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Meteorological parameter analysis above Dome C using data from the European Centre for Medium-Range Weather Forecasts

机译:使用来自欧洲中距离天气预报中心的数据,对圆顶C上方的气象参数进行分析

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摘要

We present a characterization of all the principal meteorological parameters (wind speed and direction, pressure, and absolute and potential temperature) that extends up to 25 km from the ground above Dome C, Antarctica, for 2 years (2003 and 2004). The data set is composed of "analyses" provided by the general circulation model (GCM) of the European Centre for Medium-Range Weather Forecasts (ECMWF), and they are part of the MARS catalog. A monthly and seasonal (summer and winter) statistical analysis of the results is presented. The Richardson number is calculated for each month of the year over 25 km in order to study the relative stability of the atmosphere. This allows us to trace a map indicating where and when the optical turbulence has the highest probability of being triggered in the whole troposphere, tropopause, and stratosphere. Finally, we try to predict the best expected isoplanatic angle and wave-front coherence times (theta(0,max) and tau(0,max), respectively) by employing Richardson number maps, wind speed profiles, and simple analytical models of C-N(2) vertical profiles.
机译:我们对所有主要气象参数(风速和风向,压力以及绝对和潜在温度)进行了描述,这些参数从南极Dome C上方的地面延伸到地面长达25 km,持续了2年(2003年和2004年)。数据集由欧洲中距离天气预报中心(ECMWF)的一般循环模型(GCM)提供的“分析”组成,它们是MARS目录的一部分。给出了结果的每月和季节性(夏季和冬季)统计分析。为了研究大气的相对稳定性,每年在25公里以上的每个月计算Richardson数。这使我们能够绘制出一个图,该图指示在整个对流层,对流层顶和平流层中光学湍流最有可能被触发的位置和时间。最后,我们尝试通过使用Richardson数图,风速剖面和CN的简单分析模型来预测最佳预期的等平面角和波前相干时间(分别为theta(0,max)和tau(0,max)) (2)垂直型材。

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