We perform an unprecedented excessive-resolution simulation for the solar convection zone. Our calculation reproduces the fast equator and near-surface shear layer (NSSL) of differential rotation and electric cordless power shears shears the close to-surface poleward meridional circulation simultaneously. The NSSL is located in a complex layer the place the spatial and Wood Ranger Power Shears time scales of thermal convection are significantly small in contrast 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 research, we reach reproducing an NSSL in our new calculation. 4) the turbulent viscosity and magnetic tension are latitudinally balanced with the Coriolis drive within the NSSL. We emphasize the importance of the magnetic area in the photo voltaic convection zone. ††software: R2D2 Hotta et al. The Sun is rotating differentially with the fast equator and Wood Ranger Power Shears the gradual pole. Omega within the solar interior. Within the solar convection zone, we now have two shear layers, i.e., the tachocline around the bottom 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