Flare & Jet
Structural properties of solar flare-producing coronal current system developed in emerging magnetic flux tube
Distribution characteristics of coronal current density as indicator for occurrence of solar flare
MHD simulation for investigating the evolutionary path of solar magnetic field that emerges, structures itself, erupts, and produces flare
MHD model of solar penumbral microjet
Spontaneous compression of current sheet responsible for producing solar flare
Ph.D. Thesis
Dynamics of plasmoid associated with eruptive flare
Loop-top source of solar flare