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Comparison of simultaneous wind measurements using colocated VHF meteor radar and MF spaced antenna radar systems

机译:使用共置VHF流星雷达和MF间隔天线雷达系统同时进行风测量的比较

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摘要

Comparisons of wind velocities at heights from 80 to 98 km have been made using two different techniques. The first method involves the determination of winds using meteor drifts (e.g., Avery et al., 1990; Stubbs, 1973). This was done by observing meteors using the University of Adelaide VHF radar situated approximately 40 km north of Adelaide, Australia, at Buckland Park. The second method used to determine winds was the spaced antenna technique (e.g., Briggs, 1984) using an MF radar at the same site. The two radar systems are independent, the VHF radar operating at 54.1 MHz and the MF radar at 1.98 MHz. The spatial separation of the two radars is approximately 600 m. Simultaneous data obtained from September 10 to 20, 1993, arc presented here. The agreement between the two techniques is good below 90 km, while above 90 km we find that the spaced antenna technique yields smaller wind speeds than the meteor drift technique. Several possible reasons for these discrepancies are discussed.
机译:使用两种不同的技术对80至98 km高度的风速进行了比较。第一种方法涉及使用流星漂移确定风向(例如,Avery等,1990; Stubbs,1973)。这是通过使用位于澳大利亚阿德莱德以北约40公里,位于巴克兰公园的阿德莱德大学甚高频雷达观察流星来完成的。用于确定风的第二种方法是在同一地点使用MF雷达的间隔天线技术(例如Briggs,1984)。这两个雷达系统是独立的,甚高频雷达工作在54.1 MHz,中频雷达工作在1.98 MHz。两个雷达的空间间隔约为600 m。这里提供了1993年9月10日至20日获得的同时数据。两种技术之间的一致性在90 km以下很好,而在90 km以上,我们发现间隔天线技术比流星漂移技术产生的风速更小。讨论了这些差异的几种可能原因。

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