An Analysis of the Seeing Conditions at Platform C of the Lenghu Site 后印本

摘要: This paper statistically analyzes the seeing data at the Lenghu site Platform C from 2018 to 2024, during which extensive construction modified the original landscape. The study focuses on the impacts of meteorological factors and building obstructions. The results reveal a progressive degradation in seeing as the monitoring setup passively changed: the median values were 0.″76 (the original location), 0.″83 during the Terrace, and 0.″99 at the new Dome (temporarily considered the permanent monitoring location). Once the instruments are fully deployed, wind speed and wind direction critically affect seeing quality, with optimal conditions occurring when the wind speed is 2–6 m s−1 and the wind direction is between 180° and 270°. However, in 2023 and 2024, the wind speeds decreased, and the prevailing wind direction shifted from southwest to northwest, correlating with poorer seeing. Computational Fluid Dynamics simulations reveal that the construction of the Wide Field Survey Telescope altered the local wind field, increasing turbulence around the Dome,especially when the winds blow from 225° to 255°. In contrast,Platform A,located in a higher and more open area,consistently maintained better seeing,particularly after midnight,likely due to fewer obstructions and lower nocturnal heat release.