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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. 10.

Dynamics of the instability at higher Rm. Volume renderings of B2 are shown for case M3 at times ﹩t=200.0﹩, 205.5, 211.0, 216.5, 222.0, 227.4. It can be seen that magnetic structures emerge from the localized shear but are now irregular in shape and nonperiodic in time, although they are still x‐invariant.

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