A possible model for the fast solar tachocline

Details A possible model for the fast solar tachocline A possible model for the fast solar tachocline

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002padeu..12....7f&link_type=abstract

2nd Workshop of Young Researchers in Astronomy & Astrophysics, Publications of the Astronomy Department of the Eötvös University

Astronomy and Astrophysics

Astrophysics

Scientific paper

One possible scenario for the origin of the solar tachocline, known as the "fast tachocline", assumes that the turbulent diffusivity exceeds eta> 109 cm2/s. In this case the dynamics will be governed by the dynamo-generated oscillatory magnetic field on relatively short timescales. Here, we present detailed numerical models for the fast solar tachocline with all components of the magnetic field calculated explicitly, assuming axial symmetry and a constant turbulent diffusivity and viscosity.

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