Can an inverse Λ-effect explain the thin tachocline?

Physics

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Sun: Interior, Rotation, Circulation

Scientific paper

Helioseismic measurements indicate the existence of a transition layer (the tachocline) between the differentially rotating convection zone and the rigidly rotating radiative interior. According to the theoretical models, the differential rotation should penetrate into the deep layers of the radiative interior, but, based on helioseismic measurements, the tachocline is thin. This is known as the "Thin Tachocline Problem". In this paper we examine the influence of an assumed inverse Λ-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 Λ-effect can only reduce the thickness of the tachocline to the observed value if an unrealistically high amplitude is assumed. Thus, our results practically exclude the possibility that the thin tachocline is a consequence of a Λ-effect.

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