Energy Transport by Kelvin-Helmholtz Instability at the Magnetopause

By means of the formation of vortices in the nonlinear phase, the Kelvin Helmholtz instability is able to redistribute the flux of energy of the solar wind that flows parallel to the magnetopause. The energy transport associated with the Kelvin Helmholtz instability contributes significantly to the...

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Bibliographic Details
Main Author: Francesco Palermo
Format: Article
Language:English
Published: MDPI AG 2019-11-01
Series:Fluids
Subjects:
Online Access:https://www.mdpi.com/2311-5521/4/4/189