20 citations · 37 across the 3 of their papers we have counts for
6 papers
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…
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…
The Role of a Tiny Brightening in a Huge Geo-effective Solar Eruption Leading to the St Patrick's Day Storm
Yumi Bamba, Satoshi Inoue, Keiji Hayashi
The largest magnetic storm in solar cycle 24 was caused by a fast coronal mass ejection (CME) that was related to a small C9.1 flare that occurred on 15 March 2015 in solar active…
Magnetohydrodynamic Modeling of a Solar Eruption Associated with X9.3 Flare Observed in Active Region 12673
Satoshi Inoue, Daikou Shiota, Yumi Bamba +1
On SOL2017-09-06 solar active region 12673 produced an X9.3 flare which is regarded as largest to occur in solar cycle 24. In this work we have preformed a magnetohydrodynamic (MHD…
A Study of Magnetic Field Characteristics of Flaring Active Region Based on Nonlinear Force-free Field Extrapolation
Johan Muhamad, Kanya Kusano, Satoshi Inoue +1
Coronal magnetic fields are responsible for the onset of solar flares and solar eruptions. However, the type of magnetic field parameters that can be used to measure the critical c…
Evaluation of Applicability of a Flare Trigger Model based on Comparison of Geometric Structures
Yumi Bamba, Kanya Kusano
The triggering mechanism(s) and critical condition(s) of solar flares are still not completely clarified, although various studies have attempted to elucidate them. We have also pr…