Prediction of Solar Flares Using Photospheric Magnetic Field Parameters with Deep Learning

arXiv:2606.21896 · astro-ph.SR, cs.LG · Submitted 2026-06-20 · Read on arXiv

Yash Chaudhary, Jason T. L. Wang, Chunhui Xu, Yan Xu, Sen Zhang

astro-ph.SR, cs.LG

Submitted: 2026-06-20

Comments: 7 pages, 7 figures

Project page: http://jsoc.stanford.edu

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

Interpretability — 10× in this paper · explained in 15 episodes
SHAP values — 10× in this paper · explained in 2 episodes
Feature Selection — 7× in this paper · explained in 4 episodes
Transformer — 7× in this paper · explained in 2 episodes
Accuracy — 6× in this paper · explained in 1 episode
AUC — 4× in this paper · explained in 2 episodes
Mutual Information — 3× in this paper
Activation Function — 2× in this paper · explained in 1 episode
Active Regions — 2× in this paper · explained in 1 episode
Ablation — 1× in this paper · explained in 1 episode
Ablation Studies — 1× in this paper · explained in 1 episode
Aggregation — 1× in this paper · explained in 1 episode
Area Under Curve — 1× in this paper
Attention Mechanism — 1× in this paper · explained in 3 episodes
Benchmark — 1× in this paper · explained in 2 episodes
Explainability — 1× in this paper · explained in 3 episodes
Helioseismic and Magnetic Imager — 1× in this paper
Joint Science Operations Center — 1× in this paper
Redundancy — 1× in this paper · explained in 2 episodes
Transformer Architecture — 1× in this paper · explained in 2 episodes

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