Forecasting Continuum Intensity for Solar Active Region Emergence Prediction using Transformers
Jonas Tirona, Sarang Patil, Spiridon Kasapis, Eren Dogan, John Stefan, Irina N. Kitiashvili, Alexander G. Kosovichev, Mengjia Xu

TL;DR
This paper introduces a Transformer-based model with an early detection architecture for predicting solar active region emergence, achieving earlier warnings and improved accuracy over traditional LSTM models, despite increased variance.
Contribution
The study develops a novel Transformer architecture with attention biases and a timing-aware loss for AR emergence prediction, outperforming LSTM baselines in early warning capability.
Findings
Transformer with early detection achieves 10.6% lower RMSE than LSTM.
Average warning time improved to 4.73 hours.
Model detects micro-changes, enabling earlier alerts despite higher variance.
Abstract
Early and accurate prediction of solar active region (AR) emergence is crucial for space weather forecasting. Building on established Long Short-Term Memory (LSTM) based approaches for forecasting the continuum intensity decrease associated with AR emergence, this work expands the modeling with new architectures and targets. We investigate a sliding-window Transformer architecture to forecast continuum intensity evolution up to 12 hours ahead using data from 46 ARs observed by SDO/HMI. We conduct a systematic ablation study to evaluate two key components: (1) the inclusion of a temporal 1D convolutional (Conv1D) front-end and (2) a novel `Early Detection' architecture featuring attention biases and a timing-aware loss function. Our best-performing model, combining the Early Detection architecture without the Conv1D layer, achieved a Root Mean Square Error (RMSE) of 0.1189 (representing…
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Taxonomy
TopicsIonosphere and magnetosphere dynamics · Meteorological Phenomena and Simulations · Solar and Space Plasma Dynamics
