Nonlinear evolution of the magnetized Kelvin-Helmholtz instability: From fluid to kinetic modeling-Reference-Cited by-同舟云学术

Nonlinear evolution of the magnetized Kelvin-Helmholtz instability: From fluid to kinetic modeling

Published:2013-10 Issue:10 Volume:20 Page:102118
ISSN:1070-664X
Container-title:Physics of Plasmas
language:en
Short-container-title:Physics of Plasmas

Author:

Henri P.,Cerri S. S.,Califano F.,Pegoraro F.,Rossi C.,Faganello M.,Šebek O.,Trávníček P. M.,Hellinger P.,Frederiksen J. T.,Nordlund A.,Markidis S.,Keppens R.,Lapenta G.

Publisher

AIP Publishing

Subject

Condensed Matter Physics

Link

http://aip.scitation.org/doi/pdf/10.1063/1.4826214

Reference42 articles.

1. The Solar Wind as a Turbulence Laboratory

2. Geotail observations of the Kelvin-Helmholtz instability at the equatorial magnetotail boundary for parallel northward fields

3. Transport of solar wind into Earth's magnetosphere through rolled-up Kelvin–Helmholtz vortices

4. Cassini observations of a Kelvin-Helmholtz vortex in Saturn's outer magnetosphere

5. Reconstruction of propagating Kelvin–Helmholtz vortices at Mercury's magnetopause

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