Short-Term Solar Flare Prediction Using Predictor Teams

Details Short-Term Solar Flare Prediction Using Predictor Teams Short-Term Solar Flare Prediction Using Predictor Teams

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010soph..263..175h&link_type=abstract

Solar Physics, Volume 263, Issue 1-2, pp. 175-184

Computer Science

Learning

2

Active Regions, Magnetic Fields, Flares, Forecasting, Ensemble Learning

Scientific paper

A short-term solar flare prediction model is built using predictor teams rather than an individual set of predictors. The information provided by the set of predictors could be redundant. So it is necessary to generate subsets of predictors which can keep the information constant. These subsets are called predictor teams. In the framework of rough set theory, predictor teams are constructed from sequences of the maximum horizontal gradient, the length of neutral line and the number of singular points extracted from SOHO/MDI longitudinal magnetograms. Because of the instability of the decision tree algorithm, prediction models generated by the C4.5 decision tree for different predictor teams are diverse. The flaring sample, which is incorrectly predicted by one model, can be correctly forecasted by another one. So these base prediction models are used to construct an ensemble prediction model of solar flares by the majority voting rule. The experimental results show that the predictor team can keep the distinguishability of the original set, and the ensemble prediction model can obtain better performance than the model based on the individual set of predictors.

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