We carry out an unprecedented high-resolution simulation for the solar convection zone. Our calculation reproduces the quick equator and near-floor shear layer (NSSL) of differential rotation and the close to-floor poleward meridional circulate concurrently. The NSSL is located in a posh layer where the spatial and time scales of thermal convection are considerably small in contrast with the deep convection zone. While there have been several makes an attempt to reproduce the NSSL in numerical simulation, the outcomes are nonetheless removed from reality. On this examine, we achieve reproducing an NSSL in our new calculation. 4) the turbulent viscosity and magnetic tension are latitudinally balanced with the Coriolis drive in the NSSL. We emphasize the significance of the magnetic area in the solar convection zone. ††software: R2D2 Hotta et al. The Sun is rotating differentially with the fast equator Wood Ranger Power Shears and the gradual pole. Omega in the photo voltaic interior. In the photo voltaic convection zone, we've two shear layers, i.e., the tachocline around the base of the convection zone and the close to-floor shear layer (NSSL).
The tachocline is thought to be maintained by the interaction between the convection and radiation zones (Spiegel & Zahn, 1992