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Ling Chen

5 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author2
  • last author3

Across the 5 of 5 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR4
  • physics.plasm-ph1
ORCID 0000-0001-8058-2765
same name
  • Ling Chen — 3 papers, h 35
  • Ling Chen — 1 paper
  • Ling Chen — 1 paper, h 4
  • Ling Chen — 1 paper, h 22
  • Ling Chen — 1 paper
  • Ling Chen — 1 paper, h 4

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

most citedProperties of Short-wavelength Oblique Alfven and Slow Waves

63 citations · 90 across the 5 of their papers we have counts for

collaborators

4 papers

physics.plasm-ph2016★ 3 cited

The effect of electron holes on cyclotron maser emission driven by horseshoe distributions

G. Q. Zhao, Y. H. Chu, H. Q. Feng +1

This Brief Communication presents a quantitative investigation for the effect of electron holes on electron-cyclotron maser (ECM) driven by horseshoe distributions. The investigati…

astro-ph.SR2014

Excitation of Langmuir waves by the lower energy cutoff behavior of power-law electrons

Jianfei Tang, Dejin Wu, Guoqing Zhao +2

Langmuir waves (LWs), which are believed to play a crucial role in the plasma emission of solar radio bursts, can be excited by streaming instability of energetic electron beams. H…

astro-ph.SR2014★ 63 cited

Properties of Short-wavelength Oblique Alfven and Slow Waves

J. S. Zhao, Y. Voitenko, M. Y. Yu +2

Linear properties of kinetic Alfvén waves (KAWs) and kinetic slow waves (KSWs) are studied in the framework of two-fluid magnetohydrodynamics. We obtain the wave dispersion relatio…

astro-ph.SR2014★ 12 cited

A Model for Radio Emission from Solar Coronal Shocks

G. Q. Zhao, L. Chen, D. J. Wu

Solar coronal shocks are very common phenomena in the solar atmosphere and are believed to be the drivers of solar type II radio bursts. However, the microphysical nature of these…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.