collaborators

7 papers

astro-ph.SR2026

Non-thermal Sources from Stereoscopic Hard X-ray and Earth-based Microwave Observations in a Data-Constrained Magnetohydrodynamic Simulation

Keitarou Matsumoto, Satoshi Inoue, Meiqi Wang +5

We analyze the X7.1 flare on 2024 October 1 from NOAA AR 13842 using hard X-ray (HXR) imaging, microwave observations by the Expanded Owens Valley Solar Array (EOVSA), and a three-…

astro-ph.SR2026

Stereoscopic Observations of Solar X-ray Sources Explained by a Data-Constrained Magnetohydrodynamic Simulation

Keitarou Matsumoto, Satoshi Inoue, Meiqi Wang +6

We investigated the three-dimensional (3D) magnetic structures and dynamics responsible for particle acceleration in an X7.1-class flare that occurred on October 1, 2024, in NOAA a…

astro-ph.SR2025

Driving mechanisms of solar active region geysers: The role of interacting magnetic flux

Aabha Monga, Satoshi Inoue, Jeongwoo Lee +2

Active region recurrent jets are manifestations of episodic magnetic energy release processes driven by complex interactions in the lower solar atmosphere. While magnetic flux emer…

astro-ph.SR2025

Large Magnetic Flux Rope Formation in an X2.1 Flare observed on September 6, 2011

Arpita Roddanavar, Satoshi Inoue, Keiji Hayashi +3

Solar active region 11283 produced an X2.1 flare associated with a solar eruption on September 6, 2011. Observations revealed a preflare sigmoidal structure and a circular flare ri…

astro-ph.SR2025

A Data-constrained Magnetohydrodynamic Simulation of Successive X-class Flares in Solar Active Region 13842. II. Dynamics of the Solar Eruption Associated with the X9.0 Solar Flare

Keitarou Matsumoto, Satoshi Inoue, Keiji Hayashi +5

Active region NOAA 13842 produced two successive solar flares: an X7.1-class flare on October 1, 2024, and an X9.0-class flare on October 3, 2024. This study continues our previous…

astro-ph.SR2025

Acceleration of Solar Eruptions via Enhanced Torus Instability Driven by Small-Scale Flux Emergence

Satoshi Inoue, Takahiro Miyoshi, Keiji Hayashi +4

Despite decades of research, the fundamental processes involved in the initiation and acceleration of solar eruptions remain not fully understood, making them long-standing and cha…