Showing 1–20 of 28 results
/ Date/ Name
Aug 17, 2023Understanding the Lateral Drifting of an Erupting Filament with a Data-constrained Magnetohydrodynamic SimulationFeb 25, 2025The Birth of a Major Coronal Mass Ejection with Intricate Magnetic Structure from Multiple Active RegionsJul 26, 2021Formation and Characteristics of Filament Threads in Double-Dipped Magnetic Flux TubesJul 6, 2021Magnetic Twists of Solar FilamentsNov 22, 2023Modelling the propagation of coronal mass ejections with COCONUT: implementation of the Regularized Biot-Savart Laws flux rope modelDec 12, 2023Rotation and Confined Eruption of a Double Flux-Rope SystemAug 13, 2024Recent advances in solar data-driven MHD simulations of the formation and evolution of CME flux ropesMar 23, 2026On the Constraints and Observational Manifestations of Failed Solar Eruptions in Toroidal Magnetic CageDec 6, 2023Observational study of intermittent solar jets: p-mode modulationDec 8, 2025Two-stage primary acceleration in filament initial eruption under a fan-spine magnetic configurationSep 19, 2025Flare energetics, CME launch and heliospheric propagation for the May 2024 events, as derived from ensemble MHD modellingNov 25, 2025Data-constrained magnetohydrodynamic simulation of global solar corona including solar wind effects within 2.5 $R_\odot$Feb 24, 2026Multiple Extreme Ultraviolet Peaks Attributed to Three-dimensional Magnetic Reconnection in a Long-duration Solar FlareSep 4, 2023Data-constrained Magnetohydrodynamic Simulation of an Intermediate Solar Filament EruptionDec 25, 2023A Method for Determining the Locations and Configurations of Magnetic Reconnection within 3D Turbulent PlasmasOct 24, 2024Enhanced Peak and Extended Cooling of the Extreme-ultraviolet Late Phase in a Confined Solar FlareJun 10, 2025Responses of a Coronal Hole to a Fast Flare-Driven Coronal WaveJan 31, 2026Elongation of a Solar Filament and its Three-Dimensional Numerical Reconstruction for Magnetic StructuresApr 21, 2025Data-constrained Magnetohydrodynamic Simulation of a Filament Eruption in a Decaying Active Region 13079 on a Global ScaleJun 24, 2025SIP-IFVM: An observation-based magnetohydrodynamic model of coronal mass ejection