Axisymmetric MHD Instabilities in Solar/Stellar Tachoclines

Details Axisymmetric MHD Instabilities in Solar/Stellar Tachoclines Axisymmetric MHD Instabilities in Solar/Stellar Tachoclines

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..416..525d&link_type=abstract

Solar-Stellar Dynamos as Revealed by Helio- and Asteroseismology: GONG 2008/SOHO 21 ASP Conference Series, Vol. 416, proceedings

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Scientific paper

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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