Secondary Proton Beam Instability in a Turbulent Solar Wind at 50 R ⊙

We investigate a secondary proton beam instability coexisting with the ambient solar wind turbulence at 50 R _☉ . Three-dimensional hybrid numerical simulations (particle ions and a quasi-neutralizing electron fluid) are carried out with the plasma parameters in the observed range. In the turbulent...

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Bibliographic Details
Main Authors: S. A. Markovskii, Bernard J. Vasquez
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/acf656