, J. J. Fuensalida, C. Muñoz-Tuñón, and E. Mendizabal, Monthly Not. Roy. Astron. Soc. 356, 849–858 (2005).
  3. B. García-Lorenzo, A. Eff-Darwich, J. J. Fuensalida, and J. Castro-Almazán, Monthly Not. Roy. Astron. Soc. 397, 1633–1646 (2009).
  4. Y. Hach, A. Jabiri, A. Ziad, A. Bounhir, M. Sabil, A. Abahamid, and Z. Benkhaldoun, Monthly Not. Roy. Astron. Soc. 420, 1, 637–650 (2012).
  5. L. A. Bolbasova, A. Yu. Shikhovtsev, E. A. Kopylov, A. A. Selin, V. P. Lukin, and P. G. Kovadlo, Monthly Not. Roy. Astron. Soc. 482, 2, 2619–2626 (2019).
  6. Y. Han, Q. Yang, N. Liu, K. Zhang, C. Qing, X. Li, X. Wu, and T. Luo, Monthly Not. Roy. Astron. Soc. 501, 4692–4702 (2021).
  7. M. Sarazin, E. Graham, and H. Kurlandczyk, Messenger 125, 44 (2006).
  8. The ERA5 global reanalysis: Preliminary extension to 1950 // Quarterly Journal of the Royal Meteorological Society 147, 741, 4186–4227 (2021).
  9. M. Sarazin and A. Tokovinin, Proc. ESO Workshop Beyond conventional Adaptive Optics, 321–328 (2002).
  10. J. Vernin, Astronomical Site Selection Proc. SPIE 0628, 626–628 (1986).
  11. F. Cantalloube, O. J. D. Farley, J. Milli, N. Bharmal, et al., Astron. and Astrophys. 638, A98 (2020).
  12. M. R. Kidger, J. M. Rodríguez-Espinosa, J. C. del Rosario, and G. Trancho, New Astron. Rev. 42, 537 (1998).
  13. В. Е. Зуев, В. С. Комаров Современные проблемы атмосферной оптики (Л. Гидрометеоиздат, Т. 1, 1986).
  14. А. Ю. Шиховцев, В. Б. Хайкин, П. Г. Ковадло, P. Baron, Оптика атмосферы и океана 35, 11, 956–962.https://doi.org/10.15372/AOO20221112 (2022)
  15. R. Holzlöhner, S. M. Rochester, D. Bonaccini Calia, D. Budker, J. M. Higbie, and W. Hackenberg, Astron. and Astrophys. 510, A20 (2010).
  16. M. P. Langowski, C. von Savigny, J. P. Burrows, D. Fussen, E. C. M. Dawkins, W. Feng, J. M. C. Plane, and D. R. Marsh, Atmos. Meas. Tech. 10, 2989–3006 (2017).
  17. А. Марешаль, М. Франсон, Структура оптического изображения (М.: Мир, 295, 1964).
  18. А. В. Андриенко, Сборник трудов конференции “Астрономия в Приэльбрусье”, 55–58 (2003).
  19. L. A. Bol’basova and V. P. Lukin, Atmospheric and Oceanic Optics 23, 01, 65–72 (2010).
  20. В. А. Гладких, А. Э. Макиенко, Приборы 7, 109, 21–25 (2009).

Supplementary files

Supplementary Files
Action
1. JATS XML
2.

Download (232KB)
3.

Download (114KB)
4.

Download (88KB)
5.

Download (56KB)
6.

Download (52KB)
7.

Download (53KB)
8.

Download (51KB)

Copyright (c) 2023 Л.А. Больбасова, Е.А. Копылов

This website uses cookies

You consent to our cookies if you continue to use our website.

About Cookies