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https://power2innovate.com/wp-content/uploads/2023/06/supercomputer-simulati-1.jpg800441Visualization of flow and SSD solution. Flow speed (left) and magnetic field strength (right) from a high-resolution SSD-active run with Re = 18,200 and PrM = 0.01 on the surface of the simulation box. Credit: Nature Astronomy (2023). DOI: 10.1038/s41550-023-01975-1 The sun’s strong, dynamic magnetic field can catapult huge jets of plasma known as coronal mass ejections (CMEs) out …