A study of the astroclimate in the Dagestan mountains Agul region and at the Ali Observatory in Tibet as possible locations for the Eurasian SubMM Telescopes (ESMT)

V. Khaikin, Khaikin Borisovich Vladimir Special Astrophysical✀ RAS vkhstu@mail.ru, Shikhovtsev Yurievich Artem Institute of Solar–Te✀ RAS Ashikhovtsev@iszf.irk.ru, Mironov Pavlovich Alexei Sternberg Astronomical I✀ Moscow State University almir@list.ru, Qian Xuan National Astronomical Observatories of ✀ CAS qianxuan@nao.cas.cn
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引用次数: 2

Abstract

Using the ECMWF Reanalysis v5 (ERA5) and the GNSS method as well as meteorological and observational data, the statistics of the PWV, TCC, SD, and other astroclimate indicators were obtained for a number of possible ESMT locations in the Russian Federation. These sites are compared with the Ali observatory in Tibet and the BTA location area. The first results of the GNSS PWV measurements on Mt. Kurapdag convincingly confirm the choice made earlier using the ERA5 data.
达吉斯坦山脉阿古尔地区和西藏阿里天文台作为欧亚亚毫米波望远镜(ESMT)可能位置的星象气候研究
利用ECMWF再分析v5 (ERA5)和GNSS方法以及气象和观测资料,对俄罗斯联邦一些可能的ESMT地点进行了PWV、TCC、SD和其他气象指标的统计。这些站点与西藏阿里天文台和BTA位置区域进行了比较。在Kurapdag山上的GNSS PWV测量的第一个结果令人信服地证实了早先使用ERA5数据做出的选择。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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