collaborators

7 papers

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

High-resolution Observation of Mini-Filament Eruptions Near Coronal Hole Boundary and Their Response in Solar Corona

Nengyi Huang, Haimin Wang

We investigated mini-filament (MF) eruptions near coronal hole (CH) boundaries to explore their role in coronal dynamics and their potential contributions to the solar wind. Using…

astro-ph.SR2025

Solar Alfvenic Pulses and Mesoscale Solar Wind

Jeongwoo Lee, Manolis K. Georgoulis, Rahul Sharma +3

Large-scale solar ejections are well understood, but the extent to which small-scale solar features directly influence the solar wind remains an open question, primarily due to the…

astro-ph.SR2025

MVPinn: Integrating Milne-Eddington Inversion with Physics-Informed Neural Networks for GST/NIRIS Observations

Qin Li, Bo Shen, Haodi Jiang +5

We introduce MVPinn, a Physics-Informed Neural Network (PINN) approach tailored for solving the Milne-Eddington (ME) inversion problem, specifically applied to spectropolarimetric…

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…