An analysis of the fragmentation of observing time at the Muztagh-ata site

IF 2.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Research in Astronomy and Astrophysics Pub Date : 2023-11-06 DOI:10.1088/1674-4527/ad0a32
Wenbo Gu, Jing Xu, Guojie Feng, Xuan Zhang, Letian Wang, Xinliang Wang, Ali Esamdin, Lixian Shen
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time and its continuity. Leveraging in situ measurement data gathered at the Muztagh-ata site
between 2017 and 2021, we showcase the effectiveness of our approach. The statistical result
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Abstract

Abstract Cloud cover plays a pivotal role in assessing observational conditions for astronomical site-testing. Except for the fraction of observing time, its fragmentation also wields a significant influence on the quality of nighttime sky clarity. In this article, we introduce the function Γ ∈ [0, 1], designed to comprehensively capture both the fraction of available observing
time and its continuity. Leveraging in situ measurement data gathered at the Muztagh-ata site
between 2017 and 2021, we showcase the effectiveness of our approach. The statistical result
illustrates that the Muztagh-ata site affords approximately 122 nights of absolute clear and
205 very good nights annually, corresponding to Γ ≥ 0.9 and Γ ≥ 0.36 respectively.
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Muztagh-ata站点观测时间碎片化分析
云量在天文站点测试观测条件评估中起着关键作用。除了观测时间的比例外,它的碎片化也对夜间天空清晰度的质量产生重大影响。在本文中,我们引入了函数Γ∈[0,1],该函数旨在全面捕获可用的观测 时间的百分比及其连续性。利用2017年至2021年期间在Muztagh-ata现场收集的现场测量数据,我们展示了我们方法的有效性。统计结果表明,Muztagh-ata站点每年大约有122个绝对晴朗的夜晚和205个非常晴朗的夜晚,分别对应Γ≥0.9和Γ≥0.36。
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来源期刊
Research in Astronomy and Astrophysics
Research in Astronomy and Astrophysics 地学天文-天文与天体物理
CiteScore
3.20
自引率
16.70%
发文量
2599
审稿时长
6.0 months
期刊介绍: Research in Astronomy and Astrophysics (RAA) is an international journal publishing original research papers and reviews across all branches of astronomy and astrophysics, with a particular interest in the following topics: -large-scale structure of universe formation and evolution of galaxies- high-energy and cataclysmic processes in astrophysics- formation and evolution of stars- astrogeodynamics- solar magnetic activity and heliogeospace environments- dynamics of celestial bodies in the solar system and artificial bodies- space observation and exploration- new astronomical techniques and methods
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