A Facility for the Study of Atmospheric Parameters Based on the Shack–Hartmann Sensor

—The basic principles of the development of an astroclimatic facility using commercially available standard technical solutions to allow rapid production and unlimited replication are outlined. The facility includes an equatorially-mounted mm, Ritchey–Chretien telescope with a dome, cloud sensor, an...

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Bibliographic Details
Published in:	Astrophysical bulletin Vol. 77; no. 2; pp. 214 - 221
Main Authors:	Potanin, S. A., Kornilov, M. V., Savvin, A. D., Safonov, B. S., Ibragimov, M. A., Kopylov, E. A., Nalivkin, M. A., Shmagin, V. E., Huy, L. X., Thao, N. T.
Format:	Journal Article
Language:	English
Published:	Moscow Pleiades Publishing 01-06-2022 Springer Nature B.V
Subjects:	Astronomy Astrophysics and Cosmology Atmospheric turbulence Automatic weather stations Parameters Physics Physics and Astronomy Shack-Hartmann sensors atmosphere astroclimate turbulence atmospheric effects
Online Access:	Get full text
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Summary:	—The basic principles of the development of an astroclimatic facility using commercially available standard technical solutions to allow rapid production and unlimited replication are outlined. The facility includes an equatorially-mounted mm, Ritchey–Chretien telescope with a dome, cloud sensor, and an automatic weather station. The proposed device for studying the parameters of atmospheric turbulence including the altitude profile consists only of a Shack–Hartmann sensor with a cm subaperture. The feasibility of such an approach has been confirmed by recent studies and our numerical simulations.
ISSN:	1990-3413 1990-3421
DOI:	10.1134/S1990341322020067