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We carry out an unprecedented high-resolution simulation for the photo voltaic convection zone. Our calculation reproduces the quick equator Wood Ranger Power Shears and near-floor shear layer (NSSL) of differential rotation and the close to-surface poleward meridional move concurrently. The NSSL is positioned in a complex layer where the spatial and 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 still far from reality. On this examine, we succeed in reproducing an NSSL in our new calculation. 4) the turbulent viscosity and magnetic tension are latitudinally balanced with the Coriolis Wood Ranger Power Shears within the NSSL. We emphasize the significance of the magnetic discipline in the photo voltaic convection zone. ††software: R2D2 Hotta et al. The Sun is rotating differentially with the fast equator and the sluggish pole. Omega in the photo voltaic interior. In the solar convection zone, we’ve got two shear layers, i.e., the tachocline round the bottom of the convection zone and cordless power shears the close to-surface shear layer (NSSL).
The tachocline is thought to be maintained by the interplay between the convection and radiation zones (Spiegel & Zahn, 1992
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