Appropriate knowledge of wind-speed distributions and optical turbulence at existing and
potential astronomical observatories is crucial for siting ground-based telescopes and …

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 …

The paper studies the optical turbulence structure at the Large Solar Vacuum Telescope of
the Baikal Astrophysical Observatory. Some results on the study of the wavefront distortions …

Knowledge of the turbulence spectra is of interest for describing atmospheric conditions as
applied to astronomical observations. This article discusses the deformations of the …

Atmospheric turbulence and wind speed distributions are essential in determining the
quality of astronomical sites and implementing adaptive optics systems. In this study, the …

In this paper, we present comprehensive night-time seeing statistics at the Lenghu site using
data collected between 2018 and 2021 using a differential image motion monitor. The …

Optical turbulence limits the angular resolution of ground-based astronomical telescopes.
The key parameter of optical turbulence is seeing. In this study, seasonal variations of …

Due to the space and time constraints of turbulence measurement equipment and the
experiment scene, it is difficult to obtain the atmosphere refractive index structure constant …

This article presents the results of the automatic monitoring of the concentrations of gaseous
impurities of sulfur and nitrogen oxides in the ground-level atmosphere of the urban and …

Astroclimatic conditions characterize the quality of an astronomical site. The Terskol
Observatory was founded over 42 years ago in 1980. The astronomical site (coordinates 43° …