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astro-ph2008
The generation and stability of magnetic fields in CP stars
R. Arlt
A variety of magnetohydrodynamic mechanisms that may play a role in magnetic, chemically peculiar (mCP) stars is reviewed. These involve dynamo mechanisms in laminar flows as well…
astro-ph2004
A numerical MHD model for the solar tachocline
A. Sule, R. Arlt, G. Ruediger
There are successful approaches to explain the formation of the tachocline by a poloidal magnetic field in the solar core. We present here the first MHD simulations of the solar ta…