Adaptive Forecasting of High-Energy Electron Flux at Geostationary Orbit Using ADALINE Neural Network

High-energy electron flux increases in the recovery phase after the space weather events such as a coronal mass ejection. High-energy electrons can penetrate circuits deeply and the penetration could lead to deep dielectric charging. The forecast of high-energy electron flux is vital in providing warning information for spacecraft operations. We investigate an adaptive predictor based on ADALINE neural network. The predictor can forecast the trend of the daily variations in high-energy electrons. The predictor was trained with the dataset of ten years from 1998 to 2008. We obtained the prediction efficiency approximately 0.6 each year except the first learning year 1998. Furthermore, the predictor can adapt to the changes for the satellite's location. Our model succeeded in forecasting the high-energy electron flux 24 hours ahead.

[1]  Daniel N. Baker,et al.  Linear prediction filter analysis of relativistic electron properties at 6.6 RE , 1990 .

[2]  J. B. Blake,et al.  Highly relativistic electrons in the Earth';s outer magnetosphere: 1. Lifetimes and temporal history 1979–1984 , 1986 .

[3]  Daniel N. Baker,et al.  Satellite anomalies linked to electron increase in the magnetosphere , 1994 .

[4]  Bernard Widrow,et al.  Perceptrons, adalines, and backpropagation , 1998 .

[5]  Yoshizumi Miyoshi,et al.  Flux enhancement of radiation belt electrons during geomagnetic storms driven by coronal mass ejections and corotating interaction regions , 2006 .

[6]  Lakhmi C. Jain,et al.  Knowledge-Based Intelligent Information and Engineering Systems , 2004, Lecture Notes in Computer Science.

[7]  Ahmadreza Khoogar,et al.  A Comparison of Adaline and MLP Neural Network based Predictors in SIR Estimation in Mobile DS/CDMA Systems , 2007 .

[8]  Yoshiteru Ishida Designing an Immunity-Based Sensor Network for Sensor-Based Diagnosis of Automobile Engines , 2006, KES.

[9]  Takahiro Obara,et al.  Neural network prediction of relativistic electrons at geosynchronous orbit during the storm recovery phase: effects of recurring substorms , 2002 .

[10]  Daniel N. Baker,et al.  Satellite Anomalies due to Space Storms , 2001 .

[11]  J. King,et al.  Solar wind spatial scales in and comparisons of hourly Wind and ACE plasma and magnetic field data , 2005 .

[12]  Yoshiteru Ishida,et al.  Forecast of High-energy Electron Flux at Geostationary Orbit Using Neural Network , 2009 .

[13]  Harry C. Koons,et al.  A neural network model of the relativistic electron flux at geosynchronous orbit , 1991 .

[14]  Michael W. Liemohn,et al.  Unraveling the causes of radiation belt enhancements , 2007 .