Spin-Down of Solar-Type Stars with Internal Magnetic Fields
1993 ◽
Vol 137
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pp. 464-468
Keyword(s):
AbstractWe present a selection of results from a large set of numerical simulations of the spin-down of a solar-type star containing a large scale magnetic field in its radiative interior. Our computations are dynamical, in that they take into account both the generation of the toroidal component by the wind-induced shear endits back-reaction on the azimuthal flow. Our results demonstrate the existence of classes of internal magnetic fields that can accomodate rapid spin-down near the ZAMS, and yield weak internal differential rotation by the solar age.
2012 ◽
Vol 8
(S294)
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pp. 367-368
2006 ◽
Vol 370
(1)
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pp. 468-476
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Keyword(s):
2015 ◽
Vol 11
(A29A)
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pp. 360-364
2008 ◽
Vol 4
(S259)
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pp. 75-80
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2010 ◽
Vol 6
(S274)
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pp. 381-384
Keyword(s):
2013 ◽
Vol 8
(S300)
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pp. 397-400
Keyword(s):