The Zigzag Path of Buoyant Magnetic Tubes and the Generation of Vorticity along Their Periphery
We study the generation of vorticity in the magnetic boundary layer of buoyant magnetic tubes and its consequences for the trajectory of magnetic structures rising in the solar convection zone. When the Reynolds number is well above 1, the wake trailing the tube sheds vortex rolls, producing a von Kármán vortex street, similar to the case of flows
Emonet, T. et al.
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2001