HAL (France)
open access
Electromagnetic emissions at the plasma frequency by type III solar radio bursts in solar wind and coronal plasmas
Type III solar radio bursts are produced by near-relativistic electron beams accelerated in the solar corona that propagate along open magnetic field lines into the solar wind. These beams generate Langmuir/Z-mode (LZ) wave turbulence, which is converted into electromagnetic radiation near the plasm
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