A Three-dimensional Model for the Evolution of Magnetohydrodynamic Turbulence in the Outer Heliosphere

A Three-dimensional Model for the Evolution of Magnetohydrodynamic Turbulence in the Outer Heliosphere

We present a time-dependent, three-dimensional single-fluid model for the transport of magnetohydrodynamic (MHD) turbulence that is self-consistently evolving with a dynamic large-scale solar wind in the outer heliosphere. The emphasis is on the region beyond the termination shock, where the solar w...

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Bibliographic Details
Main Authors: Jens Kleimann, Sean Oughton, Horst Fichtner, Klaus Scherer
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Heliosheath
Interplanetary turbulence
Solar wind termination
Online Access:https://doi.org/10.3847/1538-4357/acd84e

Internet

https://doi.org/10.3847/1538-4357/acd84e

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