Standard LSTM networks predict solar active region magnetic flux evolution 3-10 hours ahead from intensity and oscillation maps, outperforming encoder-decoder variants on held-out test regions.
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Prediction of Magnetic Flux Evolution During Solar Active Region Emergence using Long Short-Term Memory Networks
Standard LSTM networks predict solar active region magnetic flux evolution 3-10 hours ahead from intensity and oscillation maps, outperforming encoder-decoder variants on held-out test regions.