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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. 18.

Scalar signatures of the case VA4, where KH events are occurring continuously rather than intermittently. Plotted are the maxima of (a) u and (b) Bx (solid line) and the modulus of the minimum of Bx (dashed line) as before.

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