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Auroral Oval Boundary Modeling Based on Deep Learning Method

机译:基于深度学习方法的极光椭圆边界建模

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Research on the location of the auroral oval is important to understand the coupling processes of the Sun-Earth system. The equatorward boundary and poleward boundary of the auroral oval are significant parameters of the auroral oval location. Thus auroral oval boundary modeling is an efficient way to study the location of auroral oval. As the location of the auroral oval boundary is subject to a variety of geomagnetic factors, there are some limitations on traditional methods, which express the auroral oval boundary as a function of only one or several geomagnetic activity index. Deep learning method is used in this paper to learn the essential features of the inputs, which are a large number of geomagnetic parameters and the former locations of aurora boundary. Furthermore, a model is established to forecast the location of the auroral oval boundary. The experiment results show that our method can model and forecast the boundary of aurora oval efficiently on the data set obtained from Ultraviolet Imager (UVI) on Polar satellite and OMNI database on NASA.
机译:研究极光椭圆的位置对于理解太阳地球系统的耦合过程很重要。极光椭圆的赤道边界和极向边界是极光椭圆位置的重要参数。因此,极光椭圆形边界建模是研究极光椭圆形位置的有效方法。由于极光椭圆形边界的位置受多种地磁因素的影响,因此传统方法存在一些局限性,这些方法将极光椭圆形边界表示为仅一个或多个地磁活动指数的函数。本文使用深度学习方法来学习输入的基本特征,即大量的地磁参数和极光边界的先前位置。此外,建立了一个模型来预测极光椭圆边界的位置。实验结果表明,该方法可以有效地对极地卫星紫外成像仪和美国国家航空航天局OMNI数据库获取的数据集进行建模和预报。

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