Electromagnetic Wave Emissions from a Turbulent Plasma with Density Fluctuations

In the solar wind, Langmuir turbulence can generate electromagnetic waves at the fundamental plasma frequency p. This process can likely result from either linear wave transformations on the ambient random density inhomogeneities or resonant three-wave interactions involving Langmuir waves and ion a...

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Veröffentlicht in:	The Astrophysical journal 2018-12, Vol.868 (2), p.104
Hauptverfasser:	Volokitin, A. S., Krafft, C.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Computer simulation Electric currents Electromagnetic radiation Fluctuations Langmuir turbulence Langmuir waves Mathematical models Numerical simulations Physics Plasma Plasma density Plasma frequencies Plasma temperature plasmas Plasmas (physics) Radiation Solar radio bursts Solar wind Spacecraft Spatial distribution Sun: flares Sun: radio radiation Turbulence Wave interaction Wavelengths waves
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