The Transport and Evolution of MHD Turbulence throughout the Heliosphere: Models and Observations

A detailed study of solar wind turbulence throughout the heliosphere in both the upwind and downwind directions is presented. We use an incompressible magnetohydrodynamic (MHD) turbulence model that includes the effects of electrons, the separation of turbulence energy into proton and electron heati...

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Bibliographic Details
Main Authors: Laxman Adhikari, Gary P. Zank, Lingling Zhao
Format: Article
Language:English
Published: MDPI AG 2021-10-01
Series:Fluids
Subjects:
Online Access:https://www.mdpi.com/2311-5521/6/10/368