We present the results of kinetic numerical simulations that demonstrate the existence of a novel branchof electrostatic nonlinear waves driven by particle trapping processes. These waves have an acoustic-typedispersion with phase speed comparable to the ion thermal speed and would thus be heavily Landaudamped in the linear regime. At variance with the ion-acoustic waves, this novel electrostatic branch canexist at a small but finite amplitude even for low values of the electron to ion temperature ratio. Our resultsprovide a new interpretation of observations in space plasmas, where a significant level of electrostaticactivity is observed in the high frequency region of the solar-wind turbulent spectra.

New ion wave path in the energy cascade

VALENTINI, Francesco;VELTRI, Pierluigi
2011-01-01

Abstract

We present the results of kinetic numerical simulations that demonstrate the existence of a novel branchof electrostatic nonlinear waves driven by particle trapping processes. These waves have an acoustic-typedispersion with phase speed comparable to the ion thermal speed and would thus be heavily Landaudamped in the linear regime. At variance with the ion-acoustic waves, this novel electrostatic branch canexist at a small but finite amplitude even for low values of the electron to ion temperature ratio. Our resultsprovide a new interpretation of observations in space plasmas, where a significant level of electrostaticactivity is observed in the high frequency region of the solar-wind turbulent spectra.
2011
Vlasov simulation; electrostatic turbulence; solar wind
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.11770/147732
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