We carry out 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-surface poleward meridional stream simultaneously. The NSSL is located in a posh layer where the spatial and time scales of thermal convection are considerably small compared with the deep convection zone. While there have been a number of attempts to reproduce the NSSL in numerical simulation, the outcomes are nonetheless far from reality. In this research, we achieve reproducing an NSSL in our new calculation. 4) the turbulent viscosity and magnetic tension are latitudinally balanced with the Coriolis pressure within the NSSL. We emphasize the importance of the magnetic subject within the photo voltaic convection zone. ††software: R2D2 Hotta et al. The Sun is rotating differentially with the quick equator and Wood Ranger Power Shears the gradual pole. Omega within the photo voltaic interior. Within the solar convection zone, we have now two shear layers, i.e., Wood Ranger Power Shears the tachocline around the base of the convection zone and the near-floor shear layer (NSSL).

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