A theoretical estimate of the pole-equator temperature difference and a possible origin of the near-surface shear layer

Abstract

Convective motions in the deep layers of the solar convection zone are affected by rotation, making the convective heat transport latitude-dependent, but this is not the case in the top layers near the surface. We use the thermal wind balance condition in the deeper layers to estimate the pole-equator temperature difference. Surface observations of this temperature difference can be used for estimating the depth of the near-surface layer within which convection is not affected by rotation. If we require that the thermal wind balance holds in this layer also, then we have to conclude that this must be a layer of strong differential rotation and its characteristics which we derive are in broad agreement with the observational data of the near-surface shear layer.

arXiv commentSubmitted to Solar Physics

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Cited by in corpus (3)

• Mean field models of flux transport dynamo and meridional circulation in the Sun and stars
• A Theoretical Model of the Near Surface Shear Layer of the Sun
• The stellar thermal wind as a consequence of oblateness