Deep Flare Net (DeFN) model for solar flare prediction
Naoto Nishizuka, Komei Sugiura, Yuki Kubo, Mitsue Den, Mamoru Ishii

TL;DR
This paper introduces Deep Flare Net (DeFN), a deep neural network model that predicts solar flares with high accuracy using features extracted from solar observation data, including new operational features.
Contribution
The paper presents a novel deep neural network model for solar flare prediction that incorporates new operational features and achieves high skill scores, with interpretability of feature importance.
Findings
Achieved TSS=0.80 for M-class flare prediction
Successfully integrated new operational features into the model
Demonstrated interpretability of feature importance in predictions
Abstract
We developed a solar flare prediction model using a deep neural network (DNN), named Deep Flare Net (DeFN). The model can calculate the probability of flares occurring in the following 24 h 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 <M class or >=C class versus <C class). From 3x10^5 observation images taken during 2010-2015 by Solar Dynamic Observatory, we automatically detected sunspots and calculated 79 features for each region, to which flare occurrence labels of X-, M-, and C-class were attached. We adopted the features used in Nishizuka et al. (2017) and added some features for operational prediction: coronal hot brightening at 131 A (T>=10^7 K) and the X-ray and 131 A intensity data 1 and 2 h before an image. For operational evaluation, we divided the database into two for…
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