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- W2927594964 abstract "Streaming proton and alpha particles are permeating in the solar wind and solar atmosphere. These particles considerably affect the normal waves in electron–proton–alpha plasmas, especially inducing electrostatic and electromagnetic ion/ion beam instabilities. This paper gives a comprehensive investigation on stable and unstable parallel-propagating wave modes in plasmas with streaming proton and alpha particles. It illustrates that at a large beam velocity condition, the backward-propagating fast-magnetosonic/whistler wave (Alfvén/proton-beam or Alfvén/alpha beam mode wave) turns to forward propagation in the core proton rest frame, and couples with forward-propagating Alfvén/alpha-cyclotron and alpha-cyclotron/proton-cyclotron waves (fast-magnetosonic/whistler wave), triggering Alfvén/proton-cyclotron and fast-magnetosonic/whistler instabilities. Furthermore, as perpendicular thermal pressures of proton and alpha beams are larger than their parallel thermal pressures, several new electromagnetic instabilities arise in the case of the low ion streaming velocity, where both Alfvén/proton-cyclotron and fast-magnetosonic/whistler instabilities are stable. This paper also predicts the possible ion/ion electromagnetic instabilities in solar coronal holes, which can give a constraint on the ion differential drift velocity therein." @default.
- W2927594964 created "2019-04-11" @default.
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- W2927594964 date "2019-03-29" @default.
- W2927594964 modified "2023-10-18" @default.
- W2927594964 title "Parallel-propagating Waves and Instabilities in Plasmas with Streaming Proton and Alpha Particles" @default.
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- W2927594964 doi "https://doi.org/10.3847/1538-4357/ab0896" @default.
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