Showing 1–17 of 17 results
/ Date/ Name
Mar 29, 2022Decayless longitudinal oscillations of a solar filament maintained by quasi-periodic jetsApr 11, 2022Dynamics and Kinematics of the EUV Wave Event on 6 May 2019Sep 14, 2022Prominence fine structures in weakly twisted and highly twisted magnetic flux ropesAug 21, 2025A unified model of solar prominence formation with self-consistent heatingMay 16, 2025Dependence of the intensity of the nonwave component of EUV waves on coronal magnetic field configurationNov 24, 2023Formation of a long filament through the connection of two filament segments observed by CHASEOct 16, 2023Evaluating residual acceleration noise for TianQin gravitational waves observatory with an empirical magnetic field modelAug 30, 2024Periodic Coronal Rain Driven by Self-consistent Heating Process in a Radiative Magnetohydrodynamic SimulationDec 28, 2024The magnetic origin of the mystery of rare H$α$ Moreton wavesApr 4, 2026Preferential Appearance of H$α$ Moreton Waves along Photospheric Magnetic Network BoundariesFeb 25, 2025The Birth of a Major Coronal Mass Ejection with Intricate Magnetic Structure from Multiple Active RegionsOct 30, 2023Data-driven Modeling of a Coronal Magnetic Flux Rope: from Birth to DeathApr 28, 2021A unified model of solar prominence formationFeb 11, 2026Data-driven Magnetohydrodynamic Simulation of the Initiation of a Coronal Mass Ejection with Multiple StagesNov 22, 2023Modelling the propagation of coronal mass ejections with COCONUT: implementation of the Regularized Biot-Savart Laws flux rope modelJul 12, 2024How coronal mass ejections are influenced by the morphology and toroidal flux of their source magnetic flux ropes?Mar 23, 2026On the Constraints and Observational Manifestations of Failed Solar Eruptions in Toroidal Magnetic Cage