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Aura MLS observations of the westward-propagating s=1, 16-day planetary wave in the stratosphere, mesosphere and lower thermosphere

机译:Aura MLS观察西方传播S = 1,16天行星波在平流层,介质层和下热层中

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The Microwave Limb Sounder (MLS) on the Aura satellite has been used to measure temperatures in the stratosphere, mesosphere and lower thermosphere. The data used here are from August 2004 to December 2010 and latitudes 75° N to 75° S. The temperature data reveal the regular presence of a westward-propagating 16-day planetary wave with zonal wavenumber 1. The wave amplitudes maximise in winter at middle to high latitudes, where monthly-mean amplitudes can be as large as ~8 K. Significant wave amplitudes are also observed in the summer-time mesosphere and lower thermosphere (MLT) and at lower stratospheric heights of up to ~20 km at middle to high latitudes. Wave amplitudes in the Northern Hemisphere approach values twice as large as those in the Southern Hemisphere. Wave amplitudes are also closely related to mean zonal winds and are largest in regions of strongest eastward flow. There is a reduction in wave amplitudes at the stratopause. No significant wave amplitudes are observed near the equator or in the strongly westward background winds of the atmosphere in summer. This behaviour is interpreted as a consequence of wave/mean-flow interactions. Perturbations in wave amplitude summer MLT are compared to those simultaneously observed in the winter stratosphere of the opposite hemisphere and found to have a correlation coefficient of +0.22, suggesting a small degrees of inter-hemispheric coupling. We interpret this to mean that some of the summer-time MLT wave may originate in the winter stratosphere of the opposite hemisphere and have been ducted across the equator. We do not observe a significant QBO modulation of the 16-day wave amplitude in the polar summer-time MLT. Wave amplitudes were also observed to be suppressed during the major sudden stratospheric warming events of the Northern Hemisphere winters of 2006 and 2009.
机译:微波边缘探测器(MLS)的奥拉卫星已被用于测量温度在平流层,中间层和低热层。此处所使用的数据是从2004年8月至2010年12月和纬度75°N至75°S的温度数据揭示向西传播的16天行星波与波数纬向1中的常规存在下的波振幅在冬季在最大化中间高纬度地区,在那里月平均振幅可大如〜8 K.有效波振幅在夏季时中间层还观察到,并降低热层(MLT)并且在中间向上的下平流层的高度,以〜20公里高纬度地区。在北半球的办法值波幅的两倍那些在南半球。波振幅也密切相关,平均纬向风和是最大的最强的向东流动的区域。有一个在平流层中波振幅的降低。无显著波振幅在赤道附近,或在夏季大气中的强背景向西蜿蜒观察。这种行为被解释为波/平均流量相互作用的结果。在波振幅夏季MLT扰动的那些相比在相反的半球的冬季平流层同时观察,发现具有的0.22的相关系数,这表明小度间半球耦合。我们解释这意味着,一些在夏季时MLT波可能在相反半球的冬季平流层发起和跨赤道已经涵道。我们不会在极地夏季时MLT观察16天的波幅的显著QBO调制。也观察到波幅在2006年和2009年北半球冬季的重大突发平流层增温事件被抑制。

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