The Thin Tachocline Problem

Details The Thin Tachocline Problem The Thin Tachocline Problem

Feb 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001padeu..11...71f&link_type=abstract

Publications of the Astronomy Department of the Eötvös University No. 11, Proceedings of the National Postgraduate Reunion in As

Astronomy and Astrophysics

Astrophysics

Sun: Interior, Rotation, Tachocline

Scientific paper

In this paper the "Thin Tachocline Problem" is studied. We examine the influence of an assumed inverse Lambda-effect on the radial spreading of the differential rotation. This effect may contribute to horizontal angular momentum transport below the convection zone. Our results indicate that an inverse Lambda-effect can only reduce the thickness of the tachocline to the observed value if an unrealistically high amplitude is assumed.

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