64 citations · 535 across the 19 of their papers we have counts for
19 papers
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…
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.…
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…
Source Imaging of a Moving Type-IV Solar Radio Burst and its Role in Tracking Coronal Mass Ejection From the Inner to the Outer Corona
V. Vasanth, Yao Chen, Maoshui Lv +5
Source imaging of solar radio bursts can be used to track energetic electrons and associated magnetic structures. Here we present a combined analysis of data at different wavelengt…
An extreme ultraviolet wave generating upward secondary waves in a streamer-like solar structure
Ruisheng Zheng, Yao Chen, Shiwei Feng +2
Extreme ultraviolet (EUV) waves, spectacular horizontally propagating disturbances in the low solar corona, always trigger horizontal secondary waves (SWs) when they encounter ambi…
Harmonics of Solar Radio Spikes at Metric Wavelengths
Shiwei Feng, Yao Chen, Chuanyang Li +6
This paper presents the latest observations from the newly-built solar radio spectrograph at the \emph{Chashan Solar Observatory}. On July 18 2016, the spectrograph records a solar…
A Solar Radio Dynamic Spectrograph with Flexible Temporal-spectral Resolution
Qing-Fu Du, Lei Chen, Yue-Chang Zhao +7
The observation and research of the solar radio emission have unique scientific values in solar and space physics and related space weather forecasting applications, since the obse…
EUV and Magnetic Activities Associated with Type-I Solar Radio Bursts
Chuanyang Li, Yao Chen, Bing Wang +4
Type-I bursts (i.e. noise storms) are the earliest-known type of solar radio emission at the metre wavelength. They are believed to be excited by non-thermal energetic electrons ac…
An Eruptive Hot-Channel Structure Observed at Metric Wavelength as a Moving Type-IV Solar Radio Burst
V. Vasanth, Yao Chen, Shiwei Feng +5
Hot channel (HC) structure, observed in the high-temperature passbands of the AIA/SDO, is regarded as one candidate of coronal flux rope which is an essential element of solar erup…
Observation of a Metric Type N Solar Radio Burst
Xiangliang Kong, Yao Chen, Shiwei Feng +7
Type III and type-III-like radio bursts are produced by energetic electron beams guided along coronal magnetic fields. As a variant of type III bursts, Type N bursts appear as the…
Decameter Stationary Type IV Burst in Imaging Observations on the 6th of September 2014
Artem Koval, Aleksander Stanislavsky, Yao Chen +3
First-of-its-kind radio imaging of decameter solar stationary type IV radio burst has been presented in this paper. On 6 September 2014 the observations of type IV burst radio emis…
Electron Acceleration at a Coronal Shock Propagating Through a Large-scale Streamer-like Magnetic Field
Xiangliang Kong, Yao Chen, Fan Guo +3
With a test-particle simulation, we investigate the effect of large-scale coronal magnetic fields on electron acceleration at an outward-propagating coronal shock with a circular f…
An observational revisit of band-split solar type-II radio bursts
Guohui Du, Xiangliang Kong, Yao Chen +3
Band split of solar type II radio bursts, discovered several decades ago, is a fascinating phenomenon with the type-II lanes exhibiting two almost-parallel sub-bands with similar m…
Possible role of coronal streamer as magnetically-closed structure in shock-induced energetic electrons and metric type II radio bursts
Xiangliang Kong, Yao Chen, Fan Guo +4
Two solar type II radio bursts, separated by ~24 hours in time, are examined together. Both events are associated with coronal mass ejections (CMEs) erupting from the same active r…
A solar type II radio burst from CME-coronal ray interaction: simultaneous radio and EUV imaging
Yao Chen, Guohui Du, Li Feng +5
Simultaneous radio and extreme ultraviolet (EUV)/white-light imaging data are examined for a solar type II radio burst occurring on 2010 March 18 to deduce its source location. Usi…
A broken solar type II radio burst induced by a coronal shock propagating across the streamer boundary
Xiang-Liang Kong, Yao Chen, Gang Li +4
We discuss an intriguing type II radio burst that occurred on 2011 March 27. The dynamic spectrum was featured by a sudden break at about 43 MHz on the well-observed harmonic branc…
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…
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…
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…