87 citations · 875 across the 30 of their papers we have counts for
30 papers
Particle acceleration and their escape into the heliosphere in solar flares with open magnetic field
Mykola Gordovskyy, Philippa K. Browning, Kanya Kusano +2
Energetic particle populations in the solar corona and in the heliosphere appear to have different characteristics even when produced in the same solar flare. It is not clear what…
A Comparative Study of Solar Active Region 12371 with Data-constrained and Data-driven MHD Simulations
Satoshi Inoue, Keiji Hayashi, Takahiro Miyoshi +2
We performed two data-based magnetohydrodynamic (MHD) simulations for solar active region 12371 which produced an M6.5 flare. The first simulation is a full data-driven simulation…
A Data-constrained Magnetohydrodynamic Simulation of the X1.0 Solar Flare of 2021 October 28
Daiki Yamasaki, Satoshi Inoue, Yumi Bamba +2
The solar active region NOAA 12887 produced a strong X1.0 flare on 2021 October 28, which exhibits X-shaped flare ribbons and a circle-shaped erupting filament. To understand the e…
An Evolution and Eruption of the Coronal Magnetic Field through a Data-Driven MHD Simulation
Satoshi Inoue, Keiji Hayashi, Takahiro Miyoshi
We present a newly developed data-driven magnetohydrodynamics (MHD) simulation code under a zero-beta approximation based on a method proposed by Hayashi et al. 2018 and 2019. Alth…
An MHD Modeling of Successive X2.2 and X9.3 Solar Flares of 2017 September 6
Satoshi Inoue, Yumi Bamba
Solar active region 12673 produced two successive X-class flares (X2.2 and X9.3) approximately 3 hours apart in September 2017. The X9.3 was the recorded largest solar flare in Sol…
Evolution of the Non-potential Magnetic Field in the Solar Active Region 12673 Based on a Nonlinear Force-free Modeling
Daiki Yamasaki, Satoshi Inoue, Shin'ichi Nagata +1
Active region (AR) 12673 produced many M-class and several X-class flares, one of which being an X9.3 flare, which is recorded as the largest solar flare in solar cycle 24. We stud…