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- 5Auroral Arcs
- 5Kelvin-Helmholtz Instability
- 4Evolution
- 4Field Line Resonances
- 3Alfven Waves
- 2Dynamics
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1999
Tikhonchuk, V. T., Voronkov, I., Samson, J. C., Rankin, Robert
The three-dimensional, nonlinear evolution of a shear how (or Kelvin-Helmholtz (KH)) instability driven by a large-amplitude shear Alfven wave (SAW) in the Earth's magnetosphere is studied by using numerical solutions to the complete set of ideal magnetohydrodynamic equations. An initial setup is...
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