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