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.
Dynamics of electron beams in the solar corona plasma with density fluctuations
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abstract
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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Electromagnetic radiation by turbulent, magnetized and randomly inhomogeneous solar radio sources generated by electron beams
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.