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Cause of winter gravity wave spectrum saturation

机译:冬季重力波频谱饱和的原因

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This paper utilizes horizontal velocity measurements observed from 19 chaff rockets and nearly simultaneous temperature measurements collected from 19 falling sphere rockets to study the cause of winter gravity wave spectrum saturation. Results suggest that strong horizontal velocity shears larger than 0.04 s~(-1) are observed to be present at various heights near the winter mesopause. On one single chaff rocket flight, an extremely strong horizontal velocity shear as high as 0.33 s~(-1) is observed at 87.4 km and is believed to be the strongest value ever measured in the mesosphere. These strong horizontal velocity shears, together with Brunt-Vaeisaelae frequency squared obtained from the temperature profile, act collectively to yield two dynamical instability regions of Richardson number smaller than 1/4, suggesting that the saturated gravity wave spectrum observed by the chaff rockets in winter is a result of dynamical instability.
机译:本文利用从19枚谷壳火箭观察到的水平速度测量值和从19颗落球火箭收集的几乎同时的温度测量值来研究冬季重力波谱饱和的原因。结果表明,在冬季中绝经期附近的不同高度上均出现了大于0.04 s〜(-1)的强水平速度剪切。在一次谷壳火箭飞行中,在87.4 km处观测到极强的水平速度剪切,高达0.33 s〜(-1),被认为是有史以来在中层空间测得的最强值。这些强大的水平速度剪切力,再加上从温度分布图获得的Brunt-Vaeisaelae频率平方,共同作用,产生两个小于1/4的理查森数动态不稳定性区域,这表明谷壳火箭在冬季观测到的饱和重力波谱是动态不稳定的结果。

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