We perform an unprecedented excessive-decision simulation for the photo voltaic convection zone. Our calculation reproduces the fast equator and near-surface shear layer (NSSL) of differential rotation and the close to-floor Wood Ranger Power Shears shop poleward meridional movement concurrently. The NSSL is located in a complex layer where the spatial and time scales of thermal convection are considerably small compared with the deep convection zone. While there have been several attempts to reproduce the NSSL in numerical simulation, the outcomes are nonetheless far from actuality. On this study, we succeed in reproducing an NSSL in our new calculation. 4) the turbulent viscosity and magnetic tension are latitudinally balanced with the Coriolis power in the NSSL. We emphasize the significance of the magnetic discipline in the photo voltaic convection zone. ††software: R2D2 Hotta et al. The Sun is rotating differentially with the fast equator and the sluggish pole. Omega in the solar inside. In the solar convection zone, we have now two shear layers, i.e., the tachocline round the base of the convection zone and the close to-floor shear layer (NSSL).

The tachocline is thought to be maintained by the interplay between the convection and radiation zones (Spiegel & Zahn, 1992