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- W2020105318 abstract "In the present study, the dissipation processes of circularly polarized Alfvén waves in solar wind plasmas including beam components are numerically discussed by using a 2-D hybrid simulation code. Numerical results suggest that the parent Alfvén waves are rapidly dissipated due to the presence of the beam-induced obliquely propagating waves, such as kinetic Alfvén waves. The nonlinear wave-wave coupling is directly evaluated by using the induction equation for the parent wave. It is also observed both in the 1-D and 2-D simulations that the presence of large amplitude Alfvén waves strongly suppresses the beam instabilities." @default.
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- W2020105318 date "2012-08-01" @default.
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- W2020105318 title "Nonlinear dissipation of circularly polarized Alfvén waves due to the beam-induced obliquely propagating waves" @default.
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- W2020105318 doi "https://doi.org/10.1063/1.4748296" @default.
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