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Updated: Oct 23, 2025

Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
Published on: July 30, 2020
作为天文观测场所的西藏高原的湖
Licai Deng1,2,3, Fan Yang4,5, Xiaodian Chen6,7,8
1CAS Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China. licai@nao.cas.cn.
一个位于西藏高原的新天文站点为时间领域的天文学提供了极好的条件. 三年间的监测显示天空晴朗,气温稳定,大气透明度极高, 成为未来天文台的首选地点.
科学领域:
- 天文学
- 天体物理学
- 光学天文学
背景情况:
- 在全球范围内很少有高质量的天文遗址.
- 西藏高原提供了一个独特的机会来填补天文观测的纵向差距.
- 它的高海拔和干旱的气候表明有很好的观测条件.
研究的目的:
- 评估西藏高原萨西山的一个地点是否适合进行天文观测.
- 评估与下一代天文设施相关的大气条件.
主要方法:
- 在4200至4500米的海拔上进行了3年的环境监测.
- 测量了天空清晰度,大气观测,温度稳定性和水蒸气含量.
主要成果:
- 70%的夜晚呈现出清的光度条件.
- 天文观测的中位数为0.75弧秒.
- 平均夜间温度变化仅为2.4°C,降水蒸气低 (夜间55%的时间为2mm).
结论:
- 萨西山的气候条件非常稳定.
- 这个位置非常适合开发下一代的天文观测站,特别是时间领域的天文学.
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