activity
20232026
most citedA 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

3 citations · 3 across the 8 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2026

Statistical Analysis of Minifilament Eruptions Using Full-disk H Blue-wing Observations at Big Bear Solar Observatory

Artin Khaleghi, Qin Li, Nengyi Huang +2

This paper presents a comprehensive statistical analysis of minifilament eruptions (MFEs) using high-cadence full-disk H blue-wing observations from Big Bear Solar Observatory.…

astro-ph.SR2026

Predicting Associations between Solar Flares and Coronal Mass Ejections Using SDO/HMI Magnetograms and a Hybrid Neural Network

Jialiang Li, Vasyl Yurchyshyn, Jason T. L. Wang +6

Solar eruptions, including flares and coronal mass ejections (CMEs), have a significant impact on Earth. Some flares are associated with CMEs, and some flares are not. The associat…

astro-ph.SR2025

Fine Structures of Tiny Quiet Sun Jets Observed by Solar Orbiter and Big Bear Solar Observatory

Jeongwoo Lee, Dana Longcope, Junmu Youn +3

We present the first joint high-resolution observations of small-scale EUV jets using Solar Orbiter(SolO)'s Extreme Ultraviolet Imager and High Resolution Imager (HRI) and H ima…

astro-ph.SR2025★ 3 cited

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

Improving the Temporal Resolution of SOHO/MDI Magnetograms of Solar Active Regions Using a Deep Generative Model

Jialiang Li, Vasyl Yurchyshyn, Jason T. L. Wang +6

We present a novel deep generative model, named GenMDI, to improve the temporal resolution of line-of-sight (LOS) magnetograms of solar active regions (ARs) collected by the Michel…

astro-ph.SR2025

Prediction of Halo Coronal Mass Ejections Using SDO/HMI Vector Magnetic Data Products and a Transformer Model

Hongyang Zhang, Ju Jing, Jason T. L. Wang +6

We present a transformer model, named DeepHalo, to predict the occurrence of halo coronal mass ejections (CMEs). Our model takes as input an active region (AR) and a profile, where…

astro-ph.SR2024

Episodic energy release during the main- and post-impulsive phase of a solar flare

Yuqian Wei, Bin Chen, Sijie Yu +3

When and where the magnetic field energy is released and converted in eruptive solar flares remains an outstanding topic in solar physics. To shed light on this question, here we r…

astro-ph.SR2023

Estimating Coronal Mass Ejection Mass and Kinetic Energy by Fusion of Multiple Deep-learning Models

Khalid A. Alobaid, Yasser Abduallah, Jason T. L. Wang +5

Coronal mass ejections (CMEs) are massive solar eruptions, which have a significant impact on Earth. In this paper, we propose a new method, called DeepCME, to estimate two propert…

astro-ph.IM2023

Quantifying Energy Release in Solar Flares and Solar Eruptive Events: New Frontiers with a Next-Generation Solar Radio Facility

Bin Chen, Dale E. Gary, Sijie Yu +16

Solar flares and the often associated solar eruptive events serve as an outstanding laboratory to study the magnetic reconnection and the associated energy release and conversion p…