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20212026
most citedPlasma Emission Induced By Electron Beam in Weakly Magnetized Plasmas

20 citations · 104 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2026

Coronal Diagnostics Via Modelling Periodic-Beaded Stripes of Solar Radio Bursts

Chuanyang Li, Yao Chen, Bing Wang +11

Using high-resolution data from the Chashan Broadband Solar radio spectrometer at meter wavelengths (CBSm) of the Chinese Meridian Project-Phase II (CMP-II), Li et al. (2025) ident…

physics.space-ph2025

Particle in cell simulation on mode conversion of Saturn's 20 kHz narrowband radio emission

Zhoufan Mu, Yao Chen, Tangmu Li +3

The Z-to-O mode conversion at the density gradient is the prevailing mechanism of narrowband (NB) radio emission in planetary magnetosphere. Most previous numerical models were for…

astro-ph.SR2024

Prevalence of non-standard collapsing of strong Langmuir turbulence in solar corona plasmas

Yaokun Li, Haomin Sun, Hao Ning +4

We present a fully-kinetic simulation of the full life cycle of strong Langmuir turbulence (SLT) excited by electron beams that are accelerated under the solar corona conditions. W…

physics.plasm-ph2022★ 7 cited

Plasma emission induced by ring-distributed energetic electrons in overdense plasmas

Yao Chen, Zilong Zhang, Sulan Ni +3

According to the standard scenario of plasma emission, escaping radiations are generated by the nonlinear development of the kinetic bump-on-tail instability driven by a single bea…

physics.plasm-ph2022★ 15 cited

Verification of the standard theory of plasma emission with particle-in-cell simulations

Zilong Zhang, Yao Chen, Sulan Ni +4

The standard theory of plasma emission is based on kinetic couplings between a single beam of energetic electrons and unmagnetized thermal plasmas, involving multi-step nonlinear w…

physics.plasm-ph2022★ 20 cited

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…

astro-ph.SR2021★ 13 cited

Harmonic maser emissions from electrons with loss-cone distribution in solar active regions

Hao Ning, Yao Chen, Sulan Ni +4

Electron cyclotron maser emission (ECME) is regarded as a plausible source for the coherent radio radiations from solar active regions (e.g., solar radio spikes). In this Letter, w…

astro-ph.SR2021★ 14 cited

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…

physics.plasm-ph2021★ 16 cited

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.…

astro-ph.SR2021★ 19 cited

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…