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Operational optical turbulence forecast for the Service Mode of top-class ground based telescopes

机译:顶级地面望远镜服务模式的运行光学湍流预报

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In this contribution we present the most relevant results obtained in the context of a feasibility study (MOSE) undertaken for ESO. The principal aim of the project was to quantify the performances of an atmospherical non-hydrostatical mesoscale model (Astro-Meso-NH code) in forecasting all the main atmospherical parameters relevant for the ground-based astronomical observations and the optical turbulence (C_N~2 and associated integrated astroclimatic parameters) above Cerro Paranal (site of the VLT) and Cerro Armazones (site of the E-ELT). A detailed analysis on the score of success of the predictive capacities of the system have been carried out for all the astroclimatic as well as for the atmospherical parameters. Considering the excellent results that we obtained, this study proved the opportunity to implement on these two sites an automatic system to be run nightly in an operational configuration to support the scheduling of scientific programs as well as of astronomical facilities (particularly those supported by AO systems) of the VLT and the E-ELT. At the end of 2016 a new project for the implementation of a demonstrator of an operational system to be run on the two ESO's sites will start. The fact that the system can be run simultaneously on the two sites is an ancillary appealing feature of the system. Our team is also responsible for the implementation of a similar automatic system at Mt.Graham, site of the LBT (ALTA Project). Our system/method will permit therefore to make a step ahead in the framework of the Service Mode for new generation telescopes. Among the most exciting achieved results we cite the fact that we proved to be able to forecast C_N~2 profiles with a vertical resolution as high as 150 m. Such a feature is particularly crucial for all WFAO systems that require such detailed information on the OT vertical stratification on the whole 20 km above the ground. This important achievement tells us that all the WFAO systems can rely on automatic systems that are able to support their optimized use.
机译:在此贡献中,我们介绍了在针对ESO进行的可行性研究(MOSE)中获得的最相关的结果。该项目的主要目的是量化大气非静水中尺度模型(Astro-Meso-NH Code)的性能,以预测与地面天文观测和光学湍流(C_N〜2)相关的所有主要大气参数以及Cerro Paranal(位于VLT的站点)和Cerro Armazones(位于E-ELT的站点)上方以及相关的综合气象参数。对于所有的气象和大气参数,已经对系统的预测能力的成功分数进行了详细的分析。考虑到我们获得的出色结果,这项研究证明了有机会在这两个站点上实施一个自动系统,该系统可以按运行配置每晚运行,以支持科学程序以及天文设施(特别是由AO系统支持的那些设施)的调度)和E-ELT。在2016年底,将启动一个新的项目,以实施将在两个ESO站点上运行的操作系统演示程序。该系统可以在两个站点上同时运行的事实是该系统的一个吸引人的特征。我们的团队还负责在LBT(ALTA项目)所在地的格雷厄姆山(Mt.Graham)实施类似的自动系统。因此,我们的系统/方法将允许在新一代望远镜的服务模式框架中迈出一步。在获得的最令人兴奋的结果中,我们引用了一个事实,即事实证明我们可以预测垂直分辨率高达150 m的C_N〜2个剖面。对于所有需要在地面以上20 km的OT垂直分层方面提供此类详细信息的WFAO系统而言,此功能尤其重要。这一重要成就告诉我们,所有WFAO系统都可以依靠能够支持其优化使用的自动系统。

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