Predicting coronal mass ejection travel times using enhanced model-guided machine learning
M. Lampani, M. Rossi, S. Guastavino, M. Piana, A.M. Massone

TL;DR
This paper enhances physics-informed AI models for predicting coronal mass ejection travel times by integrating an extended drag-based model, improving applicability, robustness, and enabling real-time space weather forecasting.
Contribution
It introduces a generalized physics-driven AI framework incorporating the extended drag-based model, allowing for broader CME event applicability and improved robustness.
Findings
Achieves travel-time prediction accuracy comparable to state-of-the-art methods.
Demonstrates robustness under small variations in model parameters.
Proposes a multiclass classification for CME speed regimes for operational use.
Abstract
Coronal mass ejections (CMEs) are key drivers of space weather events, posing risks to both space-borne and ground-based systems. Accurate prediction of their arrival time at Earth is critical for impact mitigation. To this end, physics-informed artificial intelligence (AI) approaches have proven more effective than purely data-driven or physics-based methods, generally offering higher accuracy and better explainability than the former and lower computational cost than the latter. In this work, we propose a generalization of the physics-driven AI framework based on the classical drag-based model (DBM) by integrating the extended version of the drag-based model (EDBM). This enhancement allows us to include in the training process CME events whose interplanetary dynamics are incompatible with those assumed by the DBM. We achieve travel-time prediction accuracy comparable to…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Tropical and Extratropical Cyclones Research
