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Paper: |
Axisymmetric MHD Instabilities in Solar/Stellar Tachoclines |
Volume: |
416, Solar-Stellar Dynamos as Revealed by Helio- and Asteroseismology: GONG 2008/SOHO 21 |
Page: |
525 |
Authors: |
Dikpati, M.; Cally, P. S.; Gilman, P. A.; Miesch, M. S. |
Abstract: |
We show that banded toroidal fields in the tachoclines of the Sun and other stars should be unstable to 3-D axisymmetric overturning modes if the peak toroidal field is ∼100 kG or more. This instability should fragment and limit the amplitude of toroidal fields in tachoclines. |
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