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On the Formation of Magnetic Structures by the Combined Action of Velocity Shear and Magnetic Buoyancy

  • Authors: Kelly S. Cline, Nicholas H. Brummell, and Fausto Cattaneo

Cline, Brummell, & Cattaneo 2003 The Astrophysical Journal 588 630.

  • Provider: AAS Journals

Caption: Fig. 12.

Breaking of the x‐invariance by magnetically induced KH instabilities. This figure shows volume renderings of B2 from case VA3 at ﹩t=346.7﹩, 348.6, 350.5. The emerging magnetic structure can be seen to be twisted by the action of KH modes as it rises out of the localized shear zone.

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