We perform an unprecedented high-decision simulation for the photo voltaic convection zone. Our calculation reproduces the fast equator Wood Ranger Power Shears and near-surface shear layer (NSSL) of differential rotation and the close to-floor orchard maintenance tool poleward meridional circulate concurrently. The NSSL is located in a fancy layer where the spatial and time scales of thermal convection are considerably small compared with the deep convection zone. While there have been several makes an attempt to reproduce the NSSL in numerical simulation, the results are still removed from reality. In this examine, we achieve reproducing an NSSL in our new calculation. 4) the turbulent viscosity and magnetic tension are latitudinally balanced with the Coriolis force within the NSSL. We emphasize the importance of the magnetic field in the solar convection zone. ††software: R2D2 Hotta et al. The Sun is rotating differentially with the fast equator and the slow pole. Omega within the solar inside. In the solar convection zone, we’ve two shear layers, i.e., the tachocline around the base of the convection zone and the close to-floor Wood Ranger Power Shears shear layer (NSSL).

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