activity
20092026
most citedA solar type II radio burst from CME-coronal ray interaction: simultaneous radio and EUV imaging

64 citations · 1.4k across the 69 of their papers we have counts for

collaborators

69 papers

astro-ph.SR2026

Kinetic Processes to Radio Burst: First Observational-driven Study in Coronal Loops

Mehdi Yousefzadeh, Marian Karlicky, Artem Koval +3

Understanding the origin of coherent solar radio bursts requires linking macroscopic coronal structures with the kinetic processes responsible for wave generation. We investigate e…

astro-ph.SR2023

Effects of Coronal Magnetic Field Configuration on Particle Acceleration and Release during the Ground Level Enhancement Events in Solar Cycle 24

Wenlong Liu, Xiangliang Kong, Fan Guo +6

Ground level enhancements (GLEs) are extreme solar energetic particle (SEP) events that are of particular importance in space weather. In solar cycle 24, two GLEs were recorded on…

astro-ph.SR2023★ 21 cited

Why "solar tsunamis" rarely leave their imprints in the chromosphere

Ruisheng Zheng, Yihan Liu, Wenlong Liu +10

Solar coronal waves frequently appear as bright disturbances that propagate globally from the eruption center in the solar atmosphere, just like the tsunamis in the ocean on Earth.…

astro-ph.SR2023★ 2 cited

Imaging Preflare Broadband Pulsations in the Decimetric-metric Wavelengths

Maoshui Lv, Baolin Tan, Ruisheng Zheng +4

Preflare activities contain critical information about the pre-cursors and causes of solar eruptions. Here we investigate the characteristics and origin of a group of broadband pul…

astro-ph.SR2023★ 14 cited

Unveiling the mechanism for the rapid acceleration phase in a solar eruption

Ze Zhong, Yang Guo, Thomas Wiegelmann +2

Two major mechanisms have been proposed to drive the solar eruptions: the ideal magnetohydrodynamic instability and the resistive magnetic reconnection. Due to the close coupling a…

astro-ph.SR2022★ 21 cited

On the Nature of the Three-part Structure of Solar Coronal Mass Ejections

Hongqiang Song, Jie Zhang, Leping Li +4

Coronal mass ejections (CMEs) result from eruptions of magnetic flux ropes (MFRs) and can possess a three-part structure in white-light coronagraphs, including a bright front, dark…