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Dynamics of electron beams in the solar corona plasma with density fluctuations

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arxiv 1904.05650 v1 pith:R5ZFV7T5 submitted 2019-04-11 astro-ph.SR astro-ph.HEphysics.plasm-phphysics.space-ph

classification astro-ph.SRastro-ph.HEphysics.plasm-phphysics.space-ph
keywords plasmadistributionelectronwavesbeambeamsinhomogeneitiesspatial
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The problem of beam propagation in a plasma with small scale and low intensity inhomogeneities is investigated. It is shown that the electron beam propagates in a plasma as a beam-plasma structure and is a source of Langmuir waves. The plasma inhomogeneity changes the spatial distribution of the waves. The spatial distribution of the waves is fully determined by the distribution of plasma inhomogeneities. The possible applications to the theory of radio emission associated with electron beams are discussed.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Electromagnetic radiation by turbulent, magnetized and randomly inhomogeneous solar radio sources generated by electron beams

    astro-ph.SR 2025-06 conditional novelty 7.0 of 10

    Most fundamental radio emission from beam-generated turbulence in Type III sources is trapped Z-mode; the small escaping fraction is mainly O-mode, with X-mode only in weakly magnetized sources.

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