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Mesospheric semidiurnal tides and near-12?h waves through jointly analyzing observations of five specular meteor radars from three longitudinal sectors at boreal midlatitudes

机译:通过共同分析来自北半球中纬度三个纵向扇区的五个镜面流星雷达的观测结果,得出中层半日潮和近12?h波

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In the last decades, mesospheric tides have been intensively investigated with observations from both ground-based radars and satellites. Single-site radar observations provide continuous measurements at fixed locations without horizontal information, whereas single-spacecraft missions typically provide global coverage with limited temporal coverage at a given location. In this work, by combining 8 years (2009–2016) of mesospheric winds collected by five specular meteor radars from three different longitudinal sectors at boreal midlatitudes ( 49±8.5 sup°/sup N), we develop an approach to investigate the most intense global-scale oscillation, namely at the period T = 12 ± 0.5 h. Six waves are resolved: the semidiurnal westward-traveling tidal modes with zonal wave numbers 1, 2, and 3 (SW1, SW2, SW3), the lunar semidiurnal tide M2, and the upper and lower sidebands (USB and LSB) of the 16?d wave nonlinear modulation on SW2. The temporal variations of the waves are studied statistically with a special focus on their responses to sudden stratospheric warming events (SSWs) and on their climatological seasonal variations. In response to SSWs, USB, LSB, and M2 enhance, while SW2 decreases. However, SW1 and SW3 do not respond noticeably to SSWs, contrary to the broadly reported enhancements in the literature. The USB, LSB, and SW2 responses could be explained in terms of energy exchange through the nonlinear modulation, while LSB and USB might previously have been misinterpreted as SW1 and SW3, respectively. Besides, we find that LSB and M2 enhancements depend on the SSW classification with respect to the associated split or displacement of the polar vortex. In the case of seasonal variations, our results are qualitatively consistent with previous studies and show a moderate correlation with an empirical tidal model derived from satellite observations.
机译:在过去的几十年中,对中层潮汐进行了深入的研究,并结合了地面雷达和卫星的观测结果。单站点雷达观测可在固定位置进行连续测量而没有水平信息,而单飞船任务通常可在给定位置提供有限的时间覆盖范围的全球覆盖。在这项工作中,通过结合北半球中纬度(49±8.5 ° N)的三个不同纵向扇区的五个镜面流星雷达收集的8年(2009-2016)中层风,我们开发了一种研究最强烈的全球尺度振荡,即周期T = 12±0.5 h。解决了六个波浪:纬向波数为1、2和3(SW1,SW2,SW3)的半日西行潮汐模式,月半日潮M2和16个的上,下边带(USB和LSB) SW2上的d波非线性调制。对波浪的时间变化进行了统计研究,重点是对波浪对平流层突然变暖事件(SSWs)的响应及其气候季节变化。响应于SSW,USB,LSB和M2增强,而SW2减小。然而,与文献中广泛报道的增强相反,SW1和SW3对SSW的响应并不明显。 USB,LSB和SW2响应可以通过非线性调制进行能量交换来解释,而LSB和USB以前可能分别被误解为SW1和SW3。此外,我们发现LSB和M2的增强取决于极性涡旋的相关分裂或位移的SSW分类。在季节性变化的情况下,我们的结果与先前的研究在质量上是一致的,并且与从卫星观测得到的经验潮汐模型之间存在适度的相关性。

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