首页> 外文期刊>Publications of the Astronomical Society of the Pacific >The Characteristics at the Ali Observatory Based on Radiosonde Observations
【24h】

The Characteristics at the Ali Observatory Based on Radiosonde Observations

机译:基于无抗助剂观测的ALI天文台特征

获取原文
获取原文并翻译 | 示例
       

摘要

As part of the conceptual and preliminary design process of the Chinese Large Telescope, we have spent the last several years measuring and statistically analyzing the atmospheric characteristics above the high Ali Observatory region, in the most western part of the Tibetan Plateau. This is the first article in a series discussing the Ali Observatory site-testing campaign, and we analyze the radiosonde data sets for the first time in that area. The profiles of precipitable water vapor (PWV), upper wind, and optical turbulence are depicted, in addition the statistical characteristics are obtained. PWV profiles in the Ali area indicate that PWV is mainly concentrated below the altitude of 12 km above mean sea level(msl), decreasing with altitude, and has seasonal variations affected by monsoons. In 2016, the median PWV at the Ali Observatory was about 2.0 mm, and less than 1.0 mm during the winter. The wind profiles show strong seasonal variations of wind speed in the troposphere, where there is a prevailing stable west wind. The median wind speed at the height of the 200hP alpha pressure level was 27 m/s in 2016, with a mean speed over 50 m/s in February and 10 m/s in August. The optical turbulence profiles also show seasonal variations, with C-n(2) values between 10(-17) m(-2/3) and 10(-18) m(-2/3) in the free atmosphere. Three turbulent layers are found at the heights around 6-8 km, 12-13 km, and 18-20 km above msl, respectively. In 2016, the median seeing was estimated to be 0.'' 35 at the Ali Observatory, and 0.'' 24 in the summer. The results suggest that very low water vapor in winter, weak upper wind, and good seeing conditions in summer are present at the Ali Observatory, yielding high infrared transparency and high sensitivity for future ground-based optical and infrared telescopes. Given the unique longitude and high altitude, the Ali Observatory might be a promising site in the northern hemisphere for astronomical observations.
机译:作为中国大望远镜的概念和初步设计过程的一部分,我们花了过去几年的衡量和统计分析了高阿里天文台区域的大气特征,位于藏高原最大的西部地区。这是讨论ALI天文台现场测试活动的系列系列中的第一篇文章,我们将在该地区的第一次分析无线电乐库数据集。描绘了可沉淀的水蒸气(PWV),上风和光学湍流的型材,另外获得统计特征。 ALI区域的PWV曲线表明,PWV主要集中在平均海平面(MSL)上方12公里的高度,高度下降,并对季风影响季节性变化。 2016年,ALI天文台的中位数PWV在冬季约2.0毫米,小于1.0毫米。风型材在对流层中显示出强烈的风速变化,在那里存在普遍的稳定的西风。 2016年200HPα压力水平高度的中位风速为27米,2月份2月和10米/秒的平均速度超过50米/秒。光学湍流型材还显示出在自由气氛中的10(-17)m(-2/3)和10(-18)m(-2/3)之间的C-N(2)值。在6-8 km,12-13km,12-13km,18-20公里的高度上发现了三个湍流层,分别为MSL。 2016年,中位数看到估计在阿里观测所为0.''35,夏季24岁。结果表明,ALI天文台的冬季水蒸气非常低,夏季较弱,夏季良好的透明条件,产生高的红外透明度和对未来地面基光和红外望远镜的高灵敏度。鉴于独特的经度和高海拔,Ali天文台可能是北半球的有希望的遗址,用于天文观测。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号