Tarik Mouhtafid, M. Sabil, Z. Ihsane, S. Oujaoura, E.A. Siher
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引用次数: 0
Abstract
In this publication, we follow up our work in the High Atlas, in particular at of Tassemit in the Beni Mellal mountains. Our database is drawn from reanalyses ERA5 by the European Centre for Weather Forecasting, covering a period of 10 years, evaluating new parameters: precipitation water vapor (PWV), cloud cover, wind speed, geopotential, total precipitation, evaporation, coherence time , and scintillation rate . The latter are key astroclimatic parameters for qualifying of new astronomical sites.
The results highlight favorable atmospheric conditions, with a mean and median PWV of 3.68 and 3.35 mm, respectively. The site also features low cloud cover, moderate wind speeds, and low total precipitation, ensuring climatic stability suitable for advanced astronomical projects. We compared the measurements made by MASS-DIMM and calculated by ERA5 for coherence time and scintillation rate at the Observatorio del Roque de Los Muchachos ORM: The results were encouraging, as the recalculated values of and for the Tassemit site showed improved precision and consistency with expected atmospheric conditions. We have also recalculated and for the Tassemit site, and we have the medians of the values of and which are 5.93 ms and 0.00307 arcsec, respectively. This is used as a reference in astronomy.
在本出版物中,我们继续我们在高地图集的工作,特别是在贝尼梅拉尔山脉的塔塞米特。我们的数据库来自欧洲天气预报中心ERA5的再分析,涵盖了10年的时间,评估了新的参数:降水水汽(PWV)、云量、风速、位势、总降水、蒸发、相干时间τOA和闪烁率σI2。后者是确定新的天文地点的关键天文参数。结果显示大气条件有利,平均和中位数PWV分别为3.68和3.35 mm。该站点还具有低云量、中等风速和低总降水量的特点,确保了适合高级天文项目的气候稳定性。我们比较了MASS-DIMM和ERA5在Roque de Los Muchachos ORM天文台的相干时间τOA和闪烁速率σI2的测量结果,结果令人鼓舞,因为Tassemit站点的τOA和σI2的重新计算值显示出更高的精度和与预期大气条件的一致性。我们还重新计算了Tassemit站点的τOA和σI2,得到τOA和σI2的中位数分别为5.93 ms和0.00307 arcsec。这被用作天文学的参考。
Astronomy and ComputingASTRONOMY & ASTROPHYSICSCOMPUTER SCIENCE,-COMPUTER SCIENCE, INTERDISCIPLINARY APPLICATIONS
CiteScore
4.10
自引率
8.00%
发文量
67
期刊介绍:
Astronomy and Computing is a peer-reviewed journal that focuses on the broad area between astronomy, computer science and information technology. The journal aims to publish the work of scientists and (software) engineers in all aspects of astronomical computing, including the collection, analysis, reduction, visualisation, preservation and dissemination of data, and the development of astronomical software and simulations. The journal covers applications for academic computer science techniques to astronomy, as well as novel applications of information technologies within astronomy.