collaborators

6 papers

astro-ph.SR2026

Three-dimensional mapping of coronal magnetic field and plasma parameters in a solar flare

Tatyana Kaltman, Sijie Yu, Gregory D. Fleishman +1

Diagnosing solar flare conditions is essential for understanding coronal energy release. Using combined microwave and X-ray data, we reconstruct three-dimensional maps of the magne…

astro-ph.SR2026

Few Made It Out: A Multi-Messenger Study of an In Situ Solar Energetic Electron Event Driven by a Solar Jet

Meiqi Wang, Bin Chen, Mallory Wickline +4

When in situ solar energetic electron (SEE) events are closely associated with nonthermal flares, the escaping electron population is frequently observed to be much smaller than th…

astro-ph.SR2026

Dynamics of the coronal magnetic field in the 2022-10-02 X-class flare

Gregory D. Fleishman, Tatyana Kaltman, Sijie Yu

Solar flares are driven by release of free magnetic energy and often associated with restructurization of the magnetic field topology. Yet, observations of evolving magnetic field…

astro-ph.SR2025

Enigmatic centi-SFU and mSFU nonthermal radio transients detected in the middle corona

Surajit Mondal, Bin Chen, Sijie Yu +43

Decades of solar coronal observations have provided substantial evidence for accelerated particles in the corona. In most cases, the location of particle acceleration can be roughl…

astro-ph.SR2025

Measuring the Magnetic Field of a Coronal Mass Ejection from Low to Middle Corona

Xingyao Chen, Bin Chen, Sijie Yu +44

A major challenge in understanding the initiation and evolution of coronal mass ejections (CMEs) is measuring the magnetic field of the magnetic flux ropes (MFRs) that drive CMEs.…

astro-ph.SR2025

Energy Conversion and Electron Acceleration and Transport in 3D Simulations of Solar Flares

Xiaocan Li, Chengcai Shen, Xiaoyan Xie +6

Recent observations and simulations indicate that solar flares undergo extremely complex three-dimensional (3D) evolution, making 3D particle transport models essential for underst…