CME | High Altitude Observatory

Coronal Mass Ejection

Magnetic field and plasma diagnostics for solar coronal mass ejections: A case study using the forward modeling approach

Liu Fe xiii 10747 line and CME eruption

Predicting the Geoeffectiveness of CMEs Using Machine Learning

A graph showing colored dots representing: True Negative; False Positive; True Positive, False Negative

Spectropolarimetric Insight into Plasma-Sheet Dynamics of a Solar Flare

Intensity and polarization data surrounding the current sheet formed on Sept 10 2017

Convolutional Neural Networks for Predicting the strength of the Near-Earth Magnetic Field Caused by Interplanetary Coronal Mass Ejections

Examples of various initial GLOW configurations

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