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Beyond conventional G-SCIDAR - the Ground-Layer in high vertical resolution

机译:超越传统的G-SCIDAR-高垂直分辨率的地面层

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By using the SCIDAR instrument at the VATT on the top of Mt. Graham and a very wide binary star with a separtion of 35", the vertical structure of the turbulence in the first few hundred meters above the telescope was measured. When using such a binary and analysing the cross-correlation images, a vertical resolution for the turbulence profile of a few tens of meters can be achieved near the ground. This permits to determine the inner structure and the wind sheer of the single turbulent layers inside the ground-layer. We present the principles and the data-reduction process of this method and show first results obtained with this method at Mt. Graham. As an application, we estimate the fraction of the turbulence between the dome of the VATT and the primary mirror of the LBT.
机译:通过使用山顶VATT上的SCIDAR仪器。格雷厄姆(Graham)和分离度为35“的非常宽的双星,测量了望远镜上方头几百米的湍流垂直结构。当使用这种双星并分析互相关图像时,垂直分辨率为可以在地面附近获得几十米的湍流剖面,这可以确定地层内部单个湍流层的内部结构和风向,我们介绍了该方法的原理和数据缩减过程并显示了用这种方法在格雷厄姆山上获得的第一个结果作为应用,我们估计了VATT穹顶和LBT主镜之间的湍流分数。

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