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Modelling total electron content during geomagnetic storm conditions using empirical orthogonal functions and neural networks

机译:建模期间总电子含量磁暴条件使用经验正交函数和神经网络

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It has been shown in ionospheric research that modelling total electron content (TEC) during storm conditions is a big challenge. In this study, TEC modelling was performed over Sutherland (32.38°S, 20.81°E, 41.09°S geomagnetic), South Africa, during storm conditions, using a combination of empirical orthogonal function (EOF) and regression analyses techniques. The neural network (NN) technique was also applied to the same TEC data set, and its output was compared with TEC modeled using the EOF model. TEC was derived from GPS observations, and a geomagnetic storm was defined for Dst ≤ ?50 nT. The hour of the day and the day number of the year, F_(10.7p) and A indices, were chosen as inputs for the modeling techniques to take into account diurnal and seasonal variation of TEC, solar, and geomagnetic activities, respectively. Both EOF and NN models were developed using GPS TEC data for storm days counted from 1999 to 2013 and tested on different storms. For interpolation, the EOF and NN models were validated on storms that occurred during high and low solar activity periods (storms of 2000 and 2006), while for extrapolation the validation was done for the storms of 2014 and 2015, identified based on the provisional Dst index data. A comparison of the modeled TEC with the observed TEC showed that both EOF and NN models perform well for storms with nonsignificant ionospheric TEC response and storms that occurred during period of low solar activity. For storms with significant TEC response, TEC magnitude is well captured during the nighttime and early morning, but short-term features, TEC enhancement, and depression are not sufficiently captured by the models. Statistically, the NN model performs 12.79% better than the EOF model on average, over all storm periods considered. Furthermore, it has been shown that the EOF and NN models developed for a specific station can be used to estimate TEC over other locations within a latitudinal and longitudinal coverage of 8.7° and 10.6°, respectively. This is an important result as it reduces the data dimensionality problem for computational purposes.
机译:它已被证明在电离层的研究造型总电子含量(TEC)期间风暴条件是一个巨大的挑战。研究中,TEC造型了萨瑟兰(32.38°S, 20.81°E, *°S地磁),南非,在风暴的条件下,利用实证的结合正交函数(EOF)和回归分析技术。也适用于相同的TEC的数据集,和它的输出与TEC建模使用EOF模型。和磁暴的定义Dst≤? 50nT。小时的一天和一天的f(10.7英镑),和一个指数,被选为将建模技术的输入TEC账户昼夜和季节变化,太阳能、分别和地磁活动。使用GPS EOF和神经网络模型被开发TEC风暴天统计从1999年到2013年的数据和测试在不同的风暴。插值,EOF和神经网络模型在风暴发生在高和验证低的太阳活动周期(2000年风暴2006),而对于外推法验证为2014年和2015年的风暴,做确认基于临时Dst索引数据。比较建模TEC的观察TEC表明EOF和神经网络模型的执行对与无意义的电离层风暴TEC响应和风暴期间发生的低太阳活动的时期。重大TEC响应,TEC大小是好捕获在夜间和清晨,但短期特征,TEC增强,抑郁不够被模型。比EOF模型平均12.79%所有的风暴期考虑。被证明EOF和NN模型开发为一个特定的站可以用来估计侦探在纬向和在其他地方纵向覆盖8.7°和10.6°,分别。降低数据的维数问题计算的目的。

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