4.7 Article

Deep Flare Net (DeFN) Model for Solar Flare Prediction

Journal

ASTROPHYSICAL JOURNAL
Volume 858, Issue 2, Pages -

Publisher

IOP Publishing Ltd
DOI: 10.3847/1538-4357/aab9a7

Keywords

magnetic fields; methods: statistical; Sun: activity; Sun: chromosphere; Sun: flares; Sun: X-rays, gamma rays

Funding

  1. KAKENHI [JP15K17620, JP18H04451]
  2. JST CREST
  3. Grants-in-Aid for Scientific Research [15K17620] Funding Source: KAKEN

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We developed a solar flare prediction model using a deep neural network (DNN) named Deep Flare Net (DeFN). This model can calculate the probability of flares occurring in the following 24 hr in each active region, which is used to determine the most likely maximum classes of flares via a binary classification (e.g., >= M class versus = C class versus = 10(7) K) and the X-ray and 131 angstrom intensity data 1 and 2 hr before an image. For operational evaluation, we divided the database into two for training and testing: the data set in 2010-2014 for training, and the one in 2015 for testing. The DeFN model consists of deep multilayer neural networks formed by adapting skip connections and batch normalizations. To statistically predict flares, the DeFN model was trained to optimize the skill score, i.e., the true skill statistic (TSS). As a result, we succeeded in predicting flares with TSS = 0.80 for >= M-class flares and TSS = 0.63 for >= C-class flares. Note that in usual DNN models, the prediction process is a black box. However, in the DeFN model, the features are manually selected, and it is possible to analyze which features are effective for prediction after evaluation.

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