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首页> 外文期刊>Journal of Geophysical Research, D. Atmospheres: JGR >Airglow imaging observations of small-scale structures driven by convective instability in the upper mesosphere over Tirunelveli (8.7°N)
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Airglow imaging observations of small-scale structures driven by convective instability in the upper mesosphere over Tirunelveli (8.7°N)

机译:Tirunelveli(8.7°N)上方中层对流不稳定性驱动的小型结构的气辉成像观察

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摘要

Airglow imaging observations of broadband OH Meinel band emissions made on the night of 20 January 2007 from the tropical Indian site Tirunelveli (8.7°N, 77.8°E) reveal large- and small-scale wave features that are aligned perpendicular to each other and that are associated with gravity wave dynamics. The large-scale waves were the signatures of propagating quasi-monochromatic (QM) waves, whereas the small-scale features were identified to be ripples generated by convective instability in the mesosphere-lower thermosphere (MLT) region. The QM waves showed consistent propagation toward the northwest direction throughout the observation period of ~4.5 hr, whereas the ripples that manifested as short-lived patches in the airglow images were transient and did not show any prominent phase propagation. In addition to these well-resolved structures in images, we infer the presence of waves with relatively longer observed time periods (compared with the observed time period of QM waves) from the spectrum of the time series generated with zenith intensity values derived from the images. From the complementary wind and temperature data obtained with co-located MF radar and Sounding of Atmosphere with Broad band Emission Radiometry on the Thermosphere Ionosphere Mesosphere Energetics and Dynamics mission, an attempt is made to understand the dynamic processes occurring in the vicinity of the mesopause during the night of 20 January 2007. The uniqueness of the present observations is that there were short-lived ripple patches seen in various parts of the sky during the entire observation period of 4.5 hr. The precipitation rates obtained by the Tropical Rainfall Measuring Mission satellite mission suggest that the deep convective activity occurring over the equatorial eastern Indian Ocean provided a plausible source mechanism for sustained generation of the waves observed over Tirunelveli during this night.
机译:2007年1月20日晚从热带印度站点蒂鲁内尔维利(8.7°N,77.8°E)进行的宽带OH Meinel波段发射的气辉成像观察显示,大尺度和小尺度的波特征相互垂直对齐,并且与重力波动力学有关。大规模波是传播的准单色(QM)波的特征,而小尺度特征则被认为是中低层热圈(MLT)区域对流不稳定性产生的波纹。在整个〜4.5小时的观测期内,QM波显示出向西北方向一致的传播,而在气辉影像中表现为短寿命斑块的波纹是短暂的,没有任何明显的相位传播。除了图像中的这些良好解析的结构之外,我们还根据从图像得出的天顶强度值生成的时间序列频谱,推断出存在观察到的时间段相对较长(与QM波的观察到的时间段相比)的波。根据在同一个地点的中频雷达和在热圈电离层中层大气能学和动力学任务上进行的宽带发射辐射测量与大气探测的互补风和温度数据,试图了解在中途停经期间发生的动态过程。 2007年1月20日晚上。本观测的独特之处在于,在整个4.5小时的观测期内,在天空的各个部分都看到了短暂的涟漪斑。热带雨量测量任务卫星任务获得的降水速率表明,赤道东印度洋上空发生的深对流活动为今晚在Tirunelveli上观测到的海浪的持续产生提供了可能的源机制。

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