<p>A genetic algorithm-optimized random forest algorithm (GA-RF) model is constructed to impute large-scale missing data for 5-min averaged data of &gt; 2&#xa0;MeV electron integral fluxes from GOES-E/W satellites. The model inputs include V, Vx, the proton density, the SYM/H index, B, B<sub>x</sub>, B<sub>y</sub>, B<sub>z</sub>, AU, AE, and &gt; 0.6&#xa0;MeV and &gt; 2&#xa0;MeV electron integral fluxes from GOES-E/W. The target variable is the &gt; 2&#xa0;MeV electron integral flux from GOES-W/E. A comparison of the GA-RF model with other machine learning models, including the backpropagation (BP), long short-term memory (LSTM), random forest (RF), extreme learning machine (ELM), and extreme gradient boosting (XGBoost) models, reveals that the GA-RF model achieves the highest PE and LC values and the lowest RMSE and MAE values, indicating that the GA-RF model outperforms the other models in imputing large-scale missing data. Compared with commonly used interpolation methods, such as cubic spline interpolation and linear interpolation, the GA-RF model effectively captures electron flux variations and provides imputed data that closely align with satellite-detected values.</p>

错误:搜索内容不能为空,请输入英文关键词
错误:关键词超出字数限制,请精简
高级检索

Missing value imputation for > 2 MeV electron fluxes in geostationary orbit based on GA-RF model

  • Meihua Fang,
  • Dingyi Song,
  • JianFei Chen,
  • Biao Wang,
  • Mengyun He,
  • Yukuan Ma

摘要

A genetic algorithm-optimized random forest algorithm (GA-RF) model is constructed to impute large-scale missing data for 5-min averaged data of > 2 MeV electron integral fluxes from GOES-E/W satellites. The model inputs include V, Vx, the proton density, the SYM/H index, B, Bx, By, Bz, AU, AE, and > 0.6 MeV and > 2 MeV electron integral fluxes from GOES-E/W. The target variable is the > 2 MeV electron integral flux from GOES-W/E. A comparison of the GA-RF model with other machine learning models, including the backpropagation (BP), long short-term memory (LSTM), random forest (RF), extreme learning machine (ELM), and extreme gradient boosting (XGBoost) models, reveals that the GA-RF model achieves the highest PE and LC values and the lowest RMSE and MAE values, indicating that the GA-RF model outperforms the other models in imputing large-scale missing data. Compared with commonly used interpolation methods, such as cubic spline interpolation and linear interpolation, the GA-RF model effectively captures electron flux variations and provides imputed data that closely align with satellite-detected values.