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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. 4.

Buildup of the velocity and magnetic fields with time for the case M1. Shown are the maximum values over the computational domain of (a) u and (b) ﹩\left|B_{x}\right|﹩ as functions of time. Both begin at zero, increase, and then saturate in value when the nonstatic equilibrium state is reached in this case.

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