activity
20092026
most citedStreamer Waves Driven by Coronal Mass Ejections

78 citations · 329 across the 13 of their papers we have counts for

collaborators

14 papers

astro-ph.SR2026

Three-dimensional evolution of a solar filament with multipoint observations

Qingmin Zhang, Jun Dai, Beili Ying +6

In this paper, we first devise a geometrical model, featuring a torus-like flux rope based on the shape of 3DCORE model. The global shape of the torus is an ellipse, while the cros…

astro-ph.SR2025

Early Evolution of the Cavity and Core of a Coronal Mass Ejection in the Inner Corona

Shuting Li, Li Feng, Beili Ying +5

Coronal mass ejections (CMEs) typically exhibit a three-component structure in white-light (WL) coronagraphs. Utilizing the seamless observations of the inner corona ( 3 R$_\o…

astro-ph.SR2025

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…

astro-ph.SR2024

Alpha-Proton Differential Flow of A Coronal Mass Ejection at 15 Solar Radii

Xuechao Zhang, Hongqiang Song, Xiaoqian Wang +4

Alpha-proton differential flow () of coronal mass ejections (CMEs) and solar wind from the Sun to 1 au and beyond could influence the instantaneous correspondence of absolu…

astro-ph.SR2024

The differences in the origination and properties of the near-Earth solar wind between solar cycles 23 and 24

Xinzheng Shi, Hui Fu, Zhenghua Huang +5

The dependence of the sources and properties of the near-Earth solar wind on solar cycle activity is an important issue in solar and space physics. We use the improved two-step map…

astro-ph.SR2024

Comparison of Ion-Proton Differential Speed between ICMEs and Solar Wind near 1 au

Xuechao Zhang, Hongqiang Song, Chengxiao Zhang +6

The elemental abundance of ICMEs and solar wind near 1 au is often adopted to represent the abundance in the corresponding coronal sources. However, the absolute abundance of heavy…

astro-ph.SR2024

Formation of a streamer blob via the merger of multiple plasma clumps below 2Rs

Haiyi Li, Zhenghua Huang, Kaiwen Deng +7

Context. Propagating streamer blobs could be an important source of disturbances in the solar wind. Direct observations on formation of streamer blobs could be a proxy for understa…

astro-ph.SR2015★ 31 cited

Acceleration phases of a solar filament during its eruption

Hongqiang Song, Yao Chen, Jie Zhang +3

Filament eruptions often lead to coronal mass ejections (CMEs), which can affect critical technological systems in space and on the ground when they interact with the geo-magnetosp…

astro-ph.SR2015★ 15 cited

First Taste of Hot Channel in Interplanetary Space

Hongqiang Song, Jie Zhang, Yao Chen +3

Hot channel (HC) is a high temperature (10 MK) structure in the inner corona revealed first by Atmospheric Imaging Assembly (AIA) on board \textit{Solar Dynamics Observatory}…

physics.space-ph2014★ 55 cited

Temperature evolution of magnetic flux rope in a failed solar eruption

Hongqiang Song, Jie Zhang, Xin Cheng +4

In this presentation, we report for the first time the detailed temperature evolution process of the magnetic flux rope in a failed solar eruption. Occurred on January 05, 2013, th…

astro-ph.SR2011★ 35 cited

A Statistical Study on the Morphology of Rays and Dynamics of Blobs in the Wake of Coronal Mass Ejections

Hong-Qiang Song, Xiang-Liang Kong, Yao Chen +4

In this paper, with a survey through the Large Angle and Spectrometric Coronagraph (LASCO) data from 1996 to 2009, we present 11 events with plasma blobs flowing outwards sequentia…

astro-ph.SR2010★ 62 cited

A coronal seismological study with streamer waves

Y. Chen, S. W. Feng, B. Li +4

We present a novel method to evaluate the Alfven speed and the magnetic field strength along the streamer plasma sheet in the outer corona. The method is based on recent observatio…

astro-ph.SR2010★ 78 cited

Streamer Waves Driven by Coronal Mass Ejections

Y. Chen, H. Q. Song, B. Li +4

Between July 5th and July 7th 2004, two intriguing fast coronal mass ejection(CME)-streamer interaction events were recorded by the Large Angle and Spectrometric Coronagraph (LASCO…

astro-ph.SR2009★ 53 cited

Intrinsic Instability of Coronal Streamers

Y. Chen, X. Li, H. Q. Song +3

Plasma blobs are observed to be weak density enhancements as radially stretched structures emerging from the cusps of quiescent coronal streamers. In this paper, it is suggested th…