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Prediction of tropospheric scintillation on satellite links from radiosonde data

机译:利用无线电探空仪数据预测卫星对流层对流层闪烁

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摘要

On the basis of radiosonde data, a new method is proposed for predicting tropospheric scintillation effects on slant paths. It stems from a rigorous statistical development and consists of two steps. First, statistical features of tropospheric turbulence responsible for scintillation are extracted from the analysis of a large amount of radiosonde ascents. Second, long-term scintillation statistics are inferred from these turbulence characteristics, using the theory of propagation through a turbulent medium. The method is applied to a complete year of radiosonde data measured in Belgium and the predicted scintillation results are compared with measurements carried out on the same year near to the meteorological station. An agreement better than with any other usual prediction method is found. The method yields very accurate predictions of scintillation annual statistics and also adequately represents the seasonal and monthly variability of scintillation. Unlike the current prediction models, the proposed radiosonde-based method does not rest on empirical relationships derived from particular propagation experiments and could, therefore, be applied more widely.
机译:在探空资料的基础上,提出了一种预测对流层斜向路径对流闪烁效应的新方法。它源于严格的统计发展,包括两个步骤。首先,从对大量探空仪上升的分析中提取了引起闪烁的对流层湍流的统计特征。其次,使用在湍流介质中传播的理论,从这些湍流特征中推断出长期的闪烁统计数据。将该方法应用于在比利时测量的整年的无线电探空仪数据,并将预测的闪烁结果与同一年在气象站附近进行的测量结果进行比较。找到了比任何其他常用预测方法更好的一致性。该方法可以非常准确地预测闪烁年度统计数据,也可以充分表示闪烁的季节和月度变化。与当前的预测模型不同,所提出的基于探空仪的方法不依赖于从特定传播实验得出的经验关系,因此可以得到更广泛的应用。

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