Aeronomical Applications of Polar Mesospheric Summer Echoes (PMSE) at the Early Polar Cap Observatory

PI继续他对极地夏季中间层回声的研究，并有了一个新的转折：探索大气学。利用早期极帽天文台的MST雷达获得的数据，后期工作人员：(1)寻找光谱宽度和信噪比之间的相互关系，以及任何当前振荡的相位，(2)将散射特性与流星扩散时间进行比较，以确定后者中的施密特数效应(如果存在)，以及(3)使用波散散关系，通过将它们与雷达测量的风扰动进行比较，发现可以将流星温度推至的高频极限。此外，PI仍然致力于探索加拿大仪器的数据，将其作为全球变化的标志(如中间层所示)。

The PI continues his study of Polar Summer Mesospheric Echoes with a new twist: exploring the aeronomy. Using data acquired by the MST radar at the Early Polar Cap Observatory, a post-doc: (1) looks for interrelationships between spectral widths and signal-to-noise, and the phase of any present oscillations, (2) compares the scattering properties with the meteor diffusion times to locate a Schmidt Number effect in the latter (if it exists), and (3) uses the wave dispersion relationship to discover the high frequency limit to which meteor temperatures can be pushed by comparing them to wind perturbations measured with the radar. Further, the PI remains committed to exploring Canadian instrumentation's data as a marker for global change (as manifested in the mesosphere).