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astro-ph.SR2026
How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics
Zheng Sun, Julián D. Alvarado-Gómez, Hui Tian
Observations show that stellar coronal mass ejection (CME) candidates display relatively lower kinetic energies compared to expectations from solar flare-CME relations extrapolated…
astro-ph.SR2026
Fine-scale downflows above flare ribbons captured by Solar Orbiter/EUI
Zheng Sun, Alexander G. M. Pietrow, Malcolm K. Druett +8
In solar flares, flare ribbons map chromospheric footpoints where flare energy deposition occurs. These locations are associated with field aligned energy transport from the corona…