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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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.