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Medium-Term Prediction of Relativistic Electron Fluxes in a Geostationary Orbit Using Machine Learning Methods Based on Observations of Solar Coronal Holes
Geomagnetism and Aeronomy ( IF 0.6 ) Pub Date : 2020-06-22 , DOI: 10.1134/s0016793220030123 I. N. Myagkova , Yu. S. Shugai , V. V. Kalegaev , V. A. Kolmogorova , S. A. Dolenko
中文翻译:
基于太阳日冕洞观测的机器学习方法对地静止轨道相对论电子通量的中期预测
更新日期:2020-06-22
Geomagnetism and Aeronomy ( IF 0.6 ) Pub Date : 2020-06-22 , DOI: 10.1134/s0016793220030123 I. N. Myagkova , Yu. S. Shugai , V. V. Kalegaev , V. A. Kolmogorova , S. A. Dolenko
Abstract
The paper proposes a model for predicting the integral daily fluxes (fluences) of relativistic electrons (RE) (E > 2 MeV) of the Earth's outer radiation belt in a geostationary orbit using images of the Sun in the ultraviolet range. The results show that the accuracy of the forecast of the RE fluxes three or four days ahead increases significantly when adding the predicted values of solar wind speed at the Earth’s orbit, obtained by processing images of the Sun in the UV range from AIA instrument, SDO Observatory, to the input parameters of the forecasting model.中文翻译:
基于太阳日冕洞观测的机器学习方法对地静止轨道相对论电子通量的中期预测