23 citations · 23 across the 1 of their papers we have counts for
6 papers
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…
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…