25 citations · 201 across the 12 of their papers we have counts for
12 papers
Plasma Emission Induced By Electron Beam in Weakly Magnetized Plasmas
Yao Chen, Zilong Zhang, Sulan Ni +3
Previous studies on the beam-driven plasma emission process were done mainly for unmagnetized plasmas. Here we present fully-kinetic electromagnetic particle-in-cell simulations to…
Harmonic elctron-cyclotron maser emissions driven by energetic electrons of the horseshoe distribution with application to solar radio spikes
Hao Ning, Yao Chen, Sulan Ni +4
Content. Electron-cyclotron maser emission (ECME) is the favored mechanism for solar radio spikes and has been investigated extensively since the 1980s. Most studies relevant to so…
An alternative form of the fundamental plasma emission through the coalescence of Z-mode waves with whistlers
Sulan Ni, Yao Chen, Chuanyang Li +3
Plasma emission (PE), i.e., electromagnetic radiation at the plasma frequency and its second harmonic, is a general process occurring in both astrophysical and laboratory plasmas.…
PIC Simulation of Double Plasma Resonance and Zebra Pattern of Solar Radio Bursts
Chuanyang Li, Yao Chen, Sulan Ni +3
Latest study reports that plasma emission can be generated by energetic electrons of DGH distribution via the electron cyclotron maser instability (ECMI) in plasmas characterized b…
Effect of the Temperature of Background Plasma and the Energy of Energetic Electrons on Z-Mode Excitation
Chuanyang Li, Yao Chen, Xiangliang Kong +2
It has been suggested that the Z-mode instability driven by energetic electrons with a loss-cone type velocity distribution is one candidate process behind the continuum and zebra…
Formation of Large Scale Coronal Loops Interconnecting Two Active Regions Through Gradual Magnetic Reconnection and Associated Heating Process
Guohui Du, Yao Chen, Chunming Zhu +5
Coronal loops interconnecting two active regions, called as interconnecting loops (ILs), are prominent large-scale structures in the solar atmosphere. They carry a significant amou…
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…
Interaction of two filaments in a long filament channel associated with twin coronal mass ejections
Ruisheng Zheng, Qingmin Zhang, Yao Chen +4
Using the high-quality observations of the Solar Dynamics Observatory, we present the interaction of two filaments (F1 and F2) in a long filament channel associated with twin coron…
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…
Solar jet-coronal hole collision and a related coronal mass ejection
Ruisheng Zheng, Yao Chen, Guohui Du +1
Jets are defined as impulsive, well-collimated upflows, occurring in different layers of the solar atmosphere with different scales. Their relationship with coronal mass ejections…