Optical turbulence in the atmospheric surface layer at the Pamir Plateau Muztagh-ata site
Wenbo Gu, Ali Esamdin, Chunhai Bai, Xuan Zhang, Guojie Feng, Guangxin, Pu, Letian Wang, Gaowen Sun, Haozhi Wang, Lixian Shen

TL;DR
This study analyzes optical turbulence at Muztagh-ata, revealing how turbulence parameters vary with height and conditions, and suggesting the site’s potential for astronomical observations due to favorable turbulence conditions.
Contribution
The paper provides detailed measurements of optical turbulence parameters at Muztagh-ata and links turbulence behavior to environmental factors, highlighting the site's suitability for astronomy.
Findings
Nighttime seeing median of 0.24 arcseconds at 6-30m height
Optical turbulence decreases exponentially with height during the night
Temperature inversion improves seeing conditions
Abstract
In this paper, we conducted a detailed analysis of optical turbulence in the Atmospheric Surface Layer (ASL) at Muztagh-ata site during on-site testing. We utilized ultrasonic anemometers positioned on a 30-meter tower to collect and process data at five height levels, obtaining data from October 1, 2021 to the present. We investigated the behavior of optical turbulence parameters (\(C_n^2\) and seeing \(\varepsilon\)) in the ASL. Nighttime \(C_n^2\) primarily fluctuated in the range of \(10^{-16}\) to \(10^{-14}\), exhibiting an exponential decrease with height. During the day, it showed a \(h^{-0.82}\) dependency, while at night, it displayed a \(h^{-0.48}\) dependency. Additionally, we presented the distribution of seeing across different layers within the ASL, showing a gradual decrease with increasing height, with a median seeing of 0.24 arcseconds at nighttime and 0.48 arcseconds…
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