Simulating coronal mass ejections to aid space weather forecasting (IMAGE)

University of Texas at Austin, Texas Advanced Computing Center

Simulating coronal mass ejections to aid space weather forecasting

Caption

Magnetic field line configuration of the coronal mass ejection inserted at the inner boundary R = 0.1 AU, shown with the red sphere.

Credit

Talwinder Singh, Tae K. Kim , Nikolai V. Pogorelov , and Charles N. Arge

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