23 citations · 72 across the 11 of their papers we have counts for
11 papers
Solar jet-induced perturbation propagating through coronal loops and in-loop electron beam transport indicated by type II and type N radio bursts
Yingli Cui, Xiangliang Kong, Zhentong Li +12
Solar type II radio bursts are commonly attributed to coronal shocks driven by coronal mass ejections (CMEs). However, some metric type II bursts have occasionally been reported to…
A Flare-related Decimetric Type-IV Radio Burst Induced by the X2 Radiation of Electron Cyclotron Maser Emission
Maoshui Lv, Ze Zhong, Xiangliang Kong +9
The radiation mechanism of decimetric wideband and pulsating radio bursts from the Sun (in terms of decimetric type-IV (t-IVdm) burst) and other flaring stars is a long-standing pr…
A Multi-Peak Solar Flare with a High Turnover Frequency of The Gyrosynchrotron Spectra from the Loop-Top Source
Zhao Wu, Alexey Kuznetsov, Sergey Anfinogentov +8
The origin of multiple peaks in lightcurves of various wavelengths remains illusive during flares. Here we discuss the flare of SOL2023-05-09T03:54M6.5 with six flux peaks as recor…
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.…
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…
The first flare observation with a new solar microwave spectrometer working in 35-40 GHz
F. Yan, Z. Wu, Z. Shang +3
The microwave spectrum contains valuable information about solar flares. Yet, the present spectral coverage is far from complete and broad data gaps exist above 20 GHz. Here we rep…
Twin extreme ultraviolet waves in the solar corona
Ruisheng Zheng, Bing Wang, Liang Zhang +2
Solar extreme ultraviolet (EUV) waves are spectacular propagating disturbances with EUV enhancements in annular shapes in the solar corona. These EUV waves carry critical informati…
Formation and Immediate Deformation of a Small Filament Through Intermittent Magnetic Interactions
Ruisheng Zheng, Liang Zhang, Changhui Rao +4
It is generally believed that filament formation involves a process of the accumulation of magnetic energy. However, in this paper we discuss the idea that filaments will not erupt…
Compound eruptions of twin flux ropes in a solar active region
Ruisheng Zheng, Liang Zhang, Bing Wang +6
Compound eruptions represent that multiple closely spaced magnetic structures erupt consecutively within a short interval, and then lead to a single flare and a single CME. However…
Shock-wave radio probing of solar wind sources in coronal magnetic fields
A. Koval, M. Karlicky, A. Stanislavsky +3
The Space Weather effects in the near-Earth environment as well as in atmospheres of other terrestrial planets arise by corpuscular radiation from the Sun, known as the solar wind.…
The Inhomogeneity of Composition along the Magnetic Cloud Axis
Hongqiang Song, Qiang Hu, Xin Cheng +6
It is generally accepted that CMEs result from eruptions of magnetic flux ropes, which are dubbed as magnetic clouds in interplanetary space. The composition (including the ionic c…