activity
20222025
most citedFine structures of radio bursts from flare star AD Leo with FAST observations

31 citations · 72 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2025

Radio dimming associated with filament eruptions in the meter and decimeter wavebands

Zhenyong Hou, Hui Tian, Jingye Yan +12

Filament eruptions are considered to be a common phenomenon on the Sun and other stars, yet they are rarely directly imaged in the meter and decimeter wavebands. Using imaging data…

astro-ph.SR2025★ 9 cited

Location and energy of electrons producing the radio bursts from AD Leo observed by FAST in December 2021

Philippe Zarka, Corentin K. Louis, Jiale Zhang +3

In a recent paper, we presented circularly polarized radio bursts detected by the radio telescope FAST from the flare star AD Leo on December 2-3, 2021, which were attributed to th…

astro-ph.SR2023★ 31 cited

Fine structures of radio bursts from flare star AD Leo with FAST observations

Jiale Zhang, Hui Tian, Philippe Zarka +8

Radio bursts from nearby active M-dwarfs have been frequently reported and extensively studied in solar or planetary paradigms. Whereas, their sub-structures or fine structures rem…

astro-ph.SR2022★ 4 cited

Implications for additional plasma heating driving the extreme-ultraviolet late phase of a solar flare with microwave imaging spectroscopy

Jiale Zhang, Bin Chen, Sijie Yu +6

Extreme-ultraviolet late phase (ELP) refers to the second extreme-ultraviolet (EUV) radiation enhancement observed in certain solar flares, which usually occurs tens of minutes to…

astro-ph.SR2022★ 21 cited

Can we detect coronal mass ejections through asymmetries of Sun-as-a-star extreme-ultraviolet spectral line profiles?

Zihao Yang, Hui Tian, Xianyong Bai +8

Coronal mass ejections (CMEs) are the largest-scale eruptive phenomena in the solar system. Associated with enormous plasma ejections and energy release, CMEs have an important imp…

astro-ph.SR2022★ 7 cited

Doppler shifts of spectral lines formed in the solar transition region and corona

Yajie Chen, Hardi Peter, Damien Przybylski +2

Context. Emission lines formed in the transition region and corona show dominantly redshifts and blueshifts, respectively. Aims. We investigate the Doppler shifts in a 3D radiation…