Structure and evolution of active region
Quantitative characterization of active-region magnetic structure based on geometric property of force-free α
Merging and Fragmentation in the Solar Active Region 10930 Caused by Emerging Magnetic Flux Tube with Asymmetric Field-Line Twist Distribution along Its Axis
MHD Simulation for Investigating the Dynamic State Transition Responsible for Solar Eruption in Active Region 12158
Structural properties of the solar flare-producing coronal current system developed in emerging magnetic flux tube
Distribution characteristics of coronal current density as indicator for the occurrence of solar flare
MHD simulation for investigating the evolutionary path of solar magnetic field that emerges, structures itself, erupts, and produces flare
Investigation of force-freeness of emerging magnetic fields via application of virial theorem to MHD simulations
Scaling laws for magnetic flux, free magnetic energy, and relative magnetic helicity in emerging flux region
Characteristic development of magnetic shear in flare-producing sunspot
Dynamic and topological features of emerging magnetic fields
Flare-producing active region's evolution characterized by magnetic helicity
Evaluation of force-free approximation of coronal magnetic field
Comparison of MCC model of coronal magnetic field to MHD simulation
Sigmoid structure of emerging flux tube