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astro-ph.SR2026
COCONUT: Toward practical time-evolving Sun-to-Earth magnetohydrodynamic modeling
Haopeng Wang, Stefaan Poedts, Andrea Lani +16
Due to computational efficiency and numerical stability limitations, coronal simulations constrained by static magnetograms are typically performed first and then used to drive inn…
astro-ph.SR2025
Size Distributions of Arcsecond-Scale Properties of Solar Flare Ribbons
Yue Zhang, Rui Liu, Wensi Wang +1
Solar flare ribbons are believed to map the footpoints of newly reconnected magnetic flux tubes, therefore shedding light on the reconnecting current sheet, which is rarely observe…