bandeau ATST

Evidence of Langmuir/Z-mode Wave Decay into Z-mode Electromagnetic Radiation in the Solar Wind
Francisco Javier Polanco Rodríguez  1@  , Catherine Krafft  2  , Philippe Savoini  2  
1 : Laboratoire de Physique des Plasmas
Observatoire de Paris, Ecole Polytechnique, Sorbonne Université, Université Paris-Saclay, Centre National de la Recherche Scientifique
2 : Laboratoire de Physique des Plasmas
LPP, CNRS, Palaiseau, France, Sorbonne Univesité Paris 6, CNRS, Université Paris Sud, Université Paris Saclay, CNRS

The nonlinear decay of Langmuir/Z-mode waves into electromagnetic Z-mode wave radiation near the plasma frequency is studied in the framework of Particle-In-Cell simulations. Guided by the numerical study, a Langmuir wave snapshot recorded during the encounter of the Solar Orbiter satellite with an electron beam associated with a Type III radio burst is found to exhibit the generation of Z-mode waves through this process. The decay process is identified through multiple lines of evidence: satisfaction of frequency and wavevector resonance conditions, strong phase coherence and temporal coincidence between the interacting waves, exclusion of competing mechanisms, and full agreement with theoretical predictions. Two-dimensional Particle-in-cell simulations, conducted under close beam-plasma conditions, successfully reproduce the key features of the observations. Notably, they suggest that the wave packet observed by Solar Orbiter may be trapped within an extended, nearly flat-bottomed density well, where the decay process is not overcome by wave scattering on random density fluctuations and subsequent mode conversion effects.


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