We carry out an unprecedented excessive-decision simulation for the photo voltaic convection zone. Our calculation reproduces the quick equator and near-surface shear layer (NSSL) of differential rotation and the close to-floor poleward meridional circulate concurrently. The NSSL is located in a complex layer where the spatial and professional landscaping shears 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 results are still removed 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 force in the NSSL. We emphasize the significance of the magnetic area in the photo voltaic convection zone. ††software: Wood Ranger Power Shears R2D2 Hotta et al. The Sun is rotating differentially with the quick equator and Wood Ranger Power Shears the gradual pole. Omega within the solar interior. Within the solar convection zone, we have now two shear layers, i.e., the tachocline round the bottom of the convection zone and the close to-surface shear layer (NSSL).

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