I. M. Gadzhiev, O. G. Barinov, S. A. Dolenko, I. N. Myagkova
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引用次数: 0
摘要
地磁干扰是空间天气中最重要的因素之一,其作用将随着地球和近地空间的空间工业和全球数字工业的发展而增强。地磁活动通常以特殊指数为特征。最常见的地磁指数之一是 Kp 指数,由 Julius Bartels 于 1939 年首次提出。在这项研究中,我们根据太阳风和行星际磁场参数的小时值以及 Dst 指数的小时值,利用机器学习模型探索了预测第二天 Kp 指数值的可能性。我们使用的机器学习模型包括线性回归、梯度提升和多层感知器。我们测试了时间序列历史的使用在多大程度上提高了 ML 模型的性能。我们就创建和应用机器学习模型解决 Kp 指数预测问题的最佳程序得出了结论。从大多数质量指标来看,CatBoost 和具有两个隐藏层的感知器效果最好。检测到的最重要的输入特征是 Kp 指数本身的前值、太阳风速度和密度、行星际磁场的模量和 z 分量。
Comparative Analysis of the Procedures to Forecast the Kp Geomagnetic Index by Machine Learning
Geomagnetic disturbances are one of the most important factors in space weather, the role of which will increase with the development of the space industry and the global digital industry, both on Earth and in near-Earth space. Geomagnetic activity is usually characterized by special indices. One of the most common geomagnetic indices is the Kp index, first introduced by Julius Bartels in 1939. In this study, we explore the possibility of predicting the following Kp index values during the next day using machine learning models based on the hourly values of the parameters of solar wind and interplanetary magnetic field, and of the hourly Dst index. We use such ML models as linear regression, gradient boosting and multilayer perceptrons. We test to what extent the use of history of time series improves the performance of ML models. We draw conclusions about the optimal procedure of creating and applying of a machine learning model to solve the Kp index forecasting problem. The best results by most of the quality metrics were demonstrated by CatBoost and perceptron with two hidden layers. The most significant input features detected were preceding values of the Kp index itself, solar wind velocity and density, modulus and z-component of the interplanetary magnetic field.
期刊介绍:
Moscow University Physics Bulletin publishes original papers (reviews, articles, and brief communications) in the following fields of experimental and theoretical physics: theoretical and mathematical physics; physics of nuclei and elementary particles; radiophysics, electronics, acoustics; optics and spectroscopy; laser physics; condensed matter physics; chemical physics, physical kinetics, and plasma physics; biophysics and medical physics; astronomy, astrophysics, and cosmology; physics of the Earth’s, atmosphere, and hydrosphere.