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A comparison of winds measured by meteor radar systems and an MF radar at Buckland Park

机译:对巴克兰公园的流星雷达系统和mF雷达测量的风的比较

摘要

This paper describes a comparison of winds measured by the meteor echo detection and collection (MEDAC) system and a collocated spaced antenna MF radar at the Buckland Park field station near Adelaide, Australia (35°S, 138°E). A previous paper has described a detailed comparison between the MEDAC and Adelaide meteor radar system which was also operated during the campaign. In this paper, which uses only hand-classified underdense meteor echoes, the meteor horizontal zonal wind velocities were compared to the those produced by the MF spaced antenna system. Care was taken when interpreting the comparison results in light of the varying meteor data rates. A point-to-point comparison showed that the excursions seen in the meteor data tended to be larger than those in the MF data. Excellent agreement was found between the two systems and relevant model results across the observed heights for both the mean winds and tides.
机译:本文介绍了在澳大利亚阿德莱德附近(35°S,138°E)附近,由流星回声检测和收集(MEDAC)系统与并置的间隔天线中频雷达测得的风的比较。先前的一篇论文描述了MEDAC与阿德莱德流星雷达系统之间的详细比较,该系统也在战役期间使用。在本文中,仅使用手工分类的稀疏流星回声,将流星水平纬向风速与MF间隔天线系统产生的水平风速进行了比较。根据不同的流星数据速率在解释比较结果时要格外小心。点对点比较显示,在流星数据中看到的偏移往往大于在MF数据中发现的偏移。在两个系统之间发现了极好的一致性,并且在平均风和潮汐的整个观测高度上,相关的模型结果也得到了证实。

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