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20162022
most citedHarmonics of Solar Radio Spikes at Metric Wavelengths

25 citations · 201 across the 12 of their papers we have counts for

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9 papers · 1 filter

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…

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…

astro-ph.SR2019★ 8 cited

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…

astro-ph.SR2018★ 2 cited

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…

astro-ph.SR2018★ 25 cited

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…

astro-ph.SR2017★ 17 cited

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…

astro-ph.SR2017★ 23 cited

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…

astro-ph.SR2016★ 14 cited

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…

astro-ph.SR2016★ 20 cited

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…