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首页> 外文期刊>Atmospheric Measurement Techniques >Tomographic reconstruction of atmospheric gravity wave parameters from airglow observations
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Tomographic reconstruction of atmospheric gravity wave parameters from airglow observations

机译:气辉观测的大气重力波参数的层析成像重建

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Gravity waves (GWs) play an important role in the dynamics of the mesosphere and lower thermosphere (MLT). Therefore, global observations of GWs in the MLT region are of particular interest. The small scales of GWs, however, pose a major problem for the observation of GWs from space. We propose a new observation strategy for GWs in the mesopause region by combining limb and sub-limb satellite-borne remote sensing measurements for improving the spatial resolution of temperatures that are retrieved from atmospheric soundings. In our study, we simulate satellite observations of the rotational structure of the Osub2/sub A-band nightglow. A key element of the new method is the ability of the instrument or the satellite to operate in so-called qtarget mode/q, i.e. to point at a particular point in the atmosphere and collect radiances at different viewing angles. These multi-angle measurements of a selected region allow for tomographic 2-D reconstruction of the atmospheric state, in particular of GW structures. The feasibility of this tomographic retrieval approach is assessed using simulated measurements. It shows that one major advantage of this observation strategy is that GWs can be observed on a much smaller scale than conventional observations. We derive a GW sensitivity function, and it is shown that qtarget mode/q observations are able to capture GWs with horizontal wavelengths as short as ?~?50?km for a large range of vertical wavelengths. This is far better than the horizontal wavelength limit of 100–200?km obtained from conventional limb sounding.
机译:重力波(GWs)在中层和低热层(MLT)的动力学中起着重要作用。因此,对MLT地区GW的全球观测尤为重要。但是,小规模的GW构成了从太空观察GW的主要问题。我们结合中肢和近肢卫星传播的遥感测量结果,为中绝经区的GWs提出了一种新的观测策略,以提高从大气探测中获取的温度的空间分辨率。在我们的研究中,我们模拟了O 2 A波段夜光的旋转结构的卫星观测。新方法的关键要素是仪器或卫星以所谓的“目标模式”运行的能力,即指向大气中的特定点并以不同的视角收集辐射。选定区域的这些多角度测量值允许对大气状态(尤其是GW结构)进行断层扫描2D重建。使用模拟测量评估了这种断层摄影方法的可行性。它表明,这种观测策略的一个主要优点是,与传统观测相比,GW的观测范围小得多。我们推导了GW灵敏度函数,结果表明,目标模式观测值能够捕获水平波长短至λ〜?50?km的GW,且垂直波长范围很大。这远好于传统肢体测听获得的水平波长限制100–200?km。

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