Showing 1–20 of 39 results
/ Date/ Name
May 20, 2020A Solar Magnetic-fan Flaring Arch Heated by Non-thermal Particles and Hot Plasma from an X-ray Jet EruptionDec 30, 2020Magnetic reconnections in the presence of three-dimensional magnetic nulls and quasi-separatrix layersDec 4, 2024Magnetic Topology of quiet-Sun Ellerman bombs and associated Ultraviolet brighteningsJul 12, 2023Magnetohydrodynamics simulation of magnetic flux rope formation in a quadrupolar magnetic field configurationDec 8, 2022Evolution of magnetic fields and energy release processes during homologous eruptive flaresJul 23, 2020Effects of Cowling Resistivity in the Weakly-Ionized ChromosphereOct 31, 2018Successive flux rope eruptions from $δ$-Sunspots region of NOAA 12673 and associated X-class eruptive flares on 2017 September 6Jul 13, 2023Formation of an observed eruptive flux rope above the torus instability threshold through tether-cutting magnetic reconnectionJul 28, 2020An Eruptive Circular-ribbon Flare with Extended Remote BrighteningsApr 22, 2025Small-scale dynamic phenomena associated with interacting fan-spine topologies: quiet-Sun Ellerman bombs, UV brightenings, and chromospheric inverted-Y-shaped jetsOct 8, 2022Magnetohydrodynamics evolution of three-dimensional magnetic null in NOAA active region 11515 initiated using non-force-free field extrapolationOct 29, 2019Three-dimensional magnetic field structure of a flux emerging region in the solar atmosphereJul 24, 2020A data-driven MHD model of the weakly-ionized chromosphereSep 14, 2020Magnetohydrodynamic Simulation of Magnetic Null-point Reconnections and Coronal dimmings during the X2.1 flare in NOAA AR 11283Jul 26, 2021Heating of the solar chromosphere in a sunspot light bridge by electric currentsMay 25, 2025Coronal dimmings and what they tell us about solar and stellar coronal mass ejectionsFeb 14, 2020Identification of Pre-flare Processes and Their Possible Role in Driving a Large-scale Flux Rope Eruption with Complex M-class Flare in the Active Region NOAA 12371Jan 19, 2025Data-Constrained Magnetohydrodynamics Simulation of a Confined X-class Flare in NOAA Active Region 11166Feb 19, 2021Are the brightest coronal loops always rooted in mixed-polarity magnetic flux?Aug 30, 2024High-resolution observations of recurrent jets from an arch filament system