Fig. 15 from On the Formation of Magnetic Structures by the Combined Action of Velocity Shear and Magnetic Buoyancy

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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. 15.

Poloidal signature of the secondary KH instability. We show the maximum values of (a) ﹩v﹩ and (b) w within the computational domain as functions of time for case VA3. Notice that the values of the poloidal flows are small except in short intermittent bursts when the KH instability kicks in.

Other Images in This Article

Copyright and Terms & Conditions