Image Details
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.
© 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A.