Using Multiple Instance Learning for Explainable Solar Flare Prediction
C\'edric Huwyler, Martin Melchior

TL;DR
This paper employs Multiple Instance Learning on spectral data from NASA's IRIS satellite to predict solar flares with high accuracy and provide explanations for the predictions, aiding real-time flare monitoring.
Contribution
It introduces a MIL-based approach for solar flare prediction that leverages weakly-labeled spectral data and offers interpretability of the model's decisions.
Findings
Achieved around 90% accuracy in flare prediction within 25 minutes.
Identified spectral profile groups associated with flare precursors.
Demonstrated interpretability of spectral features relevant to flare prediction.
Abstract
In this work we leverage a weakly-labeled dataset of spectral data from NASAs IRIS satellite for the prediction of solar flares using the Multiple Instance Learning (MIL) paradigm. While standard supervised learning models expect a label for every instance, MIL relaxes this and only considers bags of instances to be labeled. This is ideally suited for flare prediction with IRIS data that consists of time series of bags of UV spectra measured along the instrument slit. In particular, we consider the readout window around the Mg II h&k lines that encodes information on the dynamics of the solar chromosphere. Our MIL models are not only able to predict whether flares occur within the next 25 minutes with accuracies of around 90%, but are also able to explain which spectral profiles were particularly important for their bag-level prediction. This information can be used to highlight…
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Taxonomy
TopicsSolar Radiation and Photovoltaics
Methodsk-Means Clustering
