87 citations · 875 across the 30 of their papers we have counts for
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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…