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Gravity wave ducting in the upper mesosphere and lower thermosphere duct system

机译:上部中层和下部热层导管系统中的重力波导管

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We report on a numerical study of gravity wave propagation in a pair of ducts located in a region where dramatic changes in the airglow most likely associated with ducted wave trains are observed. We examine ducting in an upper mesosphere inversion (INV) and an always present lower thermosphere stable layer (LTD) for a range of phase speeds and horizontal wavelengths characteristic of ducting events. We analyze the propagation and modal structure of ducted waves for backgrounds with increasing realism, starting with a climatological temperature profile where only the LTD is present. In succession, we add the INV based on the work of Smith et al. (2003),, climatological winds, and winds in the upper mesosphere based on the work of Smith et al. (2003). We examine ducting for phase speeds between 40 and 100 m s -1 and horizontal wavelengths between 20 and 60 km. We find that without winds, only the LTD supports ducting of waves forced from below. When observed winds and temperatures are included, strong ducting is evident in both regions. For waves forced from below, the strongest ducted modes are those with slower phase speeds, and of these the third gravest agree reasonably well with the observed phase speeds and wavelengths, indicating that the observations are consistent with linear. ducted waves. For waves forced in the INV, we find an intense and strongly dominant fundamental mode. This is a fast mode having phase speeds —100 m s -1 for a horizontal wavelength of 30 km in the INV and much faster in the LTD. That the fundamental is not seen in Smith et al.'s (2003) observations indicates that the waves were forced from below and that the lowest mode was blocked by an evanescent barrier below the INV. Our results show that the two ducts communicate: the upward extensions of waves ducted in the INV are seen in the LTD. This is particularly significant in the case of in situ forcing, where the fundamentals combine to give amplification exceeding a factor of 10 in the LTD.
机译:我们报告了关于重力波在一对管道中的传播的数值研究,该管道位于一个区域,在该区域中观察到的气辉变化很可能与管道波列有关。我们研究了上层中层反演(INV)和始终存在的下层热层稳定层(LTD)的管道,以了解管道事件的特征相速度和水平波长范围。我们以逼真度为背景的背景分析导管波的传播和模态结构,从仅存在LTD的气候温度剖面开始。接下来,我们基于Smith等人的工作添加了INV。 (2003年),根据史密斯等人的工作,气候风和中高层大气。 (2003)。我们检查导管的相速度在40到100 m s -1之间,水平波长在20到60 km之间。我们发现,没有风,只有LTD支持从下方强迫传播的波浪。如果将观察到的风和温度包括在内,则两个地区均会出现强力管道。对于从下方强行传播的波,最强的导管模式是那些具有较慢的相速度的波,其中第三个最严重的模式与观测到的相速度和波长相当吻合,这表明观测与线性一致。导管波。对于在INV中强行施加的波浪,我们找到了强烈且占主导地位的基本模式。这是一种快速模式,在INV中,对于30 km的水平波长,相位速度为-100 m s -1,而在LTD中则要快得多。 Smith等人(2003)的观测结果没有看到基本面,这表明波浪是从下方推动的,最低模式被INV下方的渐逝性屏障所阻挡。我们的结果表明,两个管道连通:在INV中传导的波浪向上延伸在LTD中可以看到。这在原位强制的情况下尤为重要,在这种情况下,基本原理相结合,使LTD中的放大倍数超过10倍。

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