ムズタグ観測所の卓越した天文学的ポテンシャルを確認(New Study Confirms Excellent Astronomical Potential of Muztagh Observation Station)

2025-09-02 中国科学院(CAS)

中国科学院新疆天文台の研究チームは、中国西部の木孜塔格観測ステーションにおける大気条件を2018~2024年にかけて体系的に調査し、この地が高精度光学観測に極めて適した環境を持つことを確認した。研究はDIMM(差動像運動モニター)、30m気象塔、自動気象観測システムを用いて「シーイング」や気温、風速・風向を計測。結果として、北2観測点(高さ10m)での中央値は0.78秒角、北1観測点(高さ6m)で0.89秒角と良好なシーイングを示した。また、夜間の地表温度差は約2℃と小さく、風速は中程度(中央値5~6 m/s)、風向は安定して南西が優勢であった。さらに解析では、風速とシーイングの間にU字型の相関があり、中程度の風速が大気乱流を抑制し最適なシーイングをもたらす一方、強い鉛直風切りや急激な変動は乱流を増大させることが判明した。これらの特徴から、木孜塔格観測ステーションは中国西部における光学天文観測の有力拠点となる潜在力を持つと結論づけられた。

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パミール高原ムズタガ・アタ観測点北1・北2地点における視程観測と気象分析 Seeing and meteorological analysis at the North-1 and North-2 points of Muztagh-Ata site on the Pamir Plateau

Wenbo Gu, Ali Esamdin, Cunhai Bai, Jicheng Zhang, Xuan Zhang, Guojie Feng, Letian Wang, Guangxin Pu, Xinliang Wang, Daiping Zhang
Monthly Notices of the Royal Astronomical Society  Published:28 July 2025
DOI:https://doi.org/10.1093/mnras/staf1210

ムズタグ観測所の卓越した天文学的ポテンシャルを確認(New Study Confirms Excellent Astronomical Potential of Muztagh Observation Station)

ABSTRACT

To support the selection of large optical/infrared telescope sites in western China, long-term monitoring of atmospheric conditions and astronomical seeing has been conducted at the Muztagh-Ata site on the Pamir Plateau since 2017. With the monitoring focus gradually shifting northward, three stations were established: the South point, North-1 point, and North-2 point. The North-1 point, selected as the site for the 1.93-m Muztagh Optical Survey Telescope, has recorded seeing and meteorological parameters since late 2018. In 2023, the North-2 point was established approximately 1.5 km north-east of the North-1 point as a candidate location for a future large-aperture telescope. A 10-m Differential Image Motion Monitor tower and a PC-4A environmental monitoring system were installed to evaluate site quality. This study presents a comparative analysis of data from the North-1 and North-2 points during 2018–2024. The median seeing is 0.89 arcsec at North-1 and 0.78 arcsec at North-2. Both points show clear seasonal and diurnal variations, with winter nights offering optimal observing conditions. On average, about 64 per cent of the nighttime duration per year is suitable for astronomical observations. Nighttime temperature variation is low:2.03℃ at 2.10℃ North-1 and  at North-2. Median wind speeds are 5–6 m s−1, with dominant directions between 210° and 300° ⁠, contributing to stable airflow. Moderate wind suppresses turbulence, while strong shear and rapid fluctuations degrade image quality. These findings confirm that both the North-1 and North-2 points offer high-quality atmospheric conditions and serve as promising sites for future ground-based optical/infrared telescopes in western China.

1701物理及び化学
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