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.

Submitted to Solar Physics

References in corpus (6)

• Persistent Magnetic Wreaths in a Rapidly Rotating Sun
• Global Seismology of the Sun
• High-resolution calculation of the solar global convection with the reduced speed of sound technique: II. Near surface shear layer with the rotation
• Helioseismic Imaging of Fast Convective Flows Throughout the Near-Surface Shear Layer
• Latitudinal variation of the solar photospheric intensity
• A theoretical model of the variation of the meridional circulation with the solar cycle

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