A simple GUI to associate an in-situ ICME to its likely solar CME source by back-propagating the event via the Drag-Based Model (DBM) and propagating uncertainties.
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Updated
Apr 30, 2026 - Python
A simple GUI to associate an in-situ ICME to its likely solar CME source by back-propagating the event via the Drag-Based Model (DBM) and propagating uncertainties.
On March 7, 2012, active region 11429 produced an X5.4 flare (00:02 UTC).
Deep learning models for predicting extreme solar activity using satellite observations.
Our submission for the IBM-Z Datathon 2024. Classifying the geoeffectiveness and predicting the arrival time of Coronal Mass Ejections (CMEs).
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