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Non-equilibrium radiative transfer in structured atmospheres

机译:结构化气氛中的非平衡辐射转移

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The nonequilibrium middle and upper atmosphere are very dynamic regions that are structured vertically and horizontally by the presence of persistent temperature inversion layers and by the passages of both atmospheric gravity waves and transient frontal disturbances or bores. The infrared emissions from this part of the atmosphere are already typically not in local thermodynamic equilibrium (LTE) and are further perturbed by the presence of this pervasive atmospheric structure. The inevitable result is highly structured atmospheric emissions that reflect the structure of the atmosphere. Understanding the structure of the atmosphere is essential to understanding the structure of the radiation that it emits. At the same understanding how atmospheric structure perturbs atmospheric radiation provides a means to sense the perturbing atmospheric processes remotely. We examine methods to calculate the LTE/non-LTE radiative response to temporal and spatial variations of the atmosphere and give examples of applications. We also compare our results with existing field data. Finally, we discuss a proposed new NASA optical / infrared experiment (Waves Explorer) to sense atmospheric gravity waves remotely from earth orbit on a global basis and characterize their sources.
机译:非QuibiBribrium和上层大气是非常动态的区域,其通过存在持续的温度反转层和通过大气重力波和瞬态前扰动或孔的通道来垂直和水平地构造。来自大气层的这部分的红外排放通常不在局部热力学平衡(LTE)中,并且通过这种普遍的大气结构的存在进一步扰乱。不可避免的结果是强大的结构化的大气排放,反映了大气的结构。了解大气的结构对于理解它发出的辐射结构至关重要。在相同的了解erturbs大气辐射的情况下,如何远程感测扰动大气过程的手段。我们研究了计算LTE /非LTE辐射响应对大气的时间和空间变化的方法,并举例说明应用的示例。我们还将结果与现有现场数据进行比较。最后,我们讨论了一个拟议的NASA光/红外实验(Waves Explorer),以在全球范围内从地球轨道远程感测大气引力波,并表征他们的来源。

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