Thermal Convection, Magnetic Field, and Differential Rotation in Solar-type Stars - Springer Theses Softcover reprint of the original 1st ed. 2015 edition

This thesis describes the studies on the solar interior where turbulent thermal convection plays an important role. The author solved, for the first time, one of the long-standing issues in solar physics, i.e., the maintenance mechanism of the solar differential rotation in the near-surface shear layer.