Showing 1–20 of 20 results
/ Date/ Name
Jan 14, 2020Continuous Null-Point Magnetic Reconnection Builds Up a Torus Unstable Magnetic Flux Rope Triggering the X9.3 Flare in Solar Active Region~12673Aug 14, 2023Data-driven MHD simulation of a sunspot rotating active region leading to solar eruptionAug 9, 2023A fundamental mechanism of solar eruption initiation in multipolar magnetic fieldJun 24, 2024Why are non-radial solar eruptions less frequent than radial ones?Feb 17, 2024A Model of Solar Magnetic Flux Rope Eruption Initiated Primarily by Magnetic ReconnectionAug 19, 2023Magnetic Reconnection as the Key Mechanism in Sunspot Rotation Leading to Solar EruptionOct 8, 2021Investigations of Sizes and Dynamical Motions of Solar Photospheric Granules by a Novel Granular Segmenting AlgorithmAug 23, 2019A Statistical Study of Solar Filament Eruptions That Forms High-Speed Coronal Mass EjectionsJul 17, 2021A fundamental mechanism of solar eruption initiationFeb 8, 2018Decipher the Three-Dimensional Magnetic Topology of a Great Solar FlareJul 29, 2023A model of failed solar eruption initiated and destructed by magnetic reconnectionOct 23, 2022Numerical Simulation of Solar Magnetic Flux Emergence Using the AMR--CESE--MHD CodeJan 9, 2022Homologous Coronal Mass Ejections Caused by Recurring Formation and Disruption of Current Sheet within a Sheared Magnetic ArcadeNov 9, 2021Numerical Simulation of a Fundamental Mechanism of Solar Eruption with Different Magnetic Flux DistributionsOct 31, 2018Magnetohydrodynamic Simulation of the X9.3 Flare on 2017 September 6: Evolving Magnetic TopologyNov 22, 2018A Two-Step Magnetic Reconnection in a Confined X-class Flare in Solar Active Region 12673Feb 12, 2020Data-driven MHD Simulation of the Formation and Initiation of a Large-scale Pre-flare Magnetic Flux Rope in Solar Active Region 12371Oct 8, 2017Reconstruction of a Large-scale Pre-flare Coronal Current Sheet Associated with an Homologous X-shaped FlareSep 24, 2025The role of photospheric magnetic flux diffusion in initiation of solar eruptionsFeb 20, 2025MHD Modeling of the Near-Sun Evolution of Coronal Mass Ejection Initiated from a Sheared Arcade