activity
20152020
most citedMagnetohydrodynamic Simulation of the X2.2 Solar Flare on 2011 February 15: II. Dynamics Connecting the Solar Flare and the Coronal Mass Ejection

69 citations · 185 across the 8 of their papers we have counts for

collaborators

10 papers

astro-ph.SR20207 cited

Extrapolation of Three-dimensional Magnetic Field Structure in Flare-productive Active Regions with Different Initial Conditions

Y. Kawabata, S. Inoue, T. Shimizu

The nonlinear force-free field (NLFFF) modeling has been extensively used as a tool to infer three-dimensional (3D) magnetic field structure. In this study, the dependency of the N…

astro-ph.SR202014 cited

Chromospheric magnetic field: A comparison of He I 10830 A observations with nonlinear force-free field extrapolation

Yusuke Kawabata, Andrés Asensio Ramos, Satoshi Inoue +1

The nonlinear force-free field (NLFFF) modeling has been extensively used to infer the three-dimensional (3D) magnetic field in the solar corona. One of the assumptions in the NLFF…

astro-ph.SR202013 cited

Intrusion of Magnetic Peninsula toward the Neighboring Opposite-polarity Region That Triggers the Largest Solar Flare in Solar Cycle 24

Yumi Bamba, Satoshi Inoue, Shinsuke Imada

The largest X9.3 solar flare in solar cycle 24 and the preceding X2.2 flare occurred on September 6, 2017, in the solar active region NOAA 12673. This study aims to understand the…

astro-ph.SR202033 cited

Comparative Study of Data-driven Solar Coronal Field Models Using a Flux Emergence Simulation as a Ground-truth Data Set

Shin Toriumi, Shinsuke Takasao, Mark C. M. Cheung +4

For a better understanding of magnetic field in the solar corona and dynamic activities such as flares and coronal mass ejections, it is crucial to measure the time-evolving corona…

astro-ph.SR201916 cited

A Magnetohydrodynamic Relaxation Method for Non-Force-Free Magnetic Field in Magnetohydrostatic Equilibrium

Takahiro Miyoshi, Kanya Kusano, Satoshi Inoue

A nonlinear force-free field (NLFFF) extrapolation is widely used to reconstruct the three-dimensional magnetic field in the solar corona from the observed photospheric magnetic fi…

astro-ph.SR2019

Onset Mechanism of M6.5 Solar Flare Observed in Active Region 12371

Jihye Kang, Satoshi Inoue, Kanya Kusano +2

We studied a flare onset process in terms of stability of a three-dimensional (3D) magnetic field in active region 12371 producing an eruptive M6.5 flare in 2015 June 22. In order…